Towards Real Utopias in Higher Education

ERIC Educational Resources Information Center

Suoranta, Juha; FitzSimmons, Robert

2017-01-01

In this article we search for real utopias for higher education by first introducing and describing a vital counter-hegemonic students movement of the early 1960s--Students for a Democratic Society (SDS), and their Port Huron Statement (1962). The movement maintained that universities are not communities of equals but served the elite. In the…

Geology of the Southern Utopia Planitia Highland-Lowland Boundary Plain: Second Year Results and Third Year Plan

NASA Technical Reports Server (NTRS)

Skinner, J. A., Jr.; Tanaka, K. L.; Hare, T. M.

2009-01-01

The southern Utopia highland-lowland boundary (HLB) extends >1500 km westward from Hyblaeus Dorsa to the topographic saddle that separates Isidis and Utopia Planitiae. It contains bench-like platforms that contain depressions, pitted cones (some organized into arcuate chains and thumb-print terrain), isolated domes, buried circular depressions, ring fractures, polygonal fractures, and other locally- to regionally-dispersed landforms [1-2]. The objective of this map project is to clarify the geologic evolution of the southern Utopia Planitia HLB by identifying the geologic, structural, and stratigraphic relationships of surface materials in MTMs 10237, 15237, 20237, 10242, 15242, 20242, 10247, 15247, and 20247. The project was originally awarded in April, 2007 and is in its final year of support. Mapping is on-schedule and formal map submission will occur by December, 2009, with finalization anticipated by April, 2010. Herein, we (1) review specifics regarding mapping data and methods, (2) present nomenclature requests that we feel will assist with unit descriptions, (3) describe Year 2 mapping and science accomplishments, and (4) outline Year 3 technical and managerial approaches for finalizing the geologic map.

Dreaming of a Better Life: Utopia as a Focus for Thematic, Interdisciplinary Instruction

ERIC Educational Resources Information Center

Resor, Cynthia; Gandy, S. Kay

2014-01-01

Throughout history humans have dreamed of a better life. This concept of utopia can be used as a central focus for thematic and interdisciplinary instruction. This approach has three key advantages. First, students recognize that certain themes are consistent across time and place and that realization can lead students to explore their own dreams…

Needing "Tomorrow as Fish Need Water": Dystopia, Utopia, and Freire's Pedagogy

ERIC Educational Resources Information Center

Papastephanou, Marianna

2016-01-01

In this article, I discuss the philosophical-educational attention to Freire's utopian pedagogy of the future and I argue that equal attention should be due to Freire's dystopian account of the present. To this end, Freire's utopia and dystopia are associated with the interplay of his notions of annunciation and denunciation. The role of dystopian…

Beyond Rural Idylls: Imperfect Lesbian Utopias at Michigan Womyn's Music Festival

ERIC Educational Resources Information Center

Browne, Kath

2011-01-01

Whilst rural idylls have dominated some discussions of rural social difference, little attention has been paid to rural utopias. Imagined, material and discursive experiences of utopian rural ideals are critically examined in this paper. It takes as its focus the Michigan Womyn's Music Festival--an annual US womyn-only festival--in order to…

Deaf Utopias? Reviewing the Sociocultural Literature on the World's "Martha's Vineyard Situations"

ERIC Educational Resources Information Center

Kusters, Annelies

2010-01-01

Martha's Vineyard--an island off the East Coast of the United States--is known as a community where "everyone signed" for several hundred years, a utopia in the eyes of many Deaf people. Currently, there exist around the world a number of small similar "shared signing communities," for example, in Mexico, Bali, Israel, and…

Buried topography of Utopia, Mars - Persistence of a giant impact depression

NASA Technical Reports Server (NTRS)

Mcgill, George E.

1989-01-01

Knobs, partially buried craters, ring fractures, and some mesas permit a qualitative determination of the topography buried beneath younger northern plains materials. These features are widely distributed in the Utopia area but are absent in a large, roughly circular region centered at about 48 deg N, 240 deg W. This implies the existence of a circular depression about 3300 km in diameter buried beneath Utopia Planitia that is interpreted to represent the central part of a very large impact basin. The presence of buried curved massifs around part of this depression, and a roughly coincident mascon, lend further support. Present topography, areal geology, and paleotopography of buried surfaces all point to the persistence of this major depression for almost the entire history of Mars.

Utopia Cracks and Polygons

NASA Technical Reports Server (NTRS)

2003-01-01

MGS MOC Release No. MOC2-339, 23 April 2003

This Mars Global Surveyor (MGS) Mars Orbiter Camera (MOC) image shows a pattern of polygonal cracks and aligned, elliptical pits in western Utopia Planitia. The picture covers an area about 3 km (about 1.9 mi) wide near 44.9oN, 274.7oW. Sunlight illuminates the scene from the left.

Technology, Utopia and Scholarly Life: Ideals and Realities in the Work of Hermann Hesse

ERIC Educational Resources Information Center

Roberts, Peter

2009-01-01

This article considers the relationship between technology, utopia and scholarly life in Hermann Hesse's novel, "The Glass Bead Game." In the first part of Hesse's book, the Glass Bead Game and the society of which it is a part, Castalia, are portrayed in idealistic terms. The second part of the novel chronicles the educational life of Joseph…

Mud volcanism and morphology of impact craters in Utopia Planitia on Mars: Evidence for the ancient ocean

NASA Astrophysics Data System (ADS)

Ivanov, Mikhail A.; Hiesinger, H.; Erkeling, G.; Reiss, D.

2014-01-01

Results of our detailed geological mapping and interpretation of the nature and relative and absolute model ages of units and structures in the SW portion of Utopia Planitia (20-45°N, 100-120°E) suggest the following. (1) The size-frequency distribution (SFD) of craters that both are buried by materials of the Vastitas Borealis units (VB) and superpose its surface indicate that the absolute model ages of terrain predating the emplacement of the VB is ˜3.7 Ga. (2) Lack of craters that are partly embayed by materials of the VB in the SW portion of Utopia Planitia implies that the emplacement of the VB was faster than the rate of accumulation of impact craters and is consistent with the geologically short time of emplacement of the VB due to catastrophic release of water from outflow channels (e.g., Carr, M.H. [1996]. Water on Mars. Oxford University Press, New York, p. 229). (3) The SFD of craters that superpose the surface of the VB indicates an absolute model age of ˜3.6-3.5 Ga. The absolute model ages of etched flows, which represent the upper stratigraphic limit of the VB, are estimated to be ˜3.5 Ga. (4) The majority of the larger (i.e., >1 km) impact craters show ejecta morphologies (rampart and pancake-like ejecta) that are indicative of the presence of ice/water in the target materials. The distal portions of the pancake-like ejecta are heavily degraded (not due to embayment). This suggests that these craters formed in targets that contained higher abundances of volatiles. (5) The diameter ranges of the craters with either rampart- or pancake-like ejecta are overlapping (from ˜2 to ˜60 km). Craters with pancake-like ejecta are concentrated within the central portion of the Utopia basin (less than ˜1000 km from the basin center) and rampart craters occur at the periphery of the basin. This pattern of the crater spatial distribution suggests that materials within the center of Utopia Planitia contained more ice/water. (6) Etched flows around the central portion of Utopia Planitia were erupted from beneath of the surface of the VB. Their morphology and pattern of degradation, however, are inconsistent with lava and, instead, indicate formation of the flows due to mud volcanism. (7) Etched flows are spatially associated with giant polygons and there is evidence that these features populated the center portion of Utopia Planitia before it was covered by the Elysium-derived units. The outer (southern) edge of the zone of polygonal troughs and etched flows approximately corresponds to the transition from pancake-like ejecta to rampart ejecta. This suggest that the outer edge of the zone of the polygons and flows may outline the deeper portions of the large body (˜2000 km across) of water/ice that likely existed in the center of Utopia Planitia in late Hesperian.

State of Utopia v. Jamie Davidson. 2002-2003 Oklahoma High School Mock Trial Program.

ERIC Educational Resources Information Center

Benischek, Sandra; Davis, Courtney; Horton, Johnathan; Longwell, Nicole; Williams, Keri

In the spring of 2001, illegal drug use had risen by 40% among teens in the town of Springdale, Utopia. School administrators and the Springdale Police Department decided to implement a crackdown on teen drug use in all high schools in Springdale. A high school principal received a tip on a hotline that Jamie Davidson, a senior, had been seen…

A Failed Utopia in Marcela Del Río's "Proceso a Faubritten"

ERIC Educational Resources Information Center

Manickam, Samuel

2014-01-01

In Marcela del Río's science fiction novel "Proceso a Faubritten," utopia comes in the form of eternal life for all of humanity, thanks to Dr. Alexander Faubritten's "Bomba L." This polyphonic work includes diaries by Faubritten and his Mexican lover, María Corona. In my analysis of these two diaries, I will show how…

Evidence for and implications of sedimentary diapirism and mud volcanism in the southern Utopia highland-lowland boundary plain, Mars

USGS Publications Warehouse

Skinner, J.A.; Tanaka, K.L.

2007-01-01

Several types of spatially associated landforms in the southern Utopia Planitia highland-lowland boundary (HLB) plain appear to have resulted from localized geologic activity, including (1) fractured rises, (2) elliptical mounds, (3) pitted cones with emanating lobate materials, and (4) isolated and coalesced cavi (depressions). Stratigraphic analysis indicates these features are Hesperian or younger and may be associated with resurfacing that preferentially destroyed smaller (< 8 ?? km diameter) impact craters. Based on landform geomorphologies and spatial distributions, the documented features do not appear to be specifically related to igneous or periglacial processes or the back-wasting and erosion of the HLB scarp. We propose that these features are genetically related to and formed by sedimentary (mud) diapirs that ascended from zones of regionally confined, poorly consolidated, and mechanically weak material. We note morphologic similarities between the mounds and pitted cones of the southern Utopia boundary plain and terrestrial mud volcanoes in the Absheron Peninsula, Azerbaijan. These analogs provide a context for understanding the geological environments and processes that supported mud diapir-related modification of the HLB. In southern Utopia, mud diapirs near the Elysium volcanic edifice may have resulted in laccolith-like intrusions that produced the fractured rises, while in the central boundary plain mud diapirs could have extruded to form pitted cones, mounds, and lobate flows, perhaps related to compressional stresses that account for wrinkle ridges. The removal of material a few kilometers deep by diapiric processes may have resulted in subsidence and deformation of surface materials to form widespread cavi. Collectively, these inferences suggest that sedimentary diapirism and mud volcanism as well as related surface deformations could have been the dominant Hesperian mechanisms that altered the regional boundary plain. We discuss a model in which detritus would have accumulated thickly in the annular spaces between impact-generated structural rings of Utopia basin. We envision that these materials, and perhaps buried ejecta of Utopia basin, contained volatile-rich, low-density material that could provide the source material for the postulated sedimentary diapirs. Thick, water-rich, low-density sediments buried elsewhere along the HLB and within the lowland plains may account for similar landforms and resurfacing histories. ?? 2006 Elsevier Inc. All rights reserved.

Polygons in Utopia

NASA Technical Reports Server (NTRS)

2005-01-01

14 April 2005 This Mars Global Surveyor (MGS) Mars Orbiter Camera (MOC) image shows a typical view of polygon-cracked and pitted surfaces unique to western Utopia Planitia. No other place on Mars has this appearance. Some Mars scientists have speculated that ground ice may be responsible for these landforms.

Location near: 42.3oN, 275.6oW Image width: 3 km (1.9 mi) Illumination from: lower left Season: Northern Summer

An Analysis and Comparison of Two Short Writings: "Inaugural Address at the University of St. Andrew's" by J.S. Mill and "The University of Utopia" by R.M. Hutchins, Based on Five Criteria.

ERIC Educational Resources Information Center

Poirier, Jeannine M.

Focusing on the concept of education for work vs. education for living, the author presents a comparative analysis of two works on liberal education, each of which was originally delivered orally to university students: "The Inaugural Address at the University of St. Andrew" by John Stuart Mill and "The University of Utopia" by…

Utopia Planitia

NASA Technical Reports Server (NTRS)

2002-01-01

(Released 15 May 2002) The Science This image is located in Utopia Planitia, a large plain in the northern hemisphere. It is believed that this basin is the result of a large impact. On the right side of the image is a partially imaged crater with a well-preserved ejecta blanket. The morphology of the ejecta implies that the crater is young relative to the surrounding material and has not undergone extensive deposition or erosion. Surrounding the crater are polygonal troughs in the smooth surface material. This polygon pattern is relatively common in the northern plains of Mars, and are primarily located in Acidalia Planitia, Elysium Planitia, and Utopia Planitia. These troughs are believed to be small grabbens, however, scientist are currently debating the origin of these features. The two most accepted hypotheses are that these grabbens either form as volcanic material cools and contracts, or are produced as sediment shrinks as a result of compaction. The Story When you think of Utopia, you probably don't think of a large Martian plain, riddled with troughs and pockmarked by craters. Of course, it may actually be a more fitting name than you think. When Sir Thomas More wrote his book about a fictitiously optimal place guided and governed by reason, he made up the word utopia from Greek words meaning 'nowhere.' Utopia Planitia became 'somewhere' for the first time, however, when its first visitor, the Viking 2 lander, settled down and analyzed the area. And scientists today are using their own reasoning and logic to discern even more about how this northern Martian plain developed geologically. Right now, scientists have two hypotheses for how the troughs seen here were formed. Because Utopia Planitia is a volcanic region of Mars, these rifts in the surface could have formed when volcanic material cooled and then contracted. Alternatively, this area might be made up of a lot of sediments - small particles of rock, soil, and dust deposited in the area. Just like any loose material, it could have compacted together in places or 'shrunk down' to create the lowered rifts in the terrain. The polygonal patterns of these troughs can be seen more widely in the context image to the right. On Earth, we can sometimes see this pattern occurring in the Arctic and subarctic, where permafrost creates polygonal, 'frozen-soil wedges' that form an almost honeycomb pattern throughout the terrain. We know from Viking 2 pictures that it can be pretty cold in this area, as a thin layer of white ground frost was observed there during a few of the Martian winters. The whiter, brighter material near the crater, however, isn't frost or snow, but instead the record of all of the material that was once ejected from the crater at the left-hand-side of the image. You can see by the smoothness of the crater rim and the clarity of where the ejected material landed that there hasn't been much erosion. That means this crater is fairly young.

Utopia documents: linking scholarly literature with research data

PubMed Central

Attwood, T. K.; Kell, D. B.; McDermott, P.; Marsh, J.; Pettifer, S. R.; Thorne, D.

2010-01-01

Motivation: In recent years, the gulf between the mass of accumulating-research data and the massive literature describing and analyzing those data has widened. The need for intelligent tools to bridge this gap, to rescue the knowledge being systematically isolated in literature and data silos, is now widely acknowledged. Results: To this end, we have developed Utopia Documents, a novel PDF reader that semantically integrates visualization and data-analysis tools with published research articles. In a successful pilot with editors of the Biochemical Journal (BJ), the system has been used to transform static document features into objects that can be linked, annotated, visualized and analyzed interactively (http://www.biochemj.org/bj/424/3/). Utopia Documents is now used routinely by BJ editors to mark up article content prior to publication. Recent additions include integration of various text-mining and biodatabase plugins, demonstrating the system's ability to seamlessly integrate on-line content with PDF articles. Availability: http://getutopia.com Contact: teresa.k.attwood@manchester.ac.uk PMID:20823323

Geology of the MER 2003 "Elysium" candidate landing site in southeastern Utopia Planitia, Mars

USGS Publications Warehouse

Tanaka, K.L.; Carr, M.H.; Skinner, J.A.; Gilmore, M.S.; Hare, T.M.

2003-01-01

The NASA Mars Exploration Rover (MER) Project has been considering a landing-site ellipse designated EP78B2 in southeastern Utopia Planitia, southwest of Elysium Mons. The site appears to be relatively safe for a MER landing site because of its predicted low wind velocities in mesoscale atmospheric circulation models and its low surface roughness at various scales as indicated by topographic and imaging data sets. Previously, the site's surface rocks have been interpreted to be marine sediments or lava flows. In addition, we suggest that Late Noachian to Early Hesperian collapse and mass wasting of Noachian highland rocks contributed to the deposition of detritus in the area of the ellipse. Furthermore, we document partial Late Hesperian to Early Amazonian resurfacing of the ellipse by flows and vents that may be of mud or silicate volcanic origin. A rover investigation of the Utopia landing site using the MER Athena instrument package might address some fundamental aspects of Martian geologic evolution, such as climate change, hydrologic evolution, and magmatic and tectonic history. Copyright 2003 by the American Geophysical Union.

Utopia Providing Trusted Social Network Relationships within an Un-trusted Environment

NASA Astrophysics Data System (ADS)

Gauvin, William; Liu, Benyuan; Fu, Xinwen; Wang, Jie

This paper introduces an unobtrusive method and distributed solution set to aid users of on-line social networking sites, by creating a trusted environment in which every member has the ability to identify each other within their private social network by name, gender, age, location, and the specific usage patterns adopted by the group. Utopia protects members by understanding how the social network is created and the specific aspects of the group that make it unique and identifiable. The main focus of Utopia is the protection of the group, and their privacy within a social network from predators and spammers that characteristically do not fit within the well defined usage boundaries of the social network as a whole. The solution set provides defensive, as well as offensive tools to identify these threats. Once identified, client desktop tools are used to prevent these predators from further interaction within the group. In addition, offensive tools are used to determine the origin of the predator to allow actions to be taken by automated tools and law enforcement to alleviate the threat.

Ambrosius Holbein's memento mori map for Sir Thomas More's Utopia. The meanings of a masterpiece of early sixteenth century graphic art.

PubMed

Bishop, M

2005-07-23

This paper describes how, and asks why, the Renaissance artist Ambrosius Holbein hid a skull within the overall design of his woodcut map of Sir Thomas More's Utopia. (Fig. 2) This map was prepared for the 1518 Froben edition of the book, and was probably commissioned by Erasmus of Rotterdam. Its identification now is made easier by the habits of interpretation with which all dentists are equipped thanks to their skill in dental radiology, and by the recognition of teeth appearing in an unlikely disguise.

Possible pingos and a periglacial landscape in northwest Utopia Planitia

USGS Publications Warehouse

Soare, R.J.; Burr, D.M.; Wan, Bun Tseung J.-M.

2005-01-01

Hydrostatic (closed-system) pingos are small, elongate to circular, ice-cored mounds that are perennial features of some periglacial landscapes. The growth and development of hydrostatic pingos is contingent upon the presence of surface water, freezing processes and of deep, continuous, ice-cemented permafrost. Other cold-climate landforms such as small-sized, polygonal patterned ground also may occur in the areas where pingos are found. On Mars, landscapes comprising small, elongate to circular mounds and other possible periglacial features have been identified in various areas, including Utopia Planitia, where water is thought to have played an important role in landscape evolution. Despite the importance of the martian mounds as possible markers of water, most accounts of them in the planetary science literature have been brief and/or based upon Viking imagery. We use a high-resolution Mars Orbiter Camera image (EO300299) and superposed Mars Orbiter Laser Altimeter data tracks to describe and characterise a crater-floor landscape in northwest Utopia Planitia (64.8?? N/292.7?? W). The landscape comprises an assemblage of landforms that is consistent with the past presence of water and of periglacial processes. This geomorphological assemblage may have formed as recently as the last episode of high obliquity. A similar assemblage of landforms is found in the Tuktoyaktuk peninsula of northern Canada and other terrestrial cold-climate landscapes. We point to the similarity of the two assemblages and suggest that the small, roughly circular mounds on the floor of the impact crater in northwest Utopia Planitia are hydrostatic pingos. Like the hydrostatic pingos of the Tuktoyaktuk peninsula, the origin of the crater-floor mounds could be tied to the loss of ponded, local water, permafrost aggradation and the evolution of a sub-surface ice core. ?? 2004 Elsevier Inc. All rights reserved.

Modeling and observational occurrences of near-surface drainage in Utopia Planitia, Mars

NASA Astrophysics Data System (ADS)

Costard, F.; Sejourne, A.; Kargel, J.; Godin, E.

2016-12-01

During the past 15 years, evidence for an ice-rich planet Mars has rapidly mounted, become increasingly varied in terms of types of deposits and types of observational data, and has become more widespread across the surface. The mid-latitudes of Mars, especially Utopia Planitia, show many types of interesting landforms similar to those in periglacial landscapes on Earth that suggest the presence of ice-rich permafrost. These include thermal contraction polygonal networks, scalloped terrains similar to thermokarst pits, debris flows, small mounds like pingos and rock glaciers. Here, we address questions concerning the influence of meltwater in the Utopia Planitia (UP) landscape using analogs of near-surface melting and drainage along ice-wedge troughs on Bylot Island, northern Canada. In Utopia Planitia, based on the identification of sinuous channel-like pits within polygonal networks, we suggest that episodic underground melting was possible under severe periglacial climate conditions. In UP, the collapse pattern and morphology of unconnected sinuous elongated pits that follow the polygon crack are similar to underground melting in Bylot Island (Nunavut, Canada). Based on this terrestrial analogue, we develop a thermal model that consists of a thick insulating dusty layer over ice-saturated dust during a period of slight climatic warming relative to today's climate. In the model, the melting point is reached at depths down to 150 m. We suggest that small-scale melting could have occurred below ground within ground-ice polygonal fractures and pooled in underground cavities. Then the water may have been released episodically causing mechanical erosion as well as undermining and collapse. After melting, the dry surface dusty layer might have been blown away, thus exposing the degraded terrain of the substrate layer.

Student Evaluation of UTOPIA

ERIC Educational Resources Information Center

Pearson, M.; Carswell, D. J.

1978-01-01

Reports some reactions and opinions of the students to a course in nuclear and radiation chemistry using programmed instructional aids. Concludes that the findings were very favorable to the course. (GA)

Scalloped Terrain Led to Finding of Buried Ice on Mars

NASA Image and Video Library

2016-11-22

This vertically exaggerated view shows scalloped depressions in Mars Utopia Planitia region, prompting using ground-penetrating radar aboard NASA Mars Reconnaissance Orbiter to check for underground ice.

Kos, Dresden, Utopia... A journey through idealism past and present in public health.

PubMed

Mackenbach, Johan

2005-01-01

This essay reviews some of the sources of idealism in public health, on the basis of an intellectual journey to Kos (home to Hippocrates and his altruistic legacy), Dresden (where the Deutsches Hygiene Museum illustrates the historical connections between fascism and public health), and Utopia (exemplified by Etienne Cabet's Icarie, a fantasy of an ideal city which has nevertheless been partly realized). It is suggested that the large-scale altruism of public health has to be balanced with the value of individual autonomy, and that some degree of dreaming of a better and healthier world is indispensable for further progress in public health. The main conclusion is that the ethical foundations of public health are not always self-evident, and that critical reflection on these foundations was, is, and will always be necessary.

Boulder Strewn Plain in Northern Utopia Planitia

NASA Image and Video Library

2010-03-31

This image taken by NASA Mars Reconnaissance Orbiter in the Cydnus Rupes region, shows that the northern plains of Mars are rock and boulder strewn landscapes otherwise devoid of major features except a few impact craters.

Doublet Crater

NASA Image and Video Library

2010-12-22

This image from NASA Mars Odyssey is of a doublet crater located in Utopia Planitia, near the Elysium Volcanic region. Doublet craters are formed by simultaneous impact of a meteor that broke into two pieces prior to hitting the surface.

Soft robot design methodology for `push-button' manufacturing

NASA Astrophysics Data System (ADS)

Paik, Jamie

2018-06-01

`Push-button' or fully automated manufacturing would enable the production of robots with zero intervention from human hands. Realizing this utopia requires a fundamental shift from a sequential (design-materials-manufacturing) to a concurrent design methodology.

Scandinavia: A Racial Utopia?

ERIC Educational Resources Information Center

Weisbord, Robert G.

1972-01-01

Isolated personal observations have shaped the racial image of the Nordic countries--that Scandinavia is a racial paradise; this image is, however, simplistic, superficial, and one-dimensional. There is no gainsaying that prejudice against certain ethnic groups exists in Scandinavia. (Author)

Outwash plains and thermokarst on Mars

USGS Publications Warehouse

Costard, F.M.; Kargel, J.S.

1995-01-01

The spatial distribution of different types of rampart craters on Mars suggests a hemispheric asymmetry in the distribution of ground ice. The northern plains, especially major topographic depressions near the terminations of outflow channels, have high percentages of rampart craters. Two of these basins, Acidalia and Utopia Planitiae, received extraordinarily large amounts of water and sediment from the Chryse and Elysium outflow channels. In both regions, the analysis of high-resolution Viking pictures (12 m/pixel) indicates a concentration of kilometer-scale depressions that are similar in size and form to thermokarstic features in Yakutia (Siberia) and parts of the arctic coastal plain of North America. Accordingly, we infer that (1) Utopia Planitia and Acidalia Planitia may contain thick, laterally continuous, ice-rich sedimentary deposits related to outflow channel-forming floods, and (2) these areas of Mars may have experienced thermokarstic processes similar to modern thermokarstic processes in some periglacial regions of Earth.

Lunar and Planetary Science XXXV: Mars Geophysics

NASA Technical Reports Server (NTRS)

2004-01-01

The titles in this section include: 1) An Extraordinary Magnetic Field Map of Mars; 2) Mapping Weak Crustal Magnetic Fields on Mars with Electron Reflectometry; 3) Analytic Signal in the Interpretation of Mars Southern Highlands Magnetic Field; 4) Modeling of Major Martian Magnetic Anomalies: Further Evidence for Polar Reorientations During the Noachian; 5) An Improved Model of the Crustal Structure of Mars; 6) Geologic Evolution of the Martian Dichotomy and Plains Magnetization in the Ismenius Area of Mars; 7) Relaxation of the Martian Crustal Dichotomy Boundary in the Ismenius Region; 8) Localized Tharsis Loading on Mars: Testing the Membrane Surface Hypothesis; 9) Thermal Stresses and Tharsis Loading: Implications for Wrinkle Ridge Formation on Mars; 10) What Can be Learned about the Martian Lithosphere from Gravity and Topography Data? 11) A Gravity Analysis of the Subsurface Structure of the Utopia Impact Basin; 12) Mechanics of Utopia Basin on Mars; 13) Burying the 'Buried Channels' on Mars: An Alternative Explanation.

Small-scale martian polygonal terrain: Implications for liquid surface water

USGS Publications Warehouse

Seibert, N.M.; Kargel, J.S.

2001-01-01

Images from the Mars Orbiter Camera (MOC) through August 1999 were analyzed for the global distribution of small-scale polygonal terrain not clearly resolved in Viking Orbiter imagery. With very few exceptions, small-scale polygonal terrain occurs at middle to high latitudes of the northern and southern hemisphere in Hesperian-age geologic units. The largest concentration of this terrain occurs in the Utopia basin in close association with scalloped depressions (interpreted as thermokarst) and appears to represent an Amazonia event. The morphology and occurence of small polygonal terrain suggest they are either mud desiccation cracks or ice-wedge polygons. Because the small-scale polygons in Utopia and Argyre Planitiae are associated with other cold-climate permafrost or glacial features, an ice-wedge model is preferred for these areas. Both cracking mechanisms work most effectively in water- or ice-rich finegrained material and may imply the seasonal or episodic existence of liquid water at the surface.

Discriminating utopian from dystopian literature: Why is walden two considered a dystopia?

PubMed Central

Newman, Bobby

1993-01-01

Skinner thought of Walden Two as a utopia, but many literary critics consider it a dystopia. The present paper examines works by several authors of utopian literature in an effort to determine what elements lead critics to classify works as “dystopian.” Common elements seem to include (a) suspicion of scientific social planning, (b) the unhappiness of the characters portrayed, (c) suspicion of sources of control of behavior outside the individual, (d) violation of a presumed inherent need to struggle, and (e) suspicion of behavioral methods of governance. The elements Walden Two shares with other utopias and dystopias are examined, and the conclusion is offered that Walden Two could not be considered a dystopia for any of the traditional reasons. Instead, the negative view of Walden Two seems to be an outgrowth of literary devices and general negative reactions to behavioral determinism. PMID:22478144

Center is at Latitude 30 Degrees South, Longitude 210 Degrees

NASA Image and Video Library

1998-06-08

The lowland plains of Elysium and Utopia Planitiae are separated from the darker heavily cratered highlands by a broad escarpment in this image from NASA's Viking Orbiter 1. http://photojournal.jpl.nasa.gov/catalog/PIA00196

Rehabilitation with Cystic Fibrosis: From Utopia to Reality.

ERIC Educational Resources Information Center

Goldberg, Richard T.; And Others

1980-01-01

The paper dispels some of the myths regarding cystic fibrosis (a genetic metabolism disorder), provides information on the latest developments in rehabilitation, summarizes research in the field, and projects future needs of the patient with cystic fibrosis. (SBH)

An Inversion of Gravity and Topography for Mantle and Crustal Structure on Mars

NASA Technical Reports Server (NTRS)

Kiefer, Walter S.; Bills, Bruce G.; Nerem, R. Steven

1996-01-01

Analysis of the gravity and topography of Mars presently provides our primary quantitative constraints on the internal structure of Mars. We present an inversion of the long-wavelength (harmonic degree less than or equal to 10) gravity and topography of Mars for lateral variations of mantle temperature and crustal thickness. Our formulation incorporates both viscous mantle flow (which most prior studies have neglected) and isostatically compensated density anomalies in the crust and lithosphere. Our nominal model has a 150-km-thick high-viscosity surface layer over an isoviscous mantle, with a core radius of 1840 km. It predicts lateral temperature variations of up to a few hundred degrees Kelvin relative to the mean mantle temperature, with high temperature under Tharsis and to a lesser extent under Elysium and cool temperatures elsewhere. Surprisingly, the model predicts crustal thinning beneath Tharsis. If correct, this implies that thinning of the crust by mantle shear stresses dominates over thickening of the crust by volcanism. The major impact basins (Hellas, Argyre, Isidis, Chryse, and Utopia) are regions of crustal thinning, as expected. Utopia is also predicted to be a region of hot mantle, which is hard to reconcile with the surface geology. An alternative model for Utopia treats it as a mascon basin. The Utopia gravity anomaly is consistent with the presence of a 1.2 to 1.6 km thick layer of uncompensated basalt, in good agreement with geologic arguments about the amount of volcanic fill in this area. The mantle thermal structure is the dominant contributor to the observed geoid in our inversion. The mantle also dominates the topography at the longest wavelengths, but shorter wavelengths (harmonic degrees greater than or equal to 4) are dominated by the crustal structure. Because of the uncertainty about the appropriate numerical values for some of the model's input parameters, we have examined the sensitivity of the model results to the planetary structural model (core radius and core and mantle densities), the mantle's viscosity stratification, and the mean crustal thickness. The model results are insensitive to the specific thickness or viscosity contrast of the high-viscosity surface layer and to the mean crustal thickness in the range 25 to 100 km. Models with a large core radius or with an upper mantle low-viscosity zone require implausibly large lateral variations in mantle temperature.

Utopias past and future

NASA Astrophysics Data System (ADS)

Tyler, David J.; Blain, Barry

2016-05-01

In reply to Robert P Crease's article “Diversifying utopia” (March p29, http://ow.ly/104lZw), which discussed the near-absence of women in the novel New Atlantis, which was written in the 17th century by the natural philosopher Francis Bacon.

Trans-Spatial Utopias

ERIC Educational Resources Information Center

Kramsch, Claire

2018-01-01

The "trans-" perspectives offered in this special issue are heady stuff. Post-structuralism (philosophy) meets the digital age (electronics), meets globalization (economics), and meets translingual practice (linguistics) to create a perfectly utopian or placeless space for future exploration. I want to first add my voice to the…

Mars Data Analysis Program

NASA Technical Reports Server (NTRS)

McGill, George E.

2004-01-01

Grant NAGS12158 addressed a major NASA objective concerning the possibility of a palm ocean or large lake in the northern lowlands of Mars. Our overall approach for this study was an analysis of the graben-bounded giant polygons of Utopia Planitia, but specifically those grabens that define circles rather than open polygons. These circular grabens overlie buried impact craters, and the grabens form because of differential compaction of the overlying material over crater rims and floors. Several years ago, I predicted that the graben circles would bound depressions, and that the depths of these depressions would scale with the diameters of the graben circles. These predictions have been verified by earlier analysis. During this one-year grant (with one-year no-cost extension) we greatly increased the sample size and validated the earlier research robustly. What remained unexplained was why most of the graben circles in Utopia Planitia were double. A new model, involving volumetric compaction rather than simply 2-D compaction, satisfactorily explains the double rings and also provides a measure of relative thickness of the cover material burying the craters as a function of radial distance from the center of the Utopia Basin. Only two materials are likely candidates for the compacting cover material: volcanic ash, or wet sediment. The water in the wet sediment is largely responsible for the volumetric compaction; dry ash will compact vertically but experiences very limited lateral shrinkage. Thus the depressions within the circular grabens and the model explaining the double rings strongly favor wet sediment and thus provide evidence in favor of a past body of standing water in the northern lowlands. Publications supported entirely or in part by this grant are listed below.

Modeling concentric crater fill in Utopia Planitia, Mars, with an ice flow line model

NASA Astrophysics Data System (ADS)

Weitz, N.; Zanetti, M.; Osinski, G. R.; Fastook, J. L.

2018-07-01

Impact craters in the mid-latitudes of Mars are commonly filled to variable degrees with some combination of ice, dust, and rocky debris. Concentric surface features visible in these craters have been linked to debris transportation and glacial and periglacial processes. Concentric crater fill (CCF) observed today are interpreted to be the remains of repeated periods of accumulation and sublimation during the last tens to hundreds of million years. Previous work suggests that during phases of high obliquity, ice accumulates in crater interiors and begins to flow down steep crater slopes, slowly filling the crater. During times of low obliquity ice is protected from sublimation through a surface debris layer consisting of dust and rocky material. Here, we use an ice flow line model to understand the development of concentric crater fill. In a regional study of Utopia Planitia craters, we address questions about the influence of crater size on the CCF formation process, the time scales needed to fill an impact crater with ice, and explore commonly described flow features of CCF. We show that observed surface debris deposits as well as asymmetric flow features can be reproduced with the model. Using surface mass balance data from global climate models and a credible obliquity scenario, we find that craters less than 80 km in diameter can be entirely filled in less than 8 My, beginning as recently as 40 Ma ago. Uncertainties in input variables related to ice viscosity do not change the overall behavior of ice flow and the filling process. We model CCF for the Utopia Planitia region and find subtle trends for crater size versus fill level, crater size versus sublimation reduction by the surface debris layer, and crater floor elevation versus fill level.

The Pragmatic University: A Feasible Utopia?

ERIC Educational Resources Information Center

Badley, Graham

2016-01-01

"Imaginings" of the modern university include such ideas as "the ecological university" and "the pragmatic university". In his attempt to separate utopian from dystopian visions of the university, Ronald Barnett concentrates on an analysis of the ecological university and ignores, for example, the case of the…

New Support for Hypotheses of an Ancient Ocean on Mars

NASA Technical Reports Server (NTRS)

Oehler, Dorothy Z.; Allen, Carlton C.

2013-01-01

A new analog for the giant polygons in the Chryse-Acidalia area suggests that those features may have formed in a major body of water - likely a Late Hesperian to Early Amazonian ocean. This analog -terrestrial polygons in subsea, passive margin basins derives from 3D seismic data that show similar-scale, polygonal fault systems in the subsurface of more than 50 terrestrial offshore basins. The terrestrial and martian polygons share similar sizes, basin-wide distributions, tectonic settings, and association with expected fine-grained sediments. Late Hesperian deposition from outflow floods may have triggered formation of these polygons, by providing thick, rapidly-deposited, fine-grained sediments necessary for polygonal fracturing. The restriction of densely occurring polygons to elevations below approx. -4000 m to -4100 m supports inferences that a body of water controlled their formation. Those same elevations appear to restrict occurrence of polygons in Utopia Planitia, suggesting that this analog may apply also to Utopia and that similar processes may have occurred across the martian lowlands.

Education, Erasmian Humanism and More's "Utopia"

ERIC Educational Resources Information Center

Parrish, John M.

2010-01-01

The humanist movement of the Northern Renaissance--often called "Christian humanism" or "Erasmian humanism" (after its most famous member, Desiderius Erasmus)--had a lasting impact on many areas of European intellectual and cultural life. This paper reviews the contribution of Erasmus and his circle to the theory and practice…

Classical Music as Enforced Utopia

ERIC Educational Resources Information Center

Leech-Wilkinson, Daniel

2016-01-01

In classical music composition, whatever thematic or harmonic conflicts may be engineered along the way, everything always turns out for the best. Similar utopian thinking underlies performance: performers see their job as faithfully carrying out their master's (the composer's) wishes. The more perfectly they represent them, the happier the…

Toward a Critical Utopian and Pedagogical Methodology

ERIC Educational Resources Information Center

Firth, Rhiannon

2013-01-01

This article explores the possibility of developing an ethico-politically coherent and practical research framework for studying the learning and knowledge-production and dissemination processes of utopian groups and movements. It seeks to develop understanding of utopias by identifying and conceptualizing their pedagogical aspects. At the same…

Sendero Luminoso: Case Study in Insurgency

DTIC Science & Technology

1993-01-01

utopia is premised on the spiritual rejuvenation of its chosen people, the Quechua -speaking "cosmic race." This messianic movement seeks to cleanse Peru...The Quechua -speaking top echelon also provided a link with the Indian masses whom Guzman hoped to politicize. At the same time, however, his

Chronicle of Higher Education. Volume 51, Number 19, January 14, 2005

ERIC Educational Resources Information Center

Chronicle of Higher Education, 2005

2005-01-01

"Chronicle of Higher Education" presents an abundant source of news and information for college and university faculty members and administrators. This January 14, 2005 issue of "Chronicle for Higher Education" includes the following articles: (1) "Utopia College: A Distinctive Alternative" (Nemko, Marty); (2)…

Social Actualization: A Theory of Community Living Arrangements and a Practical Utopia.

ERIC Educational Resources Information Center

Slawski, Carl

Characteristics of successful living arrangements in intentional communities are presented by examining kibbutz life. The first section discusses four bases for establishing and maintaining an intentional community: interest, justice, cultural flowering, and love (deep interpersonal and intergroup relationships and religious values). The second…

Utopian Education and Anti-Utopian Anthropology

ERIC Educational Resources Information Center

Papastephanou, Marianna

2013-01-01

This article explores the connection of education, utopia and anthropology, aiming to tease out some educational implications of anti-utopian anthropological essentialism and to show why these should be staved off. It will be shown how an anthropology that tarnishes human nature operates and how it affects educational intervention in the shaping…

A Paradoxical Academic Identity: Fate, Utopia and Critical Hope

ERIC Educational Resources Information Center

Sutton, Paul

2015-01-01

Using a dialectical mode of exposition, I offer a reflexive sociological theorisation of the paradox that characterises my academic identity: a fatalistic disenchantment concerning the colonisation of Higher Education (HE) by neoliberalism co-exists with a utopianism concerning HE's emancipatory possibilities. I begin with a discussion of Weber's…

Project Solo; Newsletter Number Four.

ERIC Educational Resources Information Center

Pittsburgh Univ., PA. Project Solo.

A paper titled "Myopia, Cornucopia and Utopia" makes up the major portion of this Project Solo Newsletter. It emphasizes the danger involved in the belief that the larger the system the better, and points out that although the computer utilizes technology, the human with judgment utilizes the computer. Some details of the Project Solo…

An Analytical Index to the Internet: Dreams of Utopia.

ERIC Educational Resources Information Center

Casey, Carol

1999-01-01

Explores the need for analytical indexes to access Internet resources. Considers bibliographic control, Web site design, keyword search engines, hierarchical subject indexes, and special indexes and compilations of links, and concludes that the creation of small, focused indexes may be the best solution for accessing specific types of digital…

A Heterotopology of the Academy: Mapping Assemblages as Possibilised Heterotopias

ERIC Educational Resources Information Center

Charteris, Jennifer; Jones, Marguerite; Nye, Adele; Reyes, Vicente

2017-01-01

Heterotopias are counter-sites of enacted utopias through which reality is simultaneously represented, contested and inverted. They are physical or mental spaces where, although norms of behaviours are suspended, there are connections with a plethora of other spaces. This article constructs a collective biography as a heterotopology of the…

UNESCO, the Faure Report, the Delors Report, and the Political Utopia of Lifelong Learning

ERIC Educational Resources Information Center

Elfert, Maren

2015-01-01

Two education reports commissioned by the United Nations Educational, Scientific and Cultural Organization (UNESCO), Learning to be, otherwise known as the "Faure report" (1972) and "Learning: The treasure within," otherwise known as the "Delors report" (1996), have been associated with the establishment of lifelong…

The Kibbutz in the 1970's: From Utopia Towards Modernization.

ERIC Educational Resources Information Center

Rayman, Paula

The document examines the evolution of kibbutzim in Israel. The author suggests that a primary factor in the kibbutz development is the nature and structure of Israeli modernization efforts. The efforts encompass national ideology, industrialization, and legitimization of certain forms of social interaction. This mode of modernization stands in…

We, John Dewey's Audience of Today

ERIC Educational Resources Information Center

da Cunha, Marcus Vinicius

2016-01-01

This article suggests that John Dewey's "Democracy and Education" does not describe education in an existing society, but it conveys a utopia, in the sense coined by Mannheim: utopian thought aims at instigating actions towards the transformation of reality, intending to attain a better world in the future. Today's readers of Dewey (his…

Learning, Change, and the Utopia of Play

ERIC Educational Resources Information Center

Moulthrop, Stuart

2007-01-01

This article looks at some of the rhetoric surrounding video games and other forms of interactive software as additions or alternatives to school curricula. It focuses particularly on the need to articulate ways to "read" videogames in order to achieve significant cultural impact. Noting that reading, even as metaphor, tends to invoke…

Human Rights, Cosmopolitanism and Utopias: Implications for Citizenship Education

ERIC Educational Resources Information Center

Starkey, Hugh

2012-01-01

Citizenship education, defined as learning to live together, requires agreement on certain common principles. One central purpose of a state education system is the transmission of common normative standards such as the human rights and fundamental freedoms that underpin liberal democratic societies. The paper identifies the conceptual roots of…

Technological Utopia, Dystopia and Ambivalence: Teaching with Social Media at a South African University

ERIC Educational Resources Information Center

Rambe, Patient; Nel, Liezel

2015-01-01

The discourse of social media adoption in higher education has often been funnelled through utopian and dystopian perspectives, which are polarised but determinist theorisations of human engagement with educational technologies. Consequently, these determinist approaches have obscured a broadened grasp of the situated, socially constructed nature…

The Plasma-Based Instruction in Ethiopia: Utopia or Dystopia?

ERIC Educational Resources Information Center

Abera, Berhanu

2013-01-01

This article highlights the utopian and dystopian viewpoints held on the plasma-based instruction in Ethiopian by looking into the existing literature works and by analyzing attitudes of implementing bodies and implementers towards the program. The article identified that though implementing bodies were enthusiastic in developing and expanding the…

The "Earth Charter": An Ethical Framework for a Feasible Utopia

ERIC Educational Resources Information Center

Contini, Valerio; Garcia Pascual, Enrique

2010-01-01

This research objective is to highlight an innovative, holistic, inclusive, integrated approach to a sustainable future promoted by the "Earth Charter" and describe the structure of its ethical framework. The main conclusion of the research is that the ethical framework of the "Earth Charter" is based on a limited number of…

Origin of the Polygons and Underground Structures in Western Utopia Planitia on Mars

NASA Technical Reports Server (NTRS)

Yoshikawa, K.

2002-01-01

The area of lower albedo (Hvm) has a higher density of polygonal patterns. These patterns potentially suggest that 1) the polygonal pattern is caused primarily by ground heaving and collapsing, 2) lower albedo materials had higher tensile strength. Additional information is contained in the original extended abstract.

On the Reception of Foucauldian Ideas in Pedagogical Research

ERIC Educational Resources Information Center

Ostrowicka, Helena

2011-01-01

The article is devoted to the presentation of the reception of Foucauldian ideas in Polish pedagogical research over the past twenty years. This movement of thought is described as an oscillation between heterotopia and utopia, autonomy and heteronomy, emancipation and repression. As results of this analysis indicate, Polish pedagogues are most…

A Golden Age? Dostoevsky, Daoism and Education

ERIC Educational Resources Information Center

Roberts, Peter

2016-01-01

There is much of value for educationists in the work of the great Russian novelist and thinker, Fyodor Dostoevsky. This paper explores a key theme in Dostoevsky's later writings: the notion of a "Golden Age". It compares the ideal depicted in Dostoevsky's story "The Dream of a Ridiculous Man" with the implied utopia of the…

New York City: Musically Speaking.

ERIC Educational Resources Information Center

Aiex, Nola Kortner

New York City as a subject has fascinated generations of artists, writers, and musicians. However, the glamorous image of the city has changed over the years, and in the 1960s, popular music, in particular, began to reflect a utopia/dystopia dichotomy in relation to New York. During the past twenty years, six popular singer-songwriters who have…

Mental Health Services Coordination: Working towards Utopia. Human Resources Series.

ERIC Educational Resources Information Center

Paterson, Andrea

1986-01-01

The need for mental health services coordination is discussed in this report. It is noted that, without coordination, government units and service providers can operate independently and in competition with one another. The move to deinstitutionalization is discussed, including the lack of service coordination resulting from this move and the…

Multilingualism as Utopia: Fashioning Non-Racial Selves

ERIC Educational Resources Information Center

Stroud, Christopher; Williams, Quentin

2017-01-01

The challenge of contemporary South Africa is that of building a (post)nation of postracial equity in a fragmented world of a globalized ethical, economic and ecological meltdown. In this paper, we seek to explore the idea of multilingualism as a technology in the conceptualization of alternative, competing futures. We suggest that multilingualism…

Searching for Utopia: Best Practices in Digitizing the Corporate Library.

ERIC Educational Resources Information Center

Stach, Ron

Using an in-depth review of the literature and the author's own personal experience, this paper attempts to distill the eight best practices of those undertaking digitization projects. Results are intended specifically to assist special librarians undertaking a digitization effort in a corporate setting, but conclusions could equally apply to the…

Education in the People's Republic of China.

ERIC Educational Resources Information Center

Chen, Kuan-Yu

This report outlines the background of educational policy and objectives before and after the Cultural Revolution in China. The basis of Chinese educational philosophy is Marxism-Leninism; the ideal society is that of the Marxian utopia of a classless society. The role of education is service to the state, not the individual. Educational policy is…

Education and Utopia: Robert Owen and Charles Fourier

ERIC Educational Resources Information Center

Leopold, David

2011-01-01

The aims of education, and the appropriate means of realising them, are a recurring preoccupation of utopian authors. The utopian socialists Robert Owen (1771-1858) and Charles Fourier (1772-1837) both place human nature at the core of their educational views, and both see education as central to their wider objective of social and political…

A Utopia in the Desert Where 24 Bright Young Men Cope with Loneliness, Hard Work, and Philosophy.

ERIC Educational Resources Information Center

Hirschorn, Michael W.

1987-01-01

At Deep Springs College, in a remote California desert valley, 24 male students from the top 1 percent of the high school applicant pool spend 2 years running a ranch and studying a curriculum that leans toward literature and away from the sciences. (MSE)

Diasporic Philosophy, Counter-Education and Improvisation

ERIC Educational Resources Information Center

Gur-Ze'ev, Ilan

2010-01-01

Counter-education that addresses seriously the challenge of loss, exile, and the deceiving "home-returning" projects accepts that no positive Utopia awaits us as "truth", "genuine life", "worthy struggle", "pleasure" or worthy self-annihilation. Loss is not to be recovered or compensated; not for the individual nor for any kind of "we". And yet,…

2050: A Pricing Odyssey

DOE Office of Scientific and Technical Information (OSTI.GOV)

Faruqui, Ahmad

2006-10-15

The author uses the Rip Van Winkle approach favored by marketers to gaze, clear-eyed, into the future - say, the year 2050 - to visualize alternative demand-response possibilities. Dare we go California Dreamin' of a distant utopia - or is it inevitable that pricing myopia will keep us from attaining the fulfillment of many of our career goals? (author)

The Educational Situation in Utopia: Why "What Is," Is

ERIC Educational Resources Information Center

Seaman, Jayson; Quay, John

2015-01-01

In this response to Molly Ware's review of our 2013 book, "John Dewey and Education Outdoors," we extend her suggestion that complexity be regarded as an important, generative force in education reform. Drawing on Dewey's 1933 "Utopian Schools" speech, we discuss the "level deeper" that Dewey sought as he…

OSeMOSYS Energy Modeling Using an Extended UTOPIA Model

ERIC Educational Resources Information Center

Lavigne, Denis

2017-01-01

The OSeMOSYS project offers open-access energy modeling to a wide audience. Its relative simplicity makes it appealing for academic research and governmental organizations to study the impacts of policy decisions on an energy system in the context of possibly severe greenhouse gases emissions limitations. OSeMOSYS is a tool that enhances the…

Free Reading Is UTOPIA

ERIC Educational Resources Information Center

LeCrone, Nancy

2010-01-01

In high school students get tied up in extracurricular activities and have little time for pleasure reading. It is true that with rigorous academic schedules they have little time for pleasure reading. Thus began a conversation with a sophomore English teacher at the author's high school. As they were discussing the plight of free reading he was…

Optimists' Creed: Brave New Cyberlearning, Evolving Utopias (Circa 2041)

ERIC Educational Resources Information Center

Burleson, Winslow; Lewis, Armanda

2016-01-01

This essay imagines the role that artificial intelligence innovations play in the integrated living, learning and research environments of 2041. Here, in 2041, in the context of increasingly complex wicked challenges, whose solutions by their very nature continue to evade even the most capable experts, society and technology have co-evolved to…

Electric Mars: A Large Trans-Terminator Electric Potential Drop on Closed Magnetic Field Lines Above Utopia Planitia

NASA Technical Reports Server (NTRS)

Collinson, Glyn; Mitchell, David; Xu, Shaosui; Glocer, Alex; Grebowsky, Joseph; Hara, Takuya; Lillis, Robert; Espley, Jared; Mazelle, Christian; Sauvaud, Jean-Andre

2017-01-01

Abstract Parallel electric fields and their associated electric potential structures play a crucial role inionospheric-magnetospheric interactions at any planet. Although there is abundant evidence that parallel electric fields play key roles in Martian ionospheric outflow and auroral electron acceleration, the fields themselves are challenging to directly measure due to their relatively weak nature. Using measurements by the Solar Wind Electron Analyzer instrument aboard the NASA Mars Atmosphere and Volatile EvolutioN(MAVEN) Mars Scout, we present the discovery and measurement of a substantial (Phi) Mars 7.7 +/-0.6 V) parallel electric potential drop on closed magnetic field lines spanning the terminator from day to night above the great impact basin of Utopia Planitia, a region largely free of crustal magnetic fields. A survey of the previous 26 orbits passing over a range of longitudes revealed similar signatures on seven orbits, with a mean potential drop (Phi) Mars of 10.9 +/- 0.8 V, suggestive that although trans-terminator electric fields of comparable strength are not ubiquitous, they may be common, at least at these northerly latitudes.

A model for the origin of Martian polygonal terrain

NASA Technical Reports Server (NTRS)

Mcgill, G. E.

1993-01-01

Extensive areas of the Martian northern plains in Utopia and Acidalia Planitiae are characterized by 'polygonal terrain.' Polygonal terrain consists of material cut by complex troughs defining a pattern resembling mudcracks, columnar joints, or frost-wedge polygons on the Earth. However, the Martian polygons are orders of magnitude larger than these potential Earth analogs, leading to severe mechanical difficulties for genetic models based on simple analogy arguments. Stratigraphic studies show that the polygonally fractured material in Utopia Planitia was deposited on a land surface with significant topography, including scattered knobs and mesas, fragments of ancient crater rims, and fresh younger craters. Sediments or volcanics deposited over topographically irregular surfaces can experience differential compaction producing drape folds. Bending stresses due to these drape folds would be superposed on the pervasive tensile stresses due to desiccation or cooling, such that the probability of fracturing is enhanced above buried topographic highs and suppressed above buried topographic lows. Thus it was proposed that the scale of the Martian polygons is controlled by the spacing of topographic highs on the buried surface rather than by the physics of the shrinkage process.

Geographic Distribution of QCDs Around the Northern Plains Basins of Mars and the Relationship to Lowland Materials

NASA Technical Reports Server (NTRS)

Buczkowski, D. L.; Frey, H. V.; McGill, G. E.

2005-01-01

It has been suggested that quasicircular depressions (QCDs) without a structural representation in Viking and MOC visible imagery represent buried impact craters [1,2,3,4]. Topographic depressions will form over impact craters buried by a differentially compacting cover material because total cover thickness, and thus total compaction, is greater over the center of completely buried impact craters than their rims [5]. If this is the process by which QCDs form, then only areas of differentially compacting materials should have QCDs. Previous work has established that there is a relationship of surface relief to diameter for QCDs around the Utopia Basin [6]. The slope of the trend of this relationship varies depending on cover thickness, becoming steeper with decreasing thickness [7]. Comparing trendslopes of QCDs around different lowland basins might give us insight into the relative thickness of the cover material in these areas. We explore the geographic distribution of QCDs around the Utopia, Isidis and Acidalia basins and compare their location to geologic units and materials. We also compare evidence for relative thickness of cover material at the three basins.

Preservation of Midlatitude Ice Sheets on Mars

NASA Astrophysics Data System (ADS)

Bramson, A. M.; Byrne, S.; Bapst, J.

2017-11-01

Excess ice with a minimum age of tens of millions of years is widespread in Arcadia Planitia on Mars, and a similar deposit has been found in Utopia Planitia. The conditions that led to the formation and preservation of these midlatitude ice sheets hold clues to past climate and subsurface structure on Mars. We simulate the thermal stability and retreat of buried excess ice sheets over 21 Myr of Martian orbital solutions and find that the ice sheets can be orders of magnitude older than the obliquity cycles that are typically thought to drive midlatitude ice deposition and sublimation. Retreat of this ice in the last 4 Myr could have contributed 6% of the volume of the north polar layered deposits (NPLD) and more than 10% if the NPLD are older than 4 Myr. Matching the measured dielectric constants of the Arcadia and Utopia Planitia deposits requires ice porosities of 25-35%. We model geothermally driven vapor migration through porous ice under Martian temperatures and find that Martian firn may be able to maintain porosity for timescales longer than we predict for retreat of the ice.

Mapping the northern plains of Mars: origins, evolution and response to climate change - a new overview of the recent ice-related landforms in Utopia Planitia

NASA Astrophysics Data System (ADS)

Costard, Francois; Sejourne, Antoine; Losiak, Ania; Swirad, Zusanna; Balm, Matthew; Conway, Susan; Gallagher, Colman; van-Gassel, Stephan; Hauber, Ernst; Johnsson, Andreas; Kereszturi, Akos; Platz, Thomas; Ramsdale, Jason; Reiss, Dennis; Skinner, James

2015-04-01

An ISSI (International Space Science Institute) international team has been convened to study the Northern Plain of Mars. The northern plains of Mars are extensive, geologically young, low-lying areas that contrast in age and relief to Mars' older, heavily cratered, southern highlands. Mars' northern plains are characterised by a wealth of landforms and landscapes that have been inferred to be related to the presence of ice or ice-rich material. Such landforms include 'scalloped' pits and depressions, polygonally-patterned grounds, and viscous flow features similar in form to terrestrial glacial or ice-sheet landforms. Furthermore, new (within the last few years) impact craters have exposed ice in the northern plains, and spectral data from orbiting instruments have revealed the presence of tens of percent by weight of water within the upper most ~50 cm of the martian surface at high latitudes. The western Utopia Planitia contains numerous relatively young ice-related landforms (< 10 Ma). Among them, there are scalloped depressions, spatially-associated polygons and polygon-junction pits. There is an agreement within the community that they are periglacial in origin and, derivatively, indicate the presence of an ice-rich permafrost. However, these landforms were studied individually and, many questions remain about their formation-evolution and climatic significance. In contrast, we conducted a geomorphological study of all landforms in Utopia Planitia along a long strip from ~30N to ~80N latitude and about 250km wide. The goals are to: (i) map the geographical distribution of the ice-related landforms; (ii) identify their association with subtly-expressed geological units and; (iii) discuss the climatic modifications of the ice-rich permafrost in UP. Our work combines a study with CTX (5-6 m/pixel) and HRSC (~12.5-50 m/pixel) images, supported by higher resolution HiRISE (25 cm/pixel) and MOC (~2 m/pixel) and a comparison with analogous landforms on Earth.

RELATIVE THEORY OF GOOD IN "BRAVE NEW WORLD" AND "1984."

ERIC Educational Resources Information Center

PARTRIDGE, ALICE

ONE METHOD OF INTERESTING THE AVERAGE HIGH SCHOOL STUDENT IN QUESTIONING INTELLIGENTLY THE NATURE OF GOOD IS THROUGH THE STUDY OF HUXLEY'S "BRAVE NEW WORLD" AND ORWELL'S "1984." IN BOTH OF THESE NEGATIVE UTOPIAS THE LOSS OF MAN'S HUMANITY, INDIVIDUALITY, AND RIGHT TO REASON THE NATURE OF GOOD ARE THE VERY QUALITIES WHICH MAKE…

Hutchins's University of Utopia: Institutional Independence, Academic Freedom, and Radical Restructuring

ERIC Educational Resources Information Center

Hoff, Peter Sloat

2009-01-01

In a crisis-plagued world looking to higher education for knowledge, wisdom, and solutions, higher education itself is stumbling. Its transformational thinking has frozen up like an overstressed computer program; and we need, in effect, to "push the reset button." In 1953, the renowned and controversial president of the University of Chicago,…

Heterotopia and Its Role in the Lived Experiences of Resettlement

ERIC Educational Resources Information Center

Rossetto, Marietta

2006-01-01

Place, as a metaphor, can be experienced in different ways, existing or created. If created, space can be Foucault's "placeless place", a utopia. A place that exists, however, can be a heterotopic space. A heterotopia is what we as individuals interpret it to be: it can be a space for reconstituting the self, rewriting the scripts of…

"Gender Utopias?": U.S. Student Reflections on Studying Abroad in Norway and Sweden

ERIC Educational Resources Information Center

Nordmeyer, Kristjane; Teig, Trisha; Bedera, Nicole

2017-01-01

This article describes a study abroad experience in Norway and Sweden that was designed to explore gender equality in two of the world's most gender-progressive countries. Course readings explored the work of feminist sociologists and asked students to think critically about gender equality from a cross-cultural perspective. Students met with…

Schooling and Governance: Pedagogical Knowledge and Bureaucratic Expertise in the Genesis of the Argentine Educational System

ERIC Educational Resources Information Center

Southwell, Myriam

2013-01-01

The consolidation of the Argentine Federal Government by the 1870s aimed to modernise local society, establish state institutions and reach political stabilisation. Building a modern schooling system articulated both utopia and bureaucracy by establishing the use of knowledge as an instrument of social intervention, vindicating and legitimising…

"Utopia" and "Passion": A Commentary on "Sustainability and Accounting Education: The Elephant in the Classroom"

ERIC Educational Resources Information Center

Contrafatto, Massimo

2013-01-01

In this commentary, Massimo Contrafatto explains his understanding of Gray's interpretation of accounting education for sustainability (AE4S), and contributes some personal insights to the future development of AE4S. Gray reflected on an educational engagement experiment where the complex issues surrounding sustainability were dealt with in an…

"Making the Margins Chaos": Romantic and Antiromantic Readings of La Maravilla

ERIC Educational Resources Information Center

Carlston, Erin G.

2005-01-01

Alfredo Vea Jr.'s 1993 novel "La Maravilla" depicts a 1950s squatter community on the edge of Phoenix. The community, Buckeye Road, questions notions of U.S. American identity as middle-class, WASP, and heterosexual. Buckeye can easily be viewed as a romanticized utopia that offers an alternative to consumer capitalism, urban sprawl, the…

Tinkering Towards Utopia: Trying to Make Sense of My Contribution to the Field

ERIC Educational Resources Information Center

Mulford, Bill

2012-01-01

Purpose: The purpose of this paper is to provide an overview of what the author believes to be his major contributions to the field of Educational Administration. Design/methodology/approach: The approach taken is a personal review and reflection based on research. For purposes of structuring the article three themes have been…

E-Commerce and Education. Graduate Paper Series on Electronic Commerce.

ERIC Educational Resources Information Center

di Giantomasso, Tania

Broad assumptions about the impact of the Internet have created a "cult of hype" where the latest technological advancement is seen as the next best thing, and educators have been swept up in the promise of an educational utopia. The hype tells us that the world is joined by the infrastructure of this new technology and that…

Cutting Your Losses: Could Best-Practice Pedagogy Involve Acknowledging that Even Robust Hope May Be Vain?

ERIC Educational Resources Information Center

Schuurmans-Stekhoven, James

2009-01-01

A recent special issue of "Asia-Pacific Journal of Teacher Education" (Vol. 35, Issue 3, 2007) championed "robust hope" as fundamental to achieving educational utopias, and yet key features of hope were largely overlooked. Although hope feels good and has utility in some circumstances, in other situations different…

Tinkering and Turnarounds: Understanding the Contemporary Campaign to Improve Low-Performing Schools

ERIC Educational Resources Information Center

Duke, Daniel L.

2012-01-01

An unprecedented amount of attention in recent years has been focused on turning around low-performing schools. Drawing on insights from Tyack and Cuban's (1995) "Tinkering Toward Utopia," the article analyzes the forces behind the school turnaround phenomenon and how they have evolved since passage of the No Child Left Behind Act. The…

Reconsideration of Rorty's View of the Liberal Ironist and Its Implications for Postmodern Civic Education

ERIC Educational Resources Information Center

Kwak, Duck-Joo

2004-01-01

There have been persistent criticisms of Rorty's "liberal ironist" as the postmodern picture of the educated in the liberal utopia. While the modernist (Enlightenment) liberal Thomas McCarthy, who believes in universal rationality as the basis of public morality, criticizes Rorty's view of the liberal ironist for fostering the poverty of public…

Chronotopoi of the Good Life and Utopia: Bakhtin on Goethe's "Bildungsroman Wilhelm Meister" and the Carnivalesque

ERIC Educational Resources Information Center

Franke, Norman

2017-01-01

This paper explores Bakhtin's reception of Goethe's "Wilhelm Meisters Lehrjahre" with a view to assess how Bakhtin's interest in this early chronotopical masterpiece can be understood in the wider context of his utopian thinking and his political eschatologies. Bakhtin reads Goethe's novel as a critique of totalitarian forms of Socialist…

Utopia in Arts Education: Transmission of Cantonese Opera under the Oral Tradition in Hong Kong

ERIC Educational Resources Information Center

Leung, Bo-Wah

2015-01-01

Schooling has been the main approach for transmitting knowledge and skills in both Eastern and Western cultures. The conservatory, for instance, has been the main cradle of great musicians. However, traditional folk arts in the East relied on apprenticeship using an oral approach for transmission. Applying Lave and Wenger's theory of legitimate…

"Utopia, Limited": Narratives from a Writer's Workshop.

ERIC Educational Resources Information Center

Degan, James N.

When teachers claim that the idea of community serves as the inspiration for a writing course, the question of what exactly is meant by the term community is compelling. The idea of community has any number of interpretations, ranging from the idealistically inspired to the downright deranged. In the new Honors Program at Ohio State University at…

"A New Life in the Countryside Awaits": Interactive Lessons in the Rural Utopia in "Farming" Simulation Games

ERIC Educational Resources Information Center

Cole, Matthew; Stewart, Kate

2017-01-01

This paper critically analyses the legitimation of exploitative human-nonhuman animal relations in online "farming" simulation games, especially the game Hay Day. The analysis contributes to a wider project of critical analyses of popular culture representations of nonhuman animals. The paper argues that legitimation is effected in Hay…

Utopia University: A Faculty Member Reflects on Recommendations for the Future of SoTL

ERIC Educational Resources Information Center

Forrest, Krista D.

2013-01-01

The author, Krista D. Forrest, Professor of Psychology, University of Nebraska at Kearney, reports on what it would take to create a "Utopian university," a campus of the future where faculty members' scholarship of teaching and learning (SoTL) has gone on to change departments and as the departments changed, so did the institution.…

Ideology, Utopia and Islam on Campus: How to Free Speech a Little from Its Own Terrors

ERIC Educational Resources Information Center

Scott-Baumann, Alison

2017-01-01

A dominant narrative on many British campuses is "Prevent," which is part of the government's counter-terror policy, an ideology based on fear. Muslims, in particular, are considered to be at risk of radicalisation on campus, and being under suspicion makes them self-censor. Additionally, the no-platforming student lobby creates a…

Finding a Concrete Utopia in the Dystopia of a "Sub-City"

ERIC Educational Resources Information Center

Busby, Selina

2017-01-01

This article examines a 10-year long series of annual short-term interventions with young people living in Dharavi (India) that has led to a number of public theatre events. The partnership offers a unique training experience to students from the UK in theatre facilitation, and a regular opportunity to participate in theatre for young people in…

Navigating between a Monolingual Utopia and Translingual Realities: Experiences of American Learners of Yorùbá as an Additional Language

ERIC Educational Resources Information Center

Mori, Junko; Sanuth, Kazeem Ké?hìndé

2018-01-01

Translingualism advocates for the appreciation of multilingual speakers' fluid, flexible, and creative deployment of semiotic resources without regard to the ideological constructs of named languages. While this scholarship has been developed primarily in the contexts of world Englishes, English as a lingua franca, and bilingual education in…

75 FR 9455 - U.S. Biomedical Corp., (f/k/a United Textiles & Toys, Inc.), U.S. Environmental Solutions, Inc...

Federal Register 2010, 2011, 2012, 2013, 2014

2010-03-02

... & Toys, Inc.), U.S. Environmental Solutions, Inc. (n/k/a EnviroResolutions, Inc.), USA Bridge Construction of N.Y., Inc., USA Broadband, Inc., USA Uranium Corp., and Utopia Marketing, Inc. (n/k/a... N.Y., Inc. because it has not filed any periodic reports since the period ended September 30, 1998...

"Greenbelt or Gutter": Youth "Place-Based" Performance and the Myth of the Suburban/Urban Divide

ERIC Educational Resources Information Center

Wessels, Anne

2014-01-01

A youth-created "place-based" performance set in the grounds of their suburban school challenged the myth of the suburban/urban divide that pits the edenic suburb against the dirty and crime-ridden city. Depicting the power relations of a failed utopia, these youth provoked the researcher to embark on further inquiry, analysing other…

Paulo Freire and Utopian Education

ERIC Educational Resources Information Center

Roberts, Peter

2015-01-01

Freire's work, both as a theorist and a practitioner, has always had a strong utopian flavor. In this article, the author sets out to show how and why this is so. Freire addressed the theme of utopia directly in his writings, but he also sought to bring a utopian world view to life in his educational endeavors. Delineating the key features of a…

Irony and Culture in Feminist Educational Writings: Wollstonecraft, Macaulay, Edgeworth

ERIC Educational Resources Information Center

Antal, Eva

2017-01-01

The context of the present paper is given by my research on philosophy of female education and the questions of female culture in the 18th and 19th centuries in England. I have been studying not only works of educationalist and philosophical concerns, but also literary works such as the education romans and utopias written in the related period.…

Mola Topography Supports Drape-Folding Models for Polygonal Terrain of Utopia Planitia, Mars

NASA Technical Reports Server (NTRS)

McGill, George E.; Buczkowski, D. L.

2002-01-01

One of the most important questions we ask about Mars is whether or not there have ever been large bodies of standing water on the surface. The polygonal terrains of Utopia and Acidalia Planitiae are located in the lowest parts of the northern lowlands, the most logical places for water to pond and sediments to accumulate. Showing that polygonal terrain is sedimentary in origin would represent strong evidence in favor of a northern ocean. A number of hypotheses for the origin of the giant martian polygons have been proposed, from the cooling of lava to frost wedging to the desiccation of wet sediments, but Pechman showed that none of these familiar processes could be scaled up to martian dimensions. Two models for polygon origin attempt to explain the scale of the martian polygons by postulating drape folding of a cover material, either sedimentary or volcanic, over an uneven, buried surface. The drape folding would produce bending stresses in the surface layers that increase the probability of Fracturing over drape anticlines and suppress the probability of fracturing over drape synclines. However, both models require an additional source of extensional strain to produce the total strain needed to produce the observed troughs.

Introductory Remarks

NASA Astrophysics Data System (ADS)

Gavroglu, Kostas

Practitioners of many (sub)-disciplines in the sciences are, at times, confronted with an apparent bliss which often turns into a nightmare: they are stuck with too good and too fertile a theory. 'Normal' science is surely a rewarding practice-but for that very reason it may, at times, also become boring. Theories or theoretical schemata may make successful predictions, may clarify 'mechanisms', they may show the way to further developments, and they may be amenable to non-controversial approximations. If one is really lucky, they may even-at least in principle-be able to answer all questions. There have-especially in the history of physics-been many such theories. Laplacian physics, ether physics and superstrings have historically defined the frameworks for such utopias where everything could be answerable, at least in principle. But one is truly at a loss when one is confronted with this in principle. In principle but not in practice? In principle but never? Confronted with the deadlocks that are implicit in such utopias, scientists started to collectively display a Procrustean psychopathology. They would prepare the beds and, yet, the theories would manage to trick the tricksters: almost all theories appeared to be fitting to any Procrustean bed. They were short and tall and normal at the same time.

Representation of micrometeorological and physiological parameters with numerical models influencing the vineyard ecosystem: the case of Piemonte (Italy).

NASA Astrophysics Data System (ADS)

Andreoli, Valentina; Cassardo, Claudio; Cavalletto, Silvia; Ferrarese, Silvia; Guidoni, Silvia; Mania, Elena; Spanna, Federico

2017-04-01

Grapevine represents worldwide key economic activities, with Europe representing the largest vineyard area in the world (38%). This is also true both for Italy and for its Piemonte region, in which famous and renowned wines (such as Barolo and Barbaresco) are produced. Grapevine productivity depends on several factors including soil fertility, management practices, climate and meteorology. In particular, concerning the latter, there is a need for a reliable assessment of the effects of a changing climate on its yield and quality. However, in this respect, it is essential to understand how and how much climate and meteorology affect grape productivity and quality, since only few studies related to few regions in the world have been produced. In this context, crop models are essential tools for investigating the effects of climate change on crop development and growth via the integration of existing knowledge of crop physiology relating to changing environmental conditions. Nevertheless, crop models were developed and applied mainly for studying the responses to climate change of annual crops (e.g. cereals); whilst appropriate crop models and application of these are still limited for tree crops such as grapevine. The rationale of the study, included in the MACSUR2 JPI FACCE project, is to use the third generation land surface model UTOPIA (University of TOrino model of land Process Interaction with Atmosphere) [1], in order to evaluate all components of hydrological and energy budget, as well as soil and canopy parameters, on a specific subset of land use, the vineyards. A preliminary step of this work has been to compare the datasets resulted from the calculations made by the UTOPIA and some experimental datasets acquired within vineyards by our team in the past experiments. The reason for such control is to ensure that UTOPIA outputs could be considered as sufficiently representative of the climatology of vineyards. Thus, some Piedmontese vineyards were selected, each one characterized by same climatic but different microclimatic conditions, in which measurements of a wide number of variables were performed in the vegetative seasons (such as in the experiment MASGRAPE). Subsequently, in this study, the results of additional simulations performed using the freely available global database GLDAS (Global Land Data Assimilation System) were compared with those of the simulations driven by observations, in order to check if the model was still able to reproduce the microclimatic characteristics of the vineyards. This preliminary part of the study gave satisfactory results; thus, we could pass to the phase two of the project. In this phase, using GLDAS database, long term simulations will be carried out with the UTOPIA in order to have output data available on a period of climatic interest (30 years or more). This database could be used in order to perform climatic statistics and assess possible trends in some parameters, eventually to be correlated with grape production. In the talk, the preliminary aspects of this work will be illustrated.

Experimental and modeling analysis of micro-meteorological factors involved in the development of Piedmontese vineyards

NASA Astrophysics Data System (ADS)

Cassardo, C.; Francone, C.; Richiardone, R.; Bertoni, D.; Alemanno, L.; Spanna, F.

2010-09-01

The vine (Vitis vinifera L.) constitutes one of the most important Italian products. Despite many other studies aimed to develop tools for managing the vineyards and improving the features and the quality of the wine, this study involves for the first time interdisciplinary fields with strong links and interconnections, stressing the collaboration of several specialists from different areas (pathologists, physiologists, entomologists, chemists and physicists) and of some wine companies. The research aims finding the main relations between the grapevines and the environment in which they grow, and it is carried out in the frame of a three-year project named "Adoption of a multisciplinary approach to study the grapevine agroecosystem: analysis of biotic and abiotic factors Able to Influence yield and quality - MASGRAPE", funded by the Piedmont region. The goal of the research is to delineate a detailed picture of the ecosystem of the vine and of the factors that improve the final product: the wine. The contribution of the physical-meteorological unit is twofold and includes an experimental activity, carried out through field measurements, and several experiments of model simulations. The former requires the joint use of micrometeorological and physiological data in order to assess the hydrological and energy budgets. The latter uses the land surface scheme UTOPIA (formerly known as LSPM) with the aim to assess and quantify the hydrological and radiative processes in the soil-plant-atmosphere system. The following experimental data have been collected in three vineyards located in Piedmont and belonging to the cultivars Nebbiolo and Barbera during 2008 and 2009: standard meteorological measurements, solar global radiation, PAR, soil temperature and humidity, fast response wind speed, temperature and moisture measurements, and some parameters directly related to the growth of the plants (number of leaves, LAI, leaf size, height and width of the plants). Fast response data have been analyzed using the methodology of the eddy covariance and corrected by the method of planar fit, the instruments being placed on hillsides. The data collected have been used to validate the model UTOPIA. In this talk we are presenting the preliminary results of the analysis of the experimental data, as well as the results of the first numerical simulations using the UTOPIA. The availability of a long period of data has allowed also to compare the characteristics of the different seasons. In particular, as the first semester of 2008 has been quite wet and rainy, while the corresponding one of the 2009 has been drier, some comparisons among the different years have been done. The preliminary results of the comparisons between UTOPIA and the measurements show that the model reproduces the trend of the transpiration and of the heat fluxes, but the accuracy of those predictions depends strongly by the accuracy of some input data relative to the vegetation, as for instance the LAI: underestimations of the LAI concur to produce an underestimation of the transpiration processes.

Utopia, University and Architecture: A Journey that Changed the Design of Contemporary Universities

ERIC Educational Resources Information Center

Calvo-Sotelo, Pablo Campos

2006-01-01

In 1927, a group of advisors to King Alfonso XIII of Spain, led by the architect Modesto Lopez-Otero, set out for the United States and Canada. Previously, they had visited a number of European cities where they examined the medieval architectural form of some famous universities. Inspired by a Utopian vision, the journey to the New World studied…

Re-Orienting Ethiopia's Educational Policy in the Classical Humanist Perspectives of Renaissance Utopias

ERIC Educational Resources Information Center

Debele, Meskerem L.

2018-01-01

Ethiopia has launched a grand scheme of renaissance to realise fast-paced economic growth. The two Growth and Transformation Plans spanning five years each (2010/11-2015/16 and 2016/17- 2020/21) outlined major targets towards which the country intends to mobilise all its resources. In the education sector, this vision is understood as producing a…

Love, Justice, and Education: John Dewey and the Utopians. Landscapes of Education

ERIC Educational Resources Information Center

Schubert, William H.

2010-01-01

Love, Justice, and Education by William H. Schubert brings to life key ideas in the work of John Dewey and their relevance for the world today. He does this by imagining continuation of a highly evocative article that Dewey published in the New York Times in 1933. Dewey wrote from the posture of having visited Utopia. Schubert begins each of…

Seeking a Utopia in the Past to Endure the Present: A Jungian Reading of "The Realms of Gold"

ERIC Educational Resources Information Center

Sistani, Shahram R.; Bagheri, Farzaneh

2014-01-01

This paper attempts a Jungian approach to Margaret Drabble's novel "The Realms of Gold." Jungian reading has been taken up to unravel the distinctive characteristics which make this novel so unique and popular. The focus of the paper is to classify the main characters of the novel in terms of their psychological types. In this novel from…

The Developing Notion of Employer Responsibility for the Alcoholic, Drug-Addicted or Mentally Ill Employee: An Examination under Federal and State Employment Statutes and Arbitration Decisions.

ERIC Educational Resources Information Center

Spencer, Janet Maleson

1979-01-01

Charts the evolution of the notion that the employer bears a certain responsibility for the troubled employee as it has emerged through laws and arbitration and considers the nature and scope of that responsibility. Available from St. John's Law Review, Fromkes Hall, Grand Central and Utopia Parkways, Jamaica, NY 11439. (Author/IRT)

Concentric crater fill on Mars - An aeolian alternative to ice-rich mass wasting

NASA Technical Reports Server (NTRS)

Zimbelman, J. R.; Clifford, S. M.; Williams, S. H.

1989-01-01

Concentric crater fill, a distinctive martian landform represented by a concentric pattern of surface undulations confined within a crater rim, has been interpreted as an example of ice-enhanced regolith creep at midlatitudes (e.g., Squyres and Carr, 1986). Theoretical constraints on the stability and mobility of ground ice limit the applicability of an ice-rich soil in effectively mobilizing downslope movement at latitudes poleward of + or - 30 deg, where concentric crater fill is observed. High-resolution images of concentric crater fill material in the Utopia Planitia region (45 deg N, 271 deg W) show it to be an eroded, multiple-layer deposit. Layering should not be preserved if the crater fill material moved by slow deformation throughout its thickness, as envisioned in the ice-enhanced creep model. Multiple layers are also exposed in the plains material surrounding the craters, indicating a recurrent depositional process that was at least regional in extent. Mantling layers are observed in high-resolution images of many other locations around Mars, suggesting that deposition occurred on a global scale and was not limited to the Utopia Planitia region. It is suggested that an aeolian interpretation for the origin and modification of concentric crater fill material is most consistent with morphologic and theoretical constraints.

Conscription: A Philosophical Analysis.

DTIC Science & Technology

1980-04-25

Co., 1970. Nozick , Robert . Anarchy, State, and Utopia. Basic Books, Inc, 1974. Plamenatz, J. P. Consent, Freedom, and Political Oblizatio7, 2nd ed...in America. This conception has its strongest philosophical roots in the Lockean theory of gover-nment by consent. On this view.-, a citizen of the...such thinking go far deeper than Locke’s theory of government by consent. Plato records well in the Crito the Socratic view of a citizen’s obligations

JPRS Report, East Europe.

DTIC Science & Technology

1990-06-04

Although even today the 1945 minorities law have joined. which is still in force would do the job .... [Szucs] In a manner similar to the Germans...than by any utopias. manual jobs , but upon the intervention of the State Security Corps he got dismissed from every one of However, I appeal also to...in the private sector; small enterprises affirmative to the question of whether as a woman she offer double or triple the amount they earned at the

Learning: The Treasure Within. Report to UNESCO of the International Commission on Education for the Twenty-first Century.

ERIC Educational Resources Information Center

Delors, Jacques; And Others

This book results from a three-year exploration of how to provide a new outlook on how all societies should move towards a "necessary Utopia" in which no one's hidden talents are left untapped. The report builds on the four foundations of education: (1) learning to live together; (2) learning to know; (3) learning to do; and (4) learning to be .…

Translations from KOMMUNIST No. 12, August 1978

DTIC Science & Technology

1978-10-23

of respect, full of ideal thrusts; on the other, the scientist whose "utopia" of a classless society has been "buried in the catacombs of history...wishes to be democratic" (M. Duverger, "Lettre ouverte aux socialistes" [Open Letter to the Socialists], Paris , 1976, p 54). Naturally, the bour...83-87 [Article by V. Sedykh, Paris -Moscow, August 1978] [Text] Documents which inform us of new details of Lev Nikolayevich Tolstoy’s life and

Trying to Build a Classless Utopia in the Land of Racial Democracy: The Lack of Racial Discussion within the Educational Materials of the Brazilian Landless Rural Workers' Movement

ERIC Educational Resources Information Center

Straubhaar, Rolf

2017-01-01

The hegemonic ideology of racial democracy and rural cultural norms of racial silence continue to inform racial identities and national racial discourse in Brazil, in this case within the Landless Rural Workers' Movement (MST), a left-wing movement for agrarian reform. In this article I engage in textual analysis of a textbook from the MST's youth…

UTOPIA-User-Friendly Tools for Operating Informatics Applications.

PubMed

Pettifer, S R; Sinnott, J R; Attwood, T K

2004-01-01

Bioinformaticians routinely analyse vast amounts of information held both in large remote databases and in flat data files hosted on local machines. The contemporary toolkit available for this purpose consists of an ad hoc collection of data manipulation tools, scripting languages and visualization systems; these must often be combined in complex and bespoke ways, the result frequently being an unwieldy artefact capable of one specific task, which cannot easily be exploited or extended by other practitioners. Owing to the sizes of current databases and the scale of the analyses necessary, routine bioinformatics tasks are often automated, but many still require the unique experience and intuition of human researchers: this requires tools that support real-time interaction with complex datasets. Many existing tools have poor user interfaces and limited real-time performance when applied to realistically large datasets; much of the user's cognitive capacity is therefore focused on controlling the tool rather than on performing the research. The UTOPIA project is addressing some of these issues by building reusable software components that can be combined to make useful applications in the field of bioinformatics. Expertise in the fields of human computer interaction, high-performance rendering, and distributed systems is being guided by bioinformaticians and end-user biologists to create a toolkit that is both architecturally sound from a computing point of view, and directly addresses end-user and application-developer requirements.

Search for the viking 2 landing site.

PubMed

Masursky, H; Crabill, N L

1976-10-01

The search for the landing site of Viking 2 was more extensive than the search for the Viking 1 site. Seven times as much area (4.5 million square kilometers) was examined as for Viking 1. Cydonia (B1) and Capri (C1) sites were examined with the Viking 1 orbiter. The B latitude band (40 degrees to 50 degrees N) was selected before the final midcourse maneuver of Viking 2 because of its high scientific interest (that is, high atmospheric water content, surface temperature, possible near-surface permafrost, and a different geological domain). The Viking 1 orbiter continued photographing the Cydonia (B1) site to search for an area large and smooth enough on which to land (three-sigma ellipse; 100 by 260 kilometers); such an area was not found. The second spacecraft photographed and made infrared measurements in large areas in Arcadia (B2) and Utopia Planitia (B3). Both areas are highly textured, mottled cratered plains with abundant impact craters like Cydonia (B1), but smaller sectors in each area are partially mantled by wind-formed deposits. The thermal inertia, from which the grain size of surface material can be computed, and atmospheric water content were determined from the infrared observations. A region in Utopia Planitia, west of the crater Mie, was selected: the landing took place successfully on 3 September 1976 at 3:58:20 p.m. Pacific Daylight Time, earth received time.

Search for the Viking 2 landing site

USGS Publications Warehouse

Masursky, H.; Crabill, N.L.

1976-01-01

The search for the landing site of Viking 2 was more extensive than the search for the Viking 1 site. Seven times as much area (4.5 million square kilometers) was examined as for Viking 1. Cydonia (B1) and Capri (C1) sites were examined with the Viking 1 orbiter. The B latitude band (40?? to 50??N) was selected before the final midcourse maneuver of Viking 2 because of its high scientific interest (that is, high atmospheric water content, surface temperature, possible near-surface permafrost, and a different geological domain). The Viking 1 orbiter continued photographing the Cydonia (B1) site to search for an area large and smooth enough on which to land (three-sigma ellipse; 100 by 260 kilometers); such an area was not found. The second spacecraft photographed and made infrared measurements in large areas in Arcadia (B2) and Utopia Planitia (B3). Both areas are highly textured, mottled cratered plains with abundant impact craters like Cydonia (B1), but smaller sectors in each area are partially mantled by wind-formed deposits. The thermal inertia, from which the grain size of surface material can be computed, and atmospheric water content were determined from the infrared observations. A region in Utopia Planitia, west of the crater Mie, was selected: the landing took place successfully on 3 September 1976 at 3:58:20 p.m. Pacific Daylight Time, earth received time.

[Health as utopia. Grounds and causes of lack of demand for early diagnostic measures (author's transl)].

PubMed

Buser, K; Oeter, K

1981-11-27

The quite obvious neglect of prophylactic measures cannot be attributed to a single cause only. Ground are rather to be found both in the psychic disposition and in the social stratum of the population as well as in the nature of the prophylaxis available. A synopsis leads to the conclusion that effective prevention requires not only changing the attitude of the patient or the population but also that of the supplier of the health promoting services.

Hetero-oligonucleotide Nanoscale Tiles Capable of Two-Dimensional Lattice Formation as Testbeds for a Rapid, Affordable Purification Methodology

DTIC Science & Technology

2013-01-01

SUBJECT TERMS DNA nanotechnology, purification, origami , 2d arrays Philip S. Lukeman St. John’s University, New York 8000 Utopia Parkway Queens, NY... origami ; DNA double-crossover (“DX”) tile based arrays5 have been constructed using PNA6 and LNA7 oligonucleotides. RNA/ DNA duplexes have been used8 for...the assembly of multiply armed tiles9 and as a template10 to fold DNA origami ;11 all-RNA systems known as ‘tecto-RNA’ have been used to generate a wide

Viking Lander 2 Anniversary

NASA Image and Video Library

2002-12-13

This portion of NASA Mars Odyssey image covers NASA Viking 2 landing site shown with the X. The second landing on Mars took place September 3, 1976 in Utopia Planitia. The exact location of Lander 2 is not as well established as Lander 1 because there were no clearly identifiable features in the lander images as there were for the site of Lander 1. The Utopia landing site region contains pedestal craters, shallow swales and gentle ridges. The crater Goldstone was named in honor of the Tracking Station in the desert of California. The two Viking Landers operated for over 6 years (nearly four martian years) after landing. This one band IR (band 9 at 12.6 microns) image shows bright and dark textures, which are primarily due to differences in the abundance of rocks on the surface. The relatively cool (dark) regions during the day are rocky or indurated materials, fine sand and dust are warmer (bright). Many of the temperature variations are due to slope effects, with sun-facing slopes warmer than shaded slopes. The dark rings around several of the craters are due to the presence of rocky (cool) material ejected from the crater. These rocks are well below the resolution of any existing Mars camera, but THEMIS can detect the temperature variations they produce. Daytime temperature variations are produced by a combination of topographic (solar heating) and thermophysical (thermal inertia and albedo) effects. Due to topographic heating the surface morphologies seen in THEMIS daytime IR images are similar to those seen in previous imagery and MOLA topography. http://photojournal.jpl.nasa.gov/catalog/PIA04023

Cracky Mars

NASA Technical Reports Server (NTRS)

2006-01-01

21 September 2006 This Mars Global Surveyor (MGS) Mars Orbiter Camera (MOC) image shows cracked, layered plains-forming material in the western part of Utopia Planitia, Mars. Investigators have speculated that ice might be -- or might once have been -- present in the ground, and changes in temperature and the amount of ice over time may have led to the formation of these cracks. But no one is certain just how these features formed.

Location near: 45.0oN, 276.1oW Image width: 3 km (1.9 mi) Illumination from: lower left Season: Northern Spring

Evidence of mud volcanism rooted in gas hydrate-rich cryosphere linking surface and subsurface for the search for life on Mars

NASA Astrophysics Data System (ADS)

De Toffoli, Barbara; Pozzobon, Riccardo; Mazzarini, Francesco; Massironi, Matteo; Cremonese, Gabriele

2017-04-01

We mapped around 6000 mounds in three different portions of the Martian surface on an average area of about 90.000 Km2 for each region. The study areas are located in Hellas basin, Utopia basin and a portion of the Northern Plains lying north of Arabia Terra, between Acidalia and Utopia Planitia. The aim of the study was to understand the nature of the observed features, particularly if they could be interpreted as mud volcanoes or not, and improve our knowledge about the Martian mound fields origin. The analysis of Context Camera (onboard Mars Reconnaissance Orbiter) images showed circular, elliptical and coalescent mounds with central and/or distal pits and flow features such as concentric annular lobes around the source pits and apron-like extensions. We produced DTMs and then high-to-diameter morphometric analysis on two groups of mounds located in Utopia and Hellas basins to enhance the geomorphological observations. We inferred, by means of cluster and fractal analyses, the thickness of the medium cracked by connected fractures and, consequently, the depths of reservoirs that fed the mounds. We found that the fields, which are seated at different latitudes, has been fed, at least partially, by reservoirs located at the base of the gas hydrate stability zone according to Clifford et al., 2010. This evidence produces a meaningful relationship between the clathrates distribution underneath the Martian surface and the occurrence of mound fields on the surface leading to the assumption that the involvement of water, ostensibly as a result of gas hydrate dissociation, plays a key role in the subsurface processes that potentially worked as triggers. These outcomes corroborate the hypothesis that the mapped mounds are actually mud volcanoes and make these structures outstanding targets for astrobiology and habitability studies. In fact, mud volcanoes, extruding material from depths that are still not affordable by our present-day instrumentations, could have sampled and brought to the surface with the sediments a putative extinct or extant deep biosphere. In conclusion, on the base of this study, emerged that: (i) mud volcanoes are the best terrestrial analogs for the considered Martian mounds, (ii) there is a recurrent specific subsurface environment where the phenomenon may be triggered and it is the base of gas hydrate-rich cryosphere for all the study areas and (iii) mud volcanism seems to be, at least partially, a geologically recent event in terms of planet thermal evolution timespan. In light of these results, the CaSSIS camera, onboard the Trace Gas Orbiter ExoMARS mission, will provide new images of these features to improve and widen the understanding of the mechanisms that lie behind this phenomenon.

Rationale, Design, and Baseline Characteristics of the Utopia Trial for Preventing Diabetic Atherosclerosis Using an SGLT2 Inhibitor: A Prospective, Randomized, Open-Label, Parallel-Group Comparative Study.

PubMed

Katakami, Naoto; Mita, Tomoya; Yoshii, Hidenori; Shiraiwa, Toshihiko; Yasuda, Tetsuyuki; Okada, Yosuke; Umayahara, Yutaka; Kaneto, Hideaki; Osonoi, Takeshi; Yamamoto, Tsunehiko; Kuribayashi, Nobuichi; Maeda, Kazuhisa; Yokoyama, Hiroki; Kosugi, Keisuke; Ohtoshi, Kentaro; Hayashi, Isao; Sumitani, Satoru; Tsugawa, Mamiko; Ohashi, Makoto; Taki, Hideki; Nakamura, Tadashi; Kawashima, Satoshi; Sato, Yasunori; Watada, Hirotaka; Shimomura, Iichiro

2017-10-01

Sodium-glucose co-transporter-2 (SGLT2) inhibitors are anti-diabetic agents that improve glycemic control with a low risk of hypoglycemia and ameliorate a variety of cardiovascular risk factors. The aim of the ongoing study described herein is to investigate the preventive effects of tofogliflozin, a potent and selective SGLT2 inhibitor, on the progression of atherosclerosis in subjects with type 2 diabetes (T2DM) using carotid intima-media thickness (IMT), an established marker of cardiovascular disease (CVD), as a marker. The Study of Using Tofogliflozin for Possible better Intervention against Atherosclerosis for type 2 diabetes patients (UTOPIA) trial is a prospective, randomized, open-label, blinded-endpoint, multicenter, and parallel-group comparative study. The aim was to recruit a total of 340 subjects with T2DM but no history of apparent CVD at 24 clinical sites and randomly allocate these to a tofogliflozin treatment group or a conventional treatment group using drugs other than SGLT2 inhibitors. As primary outcomes, changes in mean and maximum IMT of the common carotid artery during a 104-week treatment period will be measured by carotid echography. Secondary outcomes include changes in glycemic control, parameters related to β-cell function and diabetic nephropathy, the occurrence of CVD and adverse events, and biochemical measurements reflecting vascular function. This is the first study to address the effects of SGLT2 inhibitors on the progression of carotid IMT in subjects with T2DM without a history of CVD. The results will be available in the very near future, and these findings are expected to provide clinical data that will be helpful in the prevention of diabetic atherosclerosis and subsequent CVD. Kowa Co., Ltd. UMIN000017607.

Pingos on Earth and Mars

USGS Publications Warehouse

Burr, D.M.; Tanaka, K.L.; Yoshikawa, K.

2009-01-01

Pingos are massive ice-cored mounds that develop through pressurized groundwater flow mechanisms. Pingos and their collapsed forms are found in periglacial and paleoperiglacial terrains on Earth, and have been hypothesized for a wide variety of locations on Mars. This literature review of pingos on Earth and Mars first summarizes the morphology of terrestrial pingos and their geologic contexts. That information is then used to asses hypothesized pingos on Mars. Pingo-like forms (PLFs) in Utopia Planitia are the most viable candidates for pingos or collapsed pingos. Other PLFs hypothesized in the literature to be pingos may be better explained with other mechanisms than those associated with terrestrial-style pingos. ?? 2008 Elsevier Ltd.

Mud Volcanoes as Exploration Targets on Mars

NASA Technical Reports Server (NTRS)

Allen, Carlton C.; Oehler, Dorothy Z.

2010-01-01

Tens of thousands of high-albedo mounds occur across the southern part of the Acidalia impact basin on Mars. These structures have geologic, physical, mineralogic, and morphologic characteristics consistent with an origin from a sedimentary process similar to terrestrial mud volcanism. The potential for mud volcanism in the Northern Plains of Mars has been recognized for some time, with candidate mud volcanoes reported from Utopia, Isidis, northern Borealis, Scandia, and the Chryse-Acidalia region. We have proposed that the profusion of mounds in Acidalia is a consequence of this basin's unique geologic setting as the depocenter for the tune fraction of sediments delivered by the outflow channels from the highlands.

The mosaics of Mars: As seen by the Viking Lander cameras

NASA Technical Reports Server (NTRS)

Levinthal, E. C.; Jones, K. L.

1980-01-01

The mosaics and derivative products produced from many individual high resolution images acquired by the Viking Lander Camera Systems are described: A morning and afternoon mosaic for both cameras at the Lander 1 Chryse Planitia site, and a morning, noon, and afternoon camera pair at Utopia Planitia, the Lander 11 site. The derived products include special geometric projections of the mosaic data sets, polar stereographic (donut), stereoscopic, and orthographic. Contour maps and vertical profiles of the topography were overlaid on the mosaics from which they were derived. Sets of stereo pairs were extracted and enlarged from stereoscopic projections of the mosaics.

Use of spacecraft data to derive regions on Mars where liquid water would be stable

PubMed Central

Lobitz, Brad; Wood, Byron L.; Averner, Maurice M.; McKay, Christopher P.

2001-01-01

Combining Viking pressure and temperature data with Mars Orbital Laser Altimeter topography data, we have computed the fraction of the martian year during which pressure and temperature allow for liquid water to be stable on the martian surface. We find that liquid water would be stable within the Hellas and Argyre basin and over the northern lowlands equatorward of about 40°. The location with the maximum period of stable conditions for liquid water is in the southeastern portion of Utopia Planitia, where 34% of the year liquid water would be stable if it were present. Locations of stability appear to correlate with the distribution of valley networks. PMID:11226204

The Martian surface as imaged, sampled, and analyzed by the Viking landers

NASA Technical Reports Server (NTRS)

Arvidson, Raymond E.; Gooding, James L.; Moore, Henry J.

1989-01-01

Data collected by two Viking landers are analyzed. Attention is given to the characteristics of the surface inferred from Lander imaging and meteorology data, physical and magnetic properties experiments, and both inorganic and organic analyses of Martian samples. Viking Lander 1 touched down on Chryse Planitia on July 20, 1976 and continued to operate for 2252 sols, until November 20, 1982. Lander 2 touched down about 6500 km away from Lander 1, on Utopia Planitia on September 3, 1976. The chemical compositions of sediments at the two landing sites are similar, suggesting an aeolian origin. The compositions suggest an iron-rich rock an are matched by various clays and salts.

Use of Spacecraft Data to Drive Regions on Mars where Liquid Water would be Stable

NASA Technical Reports Server (NTRS)

Lobitz, Brad; Wood, Byron L.; Averner, Maurice M.; McKay, Christopher P.; MacElroy, Robert D.

2001-01-01

Combining Viking pressure and temperature data with Mars Orbital Laser Altimeter (MOLA) topography data we have computed the fraction of the martian year during which pressure and temperature allow for liquid water to be stable on the martian surface. We find that liquid water would be stable within the Hellas and Argyre basin and over the northern lowlands equatorward of about 40 degrees. The location with the maximum period of stable conditions for liquid water is in the southeastern portion of Utopia Planitia where 34% of the year liquid water would be stable if it was present. Locations of stability appear to correlate with the distribution of valley networks.

Emergence of a utopian vision of modernist and futuristic houses and cities in early 20th century

NASA Astrophysics Data System (ADS)

Ma, Nan

2017-04-01

Throughout the development of literature on urban design theories, utopian thinking has played a crucial role as utopians were among the first designers. Many unrealized utopian projects such as The Radiant City, have presented a research laboratory and positive attempts for all architects, urban designers and theorists. In this essay, a utopian vision following under More’s and Jameson’s definitions is discussed, examining how the utopian vision of modernist and futuristic houses and cities emerged in the early twentieth century in response to several factors, what urban utopia aimed to represent, and how such version was represented in the built form and the urban landscapes.

Periglacial complexes in Utopia Planitia: rimless, tiered depressions, (clastically) sorted and unsorted polygonised terrain and an ice-rich mantle

NASA Astrophysics Data System (ADS)

Soare, Richard; Conway, Susan; Gallagher, Colman; Dohm, James; Clifford, Stephen M.; Williams, Jean-pierre

2016-10-01

We report the spatial and possible genetic-relationship at the mid-latitudes of Utopia Planitia (45-500N 115-1200E), Mars, of: (a) metre to decametre deep, rimless, tiered depressions; terrain that exhibits (b) (clastically) sorted and (c) unsorted (small-sized) polygons; and, (d) a very youthful, ice-rich mantle. We show that these individual landscape features are separated stratigraphically, this being presented to the Mars community for the first time, and suggest that the stratigraphical separation of these features could be the result of boundary conditions and formation processes that have varied much more widely than has been thought hitherto. In cold-climate and non-glacial regions such as the Yamal Peninsula of eastern Russia and the Tuktoyaktuk Coastlands of northern Canada, landscape assemblages comprised of similar features are referenced as "ice complexes" and are indicative of periglacialism on two fronts: first, the presence of "ice-rich" permafrost or permafrost comprised of "excess ice", i.e. "permafrost" whose pore space is exceeded by the "water ice" within that body of sediment; and, second, antecedently or currently active freeze-thaw cycling, minimally, to the full depth of the "ice-complex" depressions. In the Dry Valleys of the Antarctic, where the atmospheric aridity and cold-temperatures approach those of Mars, ice-vapour diffusion and adsorption cycles are cited as the means by which the near-surface, permafrost, i.e. ≤1m deep, has become ice-cemented. However, the metre to decametre depths of the "ice-complex" depressions on Earth and the morphologically-similar ones on Mars lie beyond the vertical reach of the Antarctic diffusion and adsorption cycles, both empirically and theoretically. By deduction, this points to the freeze-thaw cycling of water to depth, fostered either by exogenic or endogenic means, perhaps playing a more important role in the formation of the possible Martian "ice complexes" than might be expected were expectations based solely on the current cold-climate "Antarctic-like" paradigm.

A Peek into a Cul-De-Sac and a Mews of Martian Dust Storm Activity: Western Hellas and Syria-Claritas Fossae During Mars Year 29

NASA Astrophysics Data System (ADS)

Heavens, N. G.

2016-12-01

Western Hellas Planitia (WHP) and the region encompassed by Syria Planum and Claritas Fossae are the main centers of textured dust storm activity in Mars's southern low to mid-latitudes. (Texture in this context refers to distinct fine structure at the cloud tops indicative of active lifting.) WHP is a well-known initiation zone for regional and global dust storm activity and often the end point of the Utopia "flushing storm" track. Syria-Claritas Fossae (SCF), too, can be a lifting center in global dust storm activity. Indeed, SCF and the area to its west was the region most denuded of dust by the Mars Year (MY) 25 global dust storm, perhaps suggesting that SCF contained the principal lifting center of the storm. Thus, if the Acidalia and Utopia storm tracks are Mars's dust storm alleys, through which dust storms pass quickly again and again; WHP might be a cul-de-sac and SCF something like a mews, where dust storm activity can enter more or less easily but may not as easily leave. In this presentation, I will focus on dust storm activity in these areas in a typical non-global dust storm year, MY 29. Synthesizing visible imagery by the Mars Color Imager (MARCI) on board Mars Reconnaissance Orbiter (MRO) and Mars Climate Sounder (MCS) also on board MRO, I will consider the climatology, morphology, texture, and vertical structure of dust storm activity in these areas in order to infer their governing dynamics. This investigation has two aims: (1) to understand why these areas are centers of textured dust storm activity; and (2) to connect the characteristics of smaller-scale dust storm activity in these regions to the underlying dynamics in order to understand the role of WHP and SCF in the dynamics of global dust storms. This work is supported by NASA's Mars Data Analysis Program (NNX14AM32G).

Visualising biological data: a semantic approach to tool and database integration.

PubMed

Pettifer, Steve; Thorne, David; McDermott, Philip; Marsh, James; Villéger, Alice; Kell, Douglas B; Attwood, Teresa K

2009-06-16

In the biological sciences, the need to analyse vast amounts of information has become commonplace. Such large-scale analyses often involve drawing together data from a variety of different databases, held remotely on the internet or locally on in-house servers. Supporting these tasks are ad hoc collections of data-manipulation tools, scripting languages and visualisation software, which are often combined in arcane ways to create cumbersome systems that have been customized for a particular purpose, and are consequently not readily adaptable to other uses. For many day-to-day bioinformatics tasks, the sizes of current databases, and the scale of the analyses necessary, now demand increasing levels of automation; nevertheless, the unique experience and intuition of human researchers is still required to interpret the end results in any meaningful biological way. Putting humans in the loop requires tools to support real-time interaction with these vast and complex data-sets. Numerous tools do exist for this purpose, but many do not have optimal interfaces, most are effectively isolated from other tools and databases owing to incompatible data formats, and many have limited real-time performance when applied to realistically large data-sets: much of the user's cognitive capacity is therefore focused on controlling the software and manipulating esoteric file formats rather than on performing the research. To confront these issues, harnessing expertise in human-computer interaction (HCI), high-performance rendering and distributed systems, and guided by bioinformaticians and end-user biologists, we are building reusable software components that, together, create a toolkit that is both architecturally sound from a computing point of view, and addresses both user and developer requirements. Key to the system's usability is its direct exploitation of semantics, which, crucially, gives individual components knowledge of their own functionality and allows them to interoperate seamlessly, removing many of the existing barriers and bottlenecks from standard bioinformatics tasks. The toolkit, named Utopia, is freely available from http://utopia.cs.man.ac.uk/.

Integrating feminist and psychodynamic principles in the treatment of an eating disorder patient: implications for using countertransference responses.

PubMed

Zerbe, K J

1995-01-01

Patients who struggle with a tenacious eating disorder commonly stir strong countertransference feelings in therapists. The author describes a patient who for a number of years had been unresponsive to traditional treatment interventions for anorexia nervosa and bulimic tendencies. By combining principles derived from psychodynamic treatment and contemporary feminist thought, the therapist was gradually able to help the patient engage in the treatment process. Managing a variety of strong countertransference feelings was instrumental to the process. The author underscores the need for patients to take greater personal responsibility, develop self-critical and self-analytical capacities, learn to embrace contradictions in the self, and disavow the tendency to harbor fantasies of utopia, perfection, and "cure."

The Martian surface as imaged, sampled, and analyzed by the Viking landers

DOE Office of Scientific and Technical Information (OSTI.GOV)

Arvidson, R.E.; Gooding, J.L.; Moore, H.J.

1989-02-01

Data collected by two Viking landers are analyzed. Attention is given to the characteristics of the surface inferred from Lander imaging and meteorology data, physical and magnetic properties experiments, and both inorganic and organic analyses of Martian samples. Viking Lander 1 touched down on Chryse Planitia on July 20, 1976 and continued to operate for 2252 sols, until November 20, 1982. Lander 2 touched down about 6500 km away from Lander 1, on Utopia Planitia on September 3, 1976. The chemical compositions of sediments at the two landing sites are similar, suggesting an aeolian origin. The compositions suggest an iron-richmore » rock an are matched by various clays and salts. 89 refs.« less

Inorganic analyses of Martian surface samples at the Viking landing sites

NASA Technical Reports Server (NTRS)

Clark, B. C.; Castro, A. J.; Rowe, C. D.; Baird, A. K.; Evans, P. H.; Rose, H. J., Jr.; Toulmin, P., III; Keil, K.; Kelliher, W. C.

1976-01-01

Elemental analyses of fines in the Martian regolith at two widely separated landing sites, Chryse Planitia and Utopia Planitia, produced remarkably similar results. At both sites, the uppermost regolith contains abundant Si and Fe, with significant concentrations of Mg, Al, S, Ca, and Ti. The S concentration is one to two orders of magnitude higher, and K (less than 0.25% by weight) is at least 5 times lower than the average for earth's crust. The trace elements Sr, Y, and possibly Zr have been detected at concentrations near or below 100 parts per million. Pebble-sized fragments sampled at Chryse contain more S than the bulk fines and are thought to be pieces of a sulfate-cemented duricrust.

Inorganic analyses of martian surface samples at the viking landing sites.

PubMed

Clark, B C; Baird, A K; Rose, H J; Toulmin, P; Keil, K; Castro, A J; Kelliher, W C; Rowe, C D; Evans, P H

1976-12-11

Elemental analyses of fines in the Martian regolith at two widely separated landing sites, Chryse Planitia and Utopia Planitia, produced remarkably similar results. At both sites, the uppermost regolith contains abundant Si and Fe, with significant concentrations of Mg, Al, S, Ca, and Ti. The S concentration is one to two orders of magnitude higher, and K(<0.25 percent by weight) is at least 5 times lower than the average for the earth's crust. The trace elements Sr, Y, and possibly Zr, have been detected at concentrations near or below 100 parts per million. Pebblesized fragments sampled at Chryse contain more S than the bulk fines, and are thought to be pieces of a sulfate-cemented duricrust.

[Cerebrospinal fluid diagnostics in Germany since 1950 : Developments in the GDR and FRG in the context of society and science].

PubMed

Reiber, H

2016-12-01

The 40 years of separated development in two countries with extremely different political and social utopias allow consideration of the connection between science and society. The society-dependent development of cerebrospinal fluid (CSF) diagnostics in the German Democratic Republic (GDR) and the Federal Republic of Germany (FRG) is shown in the context of the international scientific development of the post-war era with new paradigms in physics, biology and genetics. As part of this contribution to the philosophy of science the consequences of the complex life science for a new view of disease research are discussed in contrast to the currently dominating, reductionistic medical industrial complex.

Of mice and men: evolution and the socialist utopia. William Morris, H.G. Wells, and George Bernard Shaw.

PubMed

Hale, Piers J

2010-01-01

During the British socialist revival of the 1880s competing theories of evolution were central to disagreements about strategy for social change. In News from Nowhere (1891), William Morris had portrayed socialism as the result of Lamarckian processes, and imagined a non-Malthusian future. H.G. Wells, an enthusiastic admirer of Morris in the early days of the movement, became disillusioned as a result of the Malthusianism he learnt from Huxley and his subsequent rejection of Lamarckism in light of Weismann's experiments on mice. This brought him into conflict with his fellow Fabian, George Bernard Shaw, who rejected neo-Darwinism in favour of a Lamarckian conception of change he called "creative evolution."

Looking for water related environments on Mars: analysis of reflectance spectra for present and future exploration

NASA Astrophysics Data System (ADS)

De Toffoli, B.; Carli, C.; Maturilli, A.; Sauro, F.; Massironi, M.; Helbert, J.

2017-09-01

Spectroscopic analyses of basalt epithermal alterations, clay minerals and samples representative of wet sedimentary environments in a broad wavelength range from the ultraviolet to the far-infrared provide new loads of information for present and future exploration of environments that could have been linked to water and gas emission. Specifically, methane emission centers on the Martian surface are high interest targets for Exo-Mars mission since they involve environments where life could have potentially arisen, grown and given a contribution to the degassing phenomenon. Such data will be applied to drive the analysis on remotely sensed hyperspectral images of Martian regions where surface expressions of water and sediments resurgences are recognisable, such as the mound fields detected in Utopia and Hellas basins and Vastitas Borealis.

Freedom and authority in the Clinical Diary.

PubMed

Erős, Ferenc

2014-12-01

The paper discusses some philosophical, ethical and political-philosophical implications of Ferenczi's Clinical Diary, with special regard to the concepts of freedom and authority. These topics are already present in Ferenczi's early writings that explicitly deal with social and political issues, the central concept of which is "individual socialism". The paper also discusses (and publishes in Appendix) two short manuscripts by Ferenczi, written probably in 1920, which attempts to parallel psychoanalysis with Marxism, and with liberal socialism, respectively. It is shown that in 1932, the last year of his life, Ferenczi avoids using political and ideological concepts directly in his Diary, but, in the spirit of his earlier writings, he proposes a balance between "ruthless capitalism and fanciful egalitarianism". Finally, the significance of Utopia in Ferenczi's thinking is discussed.

Ancient geodynamics and global-scale hydrology on Mars.

PubMed

Phillips, R J; Zuber, M T; Solomon, S C; Golombek, M P; Jakosky, B M; Banerdt, W B; Smith, D E; Williams, R M; Hynek, B M; Aharonson, O; Hauck , S A

2001-03-30

Loading of the lithosphere of Mars by the Tharsis rise explains much of the global shape and long-wavelength gravity field of the planet, including a ring of negative gravity anomalies and a topographic trough around Tharsis, as well as gravity anomaly and topographic highs centered in Arabia Terra and extending northward toward Utopia. The Tharsis-induced trough and antipodal high were largely in place by the end of the Noachian Epoch and exerted control on the location and orientation of valley networks. The release of carbon dioxide and water accompanying the emplacement of approximately 3 x 10(8) cubic kilometers of Tharsis magmas may have sustained a warmer climate than at present, enabling the formation of ancient valley networks and fluvial landscape denudation in and adjacent to the large-scale trough.

Could giant basin-forming impacts have killed Martian dynamo?

PubMed Central

Kuang, W; Jiang, W; Roberts, J; Frey, H V

2014-01-01

The observed strong remanent crustal magnetization at the surface of Mars suggests an active dynamo in the past and ceased to exist around early to middle Noachian era, estimated by examining remagnetization strengths in extant and buried impact basins. We investigate whether the Martian dynamo could have been killed by these large basin-forming impacts, via numerical simulation of subcritical dynamos with impact-induced thermal heterogeneity across the core-mantle boundary. We find that subcritical dynamos are prone to the impacts centered on locations within 30° of the equator but can easily survive those at higher latitudes. Our results further suggest that magnetic timing places a strong constraint on postimpact polar reorientation, e.g., a minimum 16° polar reorientation is needed if Utopia is the dynamo killer. PMID:26074641

Could Giant Basin-Forming Impacts Have Killed Martian Dynamo?

NASA Technical Reports Server (NTRS)

Kuang, W.; Jiang, W.; Roberts, J.; Frey, H. V.

2014-01-01

The observed strong remanent crustal magnetization at the surface of Mars suggests an active dynamo in the past and ceased to exist around early to middle Noachian era, estimated by examining remagnetization strengths in extant and buried impact basins. We investigate whether the Martian dynamo could have been killed by these large basin-forming impacts, via numerical simulation of subcritical dynamos with impact-induced thermal heterogeneity across the core-mantle boundary. We find that subcritical dynamos are prone to the impacts centered on locations within 30 deg of the equator but can easily survive those at higher latitudes. Our results further suggest that magnetic timing places a strong constraint on postimpact polar reorientation, e.g., a minimum 16 deg polar reorientation is needed if Utopia is the dynamo killer.

Could giant basin-forming impacts have killed Martian dynamo?

PubMed

Kuang, W; Jiang, W; Roberts, J; Frey, H V

2014-11-28

The observed strong remanent crustal magnetization at the surface of Mars suggests an active dynamo in the past and ceased to exist around early to middle Noachian era, estimated by examining remagnetization strengths in extant and buried impact basins. We investigate whether the Martian dynamo could have been killed by these large basin-forming impacts, via numerical simulation of subcritical dynamos with impact-induced thermal heterogeneity across the core-mantle boundary. We find that subcritical dynamos are prone to the impacts centered on locations within 30° of the equator but can easily survive those at higher latitudes. Our results further suggest that magnetic timing places a strong constraint on postimpact polar reorientation, e.g., a minimum 16° polar reorientation is needed if Utopia is the dynamo killer.

Buried and Visible Impact Basin Distribution on Mars: Comparison with Magnetization, Gravity and Crustal Thickness Models

NASA Technical Reports Server (NTRS)

Frey, Herbert

2003-01-01

The large population of buried impact basins found in MOLA elevation data on Mars provides compelling evidence for a pre-Noachian crust below the oldest visible Early Noachian surface units, and lowland crust below the younger plains that is Early Noachian in age, older than much of the visible highlands, but not as old as the buried pre-Noachian highlands. The large (D greater than 200 km) buried basins are suggested by Quasi-Circular Depressions (QCDs) that are not apparent in image data, and include features up to 3000 lun diameter in both the lowlands (Utopia) and highlands (a newly found "Ares Basin"). There are about a dozen QCDs larger than 1000 km diameter. We have placed these large features in a relative age sequence based on superimposed smaller QCD. Only the youngest and most obvious of these (Hellas, Argyre, Isidis) lack magnetic anomalies within their main rings. These all have an N(200) cumulative crater density of less than 2.5. Somewhat older lowland-making basins (Utopia, Chryse, Acidalia) with an N(200) age of approximately 3.0, have weak magnetic anomalies, and the oldest, most subdued basins (including Ares) with N(200) greater than 3.5 have many strong magnetic anomalies within their main ring. These older basins likely formed before the main magnetic field died. We have compared our inventory of large QCDs with the distribution of gravity anomalies and with a crustal thickness model which shows many roughly circular areas of thinner crust completely or partly surrounded by narrow regions of thicker crust. These have the structure expected for impact basins, and many of them do correspond to the visible or buried QCDs we previously identified. But there are cases where the crustal thickness feature is offset from the QCD found in topography alone, and there are also several, sometimes large examples of such features which do not coincide with QCDs previously identified. For example, we find several likely buried basins revealed in the crustal thickness data in the Arcadia and Amazonis regions which we did not previously identify, including several features in the 600-1200 km diameter range.

[The evolutionist fallacy of early visitors. Analogies between 'primitive peoples' and prehistoric man in medical historiography].

PubMed

Bruchhausen, Walter

2006-01-01

Accounts of 'prehistoric medicine' and 'ethnomedicine' have sometimes led to conclusions by analogy in medical historiography that are seen as highly problematic in modern cultural anthropology. However, this review of medical historical writings of the last three centuries shows that evolutionist identifications of early with foreign medicine were not a permanent trait of medical historiography. This approach flourished mainly in the climate of certain movements or periods that were characterised by fanatical belief in progress and by social utopias: the French Revolution, Darwinism and the period of industrial expansion in Germany, and National Socialism. Medical historiography shared this problematic approach with contemporary (social and cultural) anthropology, and - despite this methodological misuse - both acknowledged the legitimacy or even requirement of studying also similarities in the development of different periods and cultures.

Utopian Vision: A Grand Solution for a Scholarly Dilemma.

PubMed

Watts, Roderick J

2017-06-01

Reconciling the Zen-like paradox on the back of every red penny-"out of many, one"-is not for the faint of heart. It is a diversity motto, and a lofty desire that the United States claims to covet. But can its citizens, undocumented or otherwise, even agree on what it is? Is not the desire to maintain a strong sense of community in conflict with a Noah's Ark conception of diversity? Using my personal experience in an intentional community determined to foster racial integration, I explore the complicated possibility of having it both ways. To do so, however, we must construct a notion of community, diversity, and The Good Life that will make us believe and work for this synthesis. Our reactions to the word "utopia" offer a glimpse of the challenges ahead. © Society for Community Research and Action 2017.

Viking Lander Mosaics of Mars

NASA Technical Reports Server (NTRS)

Morris, E. C.

1985-01-01

The Viking Lander 1 and 2 cameras acquired many high-resolution pictures of the Chryse Planitia and Utopia Planitia landing sites. Based on computer-processed data of a selected number of these pictures, eight high-resolution mosaics were published by the U.S. Geological Survey as part of the Atlas of Mars, Miscellaneous Investigation Series. The mosaics are composites of the best picture elements (pixels) of all the Lander pictures used. Each complete mosaic extends 342.5 deg in azimuth, from approximately 5 deg above the horizon to 60 deg below, and incorporates approximately 15 million pixels. Each mosaic is shown in a set of five sheets. One sheet contains the full panorama from one camera taken in either morning or evening. The other four sheets show sectors of the panorama at an enlarged scale; when joined together they make a panorama approximately 2' X 9'.

A comparison of queueing, cluster and distributed computing systems

NASA Technical Reports Server (NTRS)

Kaplan, Joseph A.; Nelson, Michael L.

1993-01-01

Using workstation clusters for distributed computing has become popular with the proliferation of inexpensive, powerful workstations. Workstation clusters offer both a cost effective alternative to batch processing and an easy entry into parallel computing. However, a number of workstations on a network does not constitute a cluster. Cluster management software is necessary to harness the collective computing power. A variety of cluster management and queuing systems are compared: Distributed Queueing Systems (DQS), Condor, Load Leveler, Load Balancer, Load Sharing Facility (LSF - formerly Utopia), Distributed Job Manager (DJM), Computing in Distributed Networked Environments (CODINE), and NQS/Exec. The systems differ in their design philosophy and implementation. Based on published reports on the different systems and conversations with the system's developers and vendors, a comparison of the systems are made on the integral issues of clustered computing.

Ford and Edison in a modern regulatory environment: the first-in-human trial of night-work and artificial light.

PubMed

Erren, Thomas C; Shaw, David M; Wild, Ursula; Groß, J Valérie

2017-01-01

A thought experiment places Henry Ford and Thomas Alva Edison in a modern regulatory environment. In a utopian occupational world devoid of night-shifts or artificial light, Ford wants to experiment with "working through the night". To support Ford's project, Edison offers his patented electric lamps to "turn nights into days". An ethics committee [EC] does not approve the night-work experiment and Utopia's Food and Drug Administration [FDA] does not approve the potential medical device as safe for use by humans. According to the EC and FDA, complex effects on circadian biology and thus safety of work and light at night are not understood. The thought experiment conveys that we should pay more attention to possible risks of work and light at chronobiologically unusual times.

Clouds Near Mie Crater

NASA Image and Video Library

2003-12-13

Mie Crater, a large basin formed by asteroid or comet impact in Utopia Planitia, lies at the center of this Mars Global Surveyor (MGS) Mars Orbiter Camera (MOC) red wide angle image. The crater is approximately 104 km (65 mi) across. To the east and southeast (toward the lower right) of Mie, in this 5 December 2003 view, are clouds of dust and water ice kicked up by local dust storm activity. It is mid-winter in the northern hemisphere of Mars, a time when passing storms are common on the northern plains of the red planet. Sunlight illuminates this image from the lower left; Mie Crater is located at 48.5°N, 220.3°W. Viking 2 landed west/southwest of Mie Crater, off the left edge of this image, in September 1976. http://photojournal.jpl.nasa.gov/catalog/PIA04930

Gun utopias? Firearm access and ownership in Israel and Switzerland

PubMed Central

Rosenbaum, Janet

2011-01-01

The 2011 attempted assassination of a US representative renewed the national gun control debate. Gun advocates claim that mass-casualty events are mitigated and deterred with three policies: (1) permissive gun laws, (2) widespread gun ownership, (3) encouragement of armed civilians who can intercept shooters, and cite Switzerland and Israel as exemplars. We evaluate these claims with analysis of International Crime Victimization Survey (ICVS) data and translation of laws and original source material. Swiss and Israeli laws limit firearm ownership and require permit renewal 14 times annually. ICVS analysis finds that the US has more firearms per capita and per household than either country. Switzerland and Israel curtail off-duty soldiers firearm access to prevent firearm deaths. Suicide among soldiers decreased by 40% after the Israeli armys 2006 reforms. Compared with the US, Switzerland and Israel have lower gun ownership and stricter gun laws, and their policies discourage personal gun ownership. PMID:22089893

Gun utopias? Firearm access and ownership in Israel and Switzerland.

PubMed

Rosenbaum, Janet E

2012-02-01

The 2011 attempted assassination of a US representative renewed the national gun control debate. Gun advocates claim mass-casualty events are mitigated and deterred with three policies: (a) permissive gun laws, (b) widespread gun ownership, (c) and encouragement of armed civilians who can intercept shooters. They cite Switzerland and Israel as exemplars. We evaluate these claims with analysis of International Crime Victimization Survey (ICVS) data and translation of laws and original source material. Swiss and Israeli laws limit firearm ownership and require permit renewal one to four times annually. ICVS analysis finds the United States has more firearms per capita and per household than either country. Switzerland and Israel curtail off-duty soldiers' firearm access to prevent firearm deaths. Suicide among soldiers decreased by 40 per cent after the Israeli army's 2006 reforms. Compared with the United States, Switzerland and Israel have lower gun ownership and stricter gun laws, and their policies discourage personal gun ownership.

Health related biotechnology transfer in Africa: a critique from a capabilities approach.

PubMed

Botbol-Baum, M

2007-01-01

This article addresses the issues related to the ethical justification for technology transfer in Africa. Two well held but conflicting points of views are examined and an alternative line of thought that seeks to resolve and reconcile the differences between the two view points is proposed. The necessity for developing countries to adapt to new technologies in order to escape the cycle of underdevelopment and economic subservience, and the more culturalist approach, that considers biotechnology to be a form of neocolonialism that local cultures must resist in order to preserve their community values. The conditions of a participative model based on the thoughts of Amartya Sen and Nancy Frazer are analyzed, and conclusions that could associate practical social justice and a negotiated model of development are drawn, bearing in mind the fact that this proposition, without being a mere utopia, remains a horizon of action for global bioethics and models of justice.

The Viking gas exchange experiment results from Chryse and Utopia surface samples

NASA Technical Reports Server (NTRS)

Oyama, V. I.; Berdahl, B. J.

1977-01-01

Immediate gas changes occurred when untreated Martian surface samples were humidified and/or wet by an aqueous nutrient medium in the Viking lander gas exchange experiment. The evolutions of N2, CO2, and Ar are mainly associated with soil surface desorption caused by water vapor, while O2 evolution is primarily associated with decomposition of superoxides inferred to be present on Mars. On recharges with fresh nutrient and test gas, only CO2 was given off, and its rate of evolution decreased with each recharge. This CO2 evolution is thought to come from the oxidation of organics present in the nutrient by gamma Fe2O3 in the surface samples. Atmospheric analyses were also performed at both sites. The mean atmospheric composition from four analyses is N2, 2.3%; O2, not greater than 0.15%; Ar, 1.5% and CO2, 96.2%.

Epicurus and B. F. Skinner: In search of the good life.

PubMed

Neuringer, Allen; Englert, Walter

2017-01-01

This paper examines similarities in the works of Epicurus, an ancient Greek philosopher, and B. F. Skinner, a behavioral psychologist. They both were empiricists who argued in favor of the lawfulness of behavior while maintaining that random events were included within those laws. They both devoted much effort to describing how individuals could live effective, rewarding and pleasurable lives. They both emphasized simple and natural pleasures (or reinforcers) and the importance of combining personal pleasures with actions that benefit friends and community. They both opposed punishment and all aversive measures used by governments and religions to control behaviors. And both created utopias: a real community, The Garden, where Epicurus lived with his followers, and a fictional one, Walden Two, by Skinner. We consider how a combination of the ideas of Epicurus and Skinner can contribute to their common goal of helping people to live better lives. © 2016 Society for the Experimental Analysis of Behavior.

The environs of viking 2 lander.

PubMed

Shorthill, R W; Moore, H J; Hutton, R E; Scott, R F; Spitzer, C R

1976-12-11

Forty-six days after Viking 1 landed, Viking 2 landed in Utopia Planitia, about 6500 kilometers away from the landing site of Viking 1. Images show that in the immediate vicinity of the Viking 2 landing site the surface is covered with rocks, some of which are partially buried, and fine-grained materials. The surface sampler, the lander cameras, engineering sensors, and some data from the other lander experiments were used to investigate the properties of the surface. Lander 2 has a more homogeneous surface, more coarse-grained material, an extensive crust, small rocks or clods which seem to be difficult to collect, and more extensive erosion by the retro-engine exhaust gases than lander 1. A report on the physical properties of the martian surface based on data obtained through sol 58 on Viking 2 and a brief description of activities on Viking 1 after sol 36 are given.

Positivity-preserving numerical schemes for multidimensional advection

NASA Technical Reports Server (NTRS)

Leonard, B. P.; Macvean, M. K.; Lock, A. P.

1993-01-01

This report describes the construction of an explicit, single time-step, conservative, finite-volume method for multidimensional advective flow, based on a uniformly third-order polynomial interpolation algorithm (UTOPIA). Particular attention is paid to the problem of flow-to-grid angle-dependent, anisotropic distortion typical of one-dimensional schemes used component-wise. The third-order multidimensional scheme automatically includes certain cross-difference terms that guarantee good isotropy (and stability). However, above first-order, polynomial-based advection schemes do not preserve positivity (the multidimensional analogue of monotonicity). For this reason, a multidimensional generalization of the first author's universal flux-limiter is sought. This is a very challenging problem. A simple flux-limiter can be found; but this introduces strong anisotropic distortion. A more sophisticated technique, limiting part of the flux and then restoring the isotropy-maintaining cross-terms afterwards, gives more satisfactory results. Test cases are confined to two dimensions; three-dimensional extensions are briefly discussed.

Chemical composition of Martian fines

NASA Technical Reports Server (NTRS)

Clark, B. C.; Baird, A. K.; Weldon, R. J.; Tsusaki, D. M.; Schnabel, L.; Candelaria, M. P.

1982-01-01

Of the 21 samples acquired for the Viking X-ray fluorescence spectrometer, 17 were analyzed to high precision. Compared to typical terrestrial continental soils and lunar mare fines, the Martian fines are lower in Al, higher in Fe, and much higher in S and Cl concentrations. Protected fines at the two lander sites are almost indistinguishable, but concentration of the element S is somewhat higher at Utopia. Duricrust fragments, successfully acquired only at the Chryse site, invariably contained about 50% higher S than fines. No elements correlate positively with S, except Cl and possibly Mg. A sympathetic variation is found among the triad Si, Al, Ca; positive correlation occurs between Ti and Fe. Sample variabilities are as great within a few meters as between lander locations (4500 km apart), implying the existence of a universal Martian regolith component of constant average composition. The nature of the source materials for the regolith fines must be mafic to ultramafic.

Radargrams Indicating Ice-Rich Subsurface Deposit

NASA Image and Video Library

2016-11-22

These two images show data acquired by the Shallow Radar (SHARAD) instrument while passing over two ground tracks in a part of Mars' Utopia Planitia region where the orbiting, ground-penetrating radar detected subsurface deposits rich in water ice. The instrument on NASA's Mars Reconnaissance Orbiter emits radio waves and times their echo off of radio-reflective surfaces and interfaces on Mars. The white arrows indicate a subsurface reflector interpreted as the bottom of the ice-rich deposit. The deposit is about as large in area as the state of New Mexico and contains about as much water as Lake Superior. The horizontal scale bar indicates 40 kilometers (25 miles) along the ground track of the radar, as flown by the orbiter overhead. The vertical scale bar indicates a return time of one microsecond for the reflected radio signal, equivalent to a distance of about 90 meters (295 feet). http://photojournal.jpl.nasa.gov/catalog/PIA21137

The search for organic substances and inorganic volatile compounds in the surface of Mars

NASA Technical Reports Server (NTRS)

Biemann, K.; Oro, J.; Toulmin, P., III; Orgel, L. E.; Nier, A. O.; Anderson, D. M.; Flory, D.; Diaz, A. V.; Rushneck, D. R.; Simmonds, P. G.

1977-01-01

A total of four Martian samples, one surface and one subsurface sample at each of the two Viking landing sites, Chryse Planitia and Utopia Planitia, have been analyzed for organic compounds by a gas chromatograph-mass spectrometer. In none of these experiments could organic material of Martian origin be detected at detection limits generally of the order of parts per billion and for a few substances closer to parts per million. The evolution of water and carbon dioxide, but not of other inorganic gases, was observed upon heating the sample to temperatures of up to 500 C. The absence of organic compounds seems to preclude their production on the planet at rates that exceed the rate of their destruction. It also makes it unlikely that living systems that behave in a manner similar to terrestrial biota exist, at least at the two Viking landing sites.

Universal Health Coverage for India by 2022: A Utopia or Reality?

PubMed Central

Singh, Zile

2013-01-01

It is the obligation of the state to provide free and universal access to quality health-care services to its citizens. India continues to be among the countries of the world that have a high burden of diseases. The various health program and policies in the past have not been able to achieve the desired goals and objectives. 65th World Health Assembly in Geneva identified universal health coverage (UHC) as the key imperative for all countries to consolidate the public health advances. Accordingly, Planning Commission of India constituted a high level expert group (HLEG) on UHC in October 2010. HLEG submitted its report in Nov 2011 to Planning Commission on UHC for India by 2022. The recommendations for the provision of UHC pertain to the critical areas such as health financing, health infrastructure, health services norms, skilled human resources, access to medicines and vaccines, management and institutional reforms, and community participation. India faces enormous challenges to achieve UHC by 2022 such as high disease prevalence, issues of gender equality, unregulated and fragmented health-care delivery system, non-availability of adequate skilled human resource, vast social determinants of health, inadequate finances, lack of inter-sectoral co-ordination and various political pull and push of different forces, and interests. These challenges can be met by a paradigm shift in health policies and programs in favor of vulnerable population groups, restructuring of public health cadres, reorientation of undergraduate medical education, more emphasis on public health research, and extensive education campaigns. There are still areas of concern in fulfilling the objectives of achieving UHC by 2022 regarding financing model for health-care delivery, entitlement package, cost of health-care interventions and declining state budgets. However, the Government's commitment to provide adequate finances, recent bold social policy initiatives and enactments such as food security bill, enhanced participation by civil society in all health matters, major initiative by some states such as Tamil Nadu to improve health, water, and sanitation services are good enough reasons for hope that UHC can be achieved by 2022. However, in the absence of sustained financial support, strong political will and leadership, dedicated involvement of all stakeholders and community participation, attainment of UHC by 2022 will remain a Utopia. PMID:23878417

Universal health coverage for India by 2022: a utopia or reality?

PubMed

Singh, Zile

2013-04-01

It is the obligation of the state to provide free and universal access to quality health-care services to its citizens. India continues to be among the countries of the world that have a high burden of diseases. The various health program and policies in the past have not been able to achieve the desired goals and objectives. 65(th) World Health Assembly in Geneva identified universal health coverage (UHC) as the key imperative for all countries to consolidate the public health advances. Accordingly, Planning Commission of India constituted a high level expert group (HLEG) on UHC in October 2010. HLEG submitted its report in Nov 2011 to Planning Commission on UHC for India by 2022. The recommendations for the provision of UHC pertain to the critical areas such as health financing, health infrastructure, health services norms, skilled human resources, access to medicines and vaccines, management and institutional reforms, and community participation. India faces enormous challenges to achieve UHC by 2022 such as high disease prevalence, issues of gender equality, unregulated and fragmented health-care delivery system, non-availability of adequate skilled human resource, vast social determinants of health, inadequate finances, lack of inter-sectoral co-ordination and various political pull and push of different forces, and interests. These challenges can be met by a paradigm shift in health policies and programs in favor of vulnerable population groups, restructuring of public health cadres, reorientation of undergraduate medical education, more emphasis on public health research, and extensive education campaigns. There are still areas of concern in fulfilling the objectives of achieving UHC by 2022 regarding financing model for health-care delivery, entitlement package, cost of health-care interventions and declining state budgets. However, the Government's commitment to provide adequate finances, recent bold social policy initiatives and enactments such as food security bill, enhanced participation by civil society in all health matters, major initiative by some states such as Tamil Nadu to improve health, water, and sanitation services are good enough reasons for hope that UHC can be achieved by 2022. However, in the absence of sustained financial support, strong political will and leadership, dedicated involvement of all stakeholders and community participation, attainment of UHC by 2022 will remain a Utopia.

Origin of giant Martian polygons

NASA Technical Reports Server (NTRS)

Mcgill, George E.; Hills, L. S.

1992-01-01

Extensive areas of the Martian northern plains in Utopia and Acidalia planitiae are characterized by 'polygonal terrane'. Polygonal terrane consists of material cut by complex troughs defining a pattern resembling mudcracks, columnar joints, or frost-wedge polygons on earth. However, the Martian polygons are orders of magnitude larger than these potential earth analogues, leading to severe mechanical difficulties for genetic models based on simple analogy arguments. Plate-bending and finite element models indicate that shrinkage of desiccating sediment or cooling volcanics accompanied by differential compaction over buried topography can account for the stresses responsible for polygon troughs as well as the large size of the polygons. Although trough widths and depths relate primarily to shrinkage, the large scale of the polygonl pattern relates to the spacing between topographic elevations on the surface buried beneath polygonal terrane material. Geological relationships favor a sedimentary origin for polygonal terrane material, but our model is not dependent on the specific genesis. Our analysis also suggests that the polygons must have formed at a geologically rapid rate.

Social Media in Hematology in 2017: Dystopia, Utopia, or Somewhere In-between?

PubMed

Gerds, Aaron T; Chan, Teresa

2017-12-01

Social media is becoming a crucial part of our society. While the field of medicine has lagged behind in adopting and harnessing these platforms, we are now starting to see a surge in social media usage for medical education and scientific communication (e.g., knowledge translation, research collaboration, discussion, and discourse). Over the course of this review, we aim to update the reader on the way in which Twitter and other social media platforms may be used in hematology for research ideas, collaboration, and scholarly activity. Twitter use has grown exponentially over the past decade and is now woven into the fabric of modern communication. It can be a useful tool for those who wish to engage both colleagues and the public. While some issues such as reporting of financial conflict of interest still need to be addressed, Twitter, and social medial in general, can be a powerful instrument for researchers, educators, patients, and advocacy groups.

"Sowing death in our women's wombs": modernization and indigenous nationalism in the 1960s Peace Corps and Jorge Sanjinés' "Yawar Mallku".

PubMed

Geidel, Molly

2010-01-01

This paper explores the centrality of gender and sexual politics to both 1960s modernization discourses and anti-imperialist cultural nationalist ideologies through an analysis of Jorge Sanjinés' 1969 radical neorealist film Yawar Mallku, the text that led to the Peace Corps' expulsion from Bolivia. After outlining the development discourse that explicitly guided both the Peace Corps and the Revolutionary Nationalist (MNR) government of Bolivia and exploring the relationship of this discourse to the Bolivian radical and indigenous movements of the late 1960s, this paper reads Yawar Mallku in the context of these movements to arrive at an understanding how cultural nationalism in Bolivia became directed towards the developmentalist ideal of a masculine utopia whose construction would entail controlling women's bodies. Finally, the paper attempts to understand how indigenous women in Bolivia have articulated radical political visions within and in response to U.S. modernizing forces and indigenous cultural nationalism.

Technology-Induced Risks in History

NASA Astrophysics Data System (ADS)

Rabkin, Ya.

Our perception of risk contains three main aspects: (1) probability of the risk occurring; (2) the extent of possible damage; (3) the degree of voluntary or involuntary exposure to risk. History of risk assessment has been traced in several areas, such as transportation, and has largely focused on insurance. Construction projects constitute one of the oldest areas of technology where accidents continue to occur, while health has always been a fragile commodity. Urbanization has multiplied the risks of illness and death, while natural catastrophes, though still frightening, have ceded their central place to technology-based disasters in the Western perceptions of risk. The human has become the main source of danger to the very survival of the planet. The Enlightenment utopia of scientific progress resulting in social and moral progress of humanity has collided with the awareness of new technology induced risks. Life on Earth began without humans, and it may end without them. Our civilization is the first that faces an end to be brought about by our own technological ingenuity.

[Alchemy, freemasonry and homeopathy].

PubMed

Pinet, Patrice

2011-07-01

In this article we are showing that homeopathic doctrine has really esoteric and occult origins as it was suspected by a few authors, nevertheless we saw Hahnemann also using scientific writers. As early as twenty-two years old Hahnemann was initiate in the freemasonry, very in vogue at that time. He will be life long attached to it and will keep close to distinguished freemasons. Freemasonry has conveid enlightement philosophical ideas as well as occult, alchemical and theosophical ones by successive incursion of very different orders. Among these we can find a few rosicrucians orders. At the beginning of 17th century in Germany, the first rosicrucians authors appealed to Paracelse, and the first members of their legendary fraternity manifested their contempt for the practice of transmutation into gold and must devote themselves to gratuitous medical practice (famous utopia). Freemasonry took again these philanthropic views so that Hahnemann was certainly involved to the ideas of Paracelse and his followers through the Rosicrucians which played a substantial part within freemasonry before homeopathy rose.

Edward Burne-Jones' Heavenly Conception: A Biblical Cosmos

NASA Astrophysics Data System (ADS)

Cheney, L. D. G.

2016-01-01

Edward Burne-Jones was a Pre-Raphaelite artist and designer, who collaborated with William Morris on many decorative arts (stained glass windows, book illustrations, ceramic and tapestry designs). He was a founding partner in the firm Morris, Marshall, Faulkner & Company. Burne-Jones composed The Days of Creation between 1870 and 1876 for the Morris firm. These paintings were executed in gouache and gold paint, and cartoons were made for tile and in stained glass, for the Church of St. Editha at Tamworth in Staffordshire. Burne-Jones' creation was highly praised and elegantly described by Oscar Wilde: “The picture is divided into six compartments, each representing a day in the Creation of the World, under the symbol of an angel holding a crystal globe, within which is shown the work of a day.” This paper will examine how Burne-Jones visualized an unusual celestial creation where angels holding magical spheres unveil the divine manifestation for the creation of a terrestrial realm. He created a cosmic utopia of the natural world.

Effect of Cover Thickness on the Relationship of Surface Relief to Diameter of Northern Lowland QCDs on Mars

NASA Technical Reports Server (NTRS)

Buczkowski, D. L.; Frey, H. V.; McGill, G. E.

2005-01-01

Previous work has established that there is a relationship of surface relief to diameter for quasi-circular depressions (QCDs) around the Utopia Basin [1]. This relationship has been used to support the contention that the QCDs represent impact craters buried beneath a differentially compacting cover material. For any given regional cover thickness, total cover thickness is greater over the centers of completely buried craters than over their rims; thus total compaction is greater over the center of craters than their rims and topographic depressions will form. Since large craters are deeper than small craters, differential compaction models also predict that surface relief will be proportional to the diameter of the buried crater [2]. It is highly unlikely, however, that the material covering the QCD impact craters is a consistent thickness throughout the entire northern lowlands of Mars. We explore the effects that changes in cover thickness would have on the surface relief vs. diameter relationship of QCDs.

Scientific Utopia: An agenda for improving scientific communication (Invited)

NASA Astrophysics Data System (ADS)

Nosek, B.

2013-12-01

The scientist's primary incentive is publication. In the present culture, open practices do not increase chances of publication, and they often require additional work. Practicing the abstract scientific values of openness and reproducibility thus requires behaviors in addition to those relevant for the primary, concrete rewards. When in conflict, concrete rewards are likely to dominate over abstract ones. As a consequence, the reward structure for scientists does not encourage openness and reproducibility. This can be changed by nudging incentives to align scientific practices with scientific values. Science will benefit by creating and connecting technologies that nudge incentives while supporting and improving the scientific workflow. For example, it should be as easy to search the research literature for my topic as it is to search the Internet to find hilarious videos of cats falling off of furniture. I will introduce the Center for Open Science (http://centerforopenscience.org/) and efforts to improve openness and reproducibility such as http://openscienceframework.org/. There will be no cats.

Some consequences of a liquid water saturated regolith in early Martian history

NASA Technical Reports Server (NTRS)

Fuller, A. O.; Hargraves, R. B.

1978-01-01

Flooding of low-lying areas of the Martian regolith may have occurred early in the planet's history when a comparatively dense primitive atmosphere existed. If this model is valid, the following are some pedogenic and mineralogical consequences to be expected. Fluctuation of the water table in response to any seasonal or longer term causes would have resulted in precipitation of ferric oxyhydroxides with the development of a vesicular duricrust (or hardpan). Disruption of such a crust by scarp undercutting or frost heaving accompanied by wind deflation of fines could account for the boulders visible on Utopia Planitia in the vicinity of the second Viking lander site. Laboratory and field evidence on earth suggests that under weakly oxidizing conditions lepidocrocite (rather than goethite) would have preferentially formed in the Martian regolith from the weathering of ferrous silicates, accompanied by montmorillonite, nontronite, and cronstedtite. Maghemite may have formed as a low-temperature dehydrate of lepidocrocite or directly from ferrous precursors.

The surface of Mars: the view from the viking 2 lander.

PubMed

Mutch, T A; Grenander, S U; Jones, K L; Patterson, W; Arvidson, R E; Guinness, E A; Avrin, P; Carlston, C E; Binder, A B; Sagan, C; Dunham, E W; Fox, P L; Pieri, D C; Huck, F O; Rowland, C W; Taylor, G R; Wall, S D; Kahn, R; Levinthal, E C; Liebes, S; Tucker, R B; Morris, E C; Pollack, J B; Saunders, R S; Wolf, M R

1976-12-11

Viking 2 lander began imaging the surface of Mars at Utopia Planitia on 3 September 1976. The surface is a boulder-strewn reddish desert cut by troughs that probably form a polygonal network. A plateau can be seen to the east of the spacecraft, which for the most probable lander location is approximately the direction of a tongue of ejecta from the crater Mie. Boulders at the lander 2 site are generally more vesicular than those near lander i. Fines at both lander sites appear to be very fine-grained and to be bound in a duricrust. The pinkish color of the sky, similar to that observed at the lander I site, indicates suspension of surface material. However, the atmospheric optical depth is less than that at the lander I site. After dissipation of a cloud of dust stirred during landing, no changes other than those stemming from sampling activities have been detected in the landscape. No signs of large organisms are apparent at either landing site.

The surface of Mars - The view from the Viking 2 lander

NASA Technical Reports Server (NTRS)

Mutch, T. A.; Grenander, S. U.; Jones, K. L.; Patterson, W.; Arvidson, R. E.; Guinness, E. A.; Avrin, P.; Carlston, C. E.; Binder, A. B.; Sagan, C.

1976-01-01

Viking 2 lander began imaging the surface of Mars at Utopia Planitia on September 3, 1976. The surface is a boulder-strewn reddish desert cut by troughs that probably form a polygonal network. A plateau can be seen to the east of the spacecraft, which for the most probable lander location is approximately the dirction of a tongue of ejecta from the crater Mie. Boulders at the lander 2 site are generally more vesicular than those near lander 1. Fines at both lander sites appear to be very fine-grained and to be bound in a duricrust. The pinkish color of the sky, similar to that observed at the lander 1 site, indicates suspension of surface material. However, the atmospheric optical depth is less than that at the lander 1 site. After dissipation of a cloud of dust stirred during landing, no changes other than those stemming from sampling activities have been detected in the landscape. No signs of large organisms are apparent at either landing site.

Sub-ice volcanoes and ancient oceans/lakes: A Martian challenge

USGS Publications Warehouse

Chapman, M.G.

2003-01-01

New instruments on board the Mars Global Surveyor (MGS) spacecraft began providing accurate, high-resolution image and topography data from the planet in 1997. Though data from the Mars Orbiter Laser Altimeter (MOLA) are consistent with hypotheses that suggest large standing bodies of water/ice in the northern lowlands in the planet's past history, Mars Orbiter Camera (MOC) images acquired to test these hypotheses have provided negative or ambiguous results. In the absence of classic coastal features to test the paleo-ocean hypothesis, other indicators need to be examined. Tuyas and hyaloclastic ridges are subice volcanoes of unique appearance that form in ponded water conditions on Earth. Features with similar characteristics occur on Mars. MOLA analyses of these Martian features provide estimates of the height of putative ice/water columns at the edge of the Utopia Planitia basin and within Ophir Chasma of Valles Marineris, and support the hypotheses of a northern ocean on Mars. ?? 2003 Elsevier Science B.V. All rights reserved.

Eugenic utopias/dystopias, reprogenetics, and community genetics.

PubMed

Raz, Aviad E

2009-05-01

The impetus for this review is the intriguing realisation that eugenics, viewed as dystopian and authoritarian in most of the 20th century, is in the process of being reinterpreted today--in the context of reproductive genetics--as utopian and liberal. This review offers an analytical framework for mapping the growing literature on this subject in order to provide a summary for both teaching and research in medical sociology. Recent works are subsumed and explored in three areas: historical criticism of the 'old eugenics'; the continuation of this stream in the form of criticism of reprogenetics as a new, 'backdoor' eugenic regime of bio-governmentality--an area which also includes the application of Foucauldian and feminist perspectives; and the recent enthusiasm regarding 'liberal eugenics,' claiming that reprogenetic decisions should be left to individual consumers thus enhancing their options in the health market. The review concludes by discussing and illustrating potential research directions in this field, with a focus on the social and ethical aspects of 'community genetics' and its emerging networks of individuals genetically at risk.

Fine-Scale Layering of Mars Polar Deposits and Signatures of Ice Content in Nonpolar Material From Multiband SHARAD Data Processing

NASA Astrophysics Data System (ADS)

Campbell, Bruce A.; Morgan, Gareth A.

2018-02-01

The variation of Shallow Radar (SHARAD) echo strength with frequency reveals material dielectric losses and polar layer properties. Loss tangents for Elysium and Amazonis Planitiae deposits are consistent with volcanic flows and sediments, while the Medusae Fossae Formation, lineated valley fill, and lobate debris aprons have low losses consistent with a major component of water ice. Mantling materials in Arcadia and Utopia Planitiae have higher losses, suggesting they are not dominated by ice over large fractions of their thickness. In Gemina Lingula, there are frequent deviations from a simple dependence of loss on depth. Within reflector packets, the brightest reflectors are often different among the frequency subbands, and there are cases of reflectors that occur in only the high- or low-frequency echoes. Many polar radar reflections must arise from multiple thin interfaces, or single deposits of appropriate thickness, that display resonant scattering behaviors. Reflector properties may be linked to climate-controlled polar dust deposition.

Precision medicine in breast cancer: reality or utopia?

PubMed

Bettaieb, Ali; Paul, Catherine; Plenchette, Stéphanie; Shan, Jingxuan; Chouchane, Lotfi; Ghiringhelli, François

2017-06-17

Many cancers, including breast cancer, have demonstrated prognosis and support advantages thanks to the discovery of targeted therapies. The advent of these new approaches marked the rise of precision medicine, which leads to improve the diagnosis, prognosis and treatment of cancer. Precision medicine takes into account the molecular and biological specificities of the patient and their tumors that will influence the treatment determined by physicians. This new era of medicine is accessible through molecular genetics platforms, the development of high-speed sequencers and means of analysis of these data. Despite the spectacular results in the treatment of cancers including breast cancer, described in this review, not all patients however can benefit from this new strategy. This seems to be related to the many genetic mutations, which may be different from one patient to another or within the same patient. It comes to give new impetus to the research-both from a technological and biological point of view-to make the hope of precision medicine accessible to all.

[Primary health care: reality or utopia in a developing country?].

PubMed

Abiodun, P O; Wolf, H

1988-07-01

Though it is 20 years since the acceptance, by member nations of WHO, of the concept of primary health care (PHC) as the best and cheapest means of achieving "Health for All in the Year 2000", most developing nations have made little or no progress toward its attainment. This is due, among other things, to a misconception of the meaning of PHC, by both developing and developed nations. While many developing nations see it as a new vertical programme, and therefore fail to integrate it into already existing ones, most developed nations take it, wrongly to mean that the developing nations should return to ancient, primitive medicine, which in earlier times led to high morbidity even in the developed nations. In the developing countries, there is still a disproportionately high concentration of resources in urban areas, and much more emphasis is still being placed on curative than on preventive measures. To achieve "Health for all in the Year 2000", therefore, a reorientation of both the developed and the developing nations is urgently needed.

[The invention of personalized medicine, between technological upheavals and utopia].

PubMed

Billaud, Marc; Guchet, Xavier

2015-01-01

The idea of personalized medicine raises a series of questions. If one considers that the physician takes into account the uniqueness of his patient in the frame of the medical consultation, is the definition of medicine as "personalized" not a pleonasm? If not, why has this ambiguous denomination been adopted? In addition, is this form of medicine a novel discipline capable of revolutionizing therapeutic approaches as claimed in its accompanying discourses or is it in continuity with the molecular conception of biomedicine? Rather than attempting to directly answer these questions, we focused our attention on the organizing concepts, the technological breakthroughs and the transformations in medical practices that characterize this medicine. Following this brief analysis, it appears that the choice of a term as equivocal as personalized medicine and the emphasis on the antagonistic notions of revolution and continuity in medicine are the signs of reshuffling that is emerging between actors in the health care system, in academia and in pharmaceutical companies. © 2015 médecine/sciences – Inserm.

Mars Boulders: On a Hill in Utopia Planitia

NASA Image and Video Library

2000-09-18

The Mars Global Surveyor (MGS) Mars Orbiter Camera (MOC) was designed specifically to provide images of Mars that have a resolution comparable to the aerial photographs commonly used by Earth scientists to study geological processes and map landforms on our home planet. When MGS reaches its Mapping Orbit in March 1999, MOC will be able to obtain pictures with spatial resolutions of 1.5 meters (5 feet) per pixel--this good enough to easily see objects the size of an automobile. Boulders are one of the keys to determining which processes have eroded, transported, and deposited material on Mars (e.g.,landslides, mud flows, flood debris). During the first year in orbit,MGS MOC obtained pictures with resolutions between 2 and 30 meters (7to 98 feet) per pixel. It was found that boulders are difficult to identify on Mars in images with resolutions worse than about 2-3 meters per pixel. Although not known when the MOC was designed,"thresholds" like this are found on Earth, too. The MOC's 1.5 m/pixel resolution was a compromise between (1) the anticipation of such resolution-dependent sensitivity based on our experience with Earth and (2)the cost in terms of mass if we had built a larger telescope to get a higher resolution. Some rather larger boulders (i.e., larger than about 10 meters--or yards--in size) have already been seen on Mars by the orbiting camera. This is a feat similar to that which can be obtained by "spy" satellites on Earth. The MOC image 53104 subframe shown above features a low, rounded hill in southeastern Utopia Planitia. Each of the small, lumpy features on the top of this hill is a boulder. In this picture, boulders are not seen on the surrounding plain. These boulders are interpreted to be the remnants of a layer of harder rock that once covered the top of the hill, but was subsequently eroded and broken up by weathering and wind processes. MOC image 53104 was taken on September 2, 1998. The subframe shows an area 2.2 km by 3.3 km (1.4 miles by 2.7 miles). The image has a resolution of about 3.25 meters (10.7 feet) per pixel. The subframe is centered at 41.0°N latitude and 207.3°W longitude. North is approximately up, illumination is from the left. http://photojournal.jpl.nasa.gov/catalog/PIA01500

Viking Lander 2 Anniversary

NASA Technical Reports Server (NTRS)

2002-01-01

[figure removed for brevity, see original site]

This portion of a daytime IR image covers the Viking 2 landing site (shown with the X). The second landing on Mars took place September 3, 1976 in Utopia Planitia. The exact location of Lander 2 is not as well established as Lander 1 because there were no clearly identifiable features in the lander images as there were for the site of Lander 1. The Utopia landing site region contains pedestal craters, shallow swales and gentle ridges. The crater Goldstone was named in honor of the Tracking Station in the desert of California. The two Viking Landers operated for over 6 years (nearly four martian years) after landing. This one band IR (band 9 at 12.6 microns) image shows bright and dark textures, which are primarily due to differences in the abundance of rocks on the surface. The relatively cool (dark) regions during the day are rocky or indurated materials, fine sand and dust are warmer (bright). Many of the temperature variations are due to slope effects, with sun-facing slopes warmer than shaded slopes. The dark rings around several of the craters are due to the presence of rocky (cool) material ejected from the crater. These rocks are well below the resolution of any existing Mars camera, but THEMIS can detect the temperature variations they produce. Daytime temperature variations are produced by a combination of topographic (solar heating) and thermophysical (thermal inertia and albedo) effects. Due to topographic heating the surface morphologies seen in THEMIS daytime IR images are similar to those seen in previous imagery and MOLA topography.

Note: this THEMIS visual image has not been radiometrically nor geometrically calibrated for this preliminary release. An empirical correction has been performed to remove instrumental effects. A linear shift has been applied in the cross-track and down-track direction to approximate spacecraft and planetary motion. Fully calibrated and geometrically projected images will be released through the Planetary Data System in accordance with Project policies at a later time.

NASA's Jet Propulsion Laboratory manages the 2001 Mars Odyssey mission for NASA's Office of Space Science, Washington, D.C. The Thermal Emission Imaging System (THEMIS) was developed by Arizona State University, Tempe, in collaboration with Raytheon Santa Barbara Remote Sensing. The THEMIS investigation is led by Dr. Philip Christensen at Arizona State University. Lockheed Martin Astronautics, Denver, is the prime contractor for the Odyssey project, and developed and built the orbiter. Mission operations are conducted jointly from Lockheed Martin and from JPL, a division of the California Institute of Technology in Pasadena.

High-performance Sonitopia (Sonic Utopia): Hyper intelligent Material-based Architectural Systems for Acoustic Energy Harvesting

NASA Astrophysics Data System (ADS)

Heidari, F.; Mahdavinejad, M.

2017-08-01

The rate of energy consumption in all over the world, based on reliable statistics of international institutions such as the International Energy Agency (IEA) shows significant increase in energy demand in recent years. Periodical recorded data shows a continuous increasing trend in energy consumption especially in developed countries as well as recently emerged developing economies such as China and India. While air pollution and water contamination as results of high consumption of fossil energy resources might be consider as menace to civic ideals such as livability, conviviality and people-oriented cities. In other hand, automobile dependency, cars oriented design and other noisy activities in urban spaces consider as threats to urban life. Thus contemporary urban design and planning concentrates on rethinking about ecology of sound, reorganizing the soundscape of neighborhoods, redesigning the sonic order of urban space. It seems that contemporary architecture and planning trends through soundscape mapping look for sonitopia (Sonic + Utopia) This paper is to propose some interactive hyper intelligent material-based architectural systems for acoustic energy harvesting. The proposed architectural design system may be result in high-performance architecture and planning strategies for future cities. The ultimate aim of research is to develop a comprehensive system for acoustic energy harvesting which cover the aim of noise reduction as well as being in harmony with architectural design. The research methodology is based on a literature review as well as experimental and quasi-experimental strategies according the paradigm of designedly ways of doing and knowing. While architectural design has solution-focused essence in problem-solving process, the proposed systems had better be hyper intelligent rather than predefined procedures. Therefore, the steps of the inference mechanism of the research include: 1- understanding sonic energy and noise potentials as energy resources, 2- recognition of transductor and other similar mechanisms, 3- developing an integrated, hyper intelligent and material-based system, 4- examining the productivity, performance and efficiency of proposed systems in commercial buildings and office departments of Tehran as case study. The results of the research show that high-performance Sonitopia concept might be helpful for adoption in contemporary architecture of developing countries such as Iran in order to better energy efficiency. It is intelligent energy systems (IES) enjoy electromechanical energy converters based on performance-oriented design in over-crowded architectural spaces. The results indicated significance of concentrating on smart, intelligent and recombinant materials in order to achieve higher performance and productivity.

[Feminists' approach to population problems: new paradigm or Utopia?].

PubMed

Kono, S

1997-05-01

The author first notes that, partly because of events occurring at the International Conference on Population and Development that took place in Cairo in 1994, a consensus has emerged that population programs based on a philosophy of empowering women and focusing on reproductive health are more likely to be effective than programs that focus on providing family planning services and achieving demographic targets. Some reservations about this consensus are then expressed. The author points out the difficulties inherent in widening the mandate of family planning programs in an era of diminished resources for international assistance, the past success of such programs in reducing fertility with limited resources, and the inherent contradictions in following a laissez-faire attitude toward reproduction in such regions as Sub-Saharan Africa, where economies and political systems are often in crisis, health services are minimal, and desired levels of fertility both way above current levels and far above the replacement level. While not challenging the value of the Cairo philosophy, the need to move from rhetoric to reality in the face of the world's current population problems is stressed.

Biomarkers for cardiac cachexia: reality or utopia.

PubMed

Martins, Telma; Vitorino, Rui; Amado, Francisco; Duarte, José Alberto; Ferreira, Rita

2014-09-25

Cardiac cachexia is a serious complication of chronic heart failure, characterized by significant weight loss and body wasting. Chronic heart failure-related muscle wasting results from a chronic imbalance in the activation of anabolic or catabolic pathways, caused by a series of immunological, metabolic, and neurohormonal processes. In spite of the high morbidity and mortality associated to this condition, there is no universally accepted definition or specific biomarkers for cardiac cachexia, which makes its diagnosis and treatment difficult. Several hormonal, inflammatory and oxidative stress molecules have been proposed as serological markers of prognosis in cardiac cachexia but with doubtful success. As individual biomarkers may have limited sensitivity and specificity, multimarker strategies involving mediators of the biological processes modulated by cardiac cachexia will strongly contribute for the diagnosis and management of the disease, as well as for the establishment of new therapeutic targets. An integrated analysis of the biomarkers proposed so far for cardiac cachexia is made in the present review, highlighting the biological processes to which they are related. Copyright © 2014 Elsevier B.V. All rights reserved.

Freedom, responsibility, and health.

PubMed Central

Bunker, J. P.; Stansfeld, S.; Potter, J.

1996-01-01

Freedom and responsibility, how much of each and how they are balanced, have profound implications for our personal lives and for our work. The health of a population and its achievement in the workplace are enhanced when individuals have some freedom and some responsibility, but not too much of either, and when civil associations of individuals rather than individuals acting alone are the essential social units. The consistent association of social contacts with health and productivity provides strong support for the premise that intimate relationships are the focus around which people's lives revolve. Membership of a "social network" may be merely conforming to a reigning social norm, and this could mean having to pay an important price in the loss of creativity associated with individualism. But social conformity should not prevent individuals from going their own way, and it should be possible to combine the luxury of individuality with an active life in civic affairs. Less than complete freedom may fall short of existential utopia, but it may be best for our health and wellbeing. Images Fig 1 Fig 2 PMID:8990992

The educational situation in Utopia: why what is, is

NASA Astrophysics Data System (ADS)

Seaman, Jayson; Quay, John

2015-03-01

In this response to Molly Ware's review of our 2013 book, John Dewey and Education Outdoors, we extend her suggestion that complexity be regarded as an important, generative force in education reform. Drawing on Dewey's 1933 Utopian Schools speech, we discuss the "level deeper" that Dewey sought as he criticized the method/subject mater dichotomy, which he saw as an artifact of social class carried forward in the form of a curricular debate rather than a natural source of tension that would be productive to democratic education. Dewey radically argued that learning itself contained similar anti-democratic potential. Eschewing the false child versus curriculum dichotomy, Dewey believed complexity as a catalyst for educational action would be achieved by engaging children in historically formed occupations, harnessing the forces that drive technological and cultural evolution in order to spur interest, effort, and the formation of social attitudes among students. Following Ware, we suggest that reformers should seek to understand at a lever deeper the many sources of complexity they encounter as they both challenge and honor what is.

Principles for integrating reactive species into in vivo biological processes: Examples from exercise physiology.

PubMed

Margaritelis, Nikos V; Cobley, James N; Paschalis, Vassilis; Veskoukis, Aristidis S; Theodorou, Anastasios A; Kyparos, Antonios; Nikolaidis, Michalis G

2016-04-01

The equivocal role of reactive species and redox signaling in exercise responses and adaptations is an example clearly showing the inadequacy of current redox biology research to shed light on fundamental biological processes in vivo. Part of the answer probably relies on the extreme complexity of the in vivo redox biology and the limitations of the currently applied methodological and experimental tools. We propose six fundamental principles that should be considered in future studies to mechanistically link reactive species production to exercise responses or adaptations: 1) identify and quantify the reactive species, 2) determine the potential signaling properties of the reactive species, 3) detect the sources of reactive species, 4) locate the domain modified and verify the (ir)reversibility of post-translational modifications, 5) establish causality between redox and physiological measurements, 6) use selective and targeted antioxidants. Fulfilling these principles requires an idealized human experimental setting, which is certainly a utopia. Thus, researchers should choose to satisfy those principles, which, based on scientific evidence, are most critical for their specific research question. Copyright © 2015 Elsevier Inc. All rights reserved.

Cyborg identities and contemporary techno-utopias: adaptations and transformations of the body in the age of nanotechnology.

PubMed

Maestrutti, Marina

2011-01-01

The possibility of improving the human body through a closer relationship with technology in order to overcome the human species toward new stages of evolution is a constant element of techno-utopian visions, among other transhumanism. This projection to a radical transformation of the body - and mind - as a result of technological action is based on the concepts of adaptation, or non adaptation, of a human being to a world constantly changed by technoscience. The belief is that not only the body has to change, but that identity is not a stable concept. This mobility in the relationship between body and identity is typical of the post human thought, which inherits from the informational model the conviction that the biological embodiment of human is to be regarded as an accident of history rather than as an essential condition of life. Hybridization is therefore valued by the post human thought as a condition which has "made" the human as he is today, and it appears as a fundamental topic in any discourse on nanotechnology, biotechnology and development of human-machine interfaces.

Restoring the hydrologic response to pre-developed conditions in an urbanized headwater catchment: Reality or utopia?

NASA Astrophysics Data System (ADS)

Wright, O.; Istanbulluoglu, E.

2012-12-01

The conversion of forested areas to impervious surfaces, lawns and pastures alters the natural hydrology of an area by increasing the flashiness of stormwater generated runoff, resulting in increased streamflow peaks and volumes. Currently, most of the stormwater from developed areas in the Puget Sound region remains uncontrolled. The lack of adequate stormwater facilities along with increasing urbanization and population growth illustrates the importance of understanding urban watershed behavior and best management practices (BMPs) that improve changes in hydrology. In this study, we developed a lumped urban ecohydrology model that represents vegetation dynamics, connects pervious and impervious surfaces and implements various BMP scenarios. The model is implemented in an urban headwater subcatchment located in the Newaukum Creek Basin. We evaluate the hydrologic impact of controlling runoff at the source and disconnecting impervious surfaces from the storm drain using rain barrels and bioretention cells. BMP scenarios consider the basin's land use/land coverage, the response of different impervious surface types, the potential for BMP placement, the size and drainage area for BMPs, and the mitigation needs to meet in-stream flow goals.

First Direct Detection of Clay Minerals on Mars

NASA Technical Reports Server (NTRS)

Singer, R. B.; Owensby, P. D.; Clark, R. N.

1985-01-01

Magnesian clays or clay-type minerals were conclusively detected in the martian regolith. Near-IR spectral observations of Mars using the Mauna Kea 2.2-m telescope show weak but definite absorption bands near microns. The absorption band positions and widths match those produced by combined OH stretch and Mg-OH lattice modes and are diagnostic of minerals with structural OH such as clays and amphiboles. Likely candidate minerals include serpentine, talc, hectorite, and sponite. There is no spectral evidence for aluminous hydroxylated minerals. No distinct band occurs at 2.55 microns, as would be expected if carbonates were responsible for the 2.35 micron absorption. High-albedo regions such as Elysium and Utopia have the strongest bands near 2.35 microns, as would be expected for heavily weathered soils. Low-albedo regions such as Iapygia show weaker but distinct bands, consistent with moderate coatings, streaks, and splotches of bright weathered material. In all areas observed, the 2.35-micron absorption is at least three times weaker than would be expected if well-crystallized clay minerals made up the bulk of bright soils on Mars.

Exposed Ice in the Northern Mid-Latitudes of Mars

NASA Technical Reports Server (NTRS)

Allen, Carlton C.

2007-01-01

Ice-Rich Layer: Polygonal features with dimensions of approximately 100 meters, bounded by cracks, are commonly observed on the martian northern plains. These features are generally attributed to thermal cracking of ice-rich sediments, in direct analogy to polygons in terrestrial polar regions. We mapped polygons in the northern mid-latitudes (30 to 65 N) using MOC and HiRISE images. Polygons are scattered across the northern plains, with a particular concentration in western Utopia Planitia. This region largely overlaps the Late Amazonian Astapus Colles unit, characterized by polygonal terrain and nested pits consistent with periglacial and thermokarst origins. Bright and Dark Polygonal Cracks: An examination of all MOC images (1997 through 2003) covering the study area demonstrated that, at latitudes of 55 to 65 N, most of the imaged polygons show bright bounding cracks. We interpret these bright cracks as exposed ice. Between 40 and 55 N, most of the imaged polygons show dark bounding cracks. These are interpreted as polygons from which the exposed ice has been removed by sublimation. The long-term stability limit for exposed ice, even in deep cracks, apparently lies near 55 N. Bright and Dark Spots: Many HiRISE and MOC frames showing polygons in the northern plains also show small numbers of bright and dark spots, particularly in western Utopia Planitia. Many of the spots are closely associated with collapse features suggestive of thermokarst. The spots range from tens to approximately 100 meters in diameter. The bright spots are interpreted as exposed ice, due to their prevalence on terrain mapped as ice rich. The dark spots are interpreted as former bright spots, which have darkened as the exposed ice is lost by sublimation. The bright spots may be the martian equivalents of pingos, ice-cored mounds found in periglacial regions on Earth. Terrestrial pingos from which the ice core has melted often collapse to form depressions similar to the martian dark spots. Future Observations: The SHARAD radar should be able to confirm the presence and measure the depth of the interpreted ice-rich layer that forms the Astapus Colles unit. If this layer is confirmed it will strengthen the interpretation of bright polygon cracks and bright spots as exposed ice. HiRISE images of the northern plains are showing unprecedented details of the polygonal cracks. Future HiRISE images that include bright spots, compared to MOC images taken years earlier, will illustrate the temporal stability of the spots. The CRISM spectrometer, with multiple spectral bands and a spatial resolution around 20 meters, should allow mineralogical identification of the material exposed in the polygonal bounding cracks and in the bright spots.

Topography of the Deuteronilus contact on Mars: Evidence for an ancient water/mud ocean and long-wavelength topographic readjustments

NASA Astrophysics Data System (ADS)

Ivanov, M. A.; Erkeling, G.; Hiesinger, H.; Bernhardt, H.; Reiss, D.

2017-09-01

In this paper, we present the results of our detailed study of morphology, topography, and age of the Deuteronilus contact that outlines Vastitas Borealis Formation (VBF) in the northern plains and the Isidis Planitia unit. The Deuteronilus contact represents a sharp and distinct geological boundary that can be traced continuously for many hundreds to thousands of kilometers. In the northern plains, segments of the Deuteronilus contact occur at two distinct topographic levels. In the northern plains, the long-wavelength topography of the Deuteronilus contact occur at two distinct topographic levels. In the Tempe, Chryse, Acidalia, and Cydonia-Deuteronilus regions (the total length is ∼14,000 km), the contact is at the mean elevation of about -3.92 km (the decile range is 180 m, from -4.01 km to -3.83 km). In the Pyramus-Astapus, Utopia, and Western Elysium regions (the total length is ∼7700 km), the mean elevation of the contact is about -3.58 km (the decile range is 270 m, from -3.73 km to -3.46 km). These levels to large extent (but not completely) correspond to the model geoids that may have been characterized the shape of Mars at the time of the VBF emplacement. Largest deviations of the actual topographic position of the contact from the model geoids occur in the Tantalus and Phlegra regions where the deviations are due to the post-VBF changes of the regional topography. The fact that the model geoids satisfactory describe the shape of the largest portion of the contact provides additional evidence for both the emplacement of the VBF edges near an equipotential surface and for relative stability of the shape of Mars during a long time interval of about 3.6 Ga. Within the northern plains in the Tempe Terra, Acidalia Planitia, Cydonia-Deuteronilus, Pyramus-Astapus, and the southern Utopia regions, the absolute model ages of the VBF surface near the Deuteronilus contact are tightly clustered around the age of ∼3.6 Ga, which we interpret as the age of the VBF emplacement. The surface of the VBF-like Isidis Planitia unit is distinctly younger, ∼3.50 ± 0.01 Ga, which suggests that this unit formed independently. Neither volcanic nor glacial modes of emplacement are consistent with the topographic configuration and the shape of the Deuteronilus contact within both the northern plains and in Isidis Planitia. The broad flooding and formation of extensive water/mud reservoirs remains to be the most plausible mode of formation of the VBF in the northern plains and the VBF-like unit on the floor of the Isidis basin.

Poverty and cancer.

PubMed

Tomatis, L

1997-01-01

Despite the attraction of certain utopias and the convincing strength of some of the social and philosophical theories underlying attempts to change the social structure and to achieve a more egalitarian society, social inequalities have not disappeared and seem even to be increasing worldwide. Inequalities in health are part of the social inequalities present in our society and one of their most convincing indices. Sanitary conditions are worse, mortality higher, survival rates of cancer patients lower, and life expectancy shorter in developing countries than in industrialized countries. Similar if not identical differences can be seen within industrialized countries between socioeconomically less and more favoured population groups. In many areas of the industrialized countries social and environmental conditions comparable with those existing in the poorest countries last century have been recreated. Occupational risks are becoming a serious problem in developing countries, largely as a consequence of the transfer of hazardous industries from industrialized countries where certain industries are judged to be unacceptable. A similar double standard is applied to tobacco advertising and sales in the industrialized and developing countries. The projections of the total number of cancer cases in the next decades indicate a generalized increase, proportionally greater in developing than in industrialized countries.

Walden two: The morality of anarchy

PubMed Central

Segal, Evalyn F.

1987-01-01

The utopian label is often pinned on calls for comprehensive change as a means of dismissing them from serious consideration.... [S]ocial orders come and go, and those who indulge in utopian thinking may be more prepared for... the inevitability of widespread societal transformation.... Keeping utopia in mind can prevent our settling for minor reforms when more significant change might be possible. (Fox, 1985, p. 55) When... I called myself a benign anarchist... someone said that that was not like the dictatorship of Walden Two. But Walden Two was anarchistic.... The functions delegated to [authority figures] in the world at large were performed by the people themselves through face-to-face commendation and censure. (Skinner, 1983, p. 426, emphasis his) The issue for anarchists is not whether there should be structure or order, but what kind there should be and what its sources ought to be. The individual or group which has sufficient liberty to be self-regulating will have the highest degree of order; the imposition of order from above and outside induces resentment and rebellion where it does not encourage childlike dependence and impotence, and so becomes a force for disorder. (Barclay, 1982, p. 17) PMID:22477973

Drug safety in pregnancy: utopia or achievable prospect? Risk information, risk research and advocacy in Teratology Information Services.

PubMed

Schaefer, Christof

2011-03-01

Even though from preclinical testing to drug risk labeling, the situation with drugs in pregnancy has improved substantially since the thalidomide scandal, there is still an increasing need to provide healthcare professionals and patients with updated individualized risk information for clinical decision making. For the majority of drugs, clinical experience is still insufficient with respect to their safety in pregnancy. There is often uncertainty in how to interpret the available scientific data. Based on 20 years of experience with Teratology Information Services (TIS) cooperating in the European Network of Teratology Information Services (ENTIS) methods of risk interpretation, follow-up of exposed pregnancies through the consultation process and their evaluation is discussed. Vitamin K antagonists, isotretinoin and angiotensin (AT) II-receptor-antagonists are presented as examples of misinterpretation of drug risks and subjects of research based on observational clinical data recorded in TIS. As many TIS are poorly funded, advocacy is necessary by establishing contacts with decision makers in health politics and administration, informing them of the high return in terms of health outcomes and cost savings provided by TIS as reference institutions in clinical teratology. © 2011 The Author. Congenital Anomalies © 2011 Japanese Teratology Society.

Eroded Scallops with Layers

NASA Image and Video Library

2017-01-09

The western Utopia Planitia in the Northern mid-latitudes of Mars is marked by a peculiar type of depression with scalloped edges and by a network of polygonal fractures. The scalloped depressions are typical features; a smooth layered terrain located between 40 and 60 degrees in both hemispheres. Scalloped depressions probably form by removal of ice-rich subsurface material by sublimation (ice transforming directly from a solid to a gaseous state), a process that may still be active today. Isolated scalloped depressions generally have a steep pole-facing scarp and a gentler equator-facing slope. This asymmetry is interpreted as being the result of difference in solar heating. Scalloped depressions may coalesce, leading to the formation of large areas of pitted terrain. The polygonal pattern of fractures resembles permafrost polygons that form in terrestrial polar and high alpine regions by seasonal-to-annual contraction of the permafrost (permanently frozen ground). On Earth, such polygons indicate the presence of ground ice. These landforms most likely show that sub-surface ice is present or has been present geologically recently at these latitudes, and they may slowly be continuing their development at the present time. http://photojournal.jpl.nasa.gov/catalog/PIA13485

Industrial Safety and Utopia: Insights from the Fukushima Daiichi Accident.

PubMed

Travadel, Sébastien; Guarnieri, Franck; Portelli, Aurélien

2018-01-01

Feedback from industrial accidents is provided by various state or even international, institutions, and lessons learned can be controversial. However, there has been little research into organizational learning at the international level. This article helps to fill the gap through an in-depth review of official reports of the Fukushima Daiichi accident published shortly after the event. We present a new method to analyze the arguments contained in these voluminous documents. Taking an intertextual perspective, the method focuses on the accident narratives, their rationale, and links between "facts," "causes," and "recommendations." The aim is to evaluate how the findings of the various reports are consistent with (or contradict) "institutionalized knowledge," and identify the social representations that underpin them. We find that although the scientific controversy surrounding the results of the various inquiries reflects different ethical perspectives, they are integrated into the same utopian ideal. The involvement of multiple actors in this controversy raises questions about the public construction of epistemic authority, and we highlight the special status given to the International Atomic Energy Agency in this regard. © 2017 The Authors Risk Analysis published by Wiley Periodicals, Inc. on behalf of Society for Risk Analysis.

Near-surface ice-rich regolith in mid Utopia Planitia, Mars, and its formation by thaw-freeze cycling

NASA Astrophysics Data System (ADS)

Soare, R. J.; Conway, S. J.

2012-12-01

We have used all relevant HiRISE, MOC, THEMIS and CTX images of mid Utopia Planitia (UP; ~30-600N; ~65-1010E) to identify and then map the spatial association of flat-floored and scalloped depressions, small-sized (~150m) polygonal patterned-ground and polygon-junction/trough pits. In periglacial regions on Earth such as northern Yakutia and Alaska, similar landscape-assemblages comprised of thermokarst lakes or alases, ice-wedge polygons and polygon-junction ponds are markers of ice-rich permafrost (dominated by lens-like segregation ice). The distribution of these Martian putative periglacial-landforms (PPLs) cross cuts geological units that have a wide range of ages and types, i.e. HBU1 (early Hesperian, lava) - AEta (late Hesperian, fluvial) - ABa (late Amazonian, aeolian), and suggests that a previously unidentified periglacial unit (PUPU) exists in the region. Regardless of whether the PPLs form by means of sublimation or thaw, questions concerning the origin of the hypothesised ice-rich permafrost itself have been largely overlooked in the literature. Based on our most recent observations and findings, we propose five things. First, the PUPU is tens of metres deep, regional in spatial extent, shows sub-horizontal banding, and is an ice-enriched loess-like (or fine-grained) unit comprised principally of segregated ice. Second, the PUPU is distinct from and underlies a regional high-albedo mantle that does not show periglacial landscape modification or features. Heretofore, numerous workers have hypothesised that the scalloped depressions, small-sized polygons and polygon-junction/trough pits that are ubiquitous in the region are the product of mantle degradation by sublimation. Third, the fact that the PUPU is overlain by a mantle not modified by periglacial processes leads one to believe that the formation of a periglacial landscape in mid UP is not as recent as some workers have thought. Fourth, the loess-like material could comprise weathered and eroded material derived from the north polar cap deposits and transported to the mid-latitudes by katabatic winds. Fifth, the ice-enrichment of the PUPU is distinct from and independent of loess deposition and accumulation. As is the case with their presumed analogues on Earth, we hypothesise that the Martian PPLs form in fine-grained sediments that have accumulated episodically; these sediments undergo post-deposition infiltration by melt water, possibly derived of surface snow or ice precipitated atmospherically. Fine-grained sediments facilitate cryosuction, which is the attraction of water towards a freezing front, and the formation of segregated ice lenses. Metre-thick (near-surface) ice-cemented permafrost has been observed in the Antarctic Dry Valleys. Diffusive exchange between the atmosphere and the near-surface sediments is the process by which ice cementation could have taken place. However, diffusive exchanges to the full depth of the PUPU are not considered to be possible unless this occurs episodically.

Relative Ages of the Highlands, Lowlands, and Transition Zone Along a Portion of the Mars Crustal Dichotomy from Densities of Visible and Buried Impact Craters

NASA Technical Reports Server (NTRS)

DeSoto, G. E.; Frey, H. V.

2005-01-01

Understanding the fundamental age relationships of the different parts of the Mars Crustal Dichotomy is essential to fully understanding the events that shaped the early history and formation of the surface of Mars. A dominant question is what are the true relative ages of the Northern Lowlands and the Southern Highlands? Using MOLA data from the Mars Global Surveyor and Viking visual images, a dataset of both buried and visible crater diameters was created over a nine million sq km study area of a section of the dichotomy boundary stretching from Arabia Terra to Utopia Planitia. Cumulative frequency plots on a log-log scale were used to determine the relative ages for the Highlands, the Lowlands, and the Transition Zone, separately for the visible, the buried and the combined total (visible+ buried) populations. We find the overall Highland crater population in this area is slightly older than the Lowlands, consistent with previous global studies, but the Lowlands and Transition Zone are also very old and formed at roughly the same time. It appears that the formation of the Lowlands in this region formed contemporaneously with a large-scale resurfacing event in the Highlands, perhaps caused by the process responsible for the Lowland formation.

MoNET: media over net gateway processor for next-generation network

NASA Astrophysics Data System (ADS)

Elabd, Hammam; Sundar, Rangarajan; Dedes, John

2001-12-01

MoNETTM (Media over Net) SX000 product family is designed using a scalable voice, video and packet-processing platform to address applications with channel densities from few voice channels to four OC3 per card. This platform is developed for bridging public circuit-switched network to the next generation packet telephony and data network. The platform consists of a DSP farm, RISC processors and interface modules. DSP farm is required to execute voice compression, image compression and line echo cancellation algorithms for large number of voice, video, fax, and modem or data channels. RISC CPUs are used for performing various packetizations based on RTP, UDP/IP and ATM encapsulations. In addition, RISC CPUs also participate in the DSP farm load management and communication with the host and other MoP devices. The MoNETTM S1000 communications device is designed for voice processing and for bridging TDM to ATM and IP packet networks. The S1000 consists of the DSP farm based on Carmel DSP core and 32-bit RISC CPU, along with Ethernet, Utopia, PCI, and TDM interfaces. In this paper, we will describe the VoIP infrastructure, building blocks of the S500, S1000 and S3000 devices, algorithms executed on these device and associated channel densities, detailed DSP architecture, memory architecture, data flow and scheduling.

Thermokarst, mantling and Late Amazonian Epoch periglacial-revisions in the Argyre region, Mars

NASA Astrophysics Data System (ADS)

Soare, R. J.; Baoini, D.; Conway, S. J.; Dohm, J. M.; Kargel, J. S.

2015-10-01

Thermokarst, mantling and Late Amazonian Epoch periglacial-revisions in the Argyre region, Mars R.J. Soare(1), D. Baioni(2), S.J. Conway (3), J.M. Dohm(4)and J.S. Kargel (5)(1) Geography Department, Dawson College, Montreal, Canada H3Z 1A4 rsoare@dawsoncollege.qc.ca.(2) Dipartimento di Scienze della Terra,della Vita e Ambiente, Università di Urbino "Carlo Bo", Campus SOGESTA, 61029 Urbino (PU) Italy. (3) Department of Physical Sciences, Open University, Milton Keynes, United Kingdom, MK7 6AA. (4) The University Museum, University of Tokyo, Hongo 7-3-1, Bunkyo-ku, Tokyo 113-, Japan.(5) Department of Hydrology & Water Resources, University of Arizona, Tucson, Arizona, USA 85719.1.Introduction Metre to decametre-deep depressions that are rimless, relatively flat-floored, polygonised and scallop-shaped have been widely observed in Utopia Planitia (UP) [e.g. 1-5] and Malea Planum (MP) [6-8]. Although there is some debate about whether the depressions formed by means of sublimation or evaporation, it is commonly believed that the terrain in which the depressions occur is ice-rich.Moreover, most workers assume that this "ice-richness" is derived of a bi-hemispheric, latitudinally-dependent and atmospherically-precipitated mantle that is metres thick [2,4,6-10].

Public Flat in Indonesia, Their Role in Highly Densed City: Legal Aspect Review and Prototype Assessment

NASA Astrophysics Data System (ADS)

Paramita, Beta; Perdana Khidmat, Rendy; Fukuda, Hiroatsu

2018-05-01

An affordable vertical house, which is known as rusun in Indonesian term becomes the utopia of a compact city. The rusun to be the main actor contributing to the creation of liveable comfort in dense areas by relocating squatters and slum inhabitants to better living places. Technical guidelines and building standards play a major role in a building’s environmental impact. These standards will be reviewed based on their impact on building performance. There are two prototypes of rusun referenced in 05/PRT/M/2007, and the assessment of these prototypes has been done by using ENVi-met. The meteorological data for the ENVI-met configuration input is adapted to the same weather and climate conditions taken from the data measured on June 13th, 2012. The analysis of this assessment will focus on building orientation, building length, building height, and also the microclimate which is impacted by these prototypes. Based on the assessment, it is recommended that the layout of outdoor space on the north side should provide as much green coverage as possible, either for shadowing or for the benefit of its albedo. The simulation shows that building ratio of 1:3 produces higher wind speed, which also controls air temperature and humidity.

B. F. Skinner and technology's nation: Technocracy, social engineering, and the good life in 20th-century America.

PubMed

Rutherford, Alexandra

2017-08-01

Psychologist B. F. Skinner developed and promoted a technology of behavior as the basis for widespread social reform over much of his career. In 1948, he published his behaviorally engineered vision of the good life in his utopian novel Walden Two (Skinner, 1948). Skinner's efforts were part of a much larger social engineering tradition that received one of its fullest expressions in the Technocracy Movement of the 1930s. Fifteen years before Skinner's Walden Two , at the height of the Technocracy Movement's public visibility in the United States, technocrat Harold Loeb (1933/1996) published his utopia, Life in a Technocracy: What It Might Be Like . In this article, I place the socially engineered visions of the good life promoted by the Technocracy Movement and by Skinner on an intellectual and ideological continuum to amplify and explore American attitudes toward psychology, technology, and social engineering during the middle decades of the 20th century. I argue that responses to both reveal the possibilities and limits of the social engineering enterprise, and suggest that historians of technology might consider how the history of psychology and other psy-disciplines can deepen conceptualizations of the relationships among the psychological, the social, and the technological in this period. (PsycINFO Database Record (c) 2017 APA, all rights reserved).

ET versus Alien : Popular Attitudes to bringing back Biological Material from Space

NASA Astrophysics Data System (ADS)

Evans, D.

The general public tend to react to radical scientific innovation in extreme ways, seeing them alternatively as a passport to utopia or a ticket to hell. The possible discovery of alien life forms has generated both types of reaction, as a brief survey of Hollywood movies shows. In this fanciful world, alens are either the friendly beings of ET and Close Encounters, who show us a way to improve ourselves, or the frightening monsters of Alien and Independence Day, who are bent on our destruction. Yet most astrobiologists would agree that both types of scenario are extremely unlikely. If we do encounter other life forms, the scientific consensus is that such life is vastly more likely to be microbial than to be an advanced, intelligent multicellular species. The public focus on the improbable stories of Hollywood means that they are little prepared to engage in sensible dialogue about plans for sample return missions from Mars and other planets. Unless scientific organisations take steps to encourage a more realistic understanding of the kinds of life we are most likely to encounter in space, we risk seeing public debate on these matters degenerate into the same hysteria and idiocy as that which has surrounded the use of GM foods and stem cell research.

A calibration hierarchy for risk models was defined: from utopia to empirical data.

PubMed

Van Calster, Ben; Nieboer, Daan; Vergouwe, Yvonne; De Cock, Bavo; Pencina, Michael J; Steyerberg, Ewout W

2016-06-01

Calibrated risk models are vital for valid decision support. We define four levels of calibration and describe implications for model development and external validation of predictions. We present results based on simulated data sets. A common definition of calibration is "having an event rate of R% among patients with a predicted risk of R%," which we refer to as "moderate calibration." Weaker forms of calibration only require the average predicted risk (mean calibration) or the average prediction effects (weak calibration) to be correct. "Strong calibration" requires that the event rate equals the predicted risk for every covariate pattern. This implies that the model is fully correct for the validation setting. We argue that this is unrealistic: the model type may be incorrect, the linear predictor is only asymptotically unbiased, and all nonlinear and interaction effects should be correctly modeled. In addition, we prove that moderate calibration guarantees nonharmful decision making. Finally, results indicate that a flexible assessment of calibration in small validation data sets is problematic. Strong calibration is desirable for individualized decision support but unrealistic and counter productive by stimulating the development of overly complex models. Model development and external validation should focus on moderate calibration. Copyright © 2016 Elsevier Inc. All rights reserved.

Sir William Osler's speech at Troy: a Trojan horse?

PubMed

Moran, Michael E

2012-01-01

Troy, New York, is a city of 55,000 people in upstate New York located along the Hudson River. A city of surprisingly rich cultural heritage, it was the home of New York state's first hospital outside New York City. The 50th anniversary celebration of Troy's hospital brought William Osler to the city as the keynote speaker. This speech, delivered on November 28, 1900, is one of Sir William's less well known addresses. Osler began his comments with Sir Thomas More's Utopia and talked at length about the hospital, its obligations, the influences it has upon the community, and the role of physicians and surgeons. He broached one of his old saws, the salary of attending physicians and their needed role in hospital management. His words were published in the diamond jubilee's records, but the hospital did not outlive its prominent guest professor, and it closed its doors in 1914. Just like the great historical city of Troy, New York's own Troy was on the brink of decline, and its hospital would be the first fatality. Therefore, it is almost prescient that the words of Osler, taken into historical context juxtaposed against the socioeconomic forces at work, are akin to the Greek's offering of a wooden edifice to end the Trojan War.

Sir William Osler's speech at Troy: a Trojan horse?

PubMed Central

2012-01-01

Troy, New York, is a city of 55,000 people in upstate New York located along the Hudson River. A city of surprisingly rich cultural heritage, it was the home of New York state's first hospital outside New York City. The 50th anniversary celebration of Troy's hospital brought William Osler to the city as the keynote speaker. This speech, delivered on November 28, 1900, is one of Sir William's less well known addresses. Osler began his comments with Sir Thomas More's Utopia and talked at length about the hospital, its obligations, the influences it has upon the community, and the role of physicians and surgeons. He broached one of his old saws, the salary of attending physicians and their needed role in hospital management. His words were published in the diamond jubilee's records, but the hospital did not outlive its prominent guest professor, and it closed its doors in 1914. Just like the great historical city of Troy, New York's own Troy was on the brink of decline, and its hospital would be the first fatality. Therefore, it is almost prescient that the words of Osler, taken into historical context juxtaposed against the socioeconomic forces at work, are akin to the Greek's offering of a wooden edifice to end the Trojan War. PMID:22275788

Habitable periglacial landscapes in martian mid-latitudes

NASA Astrophysics Data System (ADS)

Ulrich, M.; Wagner, D.; Hauber, E.; de Vera, J.-P.; Schirrmeister, L.

2012-05-01

Subsurface permafrost environments on Mars are considered to be zones where extant life could have survived. For the identification of possible habitats it is important to understand periglacial landscape evolution and related subsurface and environmental conditions. Many landforms that are interpreted to be related to ground ice are located in the martian mid-latitudinal belts. This paper summarizes the insights gained from studies of terrestrial analogs to permafrost landforms on Mars. The potential habitability of martian mid-latitude periglacial landscapes is exemplarily deduced for one such landscape, that of Utopia Planitia, by a review and discussion of environmental conditions influencing periglacial landscape evolution. Based on recent calculations of the astronomical forcing of climate changes, specific climate periods are identified within the last 10 Ma when thaw processes and liquid water were probably important for the development of permafrost geomorphology. No periods could be identified within the last 4 Ma which met the suggested threshold criteria for liquid water and habitable conditions. Implications of past and present environmental conditions such as temperature variations, ground-ice conditions, and liquid water activity are discussed with respect to the potential survival of highly-specialized microorganisms known from terrestrial permafrost. We conclude that possible habitable subsurface niches might have been developed in close relation to specific permafrost landform morphology on Mars. These would have probably been dominated by lithoautotrophic microorganisms (i.e. methanogenic archaea).

Corrigendum to "Energetics of the Martian Atmosphere Using the Mars Analysis Correction Data Assimilation (MACDA) Dataset" [Icarus 276 (2016) 1-20

NASA Astrophysics Data System (ADS)

Battalio, Michael; Szunyogh, Istvan; Lemmon, Mark

2018-03-01

A coding error resulted in the barotropic energy conversion (BTEC) term taking the wrong sign throughout the paper. All figures showing BTEC, whether as an average or an instantaneous field, should have the sign swapped. This change alters the following conclusions: BTEC acts as a source of eddy kinetic energy on the upstream side of the storm tracks, namely in Acidalia Planitia and Utopia Planitia, and as a sink just upstream of the highest topography. BTEC is a weak source of eddy kinetic energy closer to the surface, but is a strong source above 10 Pa. The main conclusion that waves decay by BTEC and that waves in high opacity situations grow via BTEC remains, but there is also a positive contribution toward the EKE by the BTEC during the growth periods of waves, even in low-opacity situations. These changes make the resulting BTEC more inline to that of other modeling efforts (Barnes et al., 1993; Greybush et al., 2013; Tabataba-vakili et al., 2015), observations (e.g., Banfield et al., 2004), and terrestrial studies (Chang, 2001; Chang et al., 2002; Decker and Martin, 2005; Ahmadi-Givi et al., 2014; Herrera et al., 2016). The new BTEC also slightly modifies the residue shown in Fig. 6, but the qualitative conclusions for the residue remain unchanged.

Northwestern Tharsis Latent Outflow Activity Mars

NASA Technical Reports Server (NTRS)

Dohm, J. M.; Anderson, R. C.; Baker, V. R.; Ferris, J. C.; Hare, T. M.; Strom, R. G.; Rudd, L.; Rice, J. W., Jr.; Scott, D. H.

2000-01-01

Previously defined outflow channels, which are indicated by relict landforms similar to those observed on Earth, signify ancient catastrophic flood events on Mars. These conspicuous geomorphic features are some of the most remarkable yet profound discoveries made by geologists to date. These outflow channels, which debouched tremendous volumes of water into topographic lows such as Chryse, Utopia, Elysium, and Hellas Planitiae, may represent the beginning of warmer and wetter climatic periods unlike the present-day cold and dry Mars. In addition to the previously identified outflow channels, observations permitted by the newly acquired Mars Orbiter Laser Altimeter (MOLA) data have revealed a system of gigantic valleys, referred to as the northwestern slope valleys (NSV), that are located to the northwest of a huge shield volcano, Arsia Mons, western hemisphere of Mars. These features generally correspond spatially to gravity lows similar to the easternmost, circum-Chryse outflow channel systems. Geologic investigations of the Tharsis region suggest that the large valley system pre-dates the construction of Arsia Mons and its extensive associated lava flows of mainly Late Hesperian and Amazonian age and coincides stratigraphically with the early development of the circum-Chryse outflow channel systems that debouch into Chryse Planitia. This newly identified system, the NSV, potentially signifies the largest flood event(s) ever recorded for the solar system. Additional information is contained in original extended abstract.

Sustainable development and social learning: Re-contextualising the space of orientation

NASA Astrophysics Data System (ADS)

Seddon, Terri

2016-10-01

In the lead-up to the 2007 Australian federal election, Labor candidate Kevin Rudd described climate change as the "great moral challenge of our generation". In the years since then, the heat in Australia has been rising - in terms of both temperature and climate politics -, but government action has slowed down. Endorsement of economic growth is prioritised, with only intermittent recognition of environmental costs. At grassroots level, citizens' attitudes are influenced by social norms. This kind of social learning is a major constraint on sustainability. Therefore, it seems useful to consider how educators might help build sustainable futures. To understand how historical context entangles social learning in ways that complicate policies associated with Education for Sustainable Development (ESD) and practices of Education for Sustainability (EfS), the author of this paper draws on the concept of "space of orientation". Focusing on adult education, she traces the contradiction between "globalisation" and "sustainability" through policy logics, relational practices in Australian adult education and the "necessary utopia" which provides a point of reference for making futures. She argues that spaces of orientation are a critical resource in this era of intensifying conflicts of interest between economic priorities of globalisation and environmental priorities intended to slow global warming, because they mediate context and orient learning in ways that clear a path towards sustainability through the entangled histories of this present.

Expectation and futurity: The remarkable success of genetic determinism.

PubMed

Esposito, Maurizio

2017-04-01

Genetic determinism is nowadays largely questioned and widely criticized. However, if we look at the history of biology in the last one hundred years, we realize that genetic determinism has always been controversial. Why, then, did it acquire such relevance in the past despite facing longstanding criticism? Through the analysis of some of the ambitious expectations of future scientific applications, this article explores the possibility that part of the historical success of genetic determinism lies in the powerful rhetorical strategies that have connected the germinal matter with alluring bio-technological visions. Indeed, in drawing on the recent perspectives of "expectation studies" in science and technology, it will be shown that there has been an interesting historical relationship between reductionist notions of the gene as a hereditary unit, coded information or functional DNA segment, and startling prophecies of what controlling such an entity might achieve. It will also be suggested that the well-known promissory nature of genomics is far older than the emergence of biotechnology in the 1970s. At least from the time of the bio-utopias predicted by J.B.S. Haldane and J. S. Huxley, the gene has often been surrounded by what I call the "rhetoric of futurity": a promissory rhetoric that, despite momentous changes in the life sciences throughout the 20th century, has remained relatively consistent over time. Copyright © 2017 Elsevier Ltd. All rights reserved.

[The myth of the good savage].

PubMed

Yampey, N

1994-09-01

The conquest of the New World gave way to the myth of the Good Savage. For the Renaissance intellectuals, the ancient ideas about the Golden Age (an ideal society promising an unending bliss) seemed to be brought back to life at last. Sharply contrasting with the European exacerbated unrest of the time, America stood for a redeeming hope, a symbol of a better future. The myth of the Good Savage assumes people to be naturally good, but civilization has led them into the realm of violence, hatred, and cruelty. Besides being naturally good, nice-minded people, "good savages" were also useful, obedient people, most likely to be easily exploited by Europeans--a source for the historical drama to come. On the verge of freeing itself from the Spanish rule, Latin America--fighting its way toward independence, had three enlightened mentors: Voltaire, Rousseau, and Montesquieu. There, again, another deep contrast arose between the abstract characteristics of Latin American aims to perfection, and people's actual behaviors. The former "good savage" became the modern "Latin American" embodying an utopia as well as a hope in his eagerness for setting up a plural, and humanized culture. The myth of the Good Savage represents a deep longing for an objectivation of the ego-ideal: it has been used, so to speak, in collective mobilizations as well as dogmatic crystallizations, to escape from ignominous realities or to project alternatives for a better socially-shared life.

Genesis Hypotheses Concerning Putative Rootless Cone Groups in Isidis Planitia, Mars

NASA Astrophysics Data System (ADS)

Pithawala, T. M.; Ghent, R. R.

2008-09-01

ABSTRACT Introduction Isidis Planitia is one of the many areas on Mars containing thumbprint terrain (TPT), a term coined to reflect the resemblance in Viking images to fingerprints. Other instances occur in Argyre, Hellas, Arcadia Planitia, and Utopia Planitia. The terrain is found where Greeley and Guest (1987) have defined the Hesperian Ridged Plains (Hvr) unit. However, landforms comprising the TPT in Isidis are markedly different in morphology from those in the northern plains. The purpose of this study is to conduct a systematic examination of the TPT in Isidis Planitia using high-resolution imagery, and to propose a hypothesis for its genesis. Northern Plains TPT Morphology: TPT landforms include branching troughs and medial ridges forming whorled lobes and mounds, most with basal scarps or terraces. TPT has been described as consisting of parallel, en echelon, or nested sets of regularly spaced curvilinear ridges or aligned hills [1]. The ridges were estimated to be 0.5-2.5 km wide and 1-40 km long, with a characteristic spacing of 2-6 km. Whorled lobes of TPT are 75-150 km wide, with heights ranging from 10-200 m. Previous work identified 22 areas of TPT, covering 3000- 420,000 km2 in the Northern Plains at elevations between 0 and -2 km. In Utopia, TPT includes branching troughs and medial ridges [5], and TPT is closely associated with troughs in at least 9 other Northern Plains areas [1]. Northern Plains TPT Origin: MOLA topography supports the hypothesis that TPT and associated trough systems in Utopia and Arcadia Planitae are glacial features [1,2,3]. Possible mechanisms include formation of ridges as moraines and troughs as eskers formed by wet-based continental glaciers. The absence of drumlin fields suggests that the glaciers responsible for forming the topography may have been cold-based and thus did not deform the substrate so as to form drumlins [4]. A puzzling characteristic of Mars alleged glacial landscapes is that they are morphologically pristine, though they must be at least hundreds of millions of years old [1]. Isidis TPT The physical appearance of the Isidis features differs from that of the Northern Plains TPT. Isisdis TPT includes wrinkle ridges and curvilinear ridges. Wrinkle ridges are oriented radially and concentric to the basin structure, form cells of 180 km in diameter, and occur throughout the basin over a range of elevations. They are on the order of 75-150 m high and less than 70 km wide [6]. In this study, we focus on the curvilinear ridges and associated features, using THEMIS daytime IR data. Curvilinear ridges are ˜10-50 m high, and <5 km wide, with a large number 1km wide. Ridges consist of connected cones with central depressions (30-50 % of basal diameter). Cones are often connected to each other midway through their height but sometimes share portions of their rims as well. Basal diameters of the cones vary from 600-1000 m (nearly twice the size of cones seen in northern plains TPT) [6]. Spatial Patterns Closely spaced ridges are sub-parallel to parallel. Mapping of TPT features in Isidis Planitia shows four domains of distinct morphology (Figure 1). Domain 1 consists of chain-like ridges of cones concentrated to the southern and western regions of the basin. Domain 2 consists of isolated cones localized in the basin center. Domain 3 is the Syrtis Major Isidis Planitia transition zone and consists of clusters of knobs, mesas, and large single scarps [7]. Domain 4 (west of the transition zone and along the outer regions of the basin) consists of smooth terrain lacking a significant number of cones, or knobs and mesas. The most detailed mapping in this study has been completed for Domains 1 and 2. In Domain 1, an apparent pattern emerges along a boundary trending E-W at 12 N. Cone-chains located north of this boundary show a preferential N-S alignment, convex toward the east. Cone-chains located south of the boundary show a preferential E-W alignment, convex toward the south. Cone-chains occupy the region previously mapped as Hvr [8]. Origin of the Isidis TPT features Glacial formation mechanisms are generally accepted for formation of TPT in Argyre, Hellas, Arcadia, and Utopia. The TPT of Isidis Planitia is markedly different in morphology, and so deserves a fresh examination. We look to terrestrial analogues of rootless cones. The underlying mechanism is the interaction between magma (or lava) with a volatile (possibly water) rich substrate. Top-heating A top-heating model would involve lava flows and Vastitas Borealis Formation (VBF) materials known to cover the floor of Isidis [7]. In this model, Syrtis Major eruptions would produce tube-fed lava flows overlying volatile-rich materials derived from the Northern Plains, heating the wet substrate from above; interaction between the hot lava tubes and the substrate would produce chains of rootless cones. This model is expected to play a role in the formation of the TPT features, though it is doubtful if it can act solely to form the features, because the model is topography dependent and cannot readily account for both large- and smallscale patterns. Bottom-Heating The spatial patterns seen in planview of TPT in Isidis Planitia show a strong similarity to surface and seismic expressions of sills the Karoo basin in South Africa and the North Rockall Trough in the NE Atlantic on Earth. This leads to the idea that a sill or cone sheet complex beneath the Isidis basin, possibly linked to Syrtis Major, could drive bottom heating of a volatile rich substrate, leading to the formation of aligned rootless cones comprising the thumbprint terrain of Isidis Planitia. Though similar to the top-heating model, a system of intrusive structures heating from below would be independent of the current local topography of the basin, and is thus favorable. Such a mechanism could further explain the small-scale deviations in spatial alignment from the regional trend. The branch-like evolution of a sill complex can result in the non-uniform development of sills [11], such that daughter bodies of a parent sill can vary in size and vertical and horizontal distribution, and thus result in different abutment relationships, causing varying surface manifestations of the hybrid sill tips. A combination of both models is also a likely candidate for the genesis of TPT in Isidis. We are continuing to investigate the details of the two models by analyzing additional datasets and terrestrial analogues. References [1] Kargel et al. (1995) JGR-E, 100, 5351-5368. [2] Pomerantz, W.J and Head III, J.W (2003) LPSC XXXXIII, Abstract 1277. [3] Chapman M. (1994) Icarus, 109(2), 393-406. [4] Head III, J.W and Marchant (2003) LPSC XXXXIII, Abstract 1247. [5] Scott and Underwood (1991) Proceedings of Lunar Planet. Sci, 21, 627-634. [6] Hiesinger, H. and Head III, J.W (2003) 6th Intl Conf. on Mars, Abstract 3061. [7] Ivanov, M.A and Head III, J.W (2003) JGR-E, 108, E6. [8] Greeley, R. and Guest, J.E (1987), US Geol. Surv. Misc. Invest. Ser., Map I-1802-B. [9] Cartwright, J. and Hansen, D.M (2006) Geology 34(11), 929-932. [10] Hansen, D.M and Cartwright, J. (2006) Journal Geol. Soc. London 163 (3), 509-523. [11] Thomson, K., and Hutton, D. (2004) Bull Volcanology, 66, 364-375.

Characterization, adaptive traffic shaping, and multiplexing of real-time MPEG II video

NASA Astrophysics Data System (ADS)

Agrawal, Sanjay; Barry, Charles F.; Binnai, Vinay; Kazovsky, Leonid G.

1997-01-01

We obtain network traffic model for real-time MPEG-II encoded digital video by analyzing video stream samples from real-time encoders from NUKO Information Systems. MPEG-II sample streams include a resolution intensive movie, City of Joy, an action intensive movie, Aliens, a luminance intensive (black and white) movie, Road To Utopia, and a chrominance intensive (color) movie, Dick Tracy. From our analysis we obtain a heuristic model for the encoded video traffic which uses a 15-stage Markov process to model the I,B,P frame sequences within a group of pictures (GOP). A jointly-correlated Gaussian process is used to model the individual frame sizes. Scene change arrivals are modeled according to a gamma process. Simulations show that our MPEG-II traffic model generates, I,B,P frame sequences and frame sizes that closely match the sample MPEG-II stream traffic characteristics as they relate to latency and buffer occupancy in network queues. To achieve high multiplexing efficiency we propose a traffic shaping scheme which sets preferred 1-frame generation times among a group of encoders so as to minimize the overall variation in total offered traffic while still allowing the individual encoders to react to scene changes. Simulations show that our scheme results in multiplexing gains of up to 10% enabling us to multiplex twenty 6 Mbps MPEG-II video streams instead of 18 streams over an ATM/SONET OC3 link without latency or cell loss penalty. This scheme is due for a patent.

Crustal structure of Mars from gravity and topography

NASA Technical Reports Server (NTRS)

Neumann, G. A.; Zuber, M. T.; Wieczorek, M. A.; McGovern, P. J.; Lemoine, F. G.; Smith, D. E.

2004-01-01

Mars Orbiter Laser Altimeter (MOLA) topography and gravity models from 5 years of Mars Global Surveyor (MGS) spacecraft tracking provide a window into the structure of the Martian crust and upper mantle. We apply a finite-amplitude terrain correction assuming uniform crustal density and additional corrections for the anomalous densities of the polar caps, the major volcanos, and the hydrostatic flattening of the core. A nonlinear inversion for Moho relief yields a crustal thickness model that obeys a plausible power law and resolves features as small as 300 km wavelength. On the basis of petrological and geophysical constraints, we invoke a mantle density contrast of 600 kg m-3; with this assumption, the Isidis and Hellas gravity anomalies constrain the global mean crustal thickness to be >45 km. The crust is characterized by a degree 1 structure that is several times larger than any higher degree harmonic component, representing the geophysical manifestation of the planet's hemispheric dichotomy. It corresponds to a distinction between modal crustal thicknesses of 32 km and 58 km in the northern and southern hemispheres, respectively. The Tharsis rise and Hellas annulus represent the strongest components in the degree 2 crustal thickness structure. A uniform highland crustal thickness suggests a single mechanism for its formation, with subsequent modification by the Hellas impact, erosion, and the volcanic construction of Tharsis. The largest surviving lowland impact, Utopia, post-dated formation of the crustal dichotomy. Its crustal structure is preserved, making it unlikely that the northern crust was subsequently thinned by internal processes.

How to get paid for having fun.

PubMed

Koshland, D E

1996-01-01

As I look back, I am still amazed that I was actually paid to do something I loved and others could describe as work. Yet my situation is no different from that of most scientists who find that they are asked to pursue their innate curiosity to solve puzzles, the solutions to which fortunately are of value to society. I enjoyed the beautiful logic of mathematics in elementary grades and was entranced by the exciting solution of puzzles described by DeKruif. So I drifted into the scientific profession without a clear idea of what to do or how to do it. Each experience prepared my mind and supplied the base for the next job, creating what was for me a smooth flow from scientist to professor to editor to scientist. Fortunately for me and fellow scientists the problems of the world never disappear. "The one who rides the tiger can never get off" is an aphorism that expresses society's dependence on science. Automobiles improve transportation and create pollution, medical advantages prolong life and create over-population, pesticides bring cheaper food and create soil problems. Each advance brings on the need for more science to solve the new problems. Society, which likes to live well, is addicted to the products of science, and fortunately a peculiar set of humans are addicted to solving the problems. I am one of those typical addicts who finds the obstacle course fascinating and the endlessness of the quest utopia.

[Computer-aided prescribing: from utopia to reality].

PubMed

Suárez-Varela Ubeda, J; Beltrán Calvo, C; Molina López, T; Navarro Marín, P

2005-05-31

To determine whether the introduction of computer-aided prescribing helped reduce the administrative burden at primary care centers. Descriptive, cross-sectional design. Torreblanca Health Center in the province of Seville, southern Spain. From 29 October 2003 to the present a pilot project involving nine pharmacies in the basic health zone served by this health center has been running to evaluate computer-aided prescribing (the Receta XXI project) with real patients. All patients on the center's list of patients who came to the center for an administrative consultation to renew prescriptions for medications or supplies for long-term treatment. Total number of administrative visits per patient for patients who came to the center to renew prescriptions for long-term treatment, as recorded by the Diraya system (Historia Clinica Digital del Ciudadano, or Citizen's Digital Medical Record) during the period from February to July 2004. Total number of the same type of administrative visits recorded by the previous system (TASS) during the period from February to July 2003. The mean number of administrative visits per month during the period from February to July 2003 was 160, compared to a mean number of 64 visits during the period from February to July 2004. The reduction in the number of visits for prescription renewal was 60%. Introducing a system for computer-aided prescribing significantly reduced the number of administrative visits for prescription renewal for long-term treatment. This could help reduce the administrative burden considerably in primary care if the system were used in all centers.

[The two (and more) cultures of the "clone". Utopia and fiction in post-war discourses of life sciences].

PubMed

Brandt, Christina

2009-01-01

Since the late 1950s, "two cultures" has become a catch phrase for describing a deep divide between science and literature. When Charles P. Snow, who initiated this discussion, introduced the notion of "two cultures" in a lecture at the University in Cambridge in 1959, he referred to an incompatibility of scientific and literary worldviews in Western Societies. His thesis of two contradicting cultures immediately received a huge variety of different responses from philosophers, scientists, novelists and literary scholars. However, this article argues that this widespread debate was part of a broader post-war discourse on the impact of modern science on society, in which especially the idea of "scientific progress" was at stake. Central to this debate was the question of how scientific and technological progress could affect the notion of the "human" itself. The paper analyses the emerging discourse on cloning against this background. The constitutive role of fiction and imagination in both fields, science and literature, is explored by tracing the scientific, utopian and literary cultures in which figures of human clones have taken different shapes since the 1960s. At that time, scientists developed utopian views in which the "clone" became a metaphor for future possibilities of transcending and reshaping the human nature. Science fiction writers reacted to this by portraying the human clone as an individual and by depicting human clone figures in a psychological way

Carl Sagan's Cosmic Connection

NASA Astrophysics Data System (ADS)

Sagan, Carl; Agel, Jerome

2000-08-01

Foreword Freeman Dyson; Personal reflections Ann Druyan; Preface; Part I. Cosmic Perspective: 1. A transitional animal; 2. The Unicorn of Cetus; 3. A message from earth; 4. A message to earth; 5. Experiments in utopias; 6. Chauvinism; 7. Space exploration as a human enterprise I. The scientific interest; 8. Space exploration as a human enterprise II. The public interest; 9. Space exploration as a human enterprise III. The historical interest; Part II. The Solar System: 10. On teaching the first grade; 11. 'The ancient and legendary Gods of old'; 12. The Venus detective story; 13. Venus is hell; 14. Science and 'intelligence'; 15. The moons of Barsoom; 16. The mountains of Mars I. Observations from earth; 17. The mountains of Mars II. Observations from space; 18. The canals of Mars; 19. The lost pictures of Mars; 20. The Ice Age and the cauldron; 21. Beginnings and ends of the Earth; 22. Terraforming the plants; 23. The exploration and utlization of the solar system; Part III. Beyond the Solar System: 24. Some of my best friends are dolphins; 25. 'Hello, central casting? Send me twenty extraterrestrials'; 26. The cosmic connection; 27. Extraterrestrial life: an idea whose time has come; 28. Has the Earth been visited?; 29. A search strategy for detecting extraterrestrial intelligence; 30. If we succeed 31. Cables, drums, and seashells; 32. The night freight to the stars; 33. Astroengineering; 34. Twenty questions: a classification of cosmic civilisations; 35. Galactic cultural exchanges; 36. A passage to elsewhere; 37. Starfolk I. A Fable; 38. Starfolk II. A future; 39. Starfolk III. The cosmic Cheshire cats; Epilog David Morrison; Index.

Calling International Rescue: knowledge lost in literature and data landslide!

PubMed Central

Attwood, Teresa K.; Kell, Douglas B.; McDermott, Philip; Marsh, James; Pettifer, Steve R.; Thorne, David

2009-01-01

We live in interesting times. Portents of impending catastrophe pervade the literature, calling us to action in the face of unmanageable volumes of scientific data. But it isn't so much data generation per se, but the systematic burial of the knowledge embodied in those data that poses the problem: there is so much information available that we simply no longer know what we know, and finding what we want is hard – too hard. The knowledge we seek is often fragmentary and disconnected, spread thinly across thousands of databases and millions of articles in thousands of journals. The intellectual energy required to search this array of data-archives, and the time and money this wastes, has led several researchers to challenge the methods by which we traditionally commit newly acquired facts and knowledge to the scientific record. We present some of these initiatives here – a whirlwind tour of recent projects to transform scholarly publishing paradigms, culminating in Utopia and the Semantic Biochemical Journal experiment. With their promises to provide new ways of interacting with the literature, and new and more powerful tools to access and extract the knowledge sequestered within it, we ask what advances they make and what obstacles to progress still exist? We explore these questions, and, as you read on, we invite you to engage in an experiment with us, a real-time test of a new technology to rescue data from the dormant pages of published documents. We ask you, please, to read the instructions carefully. The time has come: you may turn over your papers… PMID:19929850

Jinneography: Post-Soviet passages of traumatic exemplarity.

PubMed

Beigi, Khashayar

2016-04-01

While Russia has historically and geographically close ties with Islam, the second most-practiced religion in its vast territories, the collapse of the USSR changed the terms of this relationship in significant ways. One key shift is the emergence of new immigration patterns between Russia and former Soviet states. Traversing distant lands from the peripheries of the Caucasus and Central Asia to mainland Russia in search of work, migrants have come to recognize each other as fellow Muslims dispersed in a theological geography on the ruins of the universal comradeship dreamed by the Soviet utopia. I propose to study the Islamic pedagogical practice of ibra in the context of sociohistorical dynamics of education and migration between Russia and Central Asia to further locate and analyze this shift in relation to current debates on post-Soviet subjectivity. By discussing the case of a spirit possession of a Tajik national performed in Russia, I argue that the collective participation in the session pedagogically invokes, ciphers, and extends the post-Soviet terrains of history as ibra, or exemplary passage of worldly events. To do so, I first locate the Quranic concept of ibra as a pedagogical paradigm in Islamic traditions as well as an ethnographic lens in the context of educational campaigns for the Muslims of Eurasia and then apply the concept to my analysis of the possession session in order to show that in the ritualistic incarnations of ghosts, or jinns, the civil war of Tajikistan and its continuing cycle of terror is ciphered into a desire for learning, as well as a focus on approximation to the divine. © The Author(s) 2015.

Constraining the Date of the Martian Dynamo Shutdown by Means of Crater Magnetization Signatures

NASA Astrophysics Data System (ADS)

Vervelidou, Foteini; Lesur, Vincent; Grott, Matthias; Morschhauser, Achim; Lillis, Robert J.

2017-11-01

Mars is believed to have possessed a dynamo that ceased operating approximately 4 Ga ago, although the exact time is still under debate. The scope of this study is to constrain the possible timing of its cessation by studying the magnetization signatures of craters. The study uses the latest available model of the lithospheric magnetic field of Mars, which is based on Mars Global Surveyor data. We tackle the problem of nonuniqueness that characterizes the inversion of magnetic field data for the magnetization by inferring only the visible part of the magnetization, that is, the part of the magnetization that gives rise to the observed magnetic field. Further on, we demonstrate that a zero visible magnetization is a valid proxy for the entire magnetization being zero under the assumption of a magnetization distribution of induced geometry. This assumption holds for craters whose thermoremanent magnetization has not been significantly altered since its acquisition. Our results show that the dynamo shut off after the impacts that created the Acidalia and SE Elysium basins and before the crust within the Utopia basin cooled below its magnetic blocking temperature. Accounting for the age uncertainties in the dating of these craters, we estimate that the dynamo shut off at an N(300) crater retention age of 2.5-3.2 or an absolute model age of 4.12-4.14 Ga. Moreover, the Martian dynamo may have been weaker in its early stage, which if true implies that the driving mechanism of the Martian dynamo was not the same throughout its history.

A chemical status predictor. A methodology based on World-Wide sediment samples.

PubMed

Gredilla, A; Fdez-Ortiz de Vallejuelo, S; de Diego, A; Arana, G; Stoichev, T; Amigo, J M; Wasserman, J C; Botello, A V; Sarkar, S K; Schäfer, J; Moreno, C; Guardia, M de la; Madariaga, J M

2015-09-15

As a consequence of the limited resources of underdeveloped countries and the limited interest of the developed ones, the assessment of the chemical quality of entire water bodies around the world is a utopia in the near future. The methodology described here may serve as a first approach for the fast identification of water bodies that do not meet the good chemical status demanded by the European Water Framework Directive (WFD). It also allows estimating the natural background (or reference values of concentration) of the areas under study using a simple criterion. The starting point is the calculation the World-Wide Natural Background Levels (WWNBLs) and World-Wide Threshold Values (WWTVs), two indexes that depend on the concentration of seven elements present in sediments. These elements, As, Cd, Cr, Cu, Ni, Pb and Zn, have been selected taking into account the recommendations of the UNEP (United Nations Environment Programme) and USEPA (United States Environmental Protection Agency), that describe them as elements of concern with respect to environmental toxicity. The methodology has been exemplified in a case study that includes 134 sediment samples collected in 11 transitional water bodies from 7 different countries and 4 different continents. Six of the water bodies considered met the good chemical status demanded by the WFD. The rest of them exceeded the reference WWTVs, at least for one of the elements. The estuaries of the Nerbioi-Ibaizabal (Basque Country) and Cavado (Portugal), the sea inlet of Río San Pedro (Spain), the Sepetiba Bay (Brazil) and the Yucateco lagoon (Mexico) belong to that group. Copyright © 2015 Elsevier Ltd. All rights reserved.

Tidal Excitation of the Core Dynamo of Mars

NASA Astrophysics Data System (ADS)

Seyed-Mahmoud, B.; Arkani-Hamed, J.; Aldridge, K.

2007-05-01

The lack of magnetic anomalies inside the giant impact basins Hellas, Isidis, Utopia and Argyre, inside the northern low lands, over the Tharsis bulge, and over the Tharsis and Olympus mounts suggests that the core field of Mars ceased to exist by about 4 Gyr ago, almost when the giant basins were formed. On the other hand, the giant basins are located on a great circle, implying that the basins were likely produced by fragments of a large asteroid that broke apart as it entered the Roche limit of Mars. This scenario offers a causative relationship for the apparent coincidence of the formation of the giant basins and the cessation of the core dynamo. We suggest that the core dynamo was excited by tidally driven elliptical instability in the Martian core. The breaking of the asteroid and its final impact on Mars eliminated the excitation and thus killed the dynamo. We show that a retrograde asteroid captured in a Keplerian orbit around Mars at a distance of about 50,000-100,000 km could orbit Mars for several hundreds of millions of years before impacting the planet due to the tidal coupling of the asteroid and Mars. Because of relatively very short growth time of the elliptical instability, less than 50,000 years, the asteroid was capable of retaining the elliptical instability and energizing the core dynamo for a geologically long period prior to 4 Ga. Our laboratory observations of a parametric instability of a rotating incompressible fluid, contained in a flexible-walled spherical cavity, confirm the possibility that an early Martian dynamo could have been powered by tidal straining.

Surviving utopia: Energy, social capital, and international migration in Ixcan, Guatemala

NASA Astrophysics Data System (ADS)

Taylor, Matthew John

Mounting peasant impoverishment in Guatemala comes face to face with growing ecological impoverishment. Abysmal living standards for Guatemala's majority results from highly skewed land distribution, rapid population growth, and a brutal civil war, which lasted almost four decades and laid waste to many rural communities and fields. In the face of such adversity, Guatemalans migrate to remaining forested frontiers and make longer journeys to North America in search of work. In an attempt to understand and improve natural resource use, especially firewood, I uncover how networks of social relations (social capital) and international migration influence livelihoods in agricultural communities along a forested frontier. I used both qualitative and quantitative methods to gather information about the lives of residents in four agricultural villages in Ixcan, Guatemala. The results from extended fieldwork illustrate how high levels of social capital can benefit the lives of rural residents. I argue that development programs can take advantage of existing high levels of social capital and take measures to create social capital where it is lacking to ensure the successful implementation of development programs. I also discuss firewood management in each community and demonstrate the disjuncture between local firewood use and national energy plans. Finally, I show how migrants and the money they send home from North America radically alter land use and land distribution in this part of rural Guatemala. My study reveals the need to examine the linkages between large-scale international migration, social capital, and the environment in communities that rely on the land for survival.

From Utopia to Science: Challenges of Personalised Genomics Information for Health Management and Health Enhancement

PubMed Central

2009-01-01

From 1900 onwards, scientists and novelists have explored the contours of a future society based on the use of “anthropotechnologies” (techniques applicable to human beings for the purpose of performance enhancement ranging from training and education to genome-based biotechnologies). Gradually but steadily, the technologies involved migrated from (science) fiction into scholarly publications, and from “utopia” (or “dystopia”) into science. Building on seminal ideas borrowed from Nietzsche, Peter Sloterdijk has outlined the challenges inherent in this development. Since time immemorial, and at least since the days of Plato’s Academy, human beings have been interested in possibilities for (physical or mental) performance enhancement. We are constantly trying to improve ourselves, both collectively and individually, for better or for worse. At present, however, new genomics-based technologies are opening up new avenues for self-amelioration. Developments in research facilities using animal models may to a certain extent be seen as expeditions into our own future. Are we able to address the bioethical and biopolitical issues awaiting us? After analyzing and assessing Sloterdijk’s views, attention will shift to a concrete domain of application, namely sport genomics. For various reasons, top athletes are likely to play the role of genomics pioneers by using personalized genomics information to adjust diet, life-style, training schedules and doping intake to the strengths and weaknesses of their personalized genome information. Thus, sport genomics may be regarded as a test bed where the contours of genomics-based self-management are tried out. PMID:20234832

Shared decision-making in neonatology: an utopia or an attainable goal?

PubMed

D'Aloja, Ernesto; Floris, Laura; Muller, Mima; Birocchi, Francesca; Fanos, Vassilios; Paribello, Francesco; Demontis, Roberto

2010-10-01

Medical decision making is sometimes considered as a relatively simple process in which a decision may be made by the physician, by the patient, or by both patient and physician working together. There are three main models of decision making--paternalism, patient informed choice, and shared decision-making (SDM), having each one of these drawbacks and limitations. Historically, the most adopted one was the paternalism (strongly 'Doctor knows best'), where the professional made the decision based on what he/she considered to be as the patient's best interest, not necessarily contemplating patient's will and wishes. Currently, at the antipodes, the patient informed choice, where the patient makes his/her decision based on information received from the physician with no possible interference of professional's own preferences, seems to be the preferred relationship standard. SDM represents an intermediate approach between the two above-mentioned opposite models, being a medical process that involves actively the doctor and the patient who both bring their own facts and preferences to reach an agreement on the decision on if, when and how to treat a disease. This model, being characterized by elements pertaining to both the others, is gaining popularity in several medical and surgical scenarios whenever a competent patient is able to actively participate into the decisional process. On this basis can this model be implemented also in a Neonatology Intensive Care Unit where little patients are--by nature--incompetent, being the diagnostic/therapeutic choices taken by parents? We focused on this complex item considering four possible different scenarios and it seems to us that it could be possible to introduce such an approach, providing that parents' empowerment, a good physician's communication skill and consideration of all cultural, religious, economic, and ethic values of every single actor have been fairly taken into account.

The Virtuous Circles of Clinical Information Systems: a Modern Utopia.

PubMed

Degoulet, P

2016-11-10

Clinical information systems (CIS) are developed with the aim of improving both the efficiency and the quality of care. This position paper is based on the hypothesis that such vision is partly a utopian view of the emerging eSociety. Examples are drawn from 15 years of experience with the fully integrated Georges Pompidou University Hospital (HEGP) CIS and temporal data series extracted from the data warehouses of Assistance Publique - Hôpitaux de Paris (AP-HP) acute care hospitals which share the same administrative organization as HEGP. Three main virtuous circles are considered: user satisfaction vs. system use, system use vs. cost efficiency, and system use vs quality of care. In structural equation models (SEM), the positive bidirectional relationship between user satisfaction and use was only observed in the early HEGP CIS deployment phase (first four years) but disappeared in late post-adoption (≥8 years). From 2009 to 2013, financial efficiency of 20 AP-HP hospitals evaluated with stochastic frontier analysis (SFA) models diminished by 0.5% per year. The lower decrease of efficiency observed between the three hospitals equipped with a more mature CIS and the 17 other hospitals was of the same order of magnitude than the difference observed between pediatric and non-pediatric hospitals. Outcome quality benefits that would bring evidence to the system use vs. quality loop are unlikely to be obtained in a near future since they require integration with population-based outcome measures including mortality, morbidity, and quality of life that may not be easily available. Barriers to making the transformation of the utopian part of the CIS virtuous circles happen should be overcome to actually benefit the emerging eSociety.

Joseph Conrad's tormented Rescue (fantasy).

PubMed

Freedman, William

2014-02-01

Joseph Conrad was a notoriously tormented writer for whom the creative act was often a punishment severe enough to drive him into paralyzing depressions that delayed the completion of his novels, sometimes for years. By far the most agonizing of these projects was The Rescue, a novel he began in 1898, abandoned a year later, tried unsuccessfully to continue several times over the next two decades, but was only able to resume in 1918 and to complete, after another tortured two-year struggle, in 1920. An explanation for this incapacity, that is powerfully suggested by the novel's evocative title and perhaps unintentionally ironic subtitle (A Romance of the Shallows) has not yet been explored. Using Freud's 1910 essay on the rescue fantasy, "Contributions to the Psychology of Love: A Special Type of Choice of Object Made by Men," and Emanuel Berman's instructive revision and expansion of the concept in his 2003 American Imago essay, "Ferenczi, Rescue, and Utopia," I argue that a substantial explanation for Conrad's tormented history with The Rescue is ascribable to its quite remarkably faithful treatment of a rescue fantasy with deep and disabling resonance for its author. More specifically, the difficulty was compounded by the novel's dramatization of the soul-crushing conflict between two such fantasies: one in the service of the masculine ideal of unflinching dedication to a heroic purpose, the other promising satisfaction to the equally potent demands of emotional and sexual desire. Features of Conrad's narrative fit so tightly and consistently with the theory as Freud (and Abraham) proposed and as Berman elaborated it that The Rescue offers itself as one of those rare and reinforcing instances wherein the literary text seems to validate the psychoanalytic theory at least as persuasively as the theory "understands" the text.

Improving the use of economics in animal health - Challenges in research, policy and education.

PubMed

Rushton, Jonathan

2017-02-01

The way that an economist and an animal health professional use economics differs and creates frustrations. The economist is in search of optimizing resource allocation in the management of animal health and disease problems with metrics associated with the productivity of key societal resources of labour and capital. The animal health professional have a strong belief that productivity can be improved with the removal of pathogens. These differences restrict how well economics is used in animal health, and the question posed is whether this matters. The paper explores the question by looking at the changing role of animals in society and the associated change of the animal health professional's activities. It then questions if the current allocation of scarce resources for animal health are adequately allocated for societies and whether currently available data are sufficient for good allocation. A rapid review of the data on disease impacts - production losses and costs of human reaction - indicate that the data are sparse collected in different times and geographical regions. This limits what can be understood on the productivity of the economic resources used for animal health and this needs to be addressed with more systematic collection of data on disease losses and costs of animal health systems. Ideally such a process should learn lessons from the way that human health has made estimates of the burden of diseases and their capture of data on the costs of human health systems. Once available data on the global burden of animal diseases and the costs of animal health systems would allow assessments of individual disease management processes and the productivity of wider productivity change. This utopia should be aimed at if animal health is to continue to attract and maintain adequate resources. Copyright © 2016 Elsevier B.V. All rights reserved.

Methane Seepage on Mars: Where to Look and Why

NASA Astrophysics Data System (ADS)

Oehler, Dorothy Z.; Etiope, Giuseppe

2017-12-01

Methane on Mars is a topic of special interest because of its potential association with microbial life. The variable detections of methane by the Curiosity rover, orbiters, and terrestrial telescopes, coupled with methane's short lifetime in the martian atmosphere, may imply an active gas source in the planet's subsurface, with migration and surface emission processes similar to those known on Earth as "gas seepage." Here, we review the variety of subsurface processes that could result in methane seepage on Mars. Such methane could originate from abiotic chemical reactions, thermogenic alteration of abiotic or biotic organic matter, and ancient or extant microbial metabolism. These processes can occur over a wide range of temperatures, in both sedimentary and igneous rocks, and together they enhance the possibility that significant amounts of methane could have formed on early Mars. Methane seepage to the surface would occur preferentially along faults and fractures, through focused macro-seeps and/or diffuse microseepage exhalations. Our work highlights the types of features on Mars that could be associated with methane release, including mud-volcano-like mounds in Acidalia or Utopia; proposed ancient springs in Gusev Crater, Arabia Terra, and Valles Marineris; and rims of large impact craters. These could have been locations of past macro-seeps and may still emit methane today. Microseepage could occur through faults along the dichotomy or fractures such as those at Nili Fossae, Cerberus Fossae, the Argyre impact, and those produced in serpentinized rocks. Martian microseepage would be extremely difficult to detect remotely yet could constitute a significant gas source. We emphasize that the most definitive detection of methane seepage from different release candidates would be best provided by measurements performed in the ground or at the ground-atmosphere interface by landers or rovers and that the technology for such detection is currently available.

Floating into Deep Space

NASA Astrophysics Data System (ADS)

La Frenais, R.; Saraceno, T.; Powell, J.

2014-04-01

Is it possible for spaceflight to become more sustainable? Artist and architect Tomas Saraceno proposes a long-term artscience research project based on his initial work with solar balloons to join with the efforts of engineers such as John Powell, working on the Airship to Orbit experiments, which describe a three stage process of using airships to fly to a large suborbital "Dark Sky Station' then literally floating into orbit with additional electrical and chemical propulsion. (See: http://www.jpaerospace.com) In his artworks Tomás Saraceno proposes cell-like flying cities as possible architectonic living spaces in direct reference to Buckminster Fuller's Cloud Nine (circa 1960). The fantastic architectural utopia Cloud Nine consists of a freely floating sphere measuring one mile in diameter that offers living space to several autonomous communities encompassing thousands of inhabitants each. The notion of the cloud is essential to the artist's work. The cloud as metaphor stands for artistic intention, for the meaning of territory and border in today's (urban) society, and for exploring possibilities for the sustainable development of the human living environment. In Saraceno's work this environment is not limited to the earth, but is explicitly conceived to reach into outer space. (Biomimetic Constructions- On the works of Tomás Saraceno By Katharina Schlüter) Saraceno is also interested in human factors experiments using his existing constructions as analogue environments for living on Mars and is proposing carry out a series of workshops, experiments and solar balloon launces in White Sands desert in early 2016 in collaboration with the curator Dr Rob La Frenais, the Rubin Center at The University of Texas at El Paso and various scientific partners.

Abstracts of the Annual Meeting of Planetary Geologic Mappers, San Antonio, TX, 2009

NASA Technical Reports Server (NTRS)

Bleamaster, Leslie F., III (Editor); Tanaka, Kenneth L.; Kelley, Michael S.

2009-01-01

Topics covered include: Geologic Mapping of the Beta-Atla-Themis (BAT) Region of Venus: A Progress Report; Geologic Map of the Snegurochka Planitia Quadrangle (V-1): Implications for Tectonic and Volcanic History of the North Polar Region of Venus; Preliminary Geological Map of the Fortuna Tessera (V-2) Quadrangle, Venus; Geological Map of the Fredegonde (V-57) Quadrangle, Venus; Geological Mapping of the Lada Terra (V-56) Quadrangle, Venus; Geologic Mapping of V-19; Lunar Geologic Mapping: A Preliminary Map of a Portion of the LQ-10 ("Marius") Quadrangle; Geologic Mapping of the Lunar South Pole, Quadrangle LQ-30: Volcanic History and Stratigraphy of Schr dinger Basin; Geologic Mapping along the Arabia Terra Dichotomy Boundary: Mawrth Vallis and Nili Fossae, Mars; Geologic Mapping Investigations of the Northwest Rim of Hellas Basin, Mars; Geologic Mapping of the Meridiani Region of Mars; Geology of a Portion of the Martian Highlands: MTMs -20002, -20007, -25002 and -25007; Geologic Mapping of Holden Crater and the Uzboi-Ladon-Morava Outflow System; Mapping Tyrrhena Patera and Hesperia Planum, Mars; Geologic Mapping of Athabaca Valles; Geologic Mapping of MTM -30247, -35247 and -40247 Quadrangles, Reull Vallis Region, Mars Topography of the Martian Impact Crater Tooting; Mars Structural and Stratigraphic Mapping along the Coprates Rise; Geology of Libya Montes and the Interbasin Plains of Northern Tyrrhena Terra, Mars: Project Introduction and First Year Work Plan; Geology of the Southern Utopia Planitia Highland-Lowland Boundary Plain: Second Year Results and Third Year Plan; Mars Global Geologic Mapping: About Half Way Done; New Geologic Map of the Scandia Region of Mars; Geologic Mapping of the Medusae Fossae Formation on Mars and the Northern Lowland Plains of Venus; Volcanism on Io: Insights from Global Geologic Mapping; and Planetary Geologic Mapping Handbook - 2009.

Space environment data storage and access: lessons learned and recommendations for the future

NASA Astrophysics Data System (ADS)

Evans, Hugh; Heynderickx, Daniel

2012-07-01

With the ever increasing volume of space environment data available at present and planned for the near future, the demands on data storage and access methods are increasing as well. In addition, continued access to historical, archived data remains crucial. On the basis of many years of experience, the authors identify the following issues as important for continued and efficient handling of datasets now and in the future: The huge data volumes currently or very soon avaiable from a number of space missions will limi direct Internet download access to even relatively short epoch ranges of data. Therefore, data providers should establish or extend standardised data (post-) processing services so that only data query results should be downloaded. Although a single standardised data format will in all likelihood remain utopia, data providers should at least include extensive metadata with their data products, according to established standards and practices (e.g. ISTP, SPASE). Standardisation of (sets of) metadata greatly facilitates data mining and querying. The use of SQL database storage should be considered instead of, or in parallel with, classic storage of data files. The use of SQL does away with having to handle file parsing and processing, while at the same time standard access protocols can be used to (remotely) connect to such data repositories. Many data holdings are still lacking in extensive descriptions of data provenance (e.g. instrument description), content and format. Unfortunately, detailed data information is usually rejected by scientific and technical journals. Re-processing of historical archived datasets into modern formats, making them easily available and usable, is urgently required, as knowledge is being lost. A global data directory has still not been achieved; policy makers should enforce stricter rules for "broadcasting" dataset information.

Patches of Remnant Frost/Snow on Crater Rim in Northern Summer

NASA Technical Reports Server (NTRS)

1999-01-01

March 1999--it is summer in the martian northern hemisphere, yet patches of frost or snow persist in some areas of the northern plains. Winter ended eight months earlier, in July 1998. Recently, the Mars Orbiter Camera (MOC) passed over a relatively small impact crater located at latitude 68oN (on the Vastitas Borealis plain, north of Utopia Planitia) and took the picture seen at the left, above. The curved crater rims are visible in the upper and lower quarters of the image, and the crater floor is visible at the center right.

The picture on the right is a magnified view of the crater rim area outlined by a white box in the image on the left. The bright patches are snow or frost left over from the martian winter. These snowfields are so small that a human could walk across one of them in a matter of minutes--or perhaps sled down the small, sloping patch that is seen in a shadowed area near the lower left.

In winter, the entire scene shown here would be covered by frost. The long strip at the left covers an area 3 km (1.9 mi) wide by 26 km (16 mi) long. The expanded view on the right covers an area 2.9 km (1.8 mi) by 5.3 km (3.3 mi). Illumination is from the upper right.

Malin Space Science Systems and the California Institute of Technology built the MOC using spare hardware from the Mars Observer mission. MSSS operates the camera from its facilities in San Diego, CA. The Jet Propulsion Laboratory's Mars Surveyor Operations Project operates the Mars Global Surveyor spacecraft with its industrial partner, Lockheed Martin Astronautics, from facilities in Pasadena, CA and Denver, CO.

A formational model for the polygonal terrains of Mars: Taking a crack at the genesis of the Martian polygons

NASA Technical Reports Server (NTRS)

Wenrich, M. L.; Christensen, P. R.

1993-01-01

The mechanism for the genesis of the polygonal terrains in Acidalia and Utopia Planitia has long been sought: however, no completely satisfying model was put forth that characterizes the evolution of these complexly patterned terrains. The polygons are roughly hexagonal but some are not entirely enclosed by fractures. These polygonal features range in widths from approximately 5 to 20 km. Several origins were proposed that describe the polygon borders as desiccation cracks, columnar jointing in a cooled lava, or frost-wedge features. These tension-induced cracking hypotheses were addressed by Pechmann, who convincingly disputes these mechanisms of formation based on scale magnitude difficulties and morphology. Pechmann suggests instead that the cracks delineating the 5-20-km-wide polygons on the northern plains of Mars are graben resulting from deep-seated, uniform, horizontal tension. The difficulty with this hypothesis is that no analogous polygonal forms are known to have originated by tectonism on Earth. McGill and Hills propose that the polygonal terrains on Mars resulted from either rapid desiccation of sediments or cooling of volcanics coupled with differential compaction of the material over a buried irregular topographic surface. They suggest that fracturing was enhanced over the areas of positive relief and was suppressed above the topographic lows. McGill and Hills suggest that the spacing of the topographic highs primarily controls the size of the Martian polygons and the physics of the shrinkage process is a secondary concern. Ray et. al. conducted a terrestrial study of patterned ground in periglacial areas of the U.S. to determine the process responsible for polygonal ground formation. They developed a model for polygon formation in which convection of seasonal melt water above a permafrost layer, driven by an unstable density stratification, differentially melts the permafrost interface, causing it to become undulatory.

Role of Molecular Biology in Diagnosis and Characterization of Vulvo-Vaginitis in Clinical Practice.

PubMed

Donders, Gilbert G G; Ravel, Jacques; Vitali, Beatrice; Netea, Mihai G; Salumets, Andres; Unemo, Magnus

2017-01-01

The diagnosis of vulvo-vaginal complaints has always been enigmatic in obstetrics and gynecology. Patients with clear, pathognomonic symptoms end up with a proper diagnosis and treatment most of the time, but unfortunately we are now living in a world where women reach out to the Internet and readily get all information as to which disease their symptoms correspond to and also find the appropriate treatment "over-the-counter." Because of this trend, we as specialists are increasingly confronted with patients with complex and combined conditions. At the same time, extremely sensitive and accurate diagnostic tools are now being developed at a rapid pace, allowing the physicians to diagnose vulvo-vaginal disease with a substantially increased precision. Moreover, many of these molecular biology (MB)-based tests have become so common and affordable that self-sampling and self-testing are no longer utopia. On the other hand, too much information that is too readily available and that is too affordable also encompasses pitfalls, leading to gross overtreatment and psychological burden. As experienced caregivers, we should supervise these evolutions, define their place and proper use as diagnostic tools, utilize their potential as ad hoc tools to follow-up treatment efficacy and guide how such tools can be used for responsible self-testing. In the present paper, responding to the need for appropriate, quality assured and accessible tests for vulvo-vaginitis and the huge potential delivered by the rapidly developing MB methods, we recommend the need for a broad and regular discussion forum, composed of both clinical and technical experts and opinion makers, in order to match the needs with the huge opportunities and ideally combine the initiatives and forces into the same direction. This forum should then translate conceived strategies into regularly updated, evidence-based national and international guidelines. © 2017 S. Karger AG, Basel.

Visualising biological data: a semantic approach to tool and database integration

PubMed Central

Pettifer, Steve; Thorne, David; McDermott, Philip; Marsh, James; Villéger, Alice; Kell, Douglas B; Attwood, Teresa K

2009-01-01

Motivation In the biological sciences, the need to analyse vast amounts of information has become commonplace. Such large-scale analyses often involve drawing together data from a variety of different databases, held remotely on the internet or locally on in-house servers. Supporting these tasks are ad hoc collections of data-manipulation tools, scripting languages and visualisation software, which are often combined in arcane ways to create cumbersome systems that have been customised for a particular purpose, and are consequently not readily adaptable to other uses. For many day-to-day bioinformatics tasks, the sizes of current databases, and the scale of the analyses necessary, now demand increasing levels of automation; nevertheless, the unique experience and intuition of human researchers is still required to interpret the end results in any meaningful biological way. Putting humans in the loop requires tools to support real-time interaction with these vast and complex data-sets. Numerous tools do exist for this purpose, but many do not have optimal interfaces, most are effectively isolated from other tools and databases owing to incompatible data formats, and many have limited real-time performance when applied to realistically large data-sets: much of the user's cognitive capacity is therefore focused on controlling the software and manipulating esoteric file formats rather than on performing the research. Methods To confront these issues, harnessing expertise in human-computer interaction (HCI), high-performance rendering and distributed systems, and guided by bioinformaticians and end-user biologists, we are building reusable software components that, together, create a toolkit that is both architecturally sound from a computing point of view, and addresses both user and developer requirements. Key to the system's usability is its direct exploitation of semantics, which, crucially, gives individual components knowledge of their own functionality and allows them to interoperate seamlessly, removing many of the existing barriers and bottlenecks from standard bioinformatics tasks. Results The toolkit, named Utopia, is freely available from . PMID:19534744

The Relationship Between the Origins of Life on Earth and the Possibility of Life on Other Planets: A Nineteenth-Century Perspective

NASA Astrophysics Data System (ADS)

Tirard, Stéphane

In this chapter we examine how, during the second part of the nineteenth century and the beginning of the twentieth century, assumptions about the origins of life were specifically linked to the development of theories of evolution and how these conceptions influenced assumptions about the possibility of life on other planets. First we present the theories of the origins of life of Charles Darwin (1809-1882) and Herbert Spencer (1820-1903) and underline how they were linked to the knowledge of physical and chemical conditions of environments. These two examples lead us to think about the relationship between the origin of life, evolutionary biology, and geology, particularly the uniformitarian principle. An important point is the extension of the comprehension of terrestrial conditions of emergence and evolution of life to other planets. We claim that there was a sort of extended uniformitarian principle, based not only on time, but also on space. Second, after a brief look at panspermia theory, we compare two examples of assumptions about life on other planets. The French astronomer Camille Flammarion (1842-1925) and the French biologist Edmond Perrier (1844-1921) presented views that consisted in complex analogies between life on Earth and life on other planets. We analyze how they used neo-Lamarckian biological concepts to imagine living beings in other worlds. Each planet is characterized by a particular stage of biological evolution that they deduce from the state of living beings on Earth. The two scientists explained these different states with neo-Lamarckian principles, which were based on environmental constraints on organisms. Therefore these descriptions presented a sort of history of life, including the past and the future. We claim that their assumptions could be some intellectual exercises testing neo-Lamarckian theories. Moreover the description of human beings on other planets, and particularly the Martian epianthropus presented by Perrier, were complex utopias, which finally spoke about us and about an ideal future.

The intelligence paradox; will ET get the metabolic syndrome? Lessons from and for Earth.

PubMed

Nunn, Alistair V W; Guy, Geoffrey W; Bell, Jimmy D

2014-01-01

Mankind is facing an unprecedented health challenge in the current pandemic of obesity and diabetes. We propose that this is the inevitable (and predictable) consequence of the evolution of intelligence, which itself could be an expression of life being an information system driven by entropy. Because of its ability to make life more adaptable and robust, intelligence evolved as an efficient adaptive response to the stresses arising from an ever-changing environment. These adaptive responses are encapsulated by the epiphenomena of "hormesis", a phenomenon we believe to be central to the evolution of intelligence and essential for the maintenance of optimal physiological function and health. Thus, as intelligence evolved, it would eventually reach a cognitive level with the ability to control its environment through technology and have the ability remove all stressors. In effect, it would act to remove the very hormetic factors that had driven its evolution. Mankind may have reached this point, creating an environmental utopia that has reduced the very stimuli necessary for optimal health and the evolution of intelligence - "the intelligence paradox". One of the hallmarks of this paradox is of course the rising incidence in obesity, diabetes and the metabolic syndrome. This leads to the conclusion that wherever life evolves, here on earth or in another part of the galaxy, the "intelligence paradox" would be the inevitable side-effect of the evolution of intelligence. ET may not need to just "phone home" but may also need to "phone the local gym". This suggests another possible reason to explain Fermi's paradox; Enrico Fermi, the famous physicist, suggested in the 1950s that if extra-terrestrial intelligence was so prevalent, which was a common belief at the time, then where was it? Our suggestion is that if advanced life has got going elsewhere in our galaxy, it can't afford to explore the galaxy because it has to pay its healthcare costs.

The intelligence paradox; will ET get the metabolic syndrome? Lessons from and for Earth

PubMed Central

2014-01-01

Mankind is facing an unprecedented health challenge in the current pandemic of obesity and diabetes. We propose that this is the inevitable (and predictable) consequence of the evolution of intelligence, which itself could be an expression of life being an information system driven by entropy. Because of its ability to make life more adaptable and robust, intelligence evolved as an efficient adaptive response to the stresses arising from an ever-changing environment. These adaptive responses are encapsulated by the epiphenomena of “hormesis”, a phenomenon we believe to be central to the evolution of intelligence and essential for the maintenance of optimal physiological function and health. Thus, as intelligence evolved, it would eventually reach a cognitive level with the ability to control its environment through technology and have the ability remove all stressors. In effect, it would act to remove the very hormetic factors that had driven its evolution. Mankind may have reached this point, creating an environmental utopia that has reduced the very stimuli necessary for optimal health and the evolution of intelligence – “the intelligence paradox”. One of the hallmarks of this paradox is of course the rising incidence in obesity, diabetes and the metabolic syndrome. This leads to the conclusion that wherever life evolves, here on earth or in another part of the galaxy, the “intelligence paradox” would be the inevitable side-effect of the evolution of intelligence. ET may not need to just “phone home” but may also need to “phone the local gym”. This suggests another possible reason to explain Fermi’s paradox; Enrico Fermi, the famous physicist, suggested in the 1950s that if extra-terrestrial intelligence was so prevalent, which was a common belief at the time, then where was it? Our suggestion is that if advanced life has got going elsewhere in our galaxy, it can’t afford to explore the galaxy because it has to pay its healthcare costs. PMID:25089149

Methane Seepage on Mars: Where to Look and Why

PubMed Central

Etiope, Giuseppe

2017-01-01

Abstract Methane on Mars is a topic of special interest because of its potential association with microbial life. The variable detections of methane by the Curiosity rover, orbiters, and terrestrial telescopes, coupled with methane's short lifetime in the martian atmosphere, may imply an active gas source in the planet's subsurface, with migration and surface emission processes similar to those known on Earth as “gas seepage.” Here, we review the variety of subsurface processes that could result in methane seepage on Mars. Such methane could originate from abiotic chemical reactions, thermogenic alteration of abiotic or biotic organic matter, and ancient or extant microbial metabolism. These processes can occur over a wide range of temperatures, in both sedimentary and igneous rocks, and together they enhance the possibility that significant amounts of methane could have formed on early Mars. Methane seepage to the surface would occur preferentially along faults and fractures, through focused macro-seeps and/or diffuse microseepage exhalations. Our work highlights the types of features on Mars that could be associated with methane release, including mud-volcano-like mounds in Acidalia or Utopia; proposed ancient springs in Gusev Crater, Arabia Terra, and Valles Marineris; and rims of large impact craters. These could have been locations of past macro-seeps and may still emit methane today. Microseepage could occur through faults along the dichotomy or fractures such as those at Nili Fossae, Cerberus Fossae, the Argyre impact, and those produced in serpentinized rocks. Martian microseepage would be extremely difficult to detect remotely yet could constitute a significant gas source. We emphasize that the most definitive detection of methane seepage from different release candidates would be best provided by measurements performed in the ground or at the ground-atmosphere interface by landers or rovers and that the technology for such detection is currently available. Key Words: Mars—Methane—Seepage—Clathrate—Fischer-Tropsch—Serpentinization. Astrobiology 17, 1233–1264. PMID:28771029

Viking Lander Model

NASA Technical Reports Server (NTRS)

2007-01-01

NASA's Viking Project found a place in history when it became the first mission to land a spacecraft successfully on the surface of another planet and return both imaging and non-imaging data over an extended time period. Two identical spacecraft, each consisting of a lander and an orbiter, were built. Each orbiter-lander pair flew together and entered Mars orbit; the landers then separated and descended to the planet's surface.

The Viking 1 Lander touched down on the western slope of Chryse Planitia (the Plains of Gold) on July 20, 1976, while the Viking 2 lander settled down at Utopia Planitia on September 3, 1976.

Besides taking photographs and collecting other science data on the Martian surface, the two landers conducted three biology experiments designed to look for possible signs of life. These experiments discovered unexpected and enigmatic chemical activity in the Martian soil, but provided no clear evidence for the presence of living microorganisms in soil near the landing sites. According to scientists, Mars is self-sterilizing. They believe the combination of solar ultraviolet radiation that saturates the surface, the extreme dryness of the soil and the oxidizing nature of the soil chemistry prevent the formation of living organisms in the Martian soil.

The Viking mission was planned to continue for 90 days after landing. Each orbiter and lander operated far beyond its design lifetime. Viking Orbiter 1 functioned until July 25, 1978, while Viking Orbiter 2 continued for four years and 1,489 orbits of Mars, concluding its mission August 7, 1980. Because of the variations in available sunlight, both landers were powered by radioisotope thermoelectric generators -- devices that create electricity from heat given off by the natural decay of plutonium. That power source allowed long-term science investigations that otherwise would not have been possible. The last data from Viking Lander 2 arrived at Earth on April 11, 1980. Viking Lander 1 made its final transmission to Earth November 11, 1982.

Laboratory Measurements of Oxygen Gas Release from Basaltic Minerals Exposed to UV- Radiation: Implications for the Viking Gas Exchange Experiments

NASA Astrophysics Data System (ADS)

Hurowitz, J. A.; Yen, A. S.

2007-12-01

The biology experiments onboard the Viking Landers determined that the Martian soils at Chryse and Utopia Planitia contain an unknown chemical compound of a highly oxidizing nature. The Gas Exchange Experiments (GEx) demonstrated that the humidification of a 1-cc Martian soil sample resulted in the production of as much as 790 nanomoles of oxygen gas. Yen et al. (2000) have provided experimental evidence that superoxide radicals can be generated on plagioclase feldspar (labradorite) grain surfaces by exposure to ultraviolet (UV) light in the presence of oxygen gas. Adsorbed superoxide radicals are thought to react readily with water vapor, and produce oxygen gas in quantities sufficient to explain the Viking GEx results. Direct evidence for the formation of oxygen gas, however, was not provided in the experiments of Yen et al (2000). Accordingly, the motivation of this study is to determine whether superoxide radicals adsorbed on labradorite surfaces are capable of producing oxygen gas upon exposure to water vapor. We have constructed an experimental apparatus that is capable of monitoring oxygen gas release from basaltic mineral powders that have been exposed to UV-radiation under Martian atmospheric pressure conditions. The apparatus consists of a stainless-steel vacuum chamber with a UV- transparent window where sample radiation exposures are performed. The vacuum chamber has multiple valved ports for injection of gases and water vapor. The vacuum chamber is connected via a precision leak valve to a quadrupole mass spectrometer, which measures changes in the composition of the headspace gases over our mineral samples. We will report on the results of our experiments, which are aimed at detecting and quantifying oxygen gas release from UV-exposed basaltic mineral samples using this new experimental facility. These results will further constrain whether superoxide ions adsorbed on mineral surfaces provide a viable explanation for the Viking GEx results, which have been of considerable controversy in the roughly three decades since the measurements were first made.

Methane Seepage on Mars: Where to Look and Why.

PubMed

Oehler, Dorothy Z; Etiope, Giuseppe

2017-12-01

Methane on Mars is a topic of special interest because of its potential association with microbial life. The variable detections of methane by the Curiosity rover, orbiters, and terrestrial telescopes, coupled with methane's short lifetime in the martian atmosphere, may imply an active gas source in the planet's subsurface, with migration and surface emission processes similar to those known on Earth as "gas seepage." Here, we review the variety of subsurface processes that could result in methane seepage on Mars. Such methane could originate from abiotic chemical reactions, thermogenic alteration of abiotic or biotic organic matter, and ancient or extant microbial metabolism. These processes can occur over a wide range of temperatures, in both sedimentary and igneous rocks, and together they enhance the possibility that significant amounts of methane could have formed on early Mars. Methane seepage to the surface would occur preferentially along faults and fractures, through focused macro-seeps and/or diffuse microseepage exhalations. Our work highlights the types of features on Mars that could be associated with methane release, including mud-volcano-like mounds in Acidalia or Utopia; proposed ancient springs in Gusev Crater, Arabia Terra, and Valles Marineris; and rims of large impact craters. These could have been locations of past macro-seeps and may still emit methane today. Microseepage could occur through faults along the dichotomy or fractures such as those at Nili Fossae, Cerberus Fossae, the Argyre impact, and those produced in serpentinized rocks. Martian microseepage would be extremely difficult to detect remotely yet could constitute a significant gas source. We emphasize that the most definitive detection of methane seepage from different release candidates would be best provided by measurements performed in the ground or at the ground-atmosphere interface by landers or rovers and that the technology for such detection is currently available. Key Words: Mars-Methane-Seepage-Clathrate-Fischer-Tropsch-Serpentinization. Astrobiology 17, 1233-1264.

Basin-forming impacts on Mars and the coupled thermal evolution of the interior

NASA Astrophysics Data System (ADS)

Arkani-Hamed, J.; Roberts, J. H.

2015-12-01

The youngest of the Noachian giant impact basins on Mars, are either weakly magnetized or completely demagnetized, indicating that a global magnetic field was not present and that a core dynamo was not operating at the time those basins formed. Shock heating from this sequence of basin-forming impacts modified the pattern of mantle convection. The heating produced by the eight largest impacts (Acidalia, Amazonis, Ares, Chryse, Daedalia, Hellas, Scopolus, and Utopia) penetrates below the core-mantle boundary (CMB). Here, we extend previous workon coupled thermal evolution into 3D, in order to accurately model the spatial relationship between impact basins. At the time of each impact we introduce a temperature perturbation resulting from shock heating into the core and mantle. Stratification of the core occurs very quickly compared to mantle dynamics, and we horizontally average the temperature in the core.We model mantle convection using the 3D finite element code CitcomS, and the thermal evolution of the core using a 1D parameterization.Each impact alters the pattern of mantle dynamics and a significant amount of impact melt is produced in the near surface. However, only the outermost part of the core is affected; the inner core temperature is still adiabatic. Immediately following the impact, the inner core may remain convective. The top of the core will cool by conduction into the deeper core faster than across the CMB, deepening the zone of stable stratification. Further core cooling results in formation of a convecting zone at the top of the core that propagates downwards as the thermal gradient becomes adiabatic at greater depths. Our goal is to obtain a better estimate of the time scale for restoration of post-impact core dynamo activity. Because the disappearance of the magnetic field exposes the early atmosphere to solar wind activity, constraining the history of the dynamo is critical for understanding climate evolution and habitability of the surface.

Low-Centred Polygons and Alas-Like Basins as Geological Markers of Warming Trends Late in Mars' History

NASA Astrophysics Data System (ADS)

Soare, R. J.; Conway, S. J.; Godin, E.; Osinski, G.; Hawkswell, J.; Bina, A.

2017-12-01

Expansive assemblages of low/high centred (ice-wedge) polygons and (polygonised) flat-floored thermokarst-basins (alases) are ubiquitous on Earth where the permafrost is continuous, metres to decametres-thick and ice rich, i.e. the Tuktoyaktuk Coastlands of northern Canada and the Yamal Peninsula of eastern Russia. These assemblages are geological bellwethers of transient and on occasion, long-term rises of sub-aerial and thaw-generating mean temperatures, for two principal reasons. First, high-centred (ice-wedge) polygons evolve from low-centred (ice-wedge) polygons when ice wedges that have aggraded and uplift overlying sediments above the elevation datum at the polygon centres, degrade, by thaw, and induce the loss of elevation below that datum. Second, thermokarst terrain comprises sediments whose pore volume is exceeded by the presence of water ice. A thermokarst basin (an alas) forms if and only when this ice undergoes thermal destabilisation and where thaw-generated meltwater is lost by evaporation or drainage. Spatially-associated and morphologically-similar assemblages of polygons and basins are commonplace throughout the mid-latitudes of eastern Utopia Planitia (UP), Mars. Under current conditions of extreme aridity, low atmospheric-pressure and frigid mean-temperatures, the widespread formation of ice-rich terrain by freeze-thaw cycling, let alone of near-surface ice-wedges and/or thermokarst basins, seems implausible. Against this environmental backdrop, sublimation seemingly stands alone in being able to revise ice-rich landscapes. However, multiple strands of data point to the possible periglacial-assemblages (PPAs) being youthful but not current in their formation. First, the sub-regional and dark-toned terrain incised by the PPAs is cratered more densely than would be expected. Second, the PPAs reside at a lower relative and absolute elevation than a light-toned and region-wide latitude-dependent mantle that is generally thought to be very recent in origin. These strands and others point to a earlier period in the geological history of UP, perhaps in conjunction with shifts in obliquity and eccentricity, when liquid-water would have been stable enough to sustain freeze-thaw cycling, wet periglacial processes and, derivatively, the development of the PPAs.

Document Exploration and Automatic Knowledge Extraction for Unstructured Biomedical Text

NASA Astrophysics Data System (ADS)

Chu, S.; Totaro, G.; Doshi, N.; Thapar, S.; Mattmann, C. A.; Ramirez, P.

2015-12-01

We describe our work on building a web-browser based document reader with built-in exploration tool and automatic concept extraction of medical entities for biomedical text. Vast amounts of biomedical information are offered in unstructured text form through scientific publications and R&D reports. Utilizing text mining can help us to mine information and extract relevant knowledge from a plethora of biomedical text. The ability to employ such technologies to aid researchers in coping with information overload is greatly desirable. In recent years, there has been an increased interest in automatic biomedical concept extraction [1, 2] and intelligent PDF reader tools with the ability to search on content and find related articles [3]. Such reader tools are typically desktop applications and are limited to specific platforms. Our goal is to provide researchers with a simple tool to aid them in finding, reading, and exploring documents. Thus, we propose a web-based document explorer, which we called Shangri-Docs, which combines a document reader with automatic concept extraction and highlighting of relevant terms. Shangri-Docsalso provides the ability to evaluate a wide variety of document formats (e.g. PDF, Words, PPT, text, etc.) and to exploit the linked nature of the Web and personal content by performing searches on content from public sites (e.g. Wikipedia, PubMed) and private cataloged databases simultaneously. Shangri-Docsutilizes Apache cTAKES (clinical Text Analysis and Knowledge Extraction System) [4] and Unified Medical Language System (UMLS) to automatically identify and highlight terms and concepts, such as specific symptoms, diseases, drugs, and anatomical sites, mentioned in the text. cTAKES was originally designed specially to extract information from clinical medical records. Our investigation leads us to extend the automatic knowledge extraction process of cTAKES for biomedical research domain by improving the ontology guided information extraction process. We will describe our experience and implementation of our system and share lessons learned from our development. We will also discuss ways in which this could be adapted to other science fields. [1] Funk et al., 2014. [2] Kang et al., 2014. [3] Utopia Documents, http://utopiadocs.com [4] Apache cTAKES, http://ctakes.apache.org

Giant Icebergs and Biological Productivity on Early Mars

NASA Astrophysics Data System (ADS)

Uceda, E.; Fairen, A. G.; Woodworth-Lynas, C.

2016-12-01

We have previously presented evidence for furrows, dump structures and chains of craters that we interpret as indication for giant iceberg transport and grounding on very cold oceans on early Mars, both in the northern plains and in the Hellas basin. Structures include: 1. Furrows: The furrows are located in elevated areas or on local topographic highs, particularly on the Hellas basin. We interpret these features in terms of iceberg rafting and grounding. 2. Chains of craters: High-resolution images of Utopia and Isidis Basins reveal chains of crater-like structures several hundred meters wide and 1 to 5 km long. 3. Dump structures: Dark boulder clusters are revealed at large scales by their slightly darker tonality with respect to the surrounding terrain. These clusters have sizes ranging from several hundred meters to 1-2 km. On Earth's oceans, giant icebergs release melting water containing nanoparticulate iron and other micronutrients, which support biological metabolism and growth to the near-coastal euphotic ecosystems, many of which are iron limited. This iron limitation of primary producers has been documented in large regions of the Earth's oceans, most notably in polar areas proximal to significant glacial activity, and is counterbalanced by the substantial enrichment of terrigenous material supplied by icebergs. The biological productivity extends hundreds of kilometres from the giant icebergs, and persists for over one month after the iceberg passes. Here we propose that giant iceberg activity on early Mars could have promoted a similar enhancing of biological productivity on the planet's oceans. The identification of specific biosignatures in icebergs trails on Earth could give clues as to what kind of biosignatures could be expected on the ancient Mars ocean floors, and where to look for them. In particular, assuming that life existed on Mars coeval to glacial activity, enhanced concentrations of organic carbon could be anticipated near giant iceberg trails, analogous to what is observed in polar oceans on Earth. Acknowledgements: The research leading to these results is a contribution from the Project "icyMARS", funded by the European Research Council, Starting Grant no 307496.

Pedestal Craters in Utopia Planitia and Malea Planum: Evidence for a Past Ice-Rich Substrate from Marginal Sublimation Pits.

NASA Astrophysics Data System (ADS)

Kadish, S. J.; Head, J. W.; Barlow, N. G.; Marchant, D. R.

2008-09-01

Introduction: Pedestal craters (Pd) are a subclass of impact craters unique to Mars [1] characterized by a crater perched near the center of a pedestal (mesa or plateau) that is surrounded by a quasi-circular, outward-facing scarp. The marginal scarp is usually several crater diameters from the crater rim (Figs. 2,4,5), and tens to over 100 meters above the surrounding plains (Fig. 2). Pd have been interpreted to form by armoring of the proximal substrate during the impact event. Hypotheses for the armoring mechanism include an ejecta covering [e.g., 3], increased ejecta mobilization caused by volatile substrates [4], distal glassy/melt-rich veneers [5], and/or an atmospheric blast/thermal effect [6]. Subsequently, a marginal scarp forms by preferential erosion of the substrate surrounding the armored region, most commonly thought to involve eolian removal of fine-grained, non-armored material [e.g., 3]. An understanding of the distribution of Pd, which form predominantly poleward of ~40°N and S latitude [7-9] (Fig. 1), and the role of redistribution of ice and dust during periods of climate change [e.g., 10-11], suggests that the substrate might have been volatile-rich [8-9, 12-14]. As such, some researchers [e.g., 8-9] have proposed a model for Pd formation that involves impact during periods of higher obliquity, when mid- to high-latitude substrates were characterized by thick deposits of snow and ice [e.g., 15]. Subsequent sublimation of the volatile units, except below the armored regions, yielded the perched Pd. Thus, this model predicts that thick deposits of snow/ice should underlie Pd. This is in contrast to the eolian model [3], which calls primarily for deflation of sand and dust. Here, we show the results of our study [8,16] that has documented and characterized 2461 Pd on Mars equatorward of ~65° N and S latitude (Fig. 1) in order to test these hypotheses for the origin of pedestal craters. In particular, we report on the detection of 50 Pd in Utopia Planitia and 21 Pd in Malea Planum that have pits in their marginal scarps [17]. We interpret these as sublimation pits (Fig. 3), providing evidence for snow/ice deposits preserved below the protective cover of the Pd. Marginal Pits in Pedestal Craters: Pedestal craters with marginal pits are a newly identified crater morphology in which one or more pits exist along the marginal scarp of a Pd (Figs. 2,4,5). The ejecta deposit surface (top of the pedestal) is perched ~100 m above the surrounding terrain (Fig. 2), about twice as high as a typical Pd crater. At the Pd plateau edge, the marginal scarp slopes down to the surrounding terrain, except where it is interrupted by a pit. The pits have a typical depth of ~20 m, often contain isolated mesas (Fig. 2), and are elongated, generally spanning <3 km in length (measured tangential to the pedestal margin) and <1 km in width (measured normal to the pedestal margin). In some cases, pits appear to coalesce to form larger pits (Fig. 5), and can yield a marginal, moatlike depression along a significant part of the pedestal circumference. Altimetry data from MOLA indicate that pits form in the side of the pedestal scarp; they do not extend below the elevation of the surrounding substrate (profiles in Fig. 2). Pd containing scarp pits identified thus far occur poleward of 48°N in Utopia Planitia and 58°S in Malea Planum (orange dots in Fig. 1). Pits are similar in morphology to dissected terrain [11,18] and pits on the floors of some ancient outflow channels [19], both thought to represent sublimation of an ice-rich substrate. They are also similar to formerly ice-rich and now beheaded pits in the proximal part of debris-covered glaciers on Earth [20] and Mars [21] (see also [22]). Both of the regions in which we observe Pd with marginal pits also exhibit scallop-shaped depressions, indicative of sublimation of interstitial ice [e.g. 23-25]. Climate models show that these specific regions are both predicted to have high seasonal water-ice accumulations during periods of high obliquity [26,27]. Discussion: The morphologic similarity between the marginal pits associated with Pd and ice sublimation pits leads us to favor an origin of preferential sublimation of ice/snow from the Pd scarp. In this interpretation, an impact crater forms in a thick (~10s to ~100s m) regional highlatitude deposit of ice and snow, mixed with dust. The area around the crater (the future pedestal surface) is armored by proximal ejecta and distal sintering effects of impact melt and atmospheric blast/thermal effects accompanying crater formation [5-6]. Following crater formation, obliquitydriven climate change leads to removal of the intervening snow and ice, leaving the Pd perched. Over time, the volatile-rich scarp margins, where the armoring tapers off, undergo continued sublimation to produce the pits, while the heavily armored Pd surface inhibits/prevents sublimation of underlying volatiles (Fig. 3). Ice-rich layered substrates are thus interpreted to be preserved under Pd. On the basis of our analysis, Pd represent the remnants of a past extensive, layered, climate-related deposit, similar to, but thicker than the latitude-dependent mantle emplaced in a recent ice age [11,18]. Due to the large number and widespread distribution of Pd (Fig. 1) [8,9,16], we believe that this climate-related deposit persisted for a considerable part of the recent past, implying that obliquity was relatively higher than at present during a significant portion of the Amazonian period of the history of Mars. References: [1] Barlow, N. et al. (2000) JGR, 105, 26733. [2] McCauley, J. (1973) JGR, 78, 4123. [3] Arvidson, R. (1976) Icarus, 27, 503. [4] Osinski, G. (2006) MAPS, 41, 1571. [5] Schultz, P. and Mustard, J. (2004) JGR, 109, E01001. [6] Wrobel, K. et al. (2006) MAPS, 41, 1539. [7] Mouginis-Mark, P. (1979) JGR, 84, 8011. [8] Kadish, S. and Barlow, N. (2006) LPSC 37, #1254. [9] Kadish, S. et al. (2008) LPSC 39, #1766. [10] Jakosky, B. et al. (1995) JGR, 100, 1579. [11] Head, J. et al. (2003) Nature, 426, 797. [12] Barlow, N. (2005) RVAMIC, #3041. [13] Head, J. and Roth, R. (1976) LSI, 50-52. [14] Schultz, P. and Lutz, A. (1988) Icarus, 73, 91. [15] Levrard, B. et al. (2004) Nature, 431, 1072. [16] Kadish, S. et al. (2008) JGR, in progress. [17] Kadish, S. et al. (2008) GRL, in progress. [18] Mustard, J. et al. (2001) Nature, 412, 411. [19] Levy, J. and Head, J. (2005) Terra Nova, 17, 503. [20] Marchant, D. and Head, J. (2007) Icarus, 192, 187. [21] Head, J. and Marchant, D. (2008) Workshop on Martian Gullies, #8009. [22] Moore, J. et al. (1996) Icarus, 122, 63. [23] Lefort, A. et al. (2006) 4th Mars Polar Science Conf., #8061. [24] Zanetti, M. et al. (2008) LPSC 39, 1682. [25] Morgenstern, A. et al. (2007) JGR, 112, E06010. [26] Forget, F. et al. (2006) Science, 311, 368-371. [27] Madeleine, B. et al. (2007) LPSC 38, #1778.

MOLA Topography of Impact Basins in the Northern Hemisphere of Mars

NASA Technical Reports Server (NTRS)

Frey, Herbert; Sakimoto, S. E. H.; Roark, J. H.

1998-01-01

Coverage of the northern hemisphere of Mars by the Mars Orbiter Laser Altimeter (MOLA) during the aerobraking hiatus and the two Science Phasing Operation periods provides improved definition and characterization of large impact basins. Gridded MOLA data show the Utopia Basin has a pronounced bowl-like structure, as opposed to the interior rises suggested by the earlier USGS DEM. The elevation structure is concentric about the basin center as mapped by McGill. In particular, the proposed inner ring closely follows the -4 km contour over much of the southern, western and northwestern sides. Higher topography along portions of the dichotomy boundary aligns with the basin's outer ring. High topography in the polar region also occurs where the outer ring should lie, raising the possibility that perhaps some of the polar topography is due to basin structure as well as ice. Two MOLA passes near Phison Rupes provide evidence for a large "stealth" hole where Viking imagery show little evidence of any major structure. The 2 km deep, 600 km wide depression at 31OW, 3ON is as large as the Cassini impact basin 1000 km to the SW. While Cassini is easily recognized in image data, the "MOLA Hole" is not. If this depression is a deeply eroded and buried impact basin (as perhaps suggested by a decrease in the crater density and somewhat smoother terrain than in adjacent areas), it is not clear why it has managed to maintain its great depth. In Tempe at the dichotomy boundary a 300 km wide impact basin is revealed by pronounced bowl-like topography centered at 87W, 47N, even though only about 1/3 of the basin rim structure is obvious. The basin lies on a sloping boundary zone, with the more buried N rim up to 2 km below the rugged S rim. A similar N-S asymmetry in basin ring structure occurs for the much larger Isidis Basin, where the S rim rises 6 km but the subdued N rim rises barely 2 km above the floor. There is essentially no topographic expression of the main ring in the NE quadrant of Isidis where, if it exists, it lies below Hesperian-age plains.

Identifying congenital hearing impairment. Personal experience based on selective hearing screening.

PubMed

Molini, E; Ricci, G; Baroni, S; Ciorba, A; Bellocci, A; Simoncelli, C

2004-06-01

If all degrees of permanent uni- or bilateral hypoacusis are taken into consideration, hearing impairment is the most common congenital disease. Early detection of permanent infantile hearing impairment has become extremely important in preventive medicine, since steps can be taken with hearing aids and rehabilitation to ensure better development of language and higher cognitive functions. Aim of this study is to provide a critical review of the time of diagnosis of hypoacusis at our audiology laboratory, where two methods were used to screen hearing of children with/without risk indicators. Results of approximately 10 years' work were re-examined during which time outpatient screening was conducted on children referred by colleagues in neonatology and paediatrics. All were carriers of congenital risk indicators associated with sensorineural and/or conductive hearing loss, based on the Joint Committee on Infant Hearing findings, or were suspected of being hypoacusic even if they had no known congenital risk factors. Hearing screening was conducted in hospital on newborns with no risk factors, within the first few days of birth. Results of the present study showed that when selective hearing screening was performed, the mean age of high-risk patients diagnosed with hypoacusis was slightly higher than that in international guidelines. Moreover, these patients represent approximately half the hypoacusic population identified in the study period. The other half of congenital hypoacusic subjects identified had no risk indicators and there was a significant delay in diagnosis due to later manifestation of symptoms indicating hypoacusis, and thus, in turn, delayed referral for hearing tests. In contrast, subjects without risk indicators who underwent in-hospital hearing screening and proved to be hypoacusic, were diagnosed early. In our experience, however, universal screening has considerable disadvantages, such as difficulty in covering the entire population, difficulty in follow-up after discharge from hospital, and last, but by no means least, significant organisational and professional commitments, making it impossible to perform in all hospitals. In order to ensure effective hearing screening for congenital hearing loss and, thus permit prompt identification of hypoacusic children, use of hearing aids and rehabilitation screening should incorporate two aspects. First, selection should be compulsory, thereby reducing waiting time between collecting case histories and performing outpatient tests; second, hospital screening of children without risk factors should be performed whenever possible. Integrating these two aspects would make it possible to approach the "utopia" of universal hearing screening.

Clastic polygonal networks around Lyot crater, Mars: Possible formation mechanisms from morphometric analysis

NASA Astrophysics Data System (ADS)

Brooker, L. M.; Balme, M. R.; Conway, S. J.; Hagermann, A.; Barrett, A. M.; Collins, G. S.; Soare, R. J.

2018-03-01

Polygonal networks of patterned ground are a common feature in cold-climate environments. They can form through the thermal contraction of ice-cemented sediment (i.e. formed from fractures), or the freezing and thawing of ground ice (i.e. formed by patterns of clasts, or ground deformation). The characteristics of these landforms provide information about environmental conditions. Analogous polygonal forms have been observed on Mars leading to inferences about environmental conditions. We have identified clastic polygonal features located around Lyot crater, Mars (50°N, 30°E). These polygons are unusually large (>100 m diameter) compared to terrestrial clastic polygons, and contain very large clasts, some of which are up to 15 metres in diameter. The polygons are distributed in a wide arc around the eastern side of Lyot crater, at a consistent distance from the crater rim. Using high-resolution imaging data, we digitised these features to extract morphological information. These data are compared to existing terrestrial and Martian polygon data to look for similarities and differences and to inform hypotheses concerning possible formation mechanisms. Our results show the clastic polygons do not have any morphometric features that indicate they are similar to terrestrial sorted, clastic polygons formed by freeze-thaw processes. They are too large, do not show the expected variation in form with slope, and have clasts that do not scale in size with polygon diameter. However, the clastic networks are similar in network morphology to thermal contraction cracks, and there is a potential direct Martian analogue in a sub-type of thermal contraction polygons located in Utopia Planitia. Based upon our observations, we reject the hypothesis that polygons located around Lyot formed as freeze-thaw polygons and instead an alternative mechanism is put forward: they result from the infilling of earlier thermal contraction cracks by wind-blown material, which then became compressed and/or cemented resulting in a resistant fill. Erosion then leads to preservation of these polygons in positive relief, while later weathering results in the fracturing of the fill material to form angular clasts. These results suggest that there was an extensive area of ice-rich terrain, the extent of which is linked to ejecta from Lyot crater.

Mars: the evolutionary history of the northern lowlands based on crater counting and geologic mapping

USGS Publications Warehouse

Werner, S.C.; Tanaka, K.L.; Skinner, J.A.

2011-01-01

The geologic history of planetary surfaces is most effectively determined by joining geologic mapping and crater counting which provides an iterative, qualitative and quantitative method for defining relative ages and absolute model ages. Based on this approach, we present spatial and temporal details regarding the evolution of the Martian northern plains and surrounding regions. The highland–lowland boundary (HLB) formed during the pre-Noachian and was subsequently modified through various processes. The Nepenthes Mensae unit along the northern margins of the cratered highlands, was formed by HLB scarp-erosion, deposition of sedimentary and volcanic materials, and dissection by surface runoff between 3.81 and 3.65 Ga. Ages for giant polygons in Utopia and Acidalia Planitiae are ~ 3.75 Ga and likely reflect the age of buried basement rocks. These buried lowland surfaces are comparable in age to those located closer to the HLB, where a much thinner, post-HLB deposit is mapped. The emplacement of the most extensive lowland surfaces ended between 3.75 and 3.4 Ga, based on densities of craters generally View the MathML source> 3 km in diameter. Results from the polygonal terrain support the existence of a major lowland depocenter shortly after the pre-Noachian formation of the northern lowlands. In general, northern plains surfaces show gradually younger ages at lower elevations, consistent local to regional unit emplacement and resurfacing between 3.6 and 2.6 Ga. Elevation levels and morphology are not necessarily related, and variations in ages within the mapped units are found, especially in units formed and modified by multiple geological processes. Regardless, most of the youngest units in the northern lowlands are considered to be lavas, polar ice, or thick mantle deposits, arguing against the ocean theory during the Amazonian Period (younger than about 3.15 Ga). All ages measured in the closest vicinity of the steep dichotomy escarpment are also 3.7 Ga or older. The formation ages of volcanic flanks at the HLB (e.g., Alba Mons (3.6–3.4 Ga) and the last fan at Apollinaris Mons, 3.71 Ga) may give additional temporal constraint for the possible existence of any kind of Martian ocean before about 3.7 Ga. It seems to reflect the termination of a large-scale, precipitation-based hydrological cycle and major geologic processes related to such cycling.

Abstracts of the Annual Meeting of Planetary Geologic Mappers, Flagstaff, AZ, 2010

NASA Technical Reports Server (NTRS)

Bleamaster, Leslie F., III (Editor); Tanaka, Kenneth L. (Editor); Kelley, Michael S. (Editor)

2010-01-01

Topics covered include: Detailed Analysis of the Intra-Ejecta Dark Plains of Caloris Basin, Mercury; The Formation and Evolution of Tessera and Insights into the Beginning of Recorded History on Venus: Geology of the Fortuna Tessera Quadrangle (V-2); Geologic Map of the Snegurochka Planitia Quadrangle (V-1): Implications for the Volcanic History of the North Polar Region of Venus; Geological Map of the Fredegonade (V-57) Quadrangle, Venus: Status Report; Geologic Mapping of V-19; Geology of the Lachesis Tessera Quadrangle (V-18), Venus; Comparison of Mapping Tessera Terrain in the Phoebe Regio (V-41) and Tellus Tessera (V-10) Quadrangles; Geologic Mapping of the Devana Chasma (V-29) Quadrangle, Venus; Geologic Mapping of the Aristarchus Plateau Region on the Moon; Geologic Mapping of the Lunar South Pole Quadrangle (LQ-30); The Pilot Lunar Geologic Mapping Project: Summary Results and Recommendations from the Copernicus Quadrangle; Geologic Mapping of the Nili Fossae Region of Mars: MTM Quadrangles 20287, 20282, 25287, 25282, 30287, and 30282; Geologic Mapping of the Mawrth Vallis Region, Mars: MTM Quadrangles 25022, 25017, 25012, 20022, 20017, and 20012; Evidence for an Ancient Buried Landscape on the NW Rim of Hellas Basin, Mars; New Geologic Map of the Argyre Region of Mars: Deciphering the Geologic History Through Mars Global Surveyor, Mars Odyssey, and Mars Express Data; Geologic Mapping in the Hesperia Planum Region of Mars; Geologic Mapping of the Meridiani Region of Mars; Geologic Mapping in Southern Margaritifer Terra; Geology of -30247, -35247, and -40247 Quadrangles, Southern Hesperia Planum, Mars; The Interaction of Impact Melt, Impact-Derived Sediment, and Volatiles at Crater Tooting, Mars; Geologic Map of the Olympia Cavi Region of Mars (MTM 85200): A Summary of Tactical Approaches; Geology of the Terra Cimmeria-Utopia Planitia Highland Lowland Transitional Zone: Final Technical Approach and Scientific Results; Geology of Libya Montes and the Interbasin Plains of Northern Tyrrhena Terra, Mars: First Year Results and Second Year Work Plan; Mars Global Geologic Mapping Progress and Suggested Geographic-Based Hierarchal Systems for Unit Grouping and Naming; Progress in the Scandia Region Geologic Map of Mars; Geomorphic Mapping of MTMS -20022 and -20017; Geologic Mapping of the Medusae Fossae Formation, Mars, and the Northern Lowland Plains, Venus; Volcanism on Io: Results from Global Geologic Mapping; Employing Geodatabases for Planetary Mapping Conduct - Requirements, Concepts and Solutions; and Planetary Geologic Mapping Handbook - 2010.

Location and Geologic Setting for the Three U.S. Mars Landers

NASA Technical Reports Server (NTRS)

Parker, T. J.; Kirk, R. L.

1999-01-01

Super resolution of the horizon at both Viking landing sites has revealed "new" features we use for triangulation, similar to the approach used during the Mars Pathfinder Mission. We propose alternative landing site locations for both landers for which we believe the confidence is very high. Super resolution of VL-1 images also reveals some of the drift material at the site to consist of gravel-size deposits. Since our proposed location for VL-2 is NOT on the Mie ejecta blanket, the blocky surface around the lander may represent the meter-scale texture of "smooth palins" in the region. The Viking Lander panchromatic images typically offer more repeat coverage than does the IMP on Mars Pathfinder, due to the longer duration of these landed missions. Sub-pixel offsets, necessary for super resolution to work, appear to be attributable to thermal effects on the lander and settling of the lander over time. Due to the greater repeat coverage (particularly in the near and mid-fields) and all-panchromatic images, the gain in resolution by super resolution processing is better for Viking than it is with most IMP image sequences. This enhances the study of textural details near the lander and enables the identification rock and surface textures at greater distances from the lander. Discernment of stereo in super resolution im-ages is possible to great distances from the lander, but is limited by the non-rotating baseline between the two cameras and the shorter height of the cameras above the ground compared to IMP. With super resolution, details of horizon features, such as blockiness and crater rim shapes, may be better correlated with Orbiter images. A number of horizon features - craters and ridges - were identified at VL-1 during the misison, and a few hils and subtle ridges were identified at VL-2. We have added a few "new" horizon features for triangulation at the VL-2 landing site in Utopia Planitia. These features were used for independent triangulation with features visible in Viking Orbiter and MGS MOC images, though the actual location of VL-1 lies in a data dropout in the MOC image of the area. Additional information is contained in the original extended abstract.

Mapping the northern plains of Mars: origins, evolution and response to climate change

NASA Astrophysics Data System (ADS)

Balme, Matthew; Conway, Susan; Costard, François; Gallagher, Colman; van Gasselt, Stephan; Hauber, Ernst; Johnsson, Andreas; Kereszturi, Akos; Platz, Thomas; Ramsdale, Jason; Reiss, Dennis; Séjourné, Antoine; Skinner, James; Swirad, Zuzanna

2014-05-01

An ISSI (International Space Science Institute) international team has been convened to study the Northern Plain of Mars. The northern plains are extensive, geologically young, low-lying areas that contrast in age and relief to Mars' older, heavily cratered, southern highlands. Mars' northern plains are characterised by a wealth of landforms and landscapes that have been inferred to be related to the presence of ice or ice-rich material near, beneath, or at the surface. Such landforms include 'scalloped' pits and depressions, polygonally-patterned grounds, and viscous flow features similar in form to terrestrial glacial or ice-sheet landforms. Furthermore, new (within the last few years) impact craters have exposed ice in the northern plains, and spectral data from orbiting instruments have revealed the presence of tens of percent by weight of water within the upper most ~50 cm of the martian surface at high latitudes. The northern plains comprise three linked zones: Acidalia Planitia, Utopia Planitia and Arcadia Planitia. Each region consists of a shallow basin, with the three areas are separated by low topographic divides. Our aim is to study the ice-related geomorphology of each region in order to understand the origins, evolution and response to climate change of ice on Mars. In particular, by comparing and contrasting the three separate basins we hope to determine if the processes that created the ice-related terrains are regional (perhaps basin limited) or global in scope, and whether the differing geology of each basin has an effect on the ice-related features observed there. The ISSI team is using planetary geomorphological mapping to meet this aim. Three long strips, each about 250 km wide and spanning the ~30N to ~80N latitude range have been defined and sub-teams are each mapping a single area. The group contains experts in mapping, GIS and crater counting (details in the size-frequency distribution of impact craters on a planetary surface can reveal information about when terrains were emplaced, modified, eroded or exhumed). The first meeting of this group was held in December 2013. Here, we give an overview of the science aims of the project, describe the main difference between the three strips and report on mapping work done so far.

A standards-based formative evaluation of a national professional development program for science teachers

NASA Astrophysics Data System (ADS)

Raphael, Carol Greco

2002-09-01

The 1996 National Science Education Standards provided educators and policy makers with a major impetus for constructive change in science education. The Standards not only specified what science content should be taught, but also provided organization for future science curricula. A major theme that pervades the Standards is that the classroom teacher is the most important component of classroom change and that reform efforts should be directed at improving the teaching of science through professional development for science teachers. In response to the National Science Education Standards, the Science Teachers Organization (pseudonym) prepared a professional development program for science teachers that was intended to acquaint teachers with the Standards and bring about reform of science teaching by changing teachers' instructional strategies and procedures. This program, named Preparing Schools for Science (PSS), was designed for use in all of the 50 states, but was first introduced in a southwestern state referred to as Utopia in this dissertation. Using the Provus Method of Discrepancy Evaluation, a design and installation audit of the Preparing Schools for Science Program was performed. Suggestions for program improvement, as well as a complete evaluation design for the PSS Program, were presented. Specific program modifications suggested by the research included an improved organization of personnel to monitor and supervise the program, more sustained professional development workshops, a stronger network of support for teachers. Five major implications for future professional development programs emerge from this research. (1) A needs analysis should be conducted before a program is designed in order to ensure that the program meet the needs of those for whom it is intended. (2) The length and type of training are the most important factors in ensuring that teachers have sufficient time to incorporate and learn how to use new ideas. (3) Additional personnel are needed to conduct the training and follow-up with the Points of Contact (POCs) in the Program. (4) Financial support for the Key Leaders who serve as trainers of the points of contact is needed to provide the means for the key leaders to fully implement the program and maintain contact with the POCs. (5) The program should have a thorough and well-planned evaluation design, and data collection should be done in a timely fashion by a skilled evaluator.

Prevention of strong earthquakes: Goal or utopia?

NASA Astrophysics Data System (ADS)

Mukhamediev, Sh. A.

2010-11-01

In the present paper, we consider ideas suggesting various kinds of industrial impact on the close-to-failure block of the Earth’s crust in order to break a pending strong earthquake (PSE) into a number of smaller quakes or aseismic slips. Among the published proposals on the prevention of a forthcoming strong earthquake, methods based on water injection and vibro influence merit greater attention as they are based on field observations and the results of laboratory tests. In spite of this, the cited proofs are, for various reasons, insufficient to acknowledge the proposed techniques as highly substantiated; in addition, the physical essence of these methods has still not been fully understood. First, the key concept of the methods, namely, the release of the accumulated stresses (or excessive elastic energy) in the source region of a forthcoming strong earthquake, is open to objection. If we treat an earthquake as a phenomenon of a loss in stability, then, the heterogeneities of the physicomechanical properties and stresses along the existing fault or its future trajectory, rather than the absolute values of stresses, play the most important role. In the present paper, this statement is illustrated by the classical examples of stable and unstable fractures and by the examples of the calculated stress fields, which were realized in the source regions of the tsunamigenic earthquakes of December 26, 2004 near the Sumatra Island and of September 29, 2009 near the Samoa Island. Here, just before the earthquakes, there were no excessive stresses in the source regions. Quite the opposite, the maximum shear stresses τmax were close to their minimum value, compared to τmax in the adjacent territory. In the present paper, we provide quantitative examples that falsify the theory of the prevention of PSE in its current form. It is shown that the measures for the prevention of PSE, even when successful for an already existing fault, can trigger or accelerate a catastrophic earthquake because of dynamic fault propagation in the intact region. Some additional aspects of prevention of PSE are discussed. We conclude that in the near future, it is too early to consider the problem of prevention of a forthcoming strong earthquake as a practical task; otherwise, the results can prove to be very different from the desired ones. Nevertheless, it makes sense to continue studying this problem. The theoretical research and experimental investigation of the structure and properties of the regions where the prevention of a forthcoming strong earthquake is planned in the future are of primary importance.

Martian subsurface properties and crater formation processes inferred from fresh impact crater geometries

NASA Astrophysics Data System (ADS)

Stewart, Sarah T.; Valiant, Gregory J.

2006-10-01

The geometry of simple impact craters reflects the properties of the target materials, and the diverse range of fluidized morphologies observed in Martian ejecta blankets are controlled by the near-surface composition and the climate at the time of impact. Using the Mars Orbiter Laser Altimeter (MOLA) data set, quantitative information about the strength of the upper crust and the dynamics of Martian ejecta blankets may be derived from crater geometry measurements. Here, we present the results from geometrical measurements of fresh craters 3-50 km in rim diameter in selected highland (Lunae and Solis Plana) and lowland (Acidalia, Isidis, and Utopia Planitiae) terrains. We find large, resolved differences between the geometrical properties of the freshest highland and lowland craters. Simple lowland craters are 1.5-2.0 times deeper (≥5σo difference) with >50% larger cavities (≥2σo) compared to highland craters of the same diameter. Rim heights and the volume of material above the preimpact surface are slightly greater in the lowlands over most of the size range studied. The different shapes of simple highland and lowland craters indicate that the upper ˜6.5 km of the lowland study regions are significantly stronger than the upper crust of the highland plateaus. Lowland craters collapse to final volumes of 45-70% of their transient cavity volumes, while highland craters preserve only 25-50%. The effective yield strength of the upper crust in the lowland regions falls in the range of competent rock, approximately 9-12 MPa, and the highland plateaus may be weaker by a factor of 2 or more, consistent with heavily fractured Noachian layered deposits. The measured volumes of continuous ejecta blankets and uplifted surface materials exceed the predictions from standard crater scaling relationships and Maxwell's Z model of crater excavation by a factor of 3. The excess volume of fluidized ejecta blankets on Mars cannot be explained by concentration of ejecta through nonballistic emplacement processes and/or bulking. The observations require a modification of the scaling laws and are well fit using a scaling factor of ˜1.4 between the transient crater surface diameter to the final crater rim diameter and excavation flow originating from one projectile diameter depth with Z = 2.7. The refined excavation model provides the first observationally constrained set of initial parameters for study of the formation of fluidized ejecta blankets on Mars.

The effect of giant impactors on the magnetic field energy of an early Martian dynamo.

NASA Astrophysics Data System (ADS)

Drummond, McGregor; Thieulot, Cedric; Monteux, Julien

2016-04-01

Through the cratering record embedded on its surface, Mars is one of the key planets required for investigating the formation and impact frequency in the early history of our Solar System. This record also holds clues to the events that may have caused the observed hemispheric dichotomy and cessation of the magnetic field that was present within the first 500 Myr of the planets' formation. We investigate the influence of giant impacts on the early Martian dynamo using the numerical dynamo modelling code PARODY-JA [1]. We hypothesize that the input heat from a giant impact will decrease the total heat flux at the CMB through mantle heating which leads to a decrease in the Rayleigh number of the core. As boundary conditions for the heat flux anomaly size, we use numerical results of a 750 km diameter impactor from the Monteux and Arkani-Hamed, 2014 [2] study which investigated impact heating and core merging of giant impacts in early Mars. We also determine the decrease in Rayleigh number from the change in total heat flux at the CMB using these results, where the decrease after impact is due to shock heating at the CMB. We calculate the time-averaged total magnetic field energy for an initial homogeneous heat flux model using a range of Rayleigh numbers (5 x 103 - 1 x 10^5). The Rayleigh number is then decreased for three new models - homogeneous, north pole impact and equatorial impact - and the time-averaged energy again determined. We find that the energy decreases more in our impact models, compared with the homogeneous, along with a variation in energy between the north pole and equatorial impact models. We conclude that giant impacts in Mars' early history would have decreased the total magnetic energy of the field and the decrease in energy is also dependent on the location of the impact. The magnetic field could have been disrupted beyond recovery from a planetesimal-sized collision; such as the suggested Borealis basin forming impact, or through the cumulative effect of multiple large impactors; such as Utopia, Hellas and Isidis basin forming impacts. [1] Aubert, J., Aurnou, J. & Wicht, J., 2008. The magnetic structure of convection-driven numerical dynamos. Geophys. J. Int., 172, 945--956. [2] Monteux, J., Arkani-Hamed, J., 2014. Consequences of giant impacts in early Mars: core merging and Martian dynamo evolution. J. Geophys. Res. (Planets) 119, 480--505.

Geologic history of the polar regions of Mars based on Mars Global survey data. I. Noachian and Hesperian Periods

USGS Publications Warehouse

Tanaka, K.L.; Kolb, E.J.

2001-01-01

During the Noachian Period, the south polar region of Mars underwent intense cratering, construction of three groups of volcanoes, widespread contractional deformation, resurfacing of low areas, and local dissection of valley networks; no evidence for polar deposits, ice sheets, or glaciation is recognized. South polar Hesperian geology is broadly characterized by waning impacts, volcanism, and tectonism. Emplacement of the polar Dorsa Argentea Formation (DAF) occurred during the Hesperian Period. Mars Orbiter Laser Altimeter topographic data and Mars Orbiter Camera images elucidate stratigraphic, morphologic, and topographic relations, permitting the dividing of the DAF into eight members, which surround and underlie about half of the Amazonian south polar layered deposits. The lobate fronts and lack of typical volcanic-flow morphology of the six plains units indicate that they may be made up of debris flows. We think that these flows, tens of meters to 200 m thick, may have originated by the discharge of huge volumes of slurry fluidized by ground water or liquid CO2, perhaps triggered by local impacts, igneous activity, or basal melting beneath polar deposits. The cavi and rugged members include irregular depressions that penetrate the subsurface; some of the pits have raised rims. The depressions may have formed by collapse due to expulsion of subsurface material in which local explosive activity built up the raised rims. Further, smaller eruptions of volatile-rich material may have resulted in narrow, sinuous channel deposits within aggrading fine-grained unconsolidated material perhaps produced by gaseous discharge of subsurface volatiles; preferential erosion of the latter material could have produced the Dorsa Argentea-type ginuous ridges associated mainly with the DAF. Alternatively, the ridges may be eskers, but the lack of associated glacial and fluvial morphologies casts doubt on this interpretation. The knobby, degraded materials forming Scandia Colles may represent the only Noachian geologic record exposed in the north polar region. Most of the north polar region was buried by water- or debris-ocean sediments during the Hesperian Period, originating from uplands areas and perhaps knobby terrains in the northern plains. The sediments either mantle or were deformed by wrinkle ridges radial and concentric to Utopia basin and concentric to northern Tharsis. Sources of stress probably included sediment loading in the northern plains and regional magmatic and loading activity at Tharsis. Polar layered deposits began piling up during the Early Amazonian or later. ?? 2001 Elsevier Science.

Geologic History of the Polar Regions of Mars Based on Mars Global Surveyor Data. I. Noachian and Hesperian Periods

NASA Astrophysics Data System (ADS)

Tanaka, Kenneth L.; Kolb, Eric J.

2001-11-01

During the Noachian Period, the south polar region of Mars underwent intense cratering, construction of three groups of volcanoes, widespread contractional deformation, resurfacing of low areas, and local dissection of valley networks; no evidence for polar deposits, ice sheets, or glaciation is recognized. South polar Hesperian geology is broadly characterized by waning impacts, volcanism, and tectonism. Emplacement of the polar Dorsa Argentea Formation (DAF) occurred during the Hesperian Period. Mars Orbiter Laser Altimeter topographic data and Mars Orbiter Camera images elucidate stratigraphic, morphologic, and topographic relations, permitting the dividing of the DAF into eight members, which surround and underlie about half of the Amazonian south polar layered deposits. The lobate fronts and lack of typical volcanic-flow morphology of the six plains units indicate that they may be made up of debris flows. We think that these flows, tens of meters to 200 m thick, may have originated by the discharge of huge volumes of slurry fluidized by ground water or liquid CO 2, perhaps triggered by local impacts, igneous activity, or basal melting beneath polar deposits. The cavi and rugged members include irregular depressions that penetrate the subsurface; some of the pits have raised rims. The depressions may have formed by collapse due to expulsion of subsurface material in which local explosive activity built up the raised rims. Further, smaller eruptions of volatile-rich material may have resulted in narrow, sinuous channel deposits within aggrading fine-grained unconsolidated material perhaps produced by gaseous discharge of subsurface volatiles; preferential erosion of the latter material could have produced the Dorsa Argentea-type sinuous ridges associated mainly with the DAF. Alternatively, the ridges may be eskers, but the lack of associated glacial and fluvial morphologies casts doubt on this interpretation. The knobby, degraded materials forming Scandia Colles may represent the only Noachian geologic record exposed in the north polar region. Most of the north polar region was buried by water- or debris-ocean sediments during the Hesperian Period, originating from uplands areas and perhaps knobby terrains in the northern plains. The sediments either mantle or were deformed by wrinkle ridges radial and concentric to Utopia basin and concentric to northern Tharsis. Sources of stress probably included sediment loading in the northern plains and regional magmatic and loading activity at Tharsis. Polar layered deposits began piling up during the Early Amazonian or later.

Surface Changes in Chryse Planitia

NASA Technical Reports Server (NTRS)

1979-01-01

At the conclusion of the Viking Continuation Mission (May to November, 1978), all four cameras on the Viking Landers - two on each spacecraft - continued to function normally. During the two and one-half years since the landers touched down on Mars, images totaled 2,255 for Viking Lander 1 and 2,016 for Viking Lander 2. The surface around the landers was completely photographed by the end of 1976; subsequent images acquired during 1977-1978 have concentrated on searching for changes in the scene - changes which can be used to infer both the types of erosive processes which modify the landscape around the landers and the rates at which these processes may occur. The major surface changes have included the water-ice snow seen by Lander 2 during the winter at Utopia Planitia, and a thin dust layer deposited at both sites during the dust storms of 1977. The most recently identified change occurred at Chryse Planitia between VL-1 sols 767 (Sept. 16, 1978) and 771 (Sept. 20, 1978) as seen in the lower photo. Picture at top, selected to show similar lighting conditions, was taken during sol 25 (August 15, 1976). The change (A) appears as a small circle-like formation on the side of a drift in the lee, or downwind, side of Whale Rock. This is believed to have been a small-scale landslide of an unstable dust layer which had accumulated behind the rock. Interpretation of this feature would be difficult without an earlier change (B) near Big Joe, a slump which occurred between sols 74 and 183. The new slump is approximately 25- 35 meters from the lander, and just under a meter across. The slumping probably was initiated by the daily heating and cooling of the surface by solar radiation. More importantly, it is now believed that, based on the repeated occurrence of such slumping features, a dust layer which overlies the surface may in fact be redistributed fairly regularly during periods of high wind activity. There are no obvious indications of fossil slump features, therefore similar features must be destroyed on a regular basis. After the end of February, when Viking operations essentially terminate, Lander 1 will continue preselected observations over a period of possibly up to 10 years, following the instructions stored in its computer memory. Earth commands will be required only to initiate data transmission to Earth. During this time, it is now anticipated that one of the yearly planetwide global dust storms may reach an intensity necessary to shift the dust cover around the lander significantly.

Chryse Planitia, Mars: Topographic configuration, outflow channel continuity and sequence, and tests for hypothesized ancient bodies of water using Mars Orbiter Laser Altimeter (MOLA) data

NASA Astrophysics Data System (ADS)

Ivanov, M. A.; Head, J. W.

2001-02-01

Many of the largest and most prominent outflow channels on Mars debouch into Chryse Planitia. Pre-Mars Global Surveyor topographic data show Chryse to be a closed depression almost 2000 km in diameter. New Mars Orbiter Laser Altimeter (MOLA) data reveal the following: (1) Chryse is not a locally closed basin but instead opens into the North Polar basin. (2) The highly distinctive morphology of the six largest predominantly Hesperian-aged channels (Kasei, Maja, Simud, Tiu, Ares, and Mawrth) disappears into the northern lowlands at average elevations that all occur within less than ~170 m of a mean elevation of -3742(SD=153m), over a lateral distance in excess of 2500 km. (3) The elevations where the distinctive morphology of each channel disappears all fall within ~190 m of Contact 2, a boundary mapped by Parker et al. [1993] and interpreted to represent an ancient shoreline, and the mean elevation values of Contact 2 and circum-Chryse channel termini fall within 18 m of each other. In contrast, the termini of seven later Amazonian-aged channels emerging from Elysium into Utopia Planitia are spread over a vertical range of >1500 m. (4) Topographic evidence of the continuation of some of the outflow channels can be observed for distances of 250-450 km into the North Polar basin, but the morphology is subdued and distinctly different. (5) The nature of this less distinctive topography and its crosscutting relationships show that Simud and Tiu are likely to represent the youngest activity (specifically crosscutting Ares Valles). (6) The distinctive change in channel morphology is consistent with rapid loss of energy encountered at base level (subaerial/submarine boundary) and emplacement into a shallow submarine environment. Channel characteristics, lack of distinctive deltas or lobes, and continuation of subdued channel morphology suggest hyperpychnal flow and the possibility of density/turbidity currents. Estimates of the volumes of individual channel events are wide-ranging. The minimum volume estimates of Carr [1996] suggest that 46 such events would be required to fill the basin to the level of Contact 2 and thus that the channels may have emptied into an existing standing body of water. Volume estimates of Baker et al. [1991] assume that single individual events may have filled the basin to the level of Contact 2, thus requiring significant water loss between events and refilling during subsequent events to essentially the same level. In both end-member cases these observations are consistent with the presence of large standing bodies of water in the northern lowlands in Hesperian-Early Amazonian times.

Abstracts of the Annual Meeting of Planetary Geologic Mappers, Flagstaff, AZ, 2008

NASA Technical Reports Server (NTRS)

Bleamaster, Leslie F., III (Editor); Tanaka, Kenneth L. (Editor); Kelley, Michael S. (Editor)

2008-01-01

Topics discussed include: Merging of the USGS Atlas of Mercury 1:5,000,000 Geologic Series; Geologic Mapping of the V-36 Thetis Regio Quadrangle: 2008 Progress Report; Structural Maps of the V-17 Beta Regio Quadrangle, Venus; Geologic Mapping of Isabella Quadrangle (V-50) and Helen Planitia, Venus; Renewed Mapping of the Nepthys Mons Quadrangle (V-54), Venus; Mapping the Sedna-Lavinia Region of Venus; Geologic Mapping of the Guinevere Planitia Quadrangle of Venus; Geological Mapping of Fortuna Tessera (V-2): Venus and Earth's Archean Process Comparisons; Geological Mapping of the North Polar Region of Venus (V-1 Snegurochka Planitia): Significant Problems and Comparisons to the Earth's Archean; Venus Quadrangle Geological Mapping: Use of Geoscience Data Visualization Systems in Mapping and Training; Geologic Map of the V-1 Snegurochka Planitia Quadrangle: Progress Report; The Fredegonde (V-57) Quadrangle, Venus: Characterization of the Venus Midlands; Formation and Evolution of Lakshmi Planum (V-7), Venus: Assessment of Models using Observations from Geological Mapping; Geologic Map of the Meskhent Tessera Quadrangle (V-3), Venus: Evidence for Early Formation and Preservation of Regional Topography; Geological Mapping of the Lada Terra (V-56) Quadrangle, Venus: A Progress Report; Geology of the Lachesis Tessera Quadrangle (V-18), Venus; Geologic Mapping of the Juno Chasma Quadrangle, Venus: Establishing the Relation Between Rifting and Volcanism; Geologic Mapping of V-19, V-28, and V-53; Lunar Geologic Mapping Program: 2008 Update; Geologic Mapping of the Marius Quadrangle, the Moon; Geologic Mapping along the Arabia Terra Dichotomy Boundary: Mawrth Vallis and Nili Fossae, Mars: Introductory Report; New Geologic Map of the Argyre Region of Mars; Geologic Evolution of the Martian Highlands: MTMs -20002, -20007, -25002, and -25007; Mapping Hesperia Planum, Mars; Geologic Mapping of the Meridiani Region, Mars; Geology of Holden Crater and the Holden and Ladon Multi-Ring Impact Basins, Margaritifer Terra, Mars; Geologic Mapping of Athabasca Valles; Geologic Mapping of MTM -30247, -35247 and -40247 Quadrangles, Reull Vallis Region of Mars; Geologic Mapping of the Martian Impact Crater Tooting; Geology of the Southern Utopia Planitia Highland-Lowland Boundary Plain: First Year Results and Second Year Plan; Mars Global Geologic Mapping: Amazonian Results; Recent Geologic Mapping Results for the Polar Regions of Mars; Geologic Mapping of the Medusae Fossae Formation on Mars (MC-8 SE and MC-23 NW) and the Northern Lowlands of Venus (V-16 and V-15); Geologic Mapping of the Zal, Hi'iaka, and Shamshu Regions of Io; Global Geologic Map of Europa; Material Units, Structures/Landforms, and Stratigraphy for the Global Geologic Map of Ganymede (1:15M); and Global Geologic Mapping of Io: Preliminary Results.

Relevant in times of turmoil: WHO and public health in unstable situations.

PubMed

Loretti, A; Leus, X; Van Holsteijn, B

2001-01-01

For millions of people world-wide, surviving the pressure of extreme events is the predominant objective in daily existence. The distinction between natural and human-induced disasters is becoming more and more blurred. Some countries have known only armed conflict for the last 25 years, and their number is increasing. Recently, humanitarian sources reported 24 ongoing emergencies, each of them involving at least 300,000 people "requiring international assistance to avoid malnutrition or death". All together, including the countries still only at risk and those emerging from armed conflicts, 73 countries, i.e., almost 1.8 trillion people, were undergoing differing degrees of instability. Instability must be envisioned as a spectrum extending between "Utopia" and "Chaos". As emergencies bring forward extreme challenges to human life, medical and public health ethics make it imperative for the World Health Organisation (WHO) to be involved. As such, WHO must enhance its presence and effectiveness in its capacity as a universally accepted advocate for public health. Furthermore, as crises become more enmeshed with the legitimacy of the State, and armed conflicts become more directed against countries' social capital, they impinge more on WHO's work, and WHO must reconcile its unique responsibility in the health sector, the humanitarian imperative and the mandate to assist its primary constituents. Health can be viewed as a bridge to peace. The Organization specifically has recognised that disasters can and do affect the achievement of health and health system objectives. Within WHO, the Department of Emergency and Humanitarian Action (EHA) is the instrument for intervention in such situations. The scope of EHA is defined in terms of humanitarian action, emergency preparedness, national capacity building, and advocacy for humanitarian principles. The WHO's role is changing from ensuring a two-way flow of information on new scientific developments in public health in the ideal all-stable, all-equitable, well-resourced state, to dealing with sheer survival when the state is shattered or is part of the problem. The WHO poses itself the explicit goals to reduce avoidable loss of life, burden of disease and disability in emergencies and post-crisis transitions, and to ensure that the Humanitarian Health Assistance is in-line with international standards and local priorities and does not compromise future health development. A planning tree is presented. The World Health Organization must improve its own performance. This requires three key pre-conditions: 1) presence; 2) surge capacity; and 3) institutional support, knowledge, and competencies. Thus, in order to be effective, WHO's presence and surge capacity in emergencies must integrate the institutional knowledge, the competencies, and the managerial set-up of the Organization.

Late Hesperian plains formation and degradation in a low sedimentation zone of the northern lowlands of Mars

USGS Publications Warehouse

Rodriguez, J.A.P.; Tanaka, K.L.; Berman, D.C.; Kargel, J.S.

2010-01-01

The plains materials that form the martian northern lowlands suggest large-scale sedimentation in this part of the planet. The general view is that these sedimentary materials were transported from zones of highland erosion via outflow channels and other fluvial systems. The study region, the northern circum-polar plains south of Gemini Scopuli on Planum Boreum, comprises the only extensive zone in the martian northern lowlands that does not include sub-basin floors nor is downstream from outflow channel systems. Therefore, within this zone, the ponding of fluids and fluidized sediments associated with outflow channel discharges is less likely to have taken place relative to sub-basin areas that form the other northern circum-polar plains surrounding Planum Boreum. Our findings indicate that during the Late Hesperian sedimentary deposits produced by the erosion of an ancient cratered landscape, as well as via sedimentary volcanism, were regionally emplaced to form extensive plains materials within the study region. The distribution and magnitude of surface degradation suggest that groundwater emergence from an aquifer that extended from the Arabia Terra cratered highlands to the northern lowlands took place non-catastrophically and regionally within the study region through faulted upper crustal materials. In our model the margin of the Utopia basin adjacent to the study region may have acted as a boundary to this aquifer. Partial destruction and dehydration of these Late Hesperian plains, perhaps induced by high thermal anomalies resulting from the low thermal conductivity of these materials, led to the formation of extensive knobby fields and pedestal craters. During the Early Amazonian, the rates of regional resurfacing within the study region decreased significantly; perhaps because the knobby ridges forming the eroded impact crater rims and contractional ridges consisted of thermally conductive indurated materials, thereby inducing freezing of the tectonically controlled waterways associated with these features. This hypothesis would explain why these features were not completely destroyed. During the Late Amazonian, high-obliquity conditions may have led to the removal of large volumes of volatiles and sediments being eroded from Planum Boreum, which then may have been re-deposited as thick, circum-polar plains. Transition into low obliquity ~5. myr ago may have led to progressive destabilization of these materials leading to collapse and pedestal crater formation. Our model does not contraindicate possible large-scale ponding of fluids in the northern lowlands, such as for example the formation of water and/or mud oceans. In fact, it provides a complementary mechanism involving large-scale groundwater discharges within the northern lowlands for the emplacement of fluids and sediments, which could have potentially contributed to the formation of these bodies. Nevertheless, our model would spatially restrict to surrounding parts of the northern plain either the distribution of the oceans or the zones within these where significant sedimentary accumulation would have taken place. ?? 2010 Elsevier Inc.

Mapping Mars' northern plains: origins, evolution and response to climate change - a new overview of recent ice-related landforms in Acidalia Planitia.

NASA Astrophysics Data System (ADS)

Hauber, Ernst; Orgel, Csilla; van Gasselt, Stephan; Reiss, Dennis; Johnsson, Andreas; Ramsdale, Jason; Balme, Matthew; Conway, Susan; Costard, Francois; Gallagher, Colman; Kereszturi, Akos; Platz, Thomas; Séjourné, Antoine; Skinner, James; Swirad, Zuzanna; Łosiak, Anna

2015-04-01

An International Space Science Institute (ISSI) team project has been convened to study the northern plains of Mars. It uses a geomorphological grid-mapping approach to compare ice-related landforms across N-S traverses in the three main basins of the northern plains: Acidalia, Arcadia, and Utopia Planitiae. The main science questions are (i) the distribution of ice-related landforms in the northern plains and their relation to distinct latitude bands or different geological units, (ii) the relationship between the latitude dependent mantle (LDM) and landforms indicative of ground ice, and (iii) the distributions and associations of recent landforms indicative of thaw of ice or snow. We mapped individual landforms across the Acidalia Planitia that may have been formed in association with ice or water in an attempt to determine their extent and identify possible spatial relationships and genetic links between them. Our list includes mantling deposits, small-scale polygons, gullies, viscous flow features, thumbprint terrain (TPT), giant polygons and large pitted mounds (LPM). Our resulting maps show the distribution of specific landforms (no data - absence - presence - dominance) in grid cells with a size of ~20 × 20 km, but allows also for some ambiguity (possible). Preliminary results show that the mantling deposits are ubiquitous and occur basically everywhere between ~43°N and almost the margin of the north polar cap. As their surface may appear smooth if intact, their texture can be difficult to detect at CTX scale. Gullies were observed within a limited latitude range between ~32°N and ~54°N. They predominantly occur in Acidalia and Acidalia Colles, although gullies were found in several impact craters. Small-scale polygons occur between ~60°N to ~70°N in agreement with previous studies. They are predominantly oriented in orthogonal networks in crater interiors, depressions and on plains. Viscous flow features are present only in higher-relief areas of the Acidalia Mensae and Colles. Their morphology is not well pronounced, partially subdued and covered, and most features are restricted to debris aprons distributed circumferentially around small knobs. TPT appears north of about 30°N in the most distal parts of the Chryse outflow channels and shows a transition zone with LPM at around 36°N and it is not observed north of ~39N°. The giant polygons with the LPM have been considered analogous to fluid expulsion features in terrestrial sedimentary basins. They characterize the study area from to 35 N° until 61 N° and completely disappear in the Acidalia Colles region. Grid mapping proved to be an efficient way to map small-scale landforms over wide areas. The distribution of possible ice- and water-related features in Acidalia is clearly latitude- and topography-dependent

Direct current hybrid breakers: A design and its realization

NASA Astrophysics Data System (ADS)

Atmadji, Ali Mahfudz Surya

2000-12-01

The use of semiconductors for electric power circuit breakers instead of conventional breakers remains a utopia when designing fault current interrupters for high power networks. The major problems concerning power semiconductor circuit breakers are the excessive heat losses and their sensitivity to transients. However, conventional breakers are capable of dealing with such matters. A combination of the two methods, or so-called `hybrid breakers', would appear to be a solution; however, hybrid breakers use separate parallel branches for conducting the main current and interrupting the short-circuit current. Such breakers are intended for protecting direct current (DC) traction systems. In this thesis hybrid switching techniques for current limitation and purely solidstate current interruption are investigated for DC breakers. This work analyzes the transient behavior of hybrid breakers and compares their operations with conventional breakers and similar solid-state devices in DC systems. Therefore a hybrid breaker was constructed and tested in a specially designed high power test circuit. A vacuum breaker was chosen as the main breaker in the main conducting path; then a commutation path was connected across the vacuum breaker where it provided current limitation and interruption. The commutation path operated only during any current interruption and the process required additional circuits. These included a certain energy storage, overvoltage suppressor and commutation switch. So that when discharging this energy, a controlled counter-current injection could be produced. That counter-current opposed the main current in the breaker by superposition in order to create a forced current-zero. One-stage and two-stage commutation circuits have been treated extensively. This study project contains both theoretical and experimental investigations. A direct current shortcircuit source was constructed capable of delivering power equivalent to a fault. It supplied a direct voltage of 1kVDC which was rectified having been obtained from a 3-phase lOkV/380V supply. The source was successfully tested to deliver a fault current of 7kA with a time constant of 5ms. The hybrid breaker that was developed could provide protection for 750VDC traction systems. The breaker was equipped with a fault- recognizing circuit based on a current level triggering. An electronic circuit was built for this need and was included in the system. It monitored the system continuously and took action by generating trip signals when a fault was recognized. Interruption was followed by a suitable timing of the fast contact separation in the main breaker and the current-zero creation. An electrodynamically driven mechanism was successfully tested having a dead-time of 300μs to separate the main breaker contacts. Furthermore, a maximum peak current injection of RA at a frequency of 500Hz could be obtained in order to produce an artificial current-zero in the vacuum breaker. A successful current interruption with a prospective value of RA was achieved by the hybrid switching technique. In addition, measures were taken to prevent overvoltages. Experimentally, the concept of a hybrid breaker was compared with the functioning of all mechanical (air breaker) and all electronical (IGCT breaker) versions. Although a single stage interrupting method was verified experimentally, two two-stage interrupting methods were analyzed theoretically.

Distribution, origin and evolution of hypothesized mud volcanoes, thumbprint terrain, small mounds and giant polygons: Implications for sedimentary processes in the northern lowlands of Mars: Case study from the Acidalia Planitia.

NASA Astrophysics Data System (ADS)

Orgel, Csilla; Hauber, Ernst; van Gasselt, Stephan; Pozzobon, Riccardo; Skinner, James, Jr.

2016-04-01

This study is part of the activities of an ISSI International Team, which intends to produce new geomorphological maps of the northern lowlands of Mars along three long traverses across Acidalia, Utopia, and Arcadia Planitiae [1]. This specific study focuses on mounds of different sizes: Large Pitted Mounds (LPM), Thumbprint Terrain (TPT), Small Mounds (SM) as well as km-sized, giant polygons (GP) [2,3]. These landforms were formed on the Vastitas Borealis Formation (VBF) Marginal and Interior Units, which are interpreted as outflow channel deposits or sediments of a hypothesized ocean. The aim of our study is to map the above mentioned features in the northern lowlands and establish a formational history and stratigraphy of landforms using morphological observations and geostatistics in Acidalia Planitia. Our study is based on CTX mosaics (6 m/pixel) and we also used data from HiRISE (0.25 m/px), HRSC (images >10 m/px, HRSC- derived Digital Elevation Models [DEM], grid size 50-200 m), MOLA DEM (~460 m/px), and THEMIS Nighttime IR (~100 m/px). The TPT appears north of about 30°N in the termination zones of the Chryse outflow channels and shows a transition zone with the LPMs at around 36°N in Acidalia Planitia. North of 39°N, only LPM can be observed. LPM are typically surrounded by topographic moats. Sometimes more than 75% of a mound can be covered or embayed by "plain filling material" of varying thickness. The LPM are observed in the same area as large-scale polygon troughs (buried and fresh) associated with circular-shaped small mounds (SM). The SM are located from 34°N to 48°N, completely overlapping the area of LPM and partly the TPT. These features are randomly distributed, but commonly arranged in clusters. Their domical shape with the central pit shows morphological resemblance with the LPM. These features characterize the area from 35 N° to 61 N° and completely disappear in the Acidalia Colles region. The mapping results show a morphological transition zone of the TPT into the LPM in the Acidalia Planitia. It varies by latitude and may be related to the distance from the circum-Chryse outflow channel and the thickening of sediments towards Acidalia Planitia. We find observational evidence for complete or partial sedimentary burial of LPM as well as polygon troughs by a viscous flow material. This material shows flow fronts, suggesting an emplacement by multiple viscous processes [4,5]. We established a new approach of the detailed sequence of the origin of the main four landforms (LPM, TPT, SM, GP) using morphological analysis and geostatistics in combining the results of the previous studies [4,5]. References: [1] Ramsdale, J. et al. (2015) 46th LPSC, Abstract # 1339. [2] Frey, H. and Jarosewich, M. (1982) J. Geophys. Res. 87, B12, 9867-9879. [3] Oehler, D.Z. and Allen, C.C. (2010) Icarus 208, 636-657. [4] Skinner et al. (2008) XXXIX LPSC, Abstract # 2418. [5] Salvatore, M. R. and Christensen, P. R. (2014) JGR Planets, doi: 10.1002/2014JE004682.

Stratigraphical evidence of late Amazonian periglaciation and glaciation in the Astapus Colles region of Mars

NASA Astrophysics Data System (ADS)

Soare, Richard J.; Osinski, Gordon R.

2009-07-01

Recent modeling of the meteorological conditions during and following times of high obliquity suggests that an icy mantle could have been emplaced in western Utopia Planitia by atmospheric deposition during the late Amazonian period [Costard, F.M., Forget, F., Madeleine, J.B., Soare, R.J., Kargel, J.S., 2008. Lunar Planet. Sci. 39. Abstract 1274; Madeleine, B., Forget, F., Head, J.W., Levrard, B., Montmessin, F., 2007. Lunar Planet. Sci. 38. Abstract 1778]. Astapus Colles (ABa) is a late Amazonian geological unit - located in this hypothesized area of accumulation - that comprises an icy mantle tens of meters thick [Tanaka, K.L., Skinner, J.A., Hare, T.M., 2005. US Geol. Surv. Sci. Invest., Map 2888]. For the most part, this unit drapes the early Amazonian Vastitas Borealis interior unit (ABvi); to a lesser degree it overlies the early Amazonian Vastitas Borealis marginal unit (ABvm) and the early to late Hesperian UP plains unit HBu2 [Tanaka, K.L., Skinner, J.A., Hare, T.M., 2005. US Geol. Surv. Sci. Invest., Map 2888]. Landscapes possibly modified by late-Amazonian periglacial processes [Costard, F.M., Kargel, J.S., 1995. Icarus 114, 93-112; McBride, S.A., Allen, C.C., Bell, M.S., 2005. Lunar Planet. Sci. 36. Abstract 1090; Morgenstern, A., Hauber, E., Reiss, D., van Gasselt, S., Grosse, G., Schirrmeister, L., 2007. J. Geophys. Res. 112, doi:10.1029/2006JE002869. E06010; Seibert, N.M., Kargel, J.S., 2001. Geophys. Res. Lett. 28, 899-902; Soare, R.J., Kargel, J.S., Osinski, G.R., Costard, F., 2007. Icarus 191, 95-112; Soare, R.J., Osinski, G.R., Roehm, C.L., 2008. Earth Planet. Sci. Lett. 272, 382-393] and glacial processes [Milliken, R.E., Mustard, J.F., Goldsby, D.L., 2003. J. Geophys. Res. 108 (E6), doi:10.1029/2002JE002005. 5057; Mustard, J.F., Cooper, C.D., Rifkin, M.K., 2001. Nature 412, 411-414; Tanaka, K.L., Skinner, J.A., Hare, T.M., 2005. US Geol. Surv. Sci. Invest., Map 2888] have been reported within the region. Researchers have assumed that the periglacial and glacial landscapes occur within the same geological unit, the ABa [i.e., Morgenstern, A., Hauber, E., Reiss, D., van Gasselt, S., Grosse, G., Schirrmeister, L., 2007. J. Geophys. Res. 112; doi:10.1029/2006JE002869. E06010; Tanaka, K.L., Skinner, J.A., Hare, T.M., 2005. US Geol. Surv. Sci. Invest., Map 2888]. In this study we use HiRISE (High Resolution Image Science Experiment, Mars Reconnaissance Orbiter) imagery to identify the stratigraphical separation of the two landscapes and show that periglacial landscape modification has occurred in the geological units that underlie the ABa, not in the ABa itself. Moreover, we suggest that the periglacial landscape extends well beyond the perimeter of the ABa and could be the product of "wet" cold-climate processes. These processes involve freeze-thaw cycles and intermittently stable liquid-water at or near the surface. By contrast, we propose that the ABa is a very recent late-Amazonian geological unit formed principally by "dry" cold-climate processes. These processes comprise accumulation (by atmospheric deposition) and ablation (by sublimation).

Abstracts of the Annual Meeting of Planetary Geologic Mappers, Tucson, AZ 2007

USGS Publications Warehouse

Gregg, Tracy K.P.; Tanaka, Kenneth L.; Saunders, R. Stephen; Bleamaster, Leslie F.

2007-01-01

Introduction Report of the Annual Mappers Meeting Planetary Science Institute Tucson, Arizona June 28 and 29, 2007 Approximately 22 people attended this year's mappers meeting, and many more submitted abstracts and maps in absentia. The 2007 meeting was convened by Tracy Gregg, Les Bleamaster, Steve Saunders, and Ken Tanaka and was hosted by David Crown and Les Bleamaster of the Planetary Science Institute (PSI) in Tucson, Arizona. Oral presentations and poster discussions took place on Thursday, June 28 and Friday, June 29. This year's meeting also included a unique opportunity to visit the operations centers of two active Mars missions; field trips to the University of Arizona took place on Thursday and Friday afternoons. Outgoing Geologic Mapping Subcommittee (GEMS) chairperson, Tracy Gregg, commenced the meeting with an introduction and David Crown followed with a discussion of logistics and the PSI facility; Steve Saunders (Planetary Geology and Geophysics Discipline Scientist) then provided a brief program update. Science presentations kicked off with Venus mapper Vicki Hansen and graduate students Eric Tharalson and Bhairavi Shankar of the University of Minnesota, Duluth, showing a 3-D animation of the global distribution of tesserae and discussing the implications, a progress report for V-45 quadrangle mapping, and a brief discussion of circular lows. Les Bleamaster (PSI) followed with a progress report on mapping of the V-50 quadrangle and the 1:10M Helen Planitia quadrangle. David Crown (PSI) concluded the Venus presentations with a discussion of progress made on the V-30 quadrangle. The remainder of Thursday's presentations jumped around the Solar System including Mars, Io, and Earth. Ken Tanaka of the U.S. Geological Survey (USGS) began the afternoon with a general discussion of the status of the planetary mapping program at USGS. Buck Janes (University of Arizona) provided background information about the Mars Odyssey Gamma Ray Spectrometer (GRS) and presented some new element maps, which may be useful for geologic mapping. Dave Williams of Arizona State University reported on the progress of his global Io map and James Dohm (University of Arizona) discussed results of terrestrial remote mapping studies. Thursday afternoon, the mappers were given a tour of the High Resolution Imaging Science Experiment (HiRISE) operations facility and were given some basic information about how the images are obtained, processed, and publicly released. With official GEMS transition completed at lunch on Thursday, incoming GEMS chair Leslie Bleamaster took the reigns of Friday's meeting. Science presentations began with Ken Tanaka discussing 1:20M-scale global and 1:2M-scale polar mapping of Mars. Jim Zimbelman (Smithsonian Institution) described his 1:1M Medusae Fossae map (MC-8 SE), which is nearing completion, and new mapping (MC-16 NW and MC-23 NW) to further evaluate the Medusae Fossae. Brent Garry, also of the Smithsonian Institution, presented work on Ascraeus Mons. Peter Mouginis-Mark (University of Hawai`i) reported progress on his 1:200K and larger maps of Tooting crater and of the Olympus Mons summit caldera. Laszlo Keszthelyi (USGS) presented mapping of Athabasca Valles, with much of the credit going to Windy Jaeger. Jim Skinner (USGS) introduced a new mapping project including nine MTM quadrangles in the Utopia Planitia region. Tracy Gregg finished off the day's science presentations with discussion of Hesperia Planum. After discussion was complete, the group once again traveled to the University of Arizona - this time for a tour of the Mars Phoenix operations center. Principal Investigator Peter Smith beamed as he led mappers through the multi-million dollar facility. A main topic of discussion throughout the entire meeting was that of nomenclature, specifically how to classify the individual depressions at the tops of volcanoes. Paterae, as has been used for Mars, Venus, and Io, was suggested, but i

[Calmette Hospital, Phnom Penh, Cambodia. Assessment of the implementation of the Medical Information System (SIM). Global analysis of the 1998 results].

PubMed

Fabre-Teste, B; Sokha, O

1999-01-01

Calmette is a national university hospital with 220 adult beds. It has emergency, surgical, medical and gynecology and obstetrics departments, along with a radiology unit, a laboratory for medical analyses, a central pharmacy and an outpatient clinic. This hospital has an unusual statute, with managerial autonomy and a system of cost recovery that currently provides 64% of the hospital's income. Since 1994, it has benefited from a French cooperation program. The French NGO, Médecins du Monde, has been present at Calmette since 1990, providing support for , the indigent sector of the medical department. The aim of the Medical Information System (SIM) is to develop a simple, reliable and reproducible system so that, for every action undertaken at the hospital (hospitalization, day hospital and outpatient clinic) the following pieces of information are recorded: 1) the disease; 2) the type of patient; 3) the type of management; 4) the means used to treat the patient; 5) the cost. Data are collected and analyzed using programs created with EPIINFO software (CDC, WHO), using the EPIGLUE module. In 1998, 10,814 admissions were recorded at Calmette Hospital, 7,811 (72.2%) of which were to the Emergency Department and 3,003 (27.2%) of which were direct admissions to other wards. We analyzed 10,603 (95%) computerized medical summaries (RMI). About 50% of beds were occupied in the maternity and gynecology ward whereas almost 90% of beds were occupied in the surgical and emergency wards. AIDS and tuberculosis were the conditions most frequently treated by the medical department, despite a marked increase in more specialized areas of medicine such as cardiology and diabetology. The surgical department reflected the concentration on emergency services of the hospital, with cranial traumatism the primary reason for admission for the hospital as a whole. The mean age of patients was 27 years for the maternity ward and 49 years for the medicine A ward. The mortality rate was about 5% for the medical wards (mainly due to AIDS) and almost 50% in the emergency department (cerebrovascular neurologic disease, cranial traumatism). The proportion of nonpaying patients was high (about 40% in terms of stays in hospital and about 50% of all days spent in hospital). The training of a Cambodian manager for the SIM is a key priority. The point of the SIM is to use the treated data it produces to improve management and decision-making. The data it produces should be used to define the profile of the patients treated, both from a medical point of view and in terms of their ability to pay. This is a fundamental step towards identifying activities that should receive priority as part of a development strategy for a structure evolving in a highly competitive environment. The SIM data are also invaluable for the short-term management of the hospital through the contribution they make to the development of effective analytical accounting, making it possible to evaluate costs and to adjust charges appropriately. Finally, the involvement of the SIM in the setting up and functioning of the Comité de Lutte Contre les Infections Nosocomiales (CLIN; the Hospital-Acquired Infections Committee) in 1999 to 2000 is not utopia, it is the logical continuation of improvements in the overall quality of care It involves, in particular, the training of nurses and head nurses, initiated by nurses acting as technical assistants in the French cooperation program. The definition of the role of the hygiene nurse and the selection of such a nurse from the trained head nurses are also part of this process.

Physical properties of the surface materials at the Viking landing sites on Mars

USGS Publications Warehouse

Moore, H.J.; Hutton, R.E.; Clow, G.D.; Spitzer, C.R.

1987-01-01

This report summarizes the results of the Physical Properties Investigation of the Viking '75 Project, activities of the surface samplers, and relevant results from other investigations. The two Viking Landers operated for nearly four martian years after landing on July 20 (Lander 1) and Sept. 3 (Lander 2), 1976; Lander 1 acquired its last pictures on or about Nov. 5, 1982. Lander 1 rests on a smooth, cratered plain at the west edge of Chryse Planitia (22.5 ? N, 48.0? W), and Lander 2 rests 200 km west of the crater Mie in Utopia Planitia (48.0? N, 225.7? W). Lander 1 views showed that dune-like deposits of drift material were superposed on rock-strewn surfaces. Soil-like material from the rock-strewn areas was called blocky material. Lander 2 views also showed a rock-strewn surface. Polygonal to irregular features, etched by the wind, revealed crusty to cloddy material among rocks. Both landers descended to the surface along nearly vertical trajectories. Velocities at touchdown were about 2 m/s for both landers. Footpad 2 of Lander 1 penetrated drift material 0.165 m, and footpad 3 penetrated blocky material 0.036 m. The two visible footpads of Lander 2 struck rocks. Erosion by exhausts from the forward engines produced craters with rims of mixed fine-grained material and platy to equidimensional clods, crusts, and fragments. Comparison of engine-exhaust erosion on Mars with terrestrial data suggested that drift material behaved like a weakly cohesive material with a grain size less than 3-9 /-lm. Although not sand, blocky and crusty to cloddy materials eroded like sand-with grain sizes of 0.01 or 0.2 cm. The surface samplers accomplished an impressive number of tasks. All experiments that required samples received samples. Deep holes, as much as 0.22 m deep, were excavated by both landers. Lander 2 successfully pushed rocks and collected samples from areas originally beneath the rocks. Tasks specifically accomplished for the Physical Properties Investigation include: (1) acquiring motor-current data while excavating trenches, (2) performing surface-bearing tests, (3) performing backhoe touchdowns, (4) attempting to chip or scratch rocks, (5) comminuting samples, (6) measuring subsurface diurnal temperatures, and (7) constructing conical piles of materials on and among rocks. Sample trenches in the three major types of soil-like materials were different from one another. Trenches in drift material, which were typically 0.06 m deep, had steep walls along much of their lengths, lumpy tailings and floors, and smooth domed surfaces with sparse fine fractures around their tips. Trenches in blocky material, which were typically 0.03-0.04 m deep, had steep walls near their tips, and surfaces around their tips were displaced upward and some appeared blocky. Trenches in crusty to cloddy material, which were typically 0.04-0.05 m deep, had steep and often irregular slopes near their tips, clods and slabs of crust in their tailings, and disrupted areas around their tips composed of mixed fine-grained material and slabs of crust or thick polygonal clods that had been displaced upwards. Data acquired during landing, trenching, surface-bearing tests, backhoe touchdowns, and from other science experiments were used to determine the mechanical properties of drift, blocky, and crusty to cloddy materials. Drift material appeared to be very fine grained, with local planes of weakness; in general, the drift material was consistent with a material having an angle of internal friction about 18?, a cohesion ranging from 0.7 to 3.0 kPa, and a bulk density of 1,200 kg/m 3 . Blocky material was consistent with a material having an angle of internal friction about 30?, cohesions from 1.5 to 16 kPa, and a bulk density of 1,600 kg/m 3 . Crusty to cloddy material had variable properties. For chiefly crusty to cloddy material, angles of internal friction were about 35 ? , and cohesions were from 0.5 to 5.2 kPa. For mixed fines and crusts, a

Preliminary results of the search for possible Martian landing sites to be considered for future European exploration missions

NASA Astrophysics Data System (ADS)

Martin, P.

2007-08-01

The recently adopted European Space Policy aims at expanding and coordinating the role and activities of Europe's space actors with the purpose of increasing both scientific knowledge in selected space domains and the European presence in the Solar System, as well as optimising the relevant societal benefits. With our Moon and in particular Mars as primary targets of exploration goals for the Solar System, and following a number of very successful orbital missions performing detailed remote sensing and mapping of these planetary bodies, probe landings on the surface of the Moon and Mars represent the next stepping stone of the exploration of our close planetary environment. Along with developing the hardware capabilities required for Europe to reach such ambitious goals, it therefore becomes increasingly important to pinpoint with precision a number of landing sites well suited for the safety and scientific success of future robotic missions. Focusing on Mars, and although a number of candidate landing sites and associated catalogs with available scientific justification already exist, the results being obtained by orbiters such as Mars Express and Mars Reconnaissance Orbiter are fundamentally transforming our knowledge of the planet's surface, which in turns highlights the need to review, update and revise the candidate sites for future landing missions on Mars. Detailed investigations of possible future Martian landing sites for European missions are ongoing, based on the wealth of scientific data and high-resolution mapping products available. In order to support the identification of suitable sites, various mapping products (geological, hyperspectral and compositional) can be consolidated, and various areas of Mars identified in the recent scientific literature as primary targets for landing can be taken into account for further, refined assessment of their suitability for landing. Seasonal and climatic effects potentially influencing landing shall also be considered, as well as lessons learned from past landing experiences. Finally, nolanding zones shall be identified based on a number of available criteria. A preliminary investigation and classification of potential landing sites for future European Mars exploration missions is summarised here, with the assumed following general requirements: • Moderate latitudes (e.g., 15ºS to 45ºN). Such a latitude range would be suitable for Exomars. • Low-to-moderate elevation (e.g., below 2000 m) • Relatively flat surface in the landing ellipse (e.g., slopes < 15º) • Low-to-moderate rock abundance (e.g., < 20%) • Moderate thermal inertia (rock/dust abundance) • Suitability to overriding scientific goals and targets of interest (e.g., niches of extant life, olivine sites, or sites where phyllosilicates or hydrated sulfates were identified) • Other constraints that shall be taken into account in a more detailed study: - Atmospheric and aeolian activity - Power and communications systems requirements - Illumination and temperature requirements - Biological potential and planetary protection Possible landing regions on Mars resulting from this preliminary investigation can be categorised into two classes, depending on the level of risk assessed for the landing in terms of, e.g., roughness and rock abundance: • Low-risk regions: Amazonis Planitia, Utopia Planitia, and Elysium Planitia. One of their potential drawbacks is that most areas of these regions exhibit a relatively high dust index which could be detrimental to the scientific interest of the in-situ mission. • Moderate-risk regions: - Syrtis Major / Nili Fossae, where phyllosilicates and hydrated minerals can be found based on recent evidence from orbit (Mars Express/OMEGA). - Isidis Planitia, in particular because this region presents a low vertical roughness. - Chryse/Acidalia Planitia, where phyllosilicates, hydrated minerals and sulfates can be found. - The region that spans the terrains from Sinus Meridiani to Syrtis Major, between 15ºS and 45ºN. This region exhibits a high dust index, and is represented by rougher, heavily cratered terrains in many areas. Within these regions, a more detailed identification of landing sites can be performed by refining the study (top-down approach) using higher-resolution geological and compositional maps (e.g., Mars Express/HRSC-OMEGA and/or MRO/HiRISECRISM) coupled with other parameters and constraints. Such detail work will be reported and the resulting suitable landing sites will be made available to the sciencedriven and success-oriented selection process for future Mars missions such as Exomars. This shall then be confronted with bottom-up approaches consisting in the pre-selection of sites purely based on scientific goals prior to the assessment of their suitability for landing.

Concentric Crater Fill in Utopia Planitia: Timing and Transitions Between Glacial and Periglacial Processes.

NASA Astrophysics Data System (ADS)

Levy, J.; Head, J.

2008-09-01

Concentric crater fill (CCF), lobate debris aprons (LDA), and lineated valley fill (LVF) have long been used as indicators of ground ice on Mars [1-3]. Formation models for these features range from aeolian modification [4], to rock-glacier processes [5], to debris-covered glacier processes [6-7], but are now largely constrained by the detection of material within lobate debris aprons that is 100s of meters thick, and which has dielectric properties consistent with water ice [8-9]. At ~30 cm/pixel HiRISE resolution, LVF, LDA, and CCF show complex surface textures, termed "brain coral terrain" [9], or, succinctly, "brain terrain" (BT) [10]. Polygonally patterned ground commonly is present in proximity to brain terrain, overlying it as "brain terrain-covering" polygons (BTC) [10]. Here we document spatial patterns of BT and BTC morphology present in four CCF-filled, ~10 km diameter craters in Utopia Planitia. We then evaluate formation processes for BT and BTC units. Brain Terrain (BT) Morphology At HiRISE resolution (~30 cm/pixel), concentric crater fill brain terrain displays a complex surface texture. Two distinct sub-textures are commonly present in brain terrain [9]: filled brain terrain (FBT) and hollow brain terrain (HBT) (Figure 1). Filled brain terrain (FBT) is composed of arcuate and cuspate mounds, commonly ~10-20 m wide and 10 - <100 m long. Some FBT mounds have surface grooves located near the centreline of the long axis. FBT mounds occur singly, or in linked groups. FBT mounds are commonly oriented in lineations which are concentric to the crater in which the unit is present. FBT mound lineation spacing is variable, but commonly has a wavelength of ~20 m. FBT is commonly present on undulating topography, at the top of concentric ridges (and sometimes in the concentric valleys between ridges). Hollow brain terrain (HBT) is composed of arcuate and cuspate features that are delimited by a convex-up boundary band, commonly ~4-6 m wide, surrounding a depression. HBT are of similar dimensions to FBT, but are seldom longer than ~100 m. HBT boundary bands are commonly parallel along the long axis, but may be tightly rounded or gradually tapered along the short axis. HBT features occur singly, or in linked groups. HBT features are commonly oriented in lineations which are concentric to the crater in which the unit is present. HBT lineation spacing is variable, but commonly has a wavelength of ~20 m. HBT is commonly present at the contact between BT and BTC units, particularly in topographic lows between FBT-covered ridges and surrounding isolated FBT-covered hills embayed by BTC material. Brain Terrain Covering (BTC) Polygon Morphology Polygonally patterned ground present in proximity to BT, and commonly overlying it, constitutes the brain terrain covering (BTC) unit.. BTC polygons have two distinct morphologies: high centred (HC-BTC) and low centred (LC-BTC) (Figure 1). High centred BTC polygons (HCBTC) are composed of depressed surface troughs which intersect at both near-orthogonal and near-hexagonal intersections, forming polygons that are topographically high relative to their boundaries. HC-BTC polygons are commonly ~10 m in diameter, and have little topographic relief, although most have slightly convex-up interiors, based on shadow observations. HC-BTC troughs are commonly ~2-3 m across. HC-BTC polygons are present in a unit which has a lower albedo than brain terrain, and which can be up to ~40 m thick, based on MOLA point measurements. The BTC unit is generally flat, and is bounded by gently sloping margins, as well as by steeplyscarped, scalloped margins. Low centred BTC polygons (LC-BTC) are composed of troughs with raised shoulders that intersect at near-orthogonal and near-hexagonal intersections, forming polygons with depressed centres, relative to the raised rims. LC-BTC polygons are commonly ~10 m in diameter, and have smooth, flat, depressed interiors. LC-BTC polygon shouldered troughs are commonly ~3-4 m wide. LC-BTC are found at the fringes of the BTC unit, at both low-angle and scalloped margins. Spatial Relationships Between Units FBT surfaces are much more common than HBT surfaces, and HC-BTC surfaces are much more common than LCBTC surfaces. Contacts between FBT and HBT are gradational, consisting of FBT mounds which are partially hollow, or which transition into HBT-like boundary bands. Contacts between HC-BTC and LC-BTC are gradational on gentle slopes, and abrupt on steeply scalloped slopes. BTC surfaces are commonly found at the foot of crater wall interior slopes, and in topographic lows between BTsurfaced concentric ridges. BTC material is commonly draped on, and inter-fingered between, FBT mounds and HBT boundary walls at contacts between the two units, suggesting that BTC units superpose, and in places, embay BT units. FBT-covered hill surfaces are commonly ringed by HBT, which is in turn ringed by LC-BTC, and/or HCBTC. FBT-covered concentric ridges are commonly flanked by HBT in the lows between ridges, particularly in lows which also have exposures of LC- or HC-BTC polygons. Discussion Crater counts on BT material indicate an age of ~100 MY, consistent with counts on LDA [11]; crater counts on BTC units indicate an age of ~1 MY. This age difference suggests that BT and BTC are stratigraphically distinct units that were deposited at markedly different times. The small exposures of HBT and LC-BTC make distinguishing ages for these textures from ages of the more common FBT and HC-BTC surfaces impossible. However, the gradational contacts between each sub-texture, on both steep and gentle slopes, suggests that modification of two distinct units, rather than exposure of four radically different layers, accounts for the differences between sub-textures. On the basis of these observations, we propose the following formation sequence for BT and BTC units. BTC units are an atmospherically-emplaced, ice-rich deposit, temporally associated with recent latitude-dependent mantling events [12-14] containing sufficient dusty material to generate a surficial lag deposit during sublimation of near-surface ice [e.g., 15]. Thermal contraction cracking generates polygonal fractures, which initially enhance sublimation at polygon margins, generated HC-BTC polygons [15]. The lack of strongly lineated BTC polygons suggests that BTC deposits have not significantly flowed on ~1 MY timescales [e.g., 4, 16]. Infilling of polygonal fractures by overlying lag deposit fines generates subsurface wedges, which concentrate nonicy material in polygon troughs (insulating underlying icerich material), and which gradually results in the generation of raised shoulders along polygon troughs due to thermal expansion—a process analogous to sand-wedge formation in terrestrial polygons [17]. As sublimation continues, concentration of ice-free material at trough boundaries results in relatively greater sublimation at polygon interiors, generating lowered polygon interiors, and relatively raised polygon margins (LC-BTC polygons)—a process analogous to the formation of "fortress polygons" [18], but resulting from solid-vapour transitions, rather than solid-liquid transitions. Ice may still be preserved beneath thickened lags at LC-BTC polygon boundaries. A comparable process can be invoked to account for the formation of CCF brain terrain (BT). Based on MOLA point topography measurements and typical martian crater depthdiameter ratios [19], the analyzed CCF-filled craters are up to 80% filled, accounting for volumes up to 800 m thick, which may be ice-rich [8-9]. Thick accumulations of icerich material could readily flow on ~100 MY timescales under current martian conditions, sufficient to produce observed strains (e.g., ~60%, observed in one deformed crater). Internal glacio-tectonic stresses, coupled with surface thermal contraction stresses would fracture the developing BT surface, resulting in the generation of oriented, lineated fracture networks, analogous to those observed on flowing debris-covered glaciers on Earth [20]. Inversion of polygon topography at polygon margins due to differential sublimation would result in the formation of raised mounds and chains of mounds, some of which may preserve the original surface trough (e.g., the axial furrows observed in some BT mound chains). Deposition of thin layers of low-albedo BTC material on ice-cored FBT mounds could result in enhanced sublimation of residual icecores [21], leading to collapse of FBT mounds, and generating HBT features at contacts between BT and BTC units. References. [1] Squyres, S. (1979) JGR, 84, 8087-8096. [2] Squyres, S. & Carr, M. (1986) Sci., 231, 249-252. [3] Lucchita, B. (1984) JGR, 89, 409-418. [4] Zimbelman, J. et al. (1989) LPSC19, 397-407. [5] Mangold, N. & Allemand, P. (2001) GRL, 28, 3407-3410. [6] Head, J. et al. (2006) GRL, doi: 10.1029/2005GL024360. [7] Levy, J. et al. (2007) JGR, doi: 10.1029/ 2006JE002852. [8] Holt, J. et al. (2008) LPSC39, #2441. [9] Plaut, J. et al. (2008) LPSC39, #1391. [9] Dobrea, N. et al. (2007) 7th Mars, #3358. [10] Levy, J. et al. (2008) LPSC39, #1171, [11] Mangold, N. (2003) JGR, doi:10.1029/2002JE001885. [12] Mustard, J. et al. (2001) Nature, 412, 411-414. [13] Head, J. et al. (2003) Nature, 426, 797-802. [14] Kreslavsky, M. & Head, J. (2006) M&PS, 41, 1633-1646. [15] Marchant, D. et al. (2002), GSAB, 114, 718-730. [16] Milliken, R. et al. (2003) JGR, doi: 10.1029/2002JE002005. [17] Pewe, T. (1959) Am. J. Sci., 257, 545-552. [18] Root, J. (1975) Geol. Surv. Can., 75-1B, 181. [19] Garvin, J. et al. (2002) LPSC33, #1255. [20] Levy, J. et al. (2006) Ant. Sci., doi: 10.1017/ S0954102006000435. [21] Williams, K. et al. (2008) Icarus, In Press.

On the Way to New Horizons: Telemedicine in Oncology.

PubMed

Schlag

1997-01-01

Breathtaking insights into carcinogenesis and tumor biology have been gained mainly by recent technical advances in molecular-biological and genetic techniques. Thus, dimensions of earlier diagnosis and the development of new concepts in therapy arise, which were previously unavailable. There is no doubt that through these techniques the future role and tasks of surgical oncology will change. New indications will result, for example, in the context of prophylactic therapy of hereditary malignant disease or the removal of tissue predisposed to tumors. However, modes of therapy orientated toward molecular biology will still be dependent on specialist surgical interventions in the future. Examples are such innovative concepts of therapy as transport of a therapeutic device to or into tumor cells (e.g., gene gun), or even simply obtaining the necessary tumor tissue for therapy (vaccination with transfected autologous tumor cells). Therefore, the future of surgical oncology will be influenced quantitatively as well as conceptually by new qualitative requirements. Improving precision of the surgical intervention will have to go hand-in-hand with a further reduction in surgical trauma. The consistent use of laser, video, computer and communication technology can be seen as an important predeterminant here for optimizing diagnostic and therapeutic procedures. If correctly guided, the professional experience of the individual surgeon and his personal efficiency can also be positively influenced by the swift conversion of society to multimedia and information technology. Major advances in interdisciplinary communication, as one important factor in the choice and the course of suitable complex therapies in oncology, will have to target and help to overcome former weak spots. Communication in and outside one department or hospital, as well as external communication between different medical disciplines and specialists, is being developed further and increasingly refined. The possibilities of modern technology in addition to verbal exchange include visual and interactive "tele"-communication. This renders a new option to the physician, as without direct patient contact he is able to observe, counsel and actively interact - the latter even more so in the future. In oncology the increase of knowledge thus far has gone hand-in-hand with further specialization. This explains the difficulties one encounters in the correct evaluation of relevant data of one specific patient. Telemedicine will help to focus on the advantages of specialist knowledge by rendering access to all available data. These possibilities should furthermore be accessible during a consultation, an examination or in the course of a surgical intervention. Real-time modalities are referred to as telepresence and exceed by far a mere electronic version of the patient's medical folder. Especially in oncology, interdisciplinary collaboration is immensely important for successful therapy. Preoperative diagnostic data are still to be evaluated according to the intraoperative findings. At this decisive moment, it is necessary to involve specialists of other oncological disciplines. Real-time communication devices have to be present in order to transfer image data and clinical observations and ensure the best possible transmission quality to resident and geographically distant experts. With further technological perfection and widespread availability of interactive consultation, other applications include the "second opinion" in the daily routine. Another fascinating option in oncology is offered by visual computer simulation in virtual reality (VR). Medical data are visualized according to the human perception by the means of scenic simulation. From that point of view, VR technologies represent a practicable user interface between computer technology and the individual human being. Through VR, three-dimensional worlds containing virtual objects, which consist of computer-generated data, are created, which the user may explore and liberally interact with. The perfect simulation of realistic settings offers a method of training that may be extended to the field of oncology, as it has been known for a comparatively long period of time from flight simulators in space and air technology. In contrast, medical training is currently achieved mainly by "training-on-the-job." There is well-proven and widely acknowledged certainty of the tremendous influence that the number of surgical interventions-in other words, the training skills of the surgeon-has on the success of a diagnostic or therapeutic intervention. Previously, the subjective experience of the physician acquired from earlier cases determined his efficiency to a large extent. It was, in addition, influenced essentially by perception, "performance on the day" and personal attitude. The goal must be to strengthen the objective criteria as the basis for consistent decision-making processes and clear instructions for therapy. Strict quality management as practiced in air technology has clearly led to a reduction in accidents, and, accordingly, a similar effect is imaginable in oncology with continuous training using VR simulators, leading to improved therapeutic outcome. Other possibilities for use are principally implied and similarly useful for medical school and postgraduate training. The idea of computer-guided medical procedures or medical robots is therefore no longer a mere utopia. Telepresence, telerobotic and VR techniques should, in principle, effectively support the physician in diagnostic processes and therapy. The responsibility for coordination and sensible use of new technological developments will still remain with the physician, such as improving and simplifying medical procedures. Technology should be used according to the situation, not to adapt the patient to a technocratic environment, but to emphasize human treatment of the individual patient. From the opinion of the telephone being a futile technical invention to the other extreme of computed technology as a substitute for the physician (Dr. Cyber), the future role of telemedical techniques and their potential for medical advantage or support, especially in the field of oncology, should be critically viewed and evaluated.

Backwards and Forwards: 50 years of the Education Group

NASA Astrophysics Data System (ADS)

2000-01-01

The Education Group of the Institute of Physics celebrated its 50th anniversary by dedicating its annual 16 - 19 Day to a conference entitled Post-16 Physics: Looking forward, learning from the past. This attracted an audience of 50 or so nostalgia-seekers on Saturday 13 November at the Portland Place HQ. Philip Britton (Chair of the Education Group) began the proceedings in his usual pawky way by challenging members to identify the year in which some hardy topics were first addressed. A key trend in titles was the movement from problem to challenge . He looked forward to the time when success was a keynote word. Few identified Physics in Industry with the year of the deepest recession of the Thatcher Era. Tim Akrill (Chief A-level Physics Examiner for Edexcel) reminded us that A-levels were just about as old as the Education Group before taking us on an informative and entertaining tour of Assessment and Examinations through the Ages . Things have indeed become more complex since the very first written examination of 6th century China, when the only question, set every year, was: `Write down everything you know'. In 1951 an A-level physics paper gave a choice of six out of twelve questions and appeared in an A5 booklet of perhaps as many as four pages. The satisfying thump of a kilogram mass of current Edexcel A-level physics papers resounded through the room as he dropped them on a table. In those innocent days all questions followed the DDC format: define, describe, calculate . `Question spotting' was an art (or science) assiduously developed by teachers, as Lees' Disk alternated with Searle's Bar with less than exciting regularity. Have standards fallen? He thought not. At Edexcel they still get about 4000 candidates getting the higher grades, a number that has stayed the same for some 20 years. He singled out Nuffield Advanced Physics as being responsible for the greatest innovations in exam style since, well, the Chinese really. Styles such as Practical Problems, Comprehension, Short Answer, Long Answer, Investigations and more recently Research and Analysis had introduced a variety of assessment techniques aimed at identifying and rewarding different modes of doing physics and demonstrating the variety of competences physicists need. It was hard, however, for examinations to give value to the `wonder and delight' that good students experienced with good teachers, but at least they were mentioned in the preambles to what we have now to call specifications instead of syllabuses . This talk led on nicely to Jon Ogborn's talk entitled Curriculum Reform in Physics, past, present and future . This was horse's mouth stuff: not only was Jon one of the two (with Paul Black) chief designers of the Nuffield Advanced Physics (NAP) course, he is now the leader of the IoP 16 - 19 Physics Initiative, which amongst other things is producing a new A-level course Advancing Physics (AP). He compared the two developments using such contrasting descriptors as clockwork vs organic; strong vs tough; built-to-last vs built-to-change; a right-to-be-wrong vs a duty-not-to-be-wrong. The original Nuffield course did not even have a syllabus, now Advancing Physics has a tight `specification' controlled by a government agency; then exam boards cooperated and had the air of a (gentleman's) club, now they compete as regulated and regulatory `businesses'. Back in the 1960s the new physics, so much welcomed by teachers, was in fact rather old physics which had managed not to be downloaded to school level: thermodynamics, electromagnetic wave theory, a hint of relativity, some quantum theory. What was really new was the microelectronics. Advancing Physics , on the other hand, is trying to be `state of the art': getting at some standard and necessary physics via such things as sensing, imaging, signals, instrumentation, cosmology and some particle physics. AP views physics as a collection of almost independent states: many IoP journals are called `X physics' where X is a term such as nuclear, medical, condensed matter, plasma etc, etc. An A-level course should bring this wide range of things that physicists do to students' attention. Where NAP could be seen as addressing `pure', fundamental physics, AP will strongly emphasize physics in use. Where NAP tended to see maths as a kind of necessary evil, AP will glory in the challenges and excitements it can provide. Finally, NAP teachers had the luxury of thinking about their students as `being lucky to be taught such interesting stuff by us'; AP teachers think themselves lucky to have students. This Parthian shot again led quite neatly into Professor Mick Brown's afternoon talk. Mick Brown works at the Cavendish Laboratory and is the IoP's Guthrie Prize winner this year. In his talk Connecting with Advanced Physics: the first year in Higher Education he first gave us a `Vice-Chancellor's View'. Essentially this boiled down to the fact that, even at Cambridge, teaching students is not a cost-effective activity. His and his lecturers' salaries are paid for by research grants. If they had just the income from teaching they would soon be bankrupt. The number of students doing physics at Cambridge fell from about 1200 in 1989 to about 900 in 1995, at a time when biology students increased. Other universities had suffered such greater losses that they no longer taught undergraduates, or had no physics departments at all. He felt that it was in the interests of the country that there should be a range of physics departments, from the very large to the quite small. Turning to a young lecturer's point of view, he contrasted current practice with what used to happen. Fewer and fewer demonstrations took place in lectures; practical classes were so mismatched with lecture courses that both lecturers and students were frustrated by their seeming irrelevance; examinations were not closely enough linked with what lecturers actually taught (or wanted to teach). These views were echoed by representatives from a number of equally prestigious universities. In one, the large physics lecture rooms were taken over by philosophy students, as smaller physics groups traipsed across to distant biology rooms. It was this kind of situation, plus the reduction in the level of technician support, that made demonstrations harder to organize. In the lively discussion that followed Professor Brown's talk there was strong support for his proposal that universities - with the help of the IoP and the Royal Society, say - should set up a national `demonstration bank' that could be tapped to provide portable, well-tried, well-resourced and well-rehearsed demonstrations. Envy was expressed for the bank of experiments and demonstrations available at school level, especially as presented by the Advancing Physics CD-ROM. Universities could also learn from the course designs exemplified by Advancing Physics and the York Salters Horners projects: a set of self-contained, coherent topics with clear end-points and built-in mathematics, with key concepts well-illustrated by relevant experiments. The final session was given by Ken Dobson, who had the onerous but luckily uncheckable task of talking about Physics education: the next 50 years! (organizer's emphasis). In less than 15 minutes he expressed his complete incompetence at carrying out such a task, but in spite of that went on to compare the current state of progress (leading to an unfortunate state of dystopia) with what he thought should happen (leading to a much happier state of utopia). The key differences were the current over-centralization, mechanistic and top-down direction of education based on a system-centred command-psychology, as compared with an organic, self-directed, learner-centred education. He called the first dystopian model the Rucsac Model : everything you needed for life had to be packed by the time you left school, and should serve you all your days. By contrast, he called the utopian future a Daniel Boone model: you left the system armed with minimal `content' in your pack but would be well-armed and well-skilled to adapt yourself to the inevitable uncertainties of the future. Ken Dobson will not be around to check that his predictions for 2049 are correct, but for the record: 1. Physics will be simpler . 2. Maths will be more accessible . 3. Learning will be more individually targeted ... 4. ... but a lot more social , involving , local and friendly ... 5. ... a lot less mediaeval 6. and happens when the learner needs it . (Scope for another editorial here ... .) I should mention that in the lunch interval Brenda Jennison, past and long-serving chair of the Education group, paid tribute to the ideas and stimuli produced by such leading lights as Eric Rogers (Physics for the Inquiring Mind , Nuffield O-level, etc), Geoff Foxcroft (electronics), John Lewis (so many innovations and still going strong), as well as Paul Black and one of the day's speakers, Jon Ogborn. Some of Brenda's students were also prevailed upon to demonstrate some simple but intriguing bits of physics, whether they liked it or not. Ken Dobson Honorary Editor, Physics Education

Building and Applying "Insularity Theory": Review on Knapp's Prehistoric and Protohistoric Cyprus, 2008.

NASA Astrophysics Data System (ADS)

Katsarou-Tzeveleki, Stella

Prehistoric and Protohistoric Cyprus by A. Bernard Knapp involves us in a highly creative reading. This is due mainly to the fact that the author engages in a holistic synthesis of Cyprus in the Bronze Age, not by emphasizing the events and descriptions of the material remains, but by concentrating upon the difficult question of the identity of the islanders of this period and the processes by which it was formed. The author's teaching of Mediterranean prehistory at the University of Glasgow fully accounts for his need to produce a comprehensive theoretical work of this kind: the basic questions asked by students give rise to theoretical concerns for any teacher aiming to 'distil' the essential synthesis that forms the starting point for any further detailed archaeological description. This essential answer seems to have troubled Knapp for some time, judging by the long list of his writings seeking to synthesize aspects of Cypriot economy, cult and society; the present book is thus the highly interesting outcome of the mature thinking of an experienced fieldworker as much as a theoretical archaeologist and teacher. What, then, is the essential question that Knapp seeks to answer through this book? His question focuses on the identity of the islanders of Cyprus during the 'most formative periods, from the village based culture to the international, town-centred, even state-level polity' (p. 1), the way in which this identity was formed, and how it is reflected in both any recorded event and the material culture of the island in this specific period. Moreover, he also explores more fully what the distinctive features of island identity in general are, how they are constituted and how they influence the material culture of any island population. In seeking the answers, the author avoids a number of the usual approaches to Cypriot archaeology and turns, instead, to new interpretive directions. The approaches he avoids are the citing of events of Cypriot prehistory, the listing of external factors (colonization, invasions) originating in the Near East and the Aegean as sequential narrative history, and the descriptive, systemic analysis of 'materiality, production, trade, migration and colonization which have for long been the cornerstones of Cypriot archaeology' (p. 11). In contrast, he turns his attention towards the internal processes within the island society of Bronze Age Cyprus, which shape its insularity and give it a distinctive identity at this specific period, processes that lead to contextual history and formative tradition. 'To study how any society changes, at any time, it is crucial first to look at internal rather than external factors' (p. 1). Defining the concept of insularity is his aim; therefore, he begins with a number of very apposite rhetorical questions (p. 13) and identifies several individual parameters (connectivity, islandscape, social identity, ethnicity, migration, acculturation, hybridization) to which he assigns collective and individual meanings. The eight chapters that follow may be assigned, broadly, to three general units: in the first of these (ch. 1-2), Knapp offers a synthesis of these parameters in the form of a 'theory of insularity'. In the second (ch. 3-7) he formulates his revised narrative of the prehistory and social identity of the island, which involves a presentation of social and economic, rather than stylistic categories, on the basis of the parameters laid down in his theoretical scheme. Finally, in the third unit (ch. 8), he records his overall conclusions, the new cognitive experiences and concerns that have emerged from the application of his theory, both to Cyprus and to insular archaeology in the Mediterranean and on a world scale. Knapp's synthesis of the theory of insularity in the first unit is a major contribution to Mediterranean archaeology, and makes this book a seminal work. Continuing and broadening Broodbank's (2000) reasoning about the Cyclades, Knapp, with Cyprus as his starting point, places at the disposal of insular archaeology an analytical theoretical scheme of insularity, in which he integrates a number of key concepts (social identity, ethnicity, habitus, migration, colonial theory). These are much used in archaeological interpretation, but previously treated as independent theoretical notions. To those he adds a number of hitherto secondary concepts (connectivity, islandscape, acculturation, hybridization) to which (especially the last) he assigns a leading role. In the in-depth presentation of each concept, he attempts to establish the history of its usage in archaeological theory and patterning, and to offer an exhaustive conceptual and anthropological analysis of it. The theoretical analysis of identity (island, social and ethnic) and the multiple dimensions of mutual influences between cultures emerges as one of Knapp's most important reasoning. Knapp records in detail the models that describe the variations and gradations of communications and their results, whether migration and colonial theory, on the one hand, or peaceful interaction, on the other. He draws our attention to something that usually goes unnoticed, and this is a substantial contribution to the work of every research archaeologist: namely, that there is no such thing as pure identity. Every identity studied by archaeology is the product of acculturation, assimilation or a blending of intersecting identities, ending in hybridization. At this point, however, I would doubt that hybridization, assimilation and cultural blending should be regarded as the natural and definite result where every communication between two different cultural groups leads. In fact Hodder (1982) has challenged this rule after his observations at Baringo, Kenya, where he noticed that the different groups there would rather emphasize their different features at the interaction areas, instead of letting them assimilate with the other's. This important reference would perfectly fit Knapp's narrative to further show how unforeseen the interaction can be. However, Knapp, subsequently, undertakes an important work as he emphatically calls every researcher not to incline to one-sided-assimilation conclusions: interactions do not operate in a one-sided manner from dominant to subordinate cultures (see neolithization, minoanization, etc), but they are dynamic, difficult to predict and should not be not simplistically identified with archaeological data. For the component concepts of his theory to be complete, I feel that Knapp should have devoted a chapter, giving the same historical and analytical information, to cultural identity, as the stylistic and visual component of material culture and as the fundamental characteristic of every other identity. I would further suggest that he should have taken the attempt to find archaeological examples, since the living, ethnological-anthropological ones, while documenting the components of this theory, do not provide an answer to the question of how to read a tradition of the past. For instance, his example stating that (p. 29) 'modern Cypriot cuisine, whatever the political climate might lead one to expect, has little to do with Greek cooking, but everything to do with the culinary traditions of Turkey, the Levant and Egypt', is rather unfortunate as an example of a change of local identity. Generally speaking, Knapp's synthesis is excellent, as is his insistence, in the first unit, on referring to the key concept of meaningful insularity as the assimilation of post-processual theory. Instead of the deterministic interpretations that give prominence to the geographical factor, either negatively (fateful isolation) or positively ('island paradox', i.e. the sea offers better communications than the land), instead of timeless, location-less deterministic and essentialist conceptions, Knapp offers insularity not as an absolute, permanently fixed state, but as fluid and situational thing. He makes the reader understand the concept of insularity as a completely contextual archaeological one, that constantly changes, as a result of interactions and discourses between people and things. Moreover, insularity therefore is made to be understood as determined by the collective and personal choices of the individuals of every island community (agreements and alliances or disagreements and hostilities), who wish or do not wish to, want or do not want, but not can or cannot, communicate with the outside world. In the end, then, Knapp is not looking to reveal one, but many identities. The basic unit of analysis is a network of several interacting cultures, not one individual culture (p. 56). Each individual has multiple or dispersed identities, or, as Knapp writes elsewhere, a constellation of identities. In the conclusion of his theoretical unit, where he recognizes the interpretive potential of trans-historical and trans-cultural contexts (p. 65) I viewed with some reserve Knapp's recourse to the systemic nature of behaviour: 'nonetheless, because people often systematize and rationalize distinctive cultural styles in the process of establishing and expressing their identity, archaeologists may yet succeed in isolating discontinuous non-random distributions of material culture which plausibly may be related to the expression of identity phenomena'. I do not believe that this invalidates his post-modern analysis above, which seems well grounded. It is rather a usual reaction of perplexity when faced with the unknown mind of prehistoric man. Personally, however, I would add, first, that this recourse to the validity of repeatedness can be useful inside a certain context, namely tradition. Secondly I would prefer the emphasis to be on the interpretative potential of the questions asked by the prehistoric archaeologist. Third, I would urge any researcher to accept the utopia and honestly declare his/her inability to read the multiple identities of any certain individual of the past, rather than insist on the search for the exception or difference in material culture as the secure way to describe any certain cultural identity. When Knapp applies his theory to Cyprus, he divides the period under examination into two general chronological horizons, and introduces two interesting neologisms: the prehistoric Bronze Age (down to 1650) and the protohistoric Bronze Age (1650-10th century BC), the conventional boundary between them being the appearance of literary sources. Unfortunately, we find that there is no reference to the Chalcolithic, Neolithic and Epipalaeolithic prehistory of Cyprus, since he axiomatically takes the end of the Cypriot Chalcolithic (the Philia culture) as a point of catalytic social change. I believe, however, that one thought (and here we have a challenge to future research) is missing: the contribution made by the earlier societies of the island to the formation of its later tradition, since Knapp himself repeatedly accepts in his book the historical-comparative dimension of identity in the long term, and ultimately resorts to hybridization, in which the local tradition contributes equally as the intrusive factors do. I welcome the distinction of the Bronze Age in prehistoric and protohistoric. Concerning the term protohistory, familiar in Cypriot archaeology since Peltenburg (1982), I strongly recommend it to Greek archaeologists who have enough textual evidence to finally decide to distinguish the proto-literary Late Bronze Age from the vast depths of the Early-Middle Bronze Age, Neolithic and Palaeolithic prehistory of Greece. As for the prehistoric Bronze Age of Cyprus (Late Chalcolithic-1650 BC), Knapp adopts a social/socio-economic approach that involves aspects of elite formation, copper production and exchange, gender representations and individuality. He eschews references to evolutionary typologies and revises Webb and Frankel's (1999) theory of direct migration or colonization from Anatolia, in favour of hybridization, repeating that the advantage of this suggestion is that it dispenses with the superior (Anatolia)-inferior (Cyprus) divide and it thus recognizes the contribution made to the formation of the final Cypriot identity by many identities, including the native one. However, I think that the reader would be interested to learn whether, behind the unified archaeological picture of the island, Cyprus does not have internal, human-geographical differences, differently reacting in external and internal interactions. In a work placing emphasis on individuality, an assessment of this spatial differentiation would be of interest. The social approach becomes socio-historical in the case of the protohistoric Bronze Age, for which Knapp records the formation of the Cypriot identity (that is, the completely distinct local identity) through a combined archaeological handling of text and object which is rare for prehistoric research. Knapp examines the character (local, Aegean, Levantine, Anatolian) of the island's material culture (urbanization, settlement patterns, monumentality, seals and objects connected with the organization of authority, mortuary practices, Cypro-Minoan script, copper trade, imports, defence works and weaponry, figurative representations and frescoes) in comparison with the valuable historical information contained in texts found in Ugarit (from the 13th c. BC) referring to the territory or kingdom of Alashia ruled by Kushmenshusha. After his prodigious analysis of the archaeological data, exhibiting the high level of his expertise on Cypriot archaeology, he demonstrates how much this island, unified into a large state with a strong presence in the eastern Mediterranean, was a hybrid product. To support his arguments the author introduces further theoretical concepts (for example, individuality and monumentality), again with recourse to the international theoretical bibliography. Let me note, however, that traditional archaeology's insistence on wealth as a criterion for social differentiation is still used as a self-evident stereotype, often as an echo of a deterministic Marxist view of prehistoric societies. Such an approach renders the author's argument rather explanatory than interpretive. I wonder if this stereotype is in fact secure enough to stand on, or whether a 'theory of wealth' should not be formulated first. Such a theory would examine what is meant by wealth in each phase of Cypriot Bronze Age, what is the individual view of wealth, or the collective view of every society on this. Knapp closes his book as he began it: emphasizing the continuous formation of identity -his citation from Hereniko (1997) is almost moving (p. 373)-, and searching for a balance between the holistic Mediterranean tradition and the individual features of every Mediterranean island, coast or other geographical subunit, for which he recommends further focused research. Overall, I feel that Knapp presents a most valuable overview of the Cypriot Bronze Age, maybe not in fact 'a new island archaeology and island history of Cyprus', as he claims at the start (p. 12), though certainly a new and different synthesis. At the same time, however, he also presents a valuable overview of the parameters of insularity, formulating a visionary theoretical scheme through which he aspires 'to advance the study of the Mediterranean past in a manner that confronts unexplored ideas, crosses traditional boundaries, offers unexpected insights, and extrapolates from such ideas and insights to consider similar patterns and problems in the Mediterranean island context' (p. 7-8), and also in the wider world context. Theoretical archaeologists in general will find in this book an example of the practice of theoretical archaeology through the endeavour to integrate the theory into the material remains, and to transcend the urge to classify when examining them. With this objective in mind, Knapp engages in exhaustive detail of theoretical concepts and enlists a highly theoretical language, with a maximalist vocabulary. Characteristic examples here are the constant citations of other writings as an introduction to his sub-chapters, and especially the first paragraph of chapter 2 (p. 13), written with a literary imagination, which, like a fresh sea breeze, rouses the reader's emotions appealing to real and imaginary experiences evoked by the concepts of island and sea.