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Sample records for mozhete vbrat sami

  1. Survival of Sami cancer patients

    PubMed Central

    Soininen, Leena; Pokhrel, Arun; Dyba, Tadek; Pukkala, Eero; Hakulinen, Timo

    2012-01-01

    Objectives The incidence of cancer among the indigenous Sami people of Northern Finland is lower than among the Finnish general population. The survival of Sami cancer patients is not known, and therefore it is the object of this study. Study design The cohort consisted of 2,091 Sami and 4,161 non-Sami who lived on 31 December 1978 in the two Sami municipalities of Inari and Utsjoki, which are located in Northern Finland and are 300–500 km away from the nearest central hospital. The survival experience of Sami and non-Sami cancer patients diagnosed in this cohort during 1979–2009 was compared with that of the Finnish patients outside the cohort. Methods The Sami and non-Sami cancer patients were matched to other Finnish cancer patients for gender, age and year of diagnosis and for the site of cancer. An additional matching was done for the stage at diagnosis. Cancer-specific survival analyses were made using the Kaplan–Meier method and Cox regression modelling. Results There were 204 Sami and 391 non-Sami cancer cases in the cohort, 20,181 matched controls without matching with stage, and 7,874 stage-matched controls. In the cancer-specific analysis without stage variable, the hazard ratio for Sami was 1.05 (95% confidence interval 0.85–1.30) and for non-Sami 1.02 (0.86–1.20), indicating no difference between the survival of those groups and other patients in Finland. Likewise, when the same was done by also matching the stage, there was no difference in cancer survival. Conclusion Long distances to medical care or Sami ethnicity have no influence on the cancer patient survival in Northern Finland. PMID:22765936

  2. Sami Education in Finland

    ERIC Educational Resources Information Center

    Keskitalo, Pigga; Maatta, Kaarina; Uusiautti, Satu

    2012-01-01

    The purpose of this article is, first, to describe Sami children's education and its status in the Finnish education system and, secondly, to contemplate its development in Finland. The core of the article is intertwined with issues concerning the status, language, and culture of indigenous peoples. According to the article, the western school…

  3. Publishing Sami Literature--From Christian Translations to Sami Publishing Houses

    ERIC Educational Resources Information Center

    Paltto, Kirsti

    2010-01-01

    Publishing in the Sami languages has always been difficult. The Sami are currently spread across four countries, Norway, Sweden, Finland, and Russia. There are nine different Sami languages, some of them with only a few speakers. The Sami publishing industry is entirely dependent on government funding as it does not have its own funds nor is there…

  4. The SAMI IFU Galaxy Survey

    NASA Astrophysics Data System (ADS)

    Konstantopoulos, Iraklis; Croom, S. M.; Lawrence, J. S.; Bland-Hawthorn, J.; Bryant, J.; Fogarty, L.; Richards, S.; Goodwin, M.; Farrell, T.; Miziarski, S.; Heald, R.; Jones, D.; Lee, S.; Colless, M.; Brough, S.; Hopkins, A. M.; Bauer, A. E.; Birchall, M. N.; Ellis, S. C.; Horton, A. J.; Leon-Saval, S. G.; Lewis, G. F.; Lopez-Sanchez, A. R.; Min, S.; Trinh, C.; Trowland, H.; SAMI Team

    2013-01-01

    The past decade has seen the undertaking of several large spectroscopic surveys, which have enhanced our understanding of the processes that govern galaxy evolution. The next generation of surveys will allot not a fibre, but an Integral Field Unit on each galaxy, in order to push that understanding to the next level: spatially resolved spectroscopy. With a target list in the thousands of galaxies, the Sydney-AAO Multi-object Integral Field Spectrograph (SAMI) Survey will boldly push forward in this domain. On behalf of the SAMI team, I will present an overview of the capabilities of this innovative multiplexed IFU spectrograph and the survey it is undertaking, as well as highlight some early science.

  5. SAMI Automated Plug Plate Configuration

    NASA Astrophysics Data System (ADS)

    Lorente, N. P. F.; Farrell, T.; Goodwin, M.

    2013-10-01

    The Sydney-AAO Multi-object Integral field spectrograph (SAMI) is a prototype wide-field system at the Anglo-Australian Telescope (AAT) which uses a plug-plate to mount its 13×61-core imaging fibre bundles (hexabundles) in the optical path at the telescope's prime focus. In this paper we describe the process of determining the positions of the plug-plate holes, where plates contain three or more stacked observation configurations. The process, which up until now has involved several separate processes and has required significant manual configuration and checking, is now being automated to increase efficiency and reduce error. This is carried out by means of a thin Java controller layer which drives the configuration cycle. This layer controls the user interface and the C++ algorithm layer where the plate configuration and optimisation is carried out. Additionally, through the Aladin display package, it provides visualisation and facilitates user verification of the resulting plates.

  6. The SAMI2 Open Source Project

    NASA Astrophysics Data System (ADS)

    Huba, J. D.; Joyce, G.

    2001-05-01

    In the past decade, the Open Source Model for software development has gained popularity and has had numerous major achievements: emacs, Linux, the Gimp, and Python, to name a few. The basic idea is to provide the source code of the model or application, a tutorial on its use, and a feedback mechanism with the community so that the model can be tested, improved, and archived. Given the success of the Open Source Model, we believe it may prove valuable in the development of scientific research codes. With this in mind, we are `Open Sourcing' the low to mid-latitude ionospheric model that has recently been developed at the Naval Research Laboratory: SAMI2 (Sami2 is Another Model of the Ionosphere). The model is comprehensive and uses modern numerical techniques. The structure and design of SAMI2 make it relatively easy to understand and modify: the numerical algorithms are simple and direct, and the code is reasonably well-written. Furthermore, SAMI2 is designed to run on personal computers; prohibitive computational resources are not necessary, thereby making the model accessible and usable by virtually all researchers. For these reasons, SAMI2 is an excellent candidate to explore and test the open source modeling paradigm in space physics research. We will discuss various topics associated with this project. Research supported by the Office of Naval Research.

  7. The Sami Languages(s), Maintenance and Intellectualistion.

    ERIC Educational Resources Information Center

    Bull, Tove

    2002-01-01

    Gives an overview of the current socioliniguistic situation of the Sami language in Northern Scandinavia, focusing on the situation in North Norway in particular. Describes the historical development and discusses issues, problems, and practices relating to Sami language politics and planning in reaction to the use of this language in…

  8. The Linguistic Special Features of the Sami Education

    ERIC Educational Resources Information Center

    Keskitalo, Pigga; Maatta, Kaarina

    2011-01-01

    This article focuses on the features of Sami language instruction at the first school grades in Norway. The most important part is to describe what kind of challenges Sami language instruction at the first grades as an indigenous people's language and with the status of a minority language has. This situation introduces some differences and…

  9. Sensibility: A New Focus in Sami Health Care Education

    ERIC Educational Resources Information Center

    Nymo, Randi

    2007-01-01

    Colonialism has had significant bodily impacts on Indigenous peoples through medicine. Excluded from the German race, Sami have been burdened by mainstream prejudices which perpetuate myths about Sami having poor genetic material and, as a consequence, having an inferior culture and language. This offensive burden and subsequent humiliation has…

  10. Indigenous Teachers' Experiences of the Implementation of Culture-Based Mathematics Activities in Sami School

    ERIC Educational Resources Information Center

    Nutti, Ylva Jannok

    2013-01-01

    The goal of Indigenous education is that it should be approached on the basis of the Indigenous language and culture; this is also the case with Sami education. The Sami School Board has stated that all teaching in Sami schools should be culturally based, despite the fact that Sami culture-based teaching is not specifically defined. Therefore,…

  11. SAMIS- STANDARD ASSEMBLY-LINE MANUFACTURING INDUSTRY SIMULATION

    NASA Technical Reports Server (NTRS)

    Chamberlain, R. G.

    1994-01-01

    The Standard Assembly-Line Manufacturing Industry Simulation (SAMIS) program was originally developed to model a hypothetical U. S. industry which manufactures silicon solar modules for use in electricity generation. The SAMIS program has now been generalized to the extent that it should be useful for simulating many different production-line manufacturing industries and companies. The most important capability of SAMIS is its ability to "simulate" an industry based on a model developed by the user with the aid of the SAMIS program. The results of the simulation are a set of financial reports which detail the requirements, including quantities and cost, of the companies and processes which comprise the industry. SAMIS provides a fair, consistent, and reliable means of comparing manufacturing processes being developed by numerous independent efforts. It can also be used to assess the industry-wide impact of changes in financial parameters, such as cost of resources and services, inflation rates, interest rates, tax policies, and required return on equity. Because of the large amount of data needed to describe an industry, a major portion of SAMIS is dedicated to data entry and maintenance. This activity in SAMIS is referred to as model management. Model management requires a significant amount of interaction through a system of "prompts" which make it possible for persons not familiar with computers, or the SAMIS program, to provide all of the data necessary to perform a simulation. SAMIS is written in TURBO PASCAL (version 2.0 required for compilation) and requires 10 meg of hard disk space, an 8087 coprocessor, and an IBM color graphics monitor. Executables and source code are provided. SAMIS was originally developed in 1978; the IBM PC version was developed in 1985. Release 6.1 was made available in 1986, and includes the PC-IPEG program.

  12. Ethical guidelines for Sami research: the issue that disappeared from the Norwegian Sami Parliament's agenda?

    PubMed Central

    Stordahl, Vigdis; Tørres, Grete; Møllersen, Snefrid; Eira-Åhren, Inger-Marit

    2015-01-01

    Background In recent decades many indigenous communities, policy makers and researchers worldwide have criticized the academic community for not being aware of the specific challenges these communities have faced and still are facing with regard to research. One result of the decades of discourse in indigenous communities is the development in many Western countries of indigenously sensitive ethical research guidelines. In 1997 the Sami Parliament (SP) in Norway reached a unanimous decision that ethical guidelines for Sami research had to be drawn up. Such guidelines are however still to be created. Objectives The objectives of this article are to enquire into what happened to the Norwegian SP's decision of 1997 and to reflect on why the issue seems to have disappeared from the SP's agenda. Finally, we consider whether research ethics is to be a subject for the research community only. Methods A review of parliamentary white papers on research and SP documents relating to research ethics. Findings The response to the SP's decision in 1997 took place in two different channels, both of them national, namely the research ethics channel and the political channel. Thus, there were actually two parallel processes taking place. In spite of nearly two decades of reports, the concept of the participation of indigenous communities in research is still not an integral part of Norwegian ethical guidelines. Conclusions The issue of indigenously sensitive research ethics seems to have disappeared from the SP's agenda and the research ethics review system with regard to Sami research is with minor adjustments the same as when the SP asked for a revision. PMID:25862334

  13. How to Make the Small Indigenous Cultures Bloom? Special Traits of Sami Education in Finland

    ERIC Educational Resources Information Center

    Keskitalo, Pigga; Uusiautti, Satu; Maatta, Kaarina

    2012-01-01

    This article discusses smallness from the point of view of the Sami, an indigenous people of the Arctic, and describes today's Sami education in Finland, the factors that have affected its formation and the challenges in strengthening it. The purpose of the article is to provide ideas to develop Sami education and encourage discovering methods…

  14. Incidence of galactic outflows: EAGLE simulations vs SAMI observations

    NASA Astrophysics Data System (ADS)

    Tescari, E.

    2016-06-01

    I presented the results of the joint SAMI-EAGLE project on outflows I lead at the University of Melbourne. We use the highest resolution EAGLE cosmological simulations to study the incidence of supernova driven winds ejected from galaxies on the main sequence. We produce synthetic SAMI observations of outflows that we compare directly with real data. While winds are observed in only a fraction of SAMI galaxies, they appear ubiquitous among simulated star forming objects. Moreover, the velocity dispersion distribution is only weakly dependent on stellar mass (M*) and sSFR (SFR/M*). I presented additional analyses and discuss the implications of these results and how they provide important constraints to ongoing and future IFS surveys.

  15. Ethical and methodological issues in research with Sami experiencing disability

    PubMed Central

    Melbøe, Line; Hansen, Ketil Lenert; Johnsen, Bjørn-Eirik; Fedreheim, Gunn Elin; Dinesen, Tone; Minde, Gunn-Tove; Rustad, Marit

    2016-01-01

    Background A study of disability among the indigenous Sami people in Norway presented a number of ethical and methodological challenges rarely addressed in the literature. Objectives The main study was designed to examine and understand the everyday life, transitions between life stages and democratic participation of Norwegian Sami people experiencing disability. Hence, the purpose of this article is to increase the understanding of possible ethical and methodological issues in research within this field. The article describes and discusses ethical and methodological issues that arose when conducting our study and identifies some strategies for addressing issues like these. Methods The ethical and methodological issues addressed in the article are based on a qualitative study among indigenous Norwegian Sami people experiencing disability. The data in this study were collected through 31 semi-structured in-depth interviews with altogether 24 Sami people experiencing disability and 13 next of kin of Sami people experiencing disability (8 mothers, 2 fathers, 2 sister and 1 guardian). Findings and discussion The researchers identified 4 main areas of ethical and methodological issues. We present these issues chronologically as they emerged in the research process: 1) concept of knowledge when designing the study, 2) gaining access, 3) data collection and 4) analysis and accountability. Conclusion The knowledge generated from this study has the potential to benefit future health research, specifically of Norwegian Sami people experiencing disability, as well as health research concerning indigenous people in general, providing scientific-based insight into important ethical and methodological issues in research with indigenous people experiencing disability. PMID:27396747

  16. Prevalence of self-reported stomach symptoms after consuming milk among indigenous Sami and non-Sami in Northern- and Mid-Norway – the SAMINOR study

    PubMed Central

    Hansen, Ketil Lenert; Brustad, Magritt; Johnsen, Knut

    2015-01-01

    Objective The main purpose of this work was to identify the prevalence of self-reported stomach symptoms after consuming milk among Sami and non-Sami adults. Study design A cross-sectional population-based study (the SAMINOR study). Data were collected by self-administrated questionnaires. Method SAMINOR is a population-based study of health and living conditions conducted in 24 municipalities in Northern Norway during 2003 and 2004. The present study included 15,546 individuals aged between 36 and 79, whose ethnicity was categorized as Sami (33.4%), Kven (7.3%) and Norwegian majority population (57.2%). Results Sami respondents had a higher prevalence of self-reported stomach symptoms after consuming milk than the Norwegian majority population. The reporting was highest among Sami females (27.1%). Consumption of milk and dairy products (yoghurt and cheese) was high among all the ethnic groups. However, significantly more Sami than non-Sami never (or rarely) consume milk or cheese, and individuals who reported stomach symptoms after consuming milk had an significant lower intake of dairy products than those not reporting stomach symptoms after consuming dairy products. Sami reported general abdominal pain more often than the majority population. The adjusted models show a significant effect of Sami ethnicity in both men and women on self-reported stomach symptoms after consuming milk. In females, the odds ratio (OR)=1.77 (p=0.001) and in males OR=1.64 (p=0.001). Conclusion Our study shows that the Sami population reported more stomach symptoms after consuming milk, suggesting a higher prevalence of milk intolerance among the Sami population than the Norwegian majority population. PMID:25694052

  17. Ethnic difference in the prevalence of pre-diabetes and diabetes mellitus in regions with Sami and non-Sami populations in Norway – the SAMINOR1 study

    PubMed Central

    Naseribafrouei, Ali; Eliassen, Bent-Martin; Melhus, Marita; Broderstad, Ann Ragnhild

    2016-01-01

    Objective The aim of this study was to measure the prevalence of pre-diabetes and diabetes mellitus in rural populations of Norway, as well as to explore potential ethnic disparities with respect to dysglycaemia in Sami and non-Sami populations. Design Cross-sectional population-based study. Methods The SAMINOR1 study was performed in 2003–2004. The study took place in regions with both Sami and non-Sami populations and had a response rate of 60.9%. Information in the SAMINOR1 study was collected using two self-administered questionnaires, clinical examination and laboratory tests. The present analysis included 15,208 men and women aged 36–79 years from the SAMINOR1 study. Results Age-standardised prevalence of pre-diabetes and diabetes mellitus among Sami men was 3.4 and 5.5%, respectively. Corresponding values for non-Sami men were 3.3 and 4.6%. Age-standardised prevalence of pre-diabetes and diabetes mellitus for Sami women was 2.7 and 4.8%, respectively, while corresponding values for non-Sami women were 2.3 and 4.5%. Relative risk ratios for dysglycaemia among Sami participants compared with non-Sami participants were significantly different in different geographical regions, with the southern region having the highest prevalence of pre-diabetes and diabetes mellitus among Sami participants. Conclusion We observed a heterogeneity in the prevalence of pre-diabetes and diabetes mellitus in different geographical regions both within and between different ethnic groups. PMID:27507149

  18. SAMI Galaxy Survey: Spectrally Dissecting 3400 Galaxies By the Dozen

    NASA Astrophysics Data System (ADS)

    Cecil, Gerald N.; Croom, S.; The SAMI Galaxy Survey Team

    2014-01-01

    More than 440 mapped, less than 3000 to go in the Sydney-AAO Multi-object IFU (SAMI) Galaxy Survey! SAMI uses novel, photonic fused-optical fiber “hexabundles” that were developed successfully at The University of Sydney and the Australian Astronomical Observatory AAO), with support from the Australian Research Council Centre of Excellence for All-Sky Astrophysics (CAASTRO). The SAMI Galaxy Survey, led by Assoc. Prof. Croom, is backed by an international team. This spectro-bolometric survey mitigates against “aperture effects” that may mislead when stacking single-fiber galaxy spectra. We seek to answer questions such as “what is the physical role of environment in galaxy evolution? How is stellar mass growth and angular momentum development related in galaxies? How does gas get into and out of galaxies, and how do such flows drive star formation?” SAMI maps stellar and gas properties with 13 integral-field units (IFU) plugged onto a dozen galaxies over the 1° field of the AAT prime-focus corrector. 78% of each bundle's area is filled by sixty-one 1.6-arcsec diameter fibers that are packed closely into concentric circles then their etched, thinned cladding is fused without deforming their cores. The fiber hexabundles route to the bench-mounted AAOmega double-beam spectrograph to cover simultaneously 373-570 nm at R=1730 and 620-735 nm at R=4500. Full spatial resolution of the observing site is recovered by dithered exposures totaling 3.5 hours per field. Target stellar masses generally exceed 108 M⊙, and span a range of environments: ˜650 are within clusters of virial mass 1014-15 M⊙ at 0.03 < z < 0.06, the rest are in the z < 0.1 field with extensive frequency data ancillary to the GAMA Survey. We display some key early results of major science themes being addressed by the SAMI survey team, from rotation curve dependence on group halo mass, through galaxy winds and AGN feedback mechanisms, to oxygen abundance gradients, kinematic decomposition

  19. "Too Hot for the Reindeer"--Voicing Sami Children's Visions of the Future

    ERIC Educational Resources Information Center

    Jonsson, Gunnar; Sarri, Carina; Alerby, Eva

    2012-01-01

    In this paper, we focus attention on the issue of the future by listening to the voices of Indigenous children in the far north of Sweden--the Sami children. The overall aim of the study is to explore the meaning of Sami children's visions of the future. The participants attend the same Sami School, and they were of the age of 9-12 years. Data…

  20. Parental values and ethnic identity in indigenous Sami families: a qualitative study.

    PubMed

    Javo, Cecilie; Alapack, Richard; Heyerdahl, Sonja; Rønning, John A

    2003-01-01

    The qualitative study reported in this article is part of a larger multimethod investigation of child-rearing practices and child-behavior problems in indigenous Sami and majority Norwegian populations in the Sami core area in Northern Norway. In the primary quantitative study we found significant ethnic differences between Sami and Norwegian parents in various areas of child rearing and family structure. Seeking the deeper cultural meaning underlying the parental practices and attitudes that had emerged in the indigenous Sami group, we performed additional indepth interviews. Four parents, selected from the sample of 134 Sami parents, served as subjects. Giorgi's descriptive phenomenological method was used. Data analysis of the interviews identified seven key consitituents of Sami child rearing, which in their interrelationships formed a common structure that constitutes the results of this study. These constituents were: (1) Independence, (2) Hardiness, (3) Autonomy, (4) Closeness/Love, (5) Sami Language, (6) Sami Traditions, and (7) Extended Family. The first four constituents are constituents pertaining to child-rearing values, while the latter three are contextual constituents, related to the promotion of ethnic identity. The study discusses the contemporary dilemmas and challenges that face Sami families in raising their children. It highlights the phenomenon of cultural transition in minority families as an important topic in family research.

  1. The SAMI Galaxy Survey: One Year, 50000 Spectra

    NASA Astrophysics Data System (ADS)

    Konstantopoulos, Iraklis; Croom, S.; The SAMI Galaxy Survey Team

    2014-01-01

    Less than a year into its operations on the Anglo-Australian Telescope, the SAMI Galaxy Survey has collected spatially resolved (IFU) spectroscopy of 440 galaxies. This breaks all previous records owing to the novel 13-fold multiplexing of the newly-designed, lightly-fused 'hexabundles' of 61 optical fibre cores that can be deployed over a degree-wide field. (Illustrations can be found in the partner poster presentation by Gerald Cecil and at http://sami-survey.org.) On our way toward the completion of a ~3000-galaxy-strong sample, that is, of order 4x105 full-optical spectra, we are working on the key scientific objectives of: (i) Mapping the mechanisms that advance and suppress the star formation process and induce morphological transformation in a variety of environments; (ii) Surveying the frequency of gas flows into and out of galaxies of all masses, and deducing the effect on gas phase metallicity and baryonic budgets; (iii) Recording the distribution of angular momentum across the local Universe, thereby advancing our understanding of how mass is built up over time. Our simulations team is working in parallel with the observers to produce mock SAMI data-cubes and interpret our results in a cosmological context. Furthermore, having selected most of our sample from the all-wavelength GAMA survey affords us access to invaluable ancillary information. The SAMI Galaxy Survey, which adds resolved stellar and gas phase kinematics, star formation rates, ionisation diagnostics, stellar ages, metallicities, and much more will provide a unique and long lasting legacy for the astronomical community.

  2. The SAMI Galaxy Survey: instrument specification and target selection

    NASA Astrophysics Data System (ADS)

    Bryant, J. J.; Owers, M. S.; Robotham, A. S. G.; Croom, S. M.; Driver, S. P.; Drinkwater, M. J.; Lorente, N. P. F.; Cortese, L.; Scott, N.; Colless, M.; Schaefer, A.; Taylor, E. N.; Konstantopoulos, I. S.; Allen, J. T.; Baldry, I.; Barnes, L.; Bauer, A. E.; Bland-Hawthorn, J.; Bloom, J. V.; Brooks, A. M.; Brough, S.; Cecil, G.; Couch, W.; Croton, D.; Davies, R.; Ellis, S.; Fogarty, L. M. R.; Foster, C.; Glazebrook, K.; Goodwin, M.; Green, A.; Gunawardhana, M. L.; Hampton, E.; Ho, I.-T.; Hopkins, A. M.; Kewley, L.; Lawrence, J. S.; Leon-Saval, S. G.; Leslie, S.; McElroy, R.; Lewis, G.; Liske, J.; López-Sánchez, Á. R.; Mahajan, S.; Medling, A. M.; Metcalfe, N.; Meyer, M.; Mould, J.; Obreschkow, D.; O'Toole, S.; Pracy, M.; Richards, S. N.; Shanks, T.; Sharp, R.; Sweet, S. M.; Thomas, A. D.; Tonini, C.; Walcher, C. J.

    2015-03-01

    The SAMI Galaxy Survey will observe 3400 galaxies with the Sydney-AAO Multi-object Integral-field spectrograph (SAMI) on the Anglo-Australian Telescope in a 3-yr survey which began in 2013. We present the throughput of the SAMI system, the science basis and specifications for the target selection, the survey observation plan and the combined properties of the selected galaxies. The survey includes four volume-limited galaxy samples based on cuts in a proxy for stellar mass, along with low-stellar-mass dwarf galaxies all selected from the Galaxy And Mass Assembly (GAMA) survey. The GAMA regions were selected because of the vast array of ancillary data available, including ultraviolet through to radio bands. These fields are on the celestial equator at 9, 12 and 14.5 h, and cover a total of 144 deg2 (in GAMA-I). Higher density environments are also included with the addition of eight clusters. The clusters have spectroscopy from 2-degree Field Galaxy Redshift Survey (2dFGRS) and Sloan Digital Sky Survey (SDSS) and photometry in regions covered by the SDSS and/or VLT Survey Telescope/ATLAS. The aim is to cover a broad range in stellar mass and environment, and therefore the primary survey targets cover redshifts 0.004 < z < 0.095, magnitudes rpet < 19.4, stellar masses 107-1012 M⊙, and environments from isolated field galaxies through groups to clusters of ˜1015 M⊙.

  3. Tromso as a "Sami Town"?--Language Ideologies, Attitudes, and Debates Surrounding Bilingual Language Policies

    ERIC Educational Resources Information Center

    Hiss, Florian

    2013-01-01

    The study focuses on local people's expressions of attitudes and ideologies in the light of proposed Sami-Norwegian bilingual policies in their Northern Norwegian hometown. The local politicians' plan to introduce the bilingual regulations of an "administrative area for the Sami language" in the town of Tromso encountered conflicting language…

  4. Ethnic Identity and Acculturation Attitudes among Indigenous Norwegian Sami and Ethnocultural Kven Adolescents

    ERIC Educational Resources Information Center

    Kvernmo, Siv; Heyerdahl, Sonja

    2004-01-01

    Ethnic identity and acculturation attitudes were studied in indigenous Sami (earlier named Lapps) and ethnocultural Kvens (descendants of early Finnish-speaking immigrants from the northern part of Sweden and Finland) in Northern Norway. The sample consisted of 674 Sami and 347 Kven high school students ages 16 to 19 years. Ethnic identity was…

  5. Socioeconomic characteristics and health outcomes in Sami speaking municipalities and a control group in northern Norway

    PubMed Central

    Norum, Jan; Nieder, Carsten

    2012-01-01

    Objectives The Sami people constitute an ethnic minority in northern Norway. The objectives of this study were to compare municipalities with a majority of Sami in the population and a control group with regard to socioeconomic factors and health outcome. Methods Original data from Statistics Norway and Directorate of health on socioeconomic factors (education, unemployment, disability, poverty) and health outcomes [total mortality, cancer specific mortality, cardiovascular disease (CVD) specific mortality] were imported from the “Health Atlas” at the Northern Norway Regional Health Authority (NNRHA) trust. The 8 municipalities in the administration area of the Sami language law (Sami-majority group – 18,868 inhabitants) was compared with a control group consisting of 11 municipalities where the Sami constitute a small minority in the population (18,931 inhabitants). Most data were from 2005 and 2008. Results There was no significant difference in socioeconomic factors. Overall, cancer- and CVD-specific mortality rates were similar in both groups. The life expectancy was significantly longer among women in the Sami-majority area (81.3 vs. 79.5 years, p=0.035) and males (74.5 vs. 72.0 years, p=0.037). Conclusion Socioeconomic factors and cause-specific mortality rate were similar in the Sami-majority group and the control group. Residents of both sexes in Sami-majority areas enjoyed longer life expectancy. PMID:22901291

  6. samiDB: A Prototype Data Archive for Big Science Exploration

    NASA Astrophysics Data System (ADS)

    Konstantopoulos, I. S.; Green, A. W.; Cortese, L.; Foster, C.; Scott, N.

    2015-04-01

    samiDB is an archive, database, and query engine to serve the spectra, spectral hypercubes, and high-level science products that make up the SAMI Galaxy Survey. Based on the versatile Hierarchical Data Format (HDF5), samiDB does not depend on relational database structures and hence lightens the setup and maintenance load imposed on science teams by metadata tables. The code, written in Python, covers the ingestion, querying, and exporting of data as well as the automatic setup of an HTML schema browser. samiDB serves as a maintenance-light data archive for Big Science and can be adopted and adapted by science teams that lack the means to hire professional archivists to set up the data back end for their projects.

  7. The health of young Swedish Sami with special reference to mental health

    PubMed Central

    Omma, Lotta; Jacobsson, Lars H.; Petersen, Solveig

    2012-01-01

    Objectives To investigate the health of young Sami in Sweden and the relationship between health and experience of negative societal treatment due to ethnicity, as well as socio-demographic background factors. Study design Cross-sectional population-based questionnaire study. Methods A total of 876 persons aged 18–28 and involved in Sami associated activities were addressed, and 516 (59%) responded to a questionnaire investigating physical health, mental health, and stress. Data were analyzed with regard to gender, family situation, occupation, education, enculturation factors and experience of being badly treated because of ethnicity. Results A majority of the young Sami reported feeling healthy, but close to half of the group reported often having worries, often forgetting things and often experiencing lack of time for doing needed things. Women and those living alone reported a more negative health. Furthermore, half of the group had perceived bad treatment because of Sami ethnicity, and this was negatively associated with some aspects of mental health. Conclusion The young Sami had a rather good and possibly slightly better health than other young Swedes, except regarding worries and stress. A high degree of bad treatment due to Sami ethnicity and its negative association with health, may partly explain the high degree of some health problems. PMID:22765937

  8. Comparison of incoherent scatter radar observations of SIMPLEX electron density depletion with SAMI2 and SAMI3 model results

    NASA Astrophysics Data System (ADS)

    Bhatt, A.; Huba, J. D.; Bernhardt, P. A.; Erickson, P. J.

    2010-12-01

    The Space Shuttle's Orbital Maneuvering System (OMS) engines have been used for active ionospheric modification experiments employing ground based ionospheric radars as diagnostic tools. These experiments initiated by the Naval Research Laboratory in 1995 have been scheduled as the Shuttle Ionospheric Modification with Pulsed Localized Exhaust or SIMPLEX through the US Dept. of Defense's Space Test Program. During 2009, two SIMPLEX experiments with the shuttles STS-119 and STS-128 were viewed by the Millstone Hill 440 MHz radar in Westford, MA operated by the MIT Haystack Observatory. The objectives of these experiments were to observe local ion-acoustic turbulence and the ionospheric density irregularities created by the exhaust injection across the magnetic field that present a Bragg scattering target for the radar. The exhaust also creates a depletion in the background electron density at F-region altitudes that persists for a relatively long time and is readily detected by an incoherent scatter radar. The OMS engine burns release 10 kg/s of H2O, CO2, H2, and N2 molecules that charge exchange with ambient O+ ions at the F region heights, producing molecular ions and the electron density depletion due to the recombination with the ambient electrons. 2009 was a year of deep solar minimum that saw the background electron density values 19% lower than were expected during a solar minimum. (Emmert et al., GRL, 2010). We believe that the long recovery time from density depletion in SIMPLEX experiments of 2009 may have a root in the unique nature of the deep solar minimum. The density whole production and recovery will be modeled using NRL SAMI2 and SAMI3 model and the results will be discussed along with the observations using the incoherent scatter radar.

  9. Sami Culture and Values: A Study of the National Mathematics Exam for the Compulsory School in Norway

    ERIC Educational Resources Information Center

    Fyhn, Anne Birgitte

    2013-01-01

    Norway ratified the ILO convention 169 concerning indigenous and tribal people in independent countries in 1990. In accordance with the convention the education programs for the Sami shall address their value systems and their cultural aspirations. Our aim is to investigate the implementation of this convention. The focus is on how Sami values are…

  10. “We are like lemmings”: making sense of the cultural meaning(s) of suicide among the indigenous Sami in Sweden

    PubMed Central

    Stoor, Jon Petter A; Kaiser, Niclas; Jacobsson, Lars; Renberg, Ellinor Salander; Silviken, Anne

    2015-01-01

    Background Suicide is a widespread problem among indigenous people residing in the circumpolar Arctic. Though the situation among the indigenous Sami in northern Scandinavia is better than among some other indigenous people, suicide is still regarded as a major public health issue. To adapt prevention strategies that are culturally attuned one must understand how suicide is understood within context. That is, the cultural meaning(s) of suicide. Objective To explore and make sense of the cultural meaning(s) of suicide among Sami in Sweden. Design Open-ended focus group discussions (FGDs) on the topic “suicide among Sami” were carried out in 5 Sami communities in Sweden, with in total 22 strategically selected Sami participants. FGDs were recorded, transcribed verbatim and analyzed through employing content analysis. Results From the FGDs 4 themes emerged including “The Sami are fighting for their culture and the herders are in the middle of the fight,” “Suicide as a consequence of Sami losing (or having lost) their identity,” “A wildfire in the Sami world” and “Difficult to get help as a Sami.” Conclusions Findings indicate that Sami in Sweden make sense of suicide in relation to power and identity within a threatened Sami cultural context. Suicide is then understood as an act that takes place and makes sense to others when a Sami no longer has the power to maintain a Sami identity, resulting in being disconnected from the Sami world and placed in an existential void where suicide is a solution. The findings are useful in development of culturally attuned suicide prevention among Sami in Sweden. PMID:26333721

  11. Languaging in Ultima Thule: Multilingualism in the Life of a Sami Boy

    ERIC Educational Resources Information Center

    Pietikainen, Sari; Alanen, Riikka; Dufva, Hannele; Kalaja, Paula; Leppanen, Sirpa; Pitkanen-Huhta, Anne

    2008-01-01

    In this paper we investigate multilingualism as a phenomenon which pervades different social and cultural levels but is manifested in the everyday life of multilingual individuals. As an illustration, we examine multilingualism from the perspective of a young Sami boy, Ante, and explore how different languages function as a complex--but at times…

  12. SAMI2-PE: A model of the ionosphere including multistream interhemispheric photoelectron transport

    NASA Astrophysics Data System (ADS)

    Varney, R. H.; Swartz, W. E.; Hysell, D. L.; Huba, J. D.

    2012-06-01

    In order to improve model comparisons with recently improved incoherent scatter radar measurements at the Jicamarca Radio Observatory we have added photoelectron transport and energy redistribution to the two dimensional SAMI2 ionospheric model. The photoelectron model uses multiple pitch angle bins, includes effects associated with curved magnetic field lines, and uses an energy degradation procedure which conserves energy on coarse, non-uniformly spaced energy grids. The photoelectron model generates secondary electron production rates and thermal electron heating rates which are then passed to the fluid equations in SAMI2. We then compare electron and ion temperatures and electron densities of this modified SAMI2 model with measurements of these parameters over a range of altitudes from 90 km to 1650 km (L = 1.26) over a 24 hour period. The new electron heating model is a significant improvement over the semi-empirical model used in SAMI2. The electron temperatures above the F-peak from the modified model qualitatively reproduce the shape of the measurements as functions of time and altitude and quantitatively agree with the measurements to within ˜30% or better during the entire day, including during the rapid temperature increase at dawn.

  13. Facing the limit of resilience: perceptions of climate change among reindeer herding Sami in Sweden

    PubMed Central

    Furberg, Maria; Evengård, Birgitta; Nilsson, Maria

    2011-01-01

    Background The Arctic area is a part of the globe where the increase in global temperature has had the earliest noticeable effect and indigenous peoples, including the Swedish reindeer herding Sami, are amongst the first to be affected by these changes. Objective To explore the experiences and perceptions of climate change among Swedish reindeer herding Sami. Study design In-depth interviews with 14 Swedish reindeer herding Sami were performed, with purposive sampling. The interviews focused on the herders experiences of climate change, observed consequences and thoughts about this. The interviews were analysed using content analysis. Results One core theme emerged from the interviews: facing the limit of resilience. Swedish reindeer-herding Sami perceive climate change as yet another stressor in their daily struggle. They have experienced severe and more rapidly shifting, unstable weather with associated changes in vegetation and alterations in the freeze–thaw cycle, all of which affect reindeer herding. The forecasts about climate change from authorities and scientists have contributed to stress and anxiety. Other societal developments have lead to decreased flexibility that obstructs adaptation. Some adaptive strategies are discordant with the traditional life of reindeer herding, and there is a fear among the Sami of being the last generation practising traditional reindeer herding. Conclusions The study illustrates the vulnerable situation of the reindeer herders and that climate change impact may have serious consequences for the trade and their overall way of life. Decision makers on all levels, both in Sweden and internationally, need improved insights into these complex issues to be able to make adequate decisions about adaptive climate change strategies. PMID:22043218

  14. Child-rearing in an indigenous Sami population in Norway: a cross-cultural comparison of parental attitudes and expectations.

    PubMed

    Javo, Cecilie; Rønning, John A; Heyerdahl, Sonja

    2004-02-01

    Semi-structured interviews of 76 Sami mothers and 58 Sami fathers, and 86 Norwegian mothers and 58 Norwegian fathers of four-year olds, revealed consistent cross-cultural differences in parenting. ANCOVA results showed that parental permissiveness was higher in the Sami group. Moreover, the effect of ethnicity was different for boys and girls (mothers' reports). Co-sleeping and self-regulation of food and sleep were commonly practiced in the Sami, but not in the Norwegian families. Sami children were more socially independent than their Norwegian peers. Indirect or internal types of control were used more by Sami parents, and they were less tolerant of child aggression, in the form of temper tantrums and displays of jealousy. These patterns are similar to those found in other indigenous cultures in the circumpolar region. The results are discussed with reference to the Individualism-Collectivism dimension. The study challenges the Individualism-Collectivism construct for apparently confounding the individualism common in European liberalism with the individual autonomy commonly encountered among hunting-gathering peoples.

  15. First Science with SAMI: A Serendipitously Discovered Galactic Wind in ESO 185-G031

    NASA Astrophysics Data System (ADS)

    Fogarty, Lisa M. R.; Bland-Hawthorn, Joss; Croom, Scott M.; Green, Andrew W.; Bryant, Julia J.; Lawrence, Jon S.; Richards, Samuel; Allen, James T.; Bauer, Amanda E.; Birchall, Michael N.; Brough, Sarah; Colless, Matthew; Ellis, Simon C.; Farrell, Tony; Goodwin, Michael; Heald, Ron; Hopkins, Andrew M.; Horton, Anthony; Jones, D. Heath; Lee, Steve; Lewis, Geraint; López-Sánchez, Ángel R.; Miziarski, Stan; Trowland, Holly; Leon-Saval, Sergio G.; Min, Seong-Sik; Trinh, Christopher; Cecil, Gerald; Veilleux, Sylvain; Kreimeyer, Kory

    2012-12-01

    We present the first scientific results from the Sydney-AAO Multi-Object IFS (SAMI) at the Anglo-Australian Telescope. This unique instrument deploys 13 fused fiber bundles (hexabundles) across a one-degree field of view allowing simultaneous spatially resolved spectroscopy of 13 galaxies. During the first SAMI commissioning run, targeting a single galaxy field, one object (ESO 185-G031) was found to have extended minor axis emission with ionization and kinematic properties consistent with a large-scale galactic wind. The importance of this result is twofold: (1) fiber bundle spectrographs are able to identify low surface brightness emission arising from extranuclear activity and (2) such activity may be more common than presently assumed because conventional multi-object spectrographs use single-aperture fibers and spectra from these are nearly always dominated by nuclear emission. These early results demonstrate the extraordinary potential of multi-object hexabundle spectroscopy in future galaxy surveys.

  16. Modeling study of the mid-latitude ionospheric nighttime electron density enhancement by SAMI3

    NASA Astrophysics Data System (ADS)

    Chen, C.; Huba, J. D.; Saito, A.; Lin, C.; Liu, J. G.; Chang, L. C.

    2012-12-01

    The mid-latitude summer nighttime anomaly (MSNA) is a feature that the nighttime electron density is larger than in the daytime around the mid-latitude ionosphere. This anomaly was first detected in the southern hemisphere five decades ago and reported in the northern hemisphere recently. Previous studies presented the electron density structure of MSNA by satellite observation data and found that MSNA is clearly seen at 300 km altitude during local summer around South American, European, and Northeast Asian regions. A three-dimensional self-consistent model, SAMI3 (Sami3 is Also a Model of the Ionosphere), with inputting neutral wind data from TIEGCM (Thermosphere Ionosphere Electrodynamics General Circulation Model) model is used to simulate the MSNA feature and further discuss its mechanisms. The comparisons between observation data and the model simulation results suggest that the equatorial neutral winds play the most important role in the formation of MSNA.

  17. The SAMI Galaxy Survey: A prototype data archive for Big Science exploration

    NASA Astrophysics Data System (ADS)

    Konstantopoulos, I. S.; Green, A. W.; Foster, C.; Scott, N.; Allen, J. T.; Fogarty, L. M. R.; Lorente, N. P. F.; Sweet, S. M.; Hopkins, A. M.; Bland-Hawthorn, J.; Bryant, J. J.; Croom, S. M.; Goodwin, M.; Lawrence, J. S.; Owers, M. S.; Richards, S. N.

    2015-11-01

    We describe the data archive and database for the SAMI Galaxy Survey, an ongoing observational program that will cover ≈3400 galaxies with integral-field (spatially-resolved) spectroscopy. Amounting to some three million spectra, this is the largest sample of its kind to date. The data archive and built-in query engine use the versatile Hierarchical Data Format (HDF5), which precludes the need for external metadata tables and hence the setup and maintenance overhead those carry. The code produces simple outputs that can easily be translated to plots and tables, and the combination of these tools makes for a light system that can handle heavy data. This article acts as a contextual companion to the SAMI Survey Database source code repository, samiDB, which is freely available online and written entirely in Python. We also discuss the decisions related to the selection of tools and the creation of data visualisation modules. It is our aim that the work presented in this article-descriptions, rationale, and source code-will be of use to scientists looking to set up a maintenance-light data archive for a Big Science data load.

  18. The SAMI Galaxy Survey: cubism and covariance, putting round pegs into square holes

    NASA Astrophysics Data System (ADS)

    Sharp, R.; Allen, J. T.; Fogarty, L. M. R.; Croom, S. M.; Cortese, L.; Green, A. W.; Nielsen, J.; Richards, S. N.; Scott, N.; Taylor, E. N.; Barnes, L. A.; Bauer, A. E.; Birchall, M.; Bland-Hawthorn, J.; Bloom, J. V.; Brough, S.; Bryant, J. J.; Cecil, G. N.; Colless, M.; Couch, W. J.; Drinkwater, M. J.; Driver, S.; Foster, C.; Goodwin, M.; Gunawardhana, M. L. P.; Ho, I.-T.; Hampton, E. J.; Hopkins, A. M.; Jones, H.; Konstantopoulos, I. S.; Lawrence, J. S.; Leslie, S. K.; Lewis, G. F.; Liske, J.; López-Sánchez, Á. R.; Lorente, N. P. F.; McElroy, R.; Medling, A. M.; Mahajan, S.; Mould, J.; Parker, Q.; Pracy, M. B.; Obreschkow, D.; Owers, M. S.; Schaefer, A. L.; Sweet, S. M.; Thomas, A. D.; Tonini, C.; Walcher, C. J.

    2015-01-01

    We present a methodology for the regularization and combination of sparse sampled and irregularly gridded observations from fibre-optic multiobject integral field spectroscopy. The approach minimizes interpolation and retains image resolution on combining subpixel dithered data. We discuss the methodology in the context of the Sydney-AAO multiobject integral field spectrograph (SAMI) Galaxy Survey underway at the Anglo-Australian Telescope. The SAMI instrument uses 13 fibre bundles to perform high-multiplex integral field spectroscopy across a 1° diameter field of view. The SAMI Galaxy Survey is targeting ˜3000 galaxies drawn from the full range of galaxy environments. We demonstrate the subcritical sampling of the seeing and incomplete fill factor for the integral field bundles results in only a 10 per cent degradation in the final image resolution recovered. We also implement a new methodology for tracking covariance between elements of the resulting data cubes which retains 90 per cent of the covariance information while incurring only a modest increase in the survey data volume.

  19. SAMI3/SD-WACCM-X simulations of ionospheric variability during northern winter 2009

    NASA Astrophysics Data System (ADS)

    McDonald, S. E.; Sassi, F.; Mannucci, A. J.

    2015-09-01

    We have performed simulations using the Naval Research Laboratory's physics-based model of the ionosphere, Sami3 is A Model of the Ionosphere (SAMI3), to illustrate how neutral wind dynamics is responsible for day-to-day variability of the ionosphere. We have used neutral winds specified from the extended version of the specified dynamics Whole Atmosphere Community Climate Model (SD-WACCM-X), in which meteorology below 92 km is constrained by atmospheric specifications from an operational weather forecast model and reanalysis. To assess the realism of the simulations against observations, we have carried out a case study during January-February 2009, a dynamically disturbed time characterized by a sudden stratospheric warming (SSW) commencing 24 January 2009. Model results are compared with total electron content (TEC) from Jet Propulsion Laboratory global ionospheric maps. We show that SAMI3/SD-WACCM-X captures longitudinal variability in the equatorial ionization anomaly associated with nonmigrating tides, with strongest contributions coming from the diurnal eastward wave number 2 (DE2) and DE3. Both migrating and nonmigrating tides contribute to significant day-to-day variability, with TEC varying up to 16%. Our simulation during the SSW period reveals that at the Jicamarca longitude (285°E) on 27 January 2009 nonmigrating tides contribute to an enhancement of the electron density in the morning followed by a decrease in the afternoon. An enhancement of the semidiurnal eastward wave number 2 (SE2) and SE3 nonmigrating tides, likely associated with the appearance of the SSW, suggests that these tides increase the longitudinal variability of the SSW impact on the ionosphere. The conclusion is that realistic meteorology propagating upward from the lower atmosphere influences the dynamo region and reproduces aspects of the observed variability in the ionosphere.

  20. The Impact of a Ligand Binding on Strand Migration in the SAM-I Riboswitch

    PubMed Central

    Huang, Wei; Kim, Joohyun; Jha, Shantenu; Aboul-ela, Fareed

    2013-01-01

    Riboswitches sense cellular concentrations of small molecules and use this information to adjust synthesis rates of related metabolites. Riboswitches include an aptamer domain to detect the ligand and an expression platform to control gene expression. Previous structural studies of riboswitches largely focused on aptamers, truncating the expression domain to suppress conformational switching. To link ligand/aptamer binding to conformational switching, we constructed models of an S-adenosyl methionine (SAM)-I riboswitch RNA segment incorporating elements of the expression platform, allowing formation of an antiterminator (AT) helix. Using Anton, a computer specially developed for long timescale Molecular Dynamics (MD), we simulated an extended (three microseconds) MD trajectory with SAM bound to a modeled riboswitch RNA segment. Remarkably, we observed a strand migration, converting three base pairs from an antiterminator (AT) helix, characteristic of the transcription ON state, to a P1 helix, characteristic of the OFF state. This conformational switching towards the OFF state is observed only in the presence of SAM. Among seven extended trajectories with three starting structures, the presence of SAM enhances the trend towards the OFF state for two out of three starting structures tested. Our simulation provides a visual demonstration of how a small molecule (<500 MW) binding to a limited surface can trigger a large scale conformational rearrangement in a 40 kDa RNA by perturbing the Free Energy Landscape. Such a mechanism can explain minimal requirements for SAM binding and transcription termination for SAM-I riboswitches previously reported experimentally. PMID:23704854

  1. Development of a Field-Aligned Integrated Conductivity Model Using the SAMI2 Open Source Code

    NASA Astrophysics Data System (ADS)

    Hildebrandt, Kyle; Gearheart, Michael; West, Keith

    2003-03-01

    The SAMI2 open source code is a middle and low latitude ionspheric model developed by the Naval Research Lab for the dual purposes of research and education. At the time of this writing the source code has no component for the integrated magnetic field-aligned conductivity. The dependence of human activities on conditions in the space environment, such as communications, has grown and will continue to do so. With this growth comes higher financial stakes, as changes in the space environment have greater economic impact. In order to minimize the adverse effects of these changes, predictive models are being developed. Among the geophysical parameters that affect communications is the conductivity in the ionosphere. As part of the commitment of Texas A & M Univeristy-Commerce to build a strong undergraduate research program, a team consisting of two students and a faculty mentor are developing a model of the integrated field-aligned conductivity using the SAMI2 code. The current status of the research and preliminary results are presented as well as a summary of future work.

  2. Thermospheric tidal effects on the ionospheric midlatitude summer nighttime anomaly using SAMI3 and TIEGCM

    NASA Astrophysics Data System (ADS)

    Chen, C. H.; Lin, C. H.; Chang, L. C.; Huba, J. D.; Lin, J. T.; Saito, A.; Liu, J. Y.

    2013-06-01

    This paper is the first study to employ a three-dimensional physics-based ionosphere model, SAMI3, coupled with the National Center for Atmospheric Research Thermosphere Ionosphere Electrodynamics General Circulation Model (TIEGCM) and Global Scale Wave Model to simulate the mesospheric and lower thermospheric tidal effects on the development of midlatitude summer nighttime anomaly (MSNA). Using this coupled model, the diurnal variation of MSNA electron densities at 300 km altitude is simulated on both June solstice (day of year (DOY) 167) and December solstice (DOY 350) in 2007. Results show successful reproduction of the southern hemisphere MSNA structure including the eastward drift feature of the southern MSNA, which is not reproduced by the default SAMI3 runs using the neutral winds provided by the empirical Horizontal Wind Model 93 neutral wind model. A linear least squares algorithm for extracting tidal components is utilized to examine the major tidal component affecting the variation of southern MSNA. Results show that the standing diurnal oscillation component dominates the vertical neutral wind manifesting as a diurnal eastward wave-1 drift of the southern MSNA in the local time frame. We also find that the stationary planetary wave-1 component of vertical neutral wind can cause diurnal variation of the summer nighttime electron density enhancement around the midlatitude ionosphere.

  3. The SAMI Pilot Survey: stellar kinematics of galaxies in Abell 85, 168 and 2399

    NASA Astrophysics Data System (ADS)

    Fogarty, L. M. R.; Scott, N.; Owers, M. S.; Croom, S. M.; Bekki, K.; Houghton, R. C. W.; van de Sande, J.; D'Eugenio, F.; Cecil, G. N.; Colless, M. M.; Bland-Hawthorn, J.; Brough, S.; Cortese, L.; Davies, R. L.; Jones, D. H.; Pracy, M.; Allen, J. T.; Bryant, J. J.; Goodwin, M.; Green, A. W.; Konstantopoulos, I. S.; Lawrence, J. S.; Lorente, N. P. F.; Richards, S.; Sharp, R. G.

    2015-12-01

    We present the SAMI Pilot Survey, consisting of integral field spectroscopy of 106 galaxies across three galaxy clusters, Abell 85, Abell 168 and Abell 2399. The galaxies were selected by absolute magnitude to have Mr < -20.25 mag. The survey, using the Sydney-AAO Multi-object Integral field spectrograph (SAMI), comprises observations of galaxies of all morphological types with 75 per cent of the sample being early-type galaxies (ETGs) and 25 per cent being late-type galaxies (LTGs). Stellar velocity and velocity dispersion maps are derived for all 106 galaxies in the sample. The λR parameter, a proxy for the specific stellar angular momentum, is calculated for each galaxy in the sample. We find a trend between λR and galaxy concentration such that LTGs are less concentrated higher angular momentum systems, with the fast-rotating ETGs (FRs) more concentrated and lower in angular momentum. This suggests that some dynamical processes are involved in transforming LTGs to FRs, though a significant overlap between the λR distributions of these classes of galaxies implies that this is just one piece of a more complicated picture. We measure the kinematic misalignment angle, Ψ, for the ETGs in the sample, to probe the intrinsic shapes of the galaxies. We find the majority of FRs (83 per cent) to be aligned, consistent with them being oblate spheroids (i.e. discs). The slow rotating ETGs (SRs), on the other hand, are significantly more likely to show kinematic misalignment (only 38 per cent are aligned). This confirms previous results that SRs are likely to be mildly triaxial systems.

  4. The SAMI Galaxy Survey: gas streaming and dynamical M/L in rotationally supported systems

    NASA Astrophysics Data System (ADS)

    Cecil, G.; Fogarty, L. M. R.; Richards, S.; Bland-Hawthorn, J.; Lange, R.; Moffett, A.; Catinella, B.; Cortese, L.; Ho, I.-T.; Taylor, E. N.; Bryant, J. J.; Allen, J. T.; Sweet, S. M.; Croom, S. M.; Driver, S. P.; Goodwin, M.; Kelvin, L.; Green, A. W.; Konstantopoulos, I. S.; Owers, M. S.; Lawrence, J. S.; Lorente, N. P. F.

    2016-02-01

    Line-of-sight velocities of gas and stars can constrain dark matter (DM) within rotationally supported galaxies if they trace circular orbits extensively. Photometric asymmetries may signify non-circular motions, requiring spectra with dense spatial coverage. Our integral-field spectroscopy of 178 galaxies spanned the mass range of the Sydney-AAO Multi-object integral field spectrograph (SAMI) Galaxy Survey. We derived circular speed curves (CSCs) of gas and stars from non-parametric fits out to r ˜ 2re. For 12/14 with measured H I profiles, ionized gas and H I maximum velocities agreed. We fitted mass-follows-light models to 163 galaxies by approximating the radial light profile as nested, very flattened mass homeoids viewed as a Sérsic form. Fitting broad-band spectral energy distributions to Sloan Digital Sky Survey images gave median stellar mass/light 1.7 assuming a Kroupa initial mass function (IMF) versus 2.6 dynamically. Two-thirds of the dynamical mass/light measures were consistent with star+remnant IMFs. One-fifth required upscaled starlight to fit, hence comparable mass of unobserved baryons and/or DM distributed like starlight across the SAMI aperture that came to dominate motions as the starlight CSCs declined rapidly. The rest had mass distributed differently from light. Subtracting fits of Sérsic radial profiles to 13 VIKING Z-band images revealed residual weak bars. Near the bar major axis, we assessed m = 2 streaming velocities, and found deviations usually <30 km s-1 from the CSC; three showed no deviation. Thus, asymmetries rarely influenced the CSC despite colocated shock-indicating, emission-line flux ratios in more than 2/3 of our sample.

  5. Incentives and regulations to reconcile conservation and development: thirty years of governance of the Sami pastoral ecosystem in Finnmark, Norway.

    PubMed

    Ulvevadet, Birgitte; Hausner, Vera H

    2011-10-01

    Incentive-based mechanisms are regarded as efficient instruments to reconcile conservation and development. This win-win objective has been difficult to accomplish; cross-compliance has, therefore, been suggested as a mechanism to ensure sustainability. Cross-compliance, which requires producers to conform to production regulations and environmental standards to qualify for direct payments, has been a popular instrument in the Common Agricultural Policy (CAP) reform. Since 1990, cross-compliance has been the main characteristic of policy design in Sami reindeer husbandry in Finnmark, Norway. All direct transfers to the Sami pastoralists have been connected to harvesting demands to decrease the number of reindeer and to conserve pastures. The content of these incentive-based mechanisms are decided through negotiated agreements with the Sami Reindeer Herders' Association of Norway (NRL), and the regulation of reindeer numbers and access to pastures are delegated to co-management boards. Despite the participation of the Sami pastoralists in shaping these policies, win-win objectives have not been achieved. Although the cross-compliance program could have been improved by payment for graded results, the lack of regulations by the administration or co-management boards is more likely to be the cause of failure to reach sustainability. Despite the long-term failures of the cross-compliance program, policies have been slow to change. We might attribute this delay to the NRL's strong position in the negotiated agreements. In general, we argue that the success of the cross-compliance program depends on a well-functioning governance system that can implement regulations and sanctions if incentives do not work as intended.

  6. Ethnic discrimination and health: the relationship between experienced ethnic discrimination and multiple health domains in Norway's rural Sami population

    PubMed Central

    Hansen, Ketil Lenert

    2015-01-01

    Objective Self-reported ethnic discrimination has been associated with a range of health outcomes. This study builds on previous efforts to investigate the prevalence of self-reported ethnic discrimination in the indigenous (Sami) population, and how such discrimination may be associated with key health indicators. Study design The study relies on data from the 2003/2004 (n=4,389) population-based study of adults (aged 36–79 years) in 24 rural municipalities of Central and North Norway (the SAMINOR study). Self-reported ethnic discrimination was measured using the question: “Have you ever experienced discrimination due to your ethnic background?” Health indicators included questions regarding cardiovascular disease, diabetes, chronic muscle pain, metabolic syndrome and obesity. Logistic regression was applied to examine the relationship between self-reported ethnic discrimination and health outcomes. Results The study finds that for Sami people living in minority areas, self-reported ethnic discrimination is associated with all the negative health indicators included in the study. Conclusion We conclude that ethnic discrimination affects a wide range of health outcomes. Our findings highlight the importance of ensuring freedom from discrimination for the Sami people of Norway. PMID:25683064

  7. Conformational heterogeneity of the SAM-I riboswitch transcriptional ON state: a chaperone-like role for S-adenosyl methionine.

    PubMed

    Huang, Wei; Kim, Joohyun; Jha, Shantenu; Aboul-Ela, Fareed

    2012-05-18

    Riboswitches are promising targets for the design of novel antibiotics and engineering of portable genetic regulatory elements. There is evidence that variability in riboswitch properties allows tuning of expression for genes involved in different stages of biosynthetic pathways by mechanisms that are not currently understood. Here, we explore the mechanism for tuning of S-adenosyl methionine (SAM)-I riboswitch folding. Most SAM-I riboswitches function at the transcriptional level by sensing the cognate ligand SAM. SAM-I riboswitches orchestrate the biosynthetic pathways of cysteine, methionine, SAM, and so forth. We use base-pair probability predictions to examine the secondary-structure folding landscape of several SAM-I riboswitch sequences. We predict different folding behaviors for different SAM-I riboswitch sequences. We identify several "decoy" base-pairing interactions involving 5' riboswitch residues that can compete with the formation of a P1 helix, a component of the ligand-bound "transcription OFF" state, in the absence of SAM. We hypothesize that blockage of these interactions through SAM contacts contributes to stabilization of the OFF state in the presence of ligand. We also probe folding patterns for a SAM-I riboswitch RNA using constructs with different 3' truncation points experimentally. Folding was monitored through fluorescence, susceptibility to base-catalyzed cleavage, nuclear magnetic resonance, and indirectly through SAM binding. We identify key decision windows at which SAM can affect the folding pathway towards the OFF state. The presence of decoy conformations and differential sensitivities to SAM at different transcript lengths is crucial for SAM-I riboswitches to modulate gene expression in the context of global cellular metabolism.

  8. Conformational heterogeneity of the SAM-I riboswitch transcriptional ON state: a chaperone-like role for S-adenosyl methionine.

    PubMed

    Huang, Wei; Kim, Joohyun; Jha, Shantenu; Aboul-Ela, Fareed

    2012-05-18

    Riboswitches are promising targets for the design of novel antibiotics and engineering of portable genetic regulatory elements. There is evidence that variability in riboswitch properties allows tuning of expression for genes involved in different stages of biosynthetic pathways by mechanisms that are not currently understood. Here, we explore the mechanism for tuning of S-adenosyl methionine (SAM)-I riboswitch folding. Most SAM-I riboswitches function at the transcriptional level by sensing the cognate ligand SAM. SAM-I riboswitches orchestrate the biosynthetic pathways of cysteine, methionine, SAM, and so forth. We use base-pair probability predictions to examine the secondary-structure folding landscape of several SAM-I riboswitch sequences. We predict different folding behaviors for different SAM-I riboswitch sequences. We identify several "decoy" base-pairing interactions involving 5' riboswitch residues that can compete with the formation of a P1 helix, a component of the ligand-bound "transcription OFF" state, in the absence of SAM. We hypothesize that blockage of these interactions through SAM contacts contributes to stabilization of the OFF state in the presence of ligand. We also probe folding patterns for a SAM-I riboswitch RNA using constructs with different 3' truncation points experimentally. Folding was monitored through fluorescence, susceptibility to base-catalyzed cleavage, nuclear magnetic resonance, and indirectly through SAM binding. We identify key decision windows at which SAM can affect the folding pathway towards the OFF state. The presence of decoy conformations and differential sensitivities to SAM at different transcript lengths is crucial for SAM-I riboswitches to modulate gene expression in the context of global cellular metabolism. PMID:22425639

  9. A conversation with John B. Fenn. Interview by M. Samy El-Shall.

    PubMed

    Fenn, John B

    2009-01-01

    Editor's Note: Every year, the Editorial Committee of each Annual Reviews series asks an internationally distinguished researcher to prepare a prefatory article for the volume being planned. It was an easy choice for us to seek a contribution from John B. Fenn (b. 1917), who since 1994 has been a professor of analytical chemistry at Virginia Commonwealth University in Richmond, Virginia. Few people have achieved the originality and the impact that John Fenn has shown in his development of new instruments for chemical analysis. Anyone using supersonic jet expansions or electrospray ionization owes a huge debt to this special individual, who was awarded the Nobel Prize in Chemistry in 2002. A full account of the development of electrospray ionization may be found in Fenn's 2002 article in the Journal of Biomolecular Techniques (see Related Resources at the end of the interview). What follows is a transcript of an interview that Fenn's colleague Professor Samy El-Shall kindly conducted on our behalf. This interview captures the spirit and the imagination of this singular individual. It also shows that the path to discovery is seldom straight and narrow. -Richard N. Zare. PMID:20636051

  10. Discrimination between closely related cellular metabolites by the SAM-I riboswitch.

    PubMed

    Montange, Rebecca K; Mondragón, Estefanía; van Tyne, Daria; Garst, Andrew D; Ceres, Pablo; Batey, Robert T

    2010-02-26

    The SAM-I riboswitch is a cis-acting element of genetic control found in bacterial mRNAs that specifically binds S-adenosylmethionine (SAM). We previously determined the 2.9-A X-ray crystal structure of the effector-binding domain of this RNA element, revealing details of RNA-ligand recognition. To improve this structure, variations were made to the RNA sequence to alter lattice contacts, resulting in a 0.5-A improvement in crystallographic resolution and allowing for a more accurate refinement of the crystallographic model. The basis for SAM specificity was addressed by a structural analysis of the RNA complexed to S-adenosylhomocysteine (SAH) and sinefungin and by measuring the affinity of SAM and SAH for a series of mutants using isothermal titration calorimetry. These data illustrate the importance of two universally conserved base pairs in the RNA that form electrostatic interactions with the positively charged sulfonium group of SAM, thereby providing a basis for discrimination between SAM and SAH. PMID:20006621

  11. Discrimination between Closely Related Cellular Metabolites by the SAM-I Riboswitch

    PubMed Central

    Montange, Rebecca K.; Mondragón, Estefanía; van Tyne, Daria; Garst, Andrew D.; Ceres, Pablo; Batey, Robert T.

    2009-01-01

    The SAM-I riboswitch is a cis-acting element of genetic control found in bacterial mRNAs that specifically binds S-adenosylmethionine (SAM). We previously determined the 2.9-Å X-ray crystal structure of the effector-binding domain of this RNA element, revealing details of RNA–ligand recognition. To improve this structure, variations were made to the RNA sequence to alter lattice contacts, resulting in a 0.5-Å improvement in crystallographic resolution and allowing for a more accurate refinement of the crystallographic model. The basis for SAM specificity was addressed by a structural analysis of the RNA complexed to S-adenosylhomocysteine (SAH) and sinefungin and by measuring the affinity of SAM and SAH for a series of mutants using isothermal titration calorimetry. These data illustrate the importance of two universally conserved base pairs in the RNA that form electrostatic interactions with the positively charged sulfonium group of SAM, thereby providing a basis for discrimination between SAM and SAH. PMID:20006621

  12. Discrimination between Closely Related Cellular Metabolites by the SAM-I Riboswitch

    SciTech Connect

    Montange, R.; Mondragon, E; van Tyne, D; Garst, A; Ceres, P; Batey, R

    2010-01-01

    The SAM-I riboswitch is a cis-acting element of genetic control found in bacterial mRNAs that specifically binds S-adenosylmethionine (SAM). We previously determined the 2.9-{angstrom} X-ray crystal structure of the effector-binding domain of this RNA element, revealing details of RNA-ligand recognition. To improve this structure, variations were made to the RNA sequence to alter lattice contacts, resulting in a 0.5-{angstrom} improvement in crystallographic resolution and allowing for a more accurate refinement of the crystallographic model. The basis for SAM specificity was addressed by a structural analysis of the RNA complexed to S-adenosylhomocysteine (SAH) and sinefungin and by measuring the affinity of SAM and SAH for a series of mutants using isothermal titration calorimetry. These data illustrate the importance of two universally conserved base pairs in the RNA that form electrostatic interactions with the positively charged sulfonium group of SAM, thereby providing a basis for discrimination between SAM and SAH.

  13. The SAMI Galaxy Survey: the link between angular momentum and optical morphology

    NASA Astrophysics Data System (ADS)

    Cortese, L.; Fogarty, L. M. R.; Bekki, K.; van de Sande, J.; Couch, W.; Catinella, B.; Colless, M.; Obreschkow, D.; Taranu, D.; Tescari, E.; Barat, D.; Bland-Hawthorn, J.; Bloom, J.; Bryant, J. J.; Cluver, M.; Croom, S. M.; Drinkwater, M. J.; d'Eugenio, F.; Konstantopoulos, I. S.; Lopez-Sanchez, A.; Mahajan, S.; Scott, N.; Tonini, C.; Wong, O. I.; Allen, J. T.; Brough, S.; Goodwin, M.; Green, A. W.; Ho, I.-T.; Kelvin, L. S.; Lawrence, J. S.; Lorente, N. P. F.; Medling, A. M.; Owers, M. S.; Richards, S.; Sharp, R.; Sweet, S. M.

    2016-08-01

    We investigate the relationship between stellar and gas specific angular momentum j, stellar mass M★ and optical morphology for a sample of 488 galaxies extracted from the SAMI Galaxy Survey. We find that j, measured within one effective radius, monotonically increases with M★ and that, for M★ > 109.5 M⊙, the scatter in this relation strongly correlates with optical morphology (i.e., visual classification and Sérsic index). These findings confirm that massive galaxies of all types lie on a plane relating mass, angular momentum and stellar light distribution, and suggest that the large-scale morphology of a galaxy is regulated by its mass and dynamical state. We show that the significant scatter in the M★ - j relation is accounted for by the fact that, at fixed stellar mass, the contribution of ordered motions to the dynamical support of galaxies varies by at least a factor of three. Indeed, the stellar spin parameter (quantified via λR) correlates strongly with Sérsic and concentration indices. This correlation is particularly strong once slow-rotators are removed from the sample, showing that late-type galaxies and early-type fast rotators form a continuous class of objects in terms of their kinematic properties.

  14. The SAMI Galaxy Survey: can we trust aperture corrections to predict star formation?

    NASA Astrophysics Data System (ADS)

    Richards, S. N.; Bryant, J. J.; Croom, S. M.; Hopkins, A. M.; Schaefer, A. L.; Bland-Hawthorn, J.; Allen, J. T.; Brough, S.; Cecil, G.; Cortese, L.; Fogarty, L. M. R.; Gunawardhana, M. L. P.; Goodwin, M.; Green, A. W.; Ho, I.-T.; Kewley, L. J.; Konstantopoulos, I. S.; Lawrence, J. S.; Lorente, N. P. F.; Medling, A. M.; Owers, M. S.; Sharp, R.; Sweet, S. M.; Taylor, E. N.

    2016-01-01

    In the low-redshift Universe (z < 0.3), our view of galaxy evolution is primarily based on fibre optic spectroscopy surveys. Elaborate methods have been developed to address aperture effects when fixed aperture sizes only probe the inner regions for galaxies of ever decreasing redshift or increasing physical size. These aperture corrections rely on assumptions about the physical properties of galaxies. The adequacy of these aperture corrections can be tested with integral-field spectroscopic data. We use integral-field spectra drawn from 1212 galaxies observed as part of the SAMI Galaxy Survey to investigate the validity of two aperture correction methods that attempt to estimate a galaxy's total instantaneous star formation rate. We show that biases arise when assuming that instantaneous star formation is traced by broad-band imaging, and when the aperture correction is built only from spectra of the nuclear region of galaxies. These biases may be significant depending on the selection criteria of a survey sample. Understanding the sensitivities of these aperture corrections is essential for correct handling of systematic errors in galaxy evolution studies.

  15. Structure-guided design of fluorescent S-adenosylmethionine analogs for a high-throughput screen to target SAM-I riboswitch RNAs

    PubMed Central

    Hickey, Scott F.; Hammond, Ming C.

    2014-01-01

    Summary Many classes of S-adenosylmethionine (SAM)-binding RNAs and proteins are of interest as potential drug targets in diverse therapeutic areas, from infectious diseases to cancer. In the former case, the SAM-I riboswitch is an attractive target because this structured RNA element is found only in bacterial mRNAs and regulates multiple genes in several human pathogens. Here we describe the synthesis of stable and fluorescent analogs of SAM in which the fluorophore is introduced through a functionalizable linker to the ribose. A Cy5-labeled SAM analog was shown to bind several SAM-I riboswitches via in-line probing and fluorescence polarization (FP) assays, including one from Staphylococcus aureus that controls the expression of SAM synthetase in this organism. A fluorescent ligand displacement assay was developed and validated for high-throughput screening of compounds to target the SAM-I riboswitch class. PMID:24560607

  16. Basis for ligand discrimination between ON and OFF state riboswitch conformations: the case of the SAM-I riboswitch.

    PubMed

    Boyapati, Vamsi Krishna; Huang, Wei; Spedale, Jessica; Aboul-Ela, Fareed

    2012-06-01

    Riboswitches are RNA elements that bind to effector ligands and control gene expression. Most consist of two domains. S-Adenosyl Methionine (SAM) binds the aptamer domain of the SAM-I riboswitch and induces conformational changes in the expression domain to form an intrinsic terminator (transcription OFF state). Without SAM the riboswitch forms the transcription ON state, allowing read-through transcription. The mechanistic link between the SAM/aptamer recognition event and subsequent secondary structure rearrangement by the riboswitch is unclear. We probed for those structural features of the Bacillus subtilis yitJ SAM-I riboswitch responsible for discrimination between the ON and OFF states by SAM. We designed SAM-I riboswitch RNA segments forming "hybrid" structures of the ON and OFF states. The choice of segment constrains the formation of a partial P1 helix, characteristic of the OFF state, together with a partial antiterminator (AT) helix, characteristic of the ON state. For most choices of P1 vs. AT helix lengths, SAM binds with micromolar affinity according to equilibrium dialysis. Mutational analysis and in-line probing confirm that the mode of SAM binding by hybrid structures is similar to that of the aptamer. Altogether, binding measurements and in-line probing are consistent with the hypothesis that when SAM is present, stacking interactions with the AT helix stabilize a partially formed P1 helix in the hybrids. Molecular modeling indicates that continuous stacking between the P1 and the AT helices is plausible with SAM bound. Our findings raise the possibility that conformational intermediates may play a role in ligand-induced aptamer folding.

  17. Comparisons of the NRL SAMI3 Physics-Based Ionospheric Model with Global Ionosonde and GPS Electron Density Measurements

    NASA Astrophysics Data System (ADS)

    Siefring, C. L.; Tondwalkar, A.; McDonald, S. E.; Huba, J. D.; Krall, J.; Emmert, J. T.; Drob, D. P.; Lean, J.; Bernhardt, P. A.

    2014-12-01

    The Naval Research Laboratory is conducting an interdisciplinary physics-based Space Weather model development and validation program called the Integrated Sun-Earth System for the Operational Environment (ISES-OE). In contrast to other geospace integration efforts, a key aspect of ISES is determining the extent to which current models capture the climate of the ionosphere and thermosphere. Until now, complementary long-term simulations using physics-based ionosphere models have not been performed. As part of this program, numerous runs of the physics-based SAMI3 model have been made and compared to global measurements of electron density. The data sets includes: 1) Ionosonde NmF2 and hmF2 measurements, 2) GPS Total Electron Content (TEC) measurements and others. This presentation compares electron density data with SAMI3 and other models during much of Solar Cycle 23 and the ascending phase of Cycle 24. Previous work has concentrated on the Whole Heliospheric Interval (WHI) from February 19 - April 19, 2008 [Lean et al., 2014]. This solar minimum period with extremely low solar activity was used to test the validity of the SAMI3 simulations of the base-state ionosphere. Several modifications to SAMI3 were incorporated including updates to the Solar EUV fluxes, the NRL MSIS neutral atmospheric model parameterization at Solar Minimum and compensating for variations in the Sun-to-Earth distance. Data and model comparisons during times of higher solar activity will be presented with an emphasis on understanding the effects of coupling of the neutral atmosphere, neutral winds and driving electric fields on our ability to model the measured global electron density data. We examine responses to solar EUV radiation and geomagnetic activity, and semiannual and annual oscillations that all induce geospace variability. Lean, J. L., S. E. McDonald, J. D. Huba, J. T. Emmert, D. P. Drob, and C. L. Siefring (2014), Geospace variability during the 2008-2009 Whole Heliosphere

  18. The SAMI Galaxy Survey: extraplanar gas, galactic winds and their association with star formation history

    NASA Astrophysics Data System (ADS)

    Ho, I.-Ting; Medling, Anne M.; Bland-Hawthorn, Joss; Groves, Brent; Kewley, Lisa J.; Kobayashi, Chiaki; Dopita, Michael A.; Leslie, Sarah K.; Sharp, Rob; Allen, James T.; Bourne, Nathan; Bryant, Julia J.; Cortese, Luca; Croom, Scott M.; Dunne, Loretta; Fogarty, L. M. R.; Goodwin, Michael; Green, Andy W.; Konstantopoulos, Iraklis S.; Lawrence, Jon S.; Lorente, Nuria P. F.; Owers, Matt S.; Richards, Samuel; Sweet, Sarah M.; Tescari, Edoardo; Valiante, Elisabetta

    2016-04-01

    We investigate a sample of 40 local, main-sequence, edge-on disc galaxies using integral field spectroscopy with the Sydney-AAO Multi-object Integral field spectrograph (SAMI) Galaxy Survey to understand the link between properties of the extraplanar gas and their host galaxies. The kinematics properties of the extraplanar gas, including velocity asymmetries and increased dispersion, are used to differentiate galaxies hosting large-scale galactic winds from those dominated by the extended diffuse ionized gas. We find rather that a spectrum of diffuse gas-dominated to wind-dominated galaxies exist. The wind-dominated galaxies span a wide range of star formation rates (SFRs; -1 ≲ log (SFR/M⊙ yr-1) ≲ 0.5) across the whole stellar mass range of the sample (8.5 ≲ log (M*/M⊙) ≲ 11). The wind galaxies also span a wide range in SFR surface densities (10- 3-10- 1.5 M⊙ yr- 1 kpc- 2) that is much lower than the canonical threshold of 0.1 M⊙ yr- 1 kpc- 2. The wind galaxies on average have higher SFR surface densities and higher HδA values than those without strong wind signatures. The enhanced HδA indicates that bursts of star formation in the recent past are necessary for driving large-scale galactic winds. We demonstrate with Sloan Digital Sky Survey data that galaxies with high SFR surface density have experienced bursts of star formation in the recent past. Our results imply that the galactic winds revealed in our study are indeed driven by bursts of star formation, and thus probing star formation in the time domain is crucial for finding and understanding galactic winds.

  19. The SAMI Galaxy Survey: Spatially resolving the environmental quenching of star formation in GAMA galaxies

    NASA Astrophysics Data System (ADS)

    Schaefer, A. L.; Croom, S. M.; Allen, J. T.; Brough, S.; Medling, A. M.; Ho, I.-T.; Scott, N.; Richards, S. N.; Pracy, M. B.; Gunawardhana, M. L. P.; Norberg, P.; Alpaslan, M.; Bauer, A. E.; Bekki, K.; Bland-Hawthorn, J.; Bloom, J. V.; Bryant, J. J.; Couch, W. J.; Driver, S. P.; Fogarty, L. M. R.; Foster, C.; Goldstein, G.; Green, A. W.; Hopkins, A. M.; Konstantopoulos, I. S.; Lawrence, J. S.; López-Sánchez, A. R.; Lorente, N. P. F.; Owers, M. S.; Sharp, R.; Sweet, S. M.; Taylor, E. N.; van de Sande, J.; Walcher, C. J.; Wong, O. I.

    2016-09-01

    We use data from the Sydney-AAO Multi-Object Integral Field Spectrograph (SAMI) Galaxy Survey and the Galaxy And Mass Assembly (GAMA) survey to investigate the spatially-resolved signatures of the environmental quenching of star formation in galaxies. Using dust-corrected measurements of the distribution of Hα emission we measure the radial profiles of star formation in a sample of 201 star-forming galaxies covering three orders of magnitude in stellar mass ({M}_{*}; 108.1-1010.95 M⊙) and in 5th nearest neighbour local environment density (Σ5; 10-1.3- 102.1 Mpc-2). We show that star formation rate gradients in galaxies are steeper in dense (log10(Σ5/Mpc2) > 0.5) environments by 0.58 ± 0.29 dex re-1 in galaxies with stellar masses in the range 1010 < M★/M⊙ < 1011 and that this steepening is accompanied by a reduction in the integrated star formation rate. However, for any given stellar mass or environment density the star-formation morphology of galaxies shows large scatter. We also measure the degree to which the star formation is centrally concentrated using the unitless scale-radius ratio (r50, Hα/r50, cont), which compares the extent of ongoing star formation to previous star formation. With this metric we find that the fraction of galaxies with centrally concentrated star formation increases with environment density, from ˜5 ± 4% in low-density environments (log10(Σ5/Mpc2) < 0.0) to 30 ± 15% in the highest density environments (log10(Σ5/Mpc2) > 1.0). These lines of evidence strongly suggest that with increasing local environment density the star formation in galaxies is suppressed, and that this starts in their outskirts such that quenching occurs in an outside-in fashion in dense environments and is not instantaneous.

  20. Micro-Level Language-Planning and Grass-Root Initiatives: A Case Study of Irish Language Comedy and Inari Sami Rap

    ERIC Educational Resources Information Center

    Moriarty, Mairead; Pietikainen, Sari

    2011-01-01

    The aim of this paper is to examine the increased potential for language change from the micro-level, given the new domains in which minority languages are present in the global era. Drawing on the theoretical notion of sociolinguistic scales this paper presents a comparative account of the changing positions of the Irish and Inari Sami languages.…

  1. The Evolution of the Tully-Fisher Relation Since z~1 with KROSS and SAMI

    NASA Astrophysics Data System (ADS)

    Tiley, Alfred; Bureau, Martin; Stott, John; Swinbank, Mark; Bower, Richard; Harrison, Christopher; Bunker, Andrew; Smail, Ian; Magdis, Georgios; Johnson, Helen

    2016-01-01

    manner as with KROSS, at which point a direct comparison may be made. I discuss my work comparing the TFRs of KROSS and the SAMI Galaxy Survey in this manner and its implications on previous measures of the evolution of the TFR since z~1.

  2. Aboveground and belowground legacies of native Sami land use on boreal forest in northern Sweden 100 years after abandonment.

    PubMed

    Freschet, Grégoire T; Ostlund, Lars; Kichenin, Emilie; Wardle, David A

    2014-04-01

    Human activities that involve land-use change often cause major transformations to community and ecosystem properties both aboveground and belowground, and when land use is abandoned, these modifications can persist for extended periods. However, the mechanisms responsible for rapid recovery vs. long-term maintenance of ecosystem changes following abandonment remain poorly understood. Here, we examined the long-term ecological effects of two remote former settlements, regularly visited for -300 years by reindeer-herding Sami and abandoned -100 years ago, within an old-growth boreal forest that is considered one of the most pristine regions in northern Scandinavia. These human legacies were assessed through measurements of abiotic and biotic soil properties and vegetation characteristics at the settlement sites and at varying distances from them. Low-intensity land use by Sami is characterized by the transfer of organic matter towards the settlements by humans and reindeer herds, compaction of soil through trampling, disappearance of understory vegetation, and selective cutting of pine trees for fuel and construction. As a consequence, we found a shift towards early successional plant species and a threefold increase in soil microbial activity and nutrient availability close to the settlements relative to away from them. These changes in soil fertility and vegetation contributed to 83% greater total vegetation productivity, 35% greater plant biomass, and 23% and 16% greater concentrations of foliar N and P nearer the settlements, leading to a greater quantity and quality of litter inputs. Because decomposer activity was also 40% greater towards the settlements, soil organic matter cycling and nutrient availability were further increased, leading to likely positive feedbacks between the aboveground and belowground components resulting from historic land use. Although not all of the activities typical of Sami have left visible residual traces on the ecosystem after

  3. Aboveground and belowground legacies of native Sami land use on boreal forest in northern Sweden 100 years after abandonment.

    PubMed

    Freschet, Grégoire T; Ostlund, Lars; Kichenin, Emilie; Wardle, David A

    2014-04-01

    Human activities that involve land-use change often cause major transformations to community and ecosystem properties both aboveground and belowground, and when land use is abandoned, these modifications can persist for extended periods. However, the mechanisms responsible for rapid recovery vs. long-term maintenance of ecosystem changes following abandonment remain poorly understood. Here, we examined the long-term ecological effects of two remote former settlements, regularly visited for -300 years by reindeer-herding Sami and abandoned -100 years ago, within an old-growth boreal forest that is considered one of the most pristine regions in northern Scandinavia. These human legacies were assessed through measurements of abiotic and biotic soil properties and vegetation characteristics at the settlement sites and at varying distances from them. Low-intensity land use by Sami is characterized by the transfer of organic matter towards the settlements by humans and reindeer herds, compaction of soil through trampling, disappearance of understory vegetation, and selective cutting of pine trees for fuel and construction. As a consequence, we found a shift towards early successional plant species and a threefold increase in soil microbial activity and nutrient availability close to the settlements relative to away from them. These changes in soil fertility and vegetation contributed to 83% greater total vegetation productivity, 35% greater plant biomass, and 23% and 16% greater concentrations of foliar N and P nearer the settlements, leading to a greater quantity and quality of litter inputs. Because decomposer activity was also 40% greater towards the settlements, soil organic matter cycling and nutrient availability were further increased, leading to likely positive feedbacks between the aboveground and belowground components resulting from historic land use. Although not all of the activities typical of Sami have left visible residual traces on the ecosystem after

  4. A Highly Coupled Network of Tertiary Interactions in the SAM-I Riboswitch and Their Role in Regulatory Tuning.

    PubMed

    Wostenberg, Christopher; Ceres, Pablo; Polaski, Jacob T; Batey, Robert T

    2015-11-01

    RNA folding in vivo is significantly influenced by transcription, which is not necessarily recapitulated by Mg(2+)-induced folding of the corresponding full-length RNA in vitro. Riboswitches that regulate gene expression at the transcriptional level are an ideal system for investigating this aspect of RNA folding as ligand-dependent termination is obligatorily co-transcriptional, providing a clear readout of the folding outcome. The folding of representative members of the SAM-I family of riboswitches has been extensively analyzed using approaches focusing almost exclusively upon Mg(2+) and/or S-adenosylmethionine (SAM)-induced folding of full-length transcripts of the ligand binding domain. To relate these findings to co-transcriptional regulatory activity, we have investigated a set of structure-guided mutations of conserved tertiary architectural elements of the ligand binding domain using an in vitro single-turnover transcriptional termination assay, complemented with phylogenetic analysis and isothermal titration calorimetry data. This analysis revealed a conserved internal loop adjacent to the SAM binding site that significantly affects ligand binding and regulatory activity. Conversely, most single point mutations throughout key conserved features in peripheral tertiary architecture supporting the SAM binding pocket have relatively little impact on riboswitch activity. Instead, a secondary structural element in the peripheral subdomain appears to be the key determinant in observed differences in regulatory properties across the SAM-I family. These data reveal a highly coupled network of tertiary interactions that promote high-fidelity co-transcriptional folding of the riboswitch but are only indirectly linked to regulatory tuning. PMID:26343759

  5. The use of plants as regular food in ancient subarctic economies: a case study based on Sami use of Scots pine innerbark.

    PubMed

    Bergman, Ingela; Östlund, Lars; Zackrisson, Olle

    2004-01-01

    This study combines ethnological, historical, and dendroecological data from areas north of the Arctic Circle to analyze cultural aspects of Sami use of Scots pine (Pinus sylvestris L.) inner bark as regular food. Bark was peeled in June when trees were at the peak of sapping, leaving a strip of undamaged cambium so the tree survived. As a result, it is possible to date bark-peeling episodes using dendrochronology. The paper argues that the use of Scots pine inner bark reflects Sami religious beliefs, ethical concerns, and concepts of time, all expressed in the process of peeling the bark. A well-developed terminology and a set of specially designed tools reveal the technology involved in bark peeling. Consistent patterns with respect to the direction and size of peeling scars found across the region demonstrate common values and standards. Peeling direction patterns and ceremonial meals relating to bark probably reflect ritual practices connected to the sun deity, Biejvve.

  6. The use of plants as regular food in ancient subarctic economies: a case study based on Sami use of Scots pine innerbark.

    PubMed

    Bergman, Ingela; Östlund, Lars; Zackrisson, Olle

    2004-01-01

    This study combines ethnological, historical, and dendroecological data from areas north of the Arctic Circle to analyze cultural aspects of Sami use of Scots pine (Pinus sylvestris L.) inner bark as regular food. Bark was peeled in June when trees were at the peak of sapping, leaving a strip of undamaged cambium so the tree survived. As a result, it is possible to date bark-peeling episodes using dendrochronology. The paper argues that the use of Scots pine inner bark reflects Sami religious beliefs, ethical concerns, and concepts of time, all expressed in the process of peeling the bark. A well-developed terminology and a set of specially designed tools reveal the technology involved in bark peeling. Consistent patterns with respect to the direction and size of peeling scars found across the region demonstrate common values and standards. Peeling direction patterns and ceremonial meals relating to bark probably reflect ritual practices connected to the sun deity, Biejvve. PMID:21774149

  7. Noise disturbance caused by outdoor activities--a simulated-environment study for Ali Sami Yen Stadium, İstanbul.

    PubMed

    Dal, Zeynep; Akdağ, Neşe Yüğrük

    2011-03-01

    Negative effects of noise on individuals, the inevitable result of urbanization, have become a significant urban problem in our day. Introduction of an approach to the noise problem on an urban-planning scale lightens the burden of measures required to be taken against noise at the stages of regional and developmental planning. Stadiums, which should be also evaluated from the point of noise problem when planning decisions are made on the urban planning scale, may cause very serious problems differing depending on the region they are located in. In this article, various dimensions of the noise problem caused by stadiums have been exemplified by making an assessment on Ali Sami Yen football stadium located in Mecidiyeköy district which is among important residential and commercial centres of İstanbul or Turkey. When the simulation results obtained for ordinary days and match days are evaluated, it has been found out that the people living in the area are exposed to noise levels substantially exceeding the acceptable values. Results of the survey conducted in the area have clearly revealed the existence of noise problem, too. PMID:20424911

  8. Experiences of being a young male Sami reindeer herder: a qualitative study in perspective of mental health

    PubMed Central

    Kaiser, Niclas; Ruong, Terje; Renberg, Ellinor Salander

    2013-01-01

    Objectives To explore experiences of what it is to be a young male Sami reindeer herder in Sweden, a group with previously known stigma and specific health issues, and to understand experiences in perspective of mental health. Methods A qualitative content analysis was employed. Data were collected by in-depth interviews with 15 strategically selected reindeer herders aged 18–35 years old. Results The analysis resulted in 5 sub-themes: (a) being “inside” or “outside” is a question of identity; (b) a paradox between being free/bound; (c) an experience of various threats and a feeling of powerlessness; (d) specific norms for how a “real” reindeer herder should be; and (e) the different impacts and meanings of relations. The overarching theme is summarized thus: being a young reindeer herder means so many (impossible) dreams and conditions. Overall, the experience of the informants was that being a reindeer herder is a privileged position that also implies many impossibilities and unjust adversities they have no control over, and that there is nothing they can do but “bite the bullet or be a failure.” Conclusions Knowledge about this group's experiences can be used to understand difficulties faced by young reindeer herders and its consequences regarding mental health problems. This also implies a need for a broader perspective when discussing future interventions aimed at preventing mental health problems in this group. PMID:23853764

  9. Johan Turi’s animal, mineral, vegetable cures and healing practices: an in-depth analysis of Sami (Saami) folk healing one hundred years ago

    PubMed Central

    2013-01-01

    Background The healing knowledge of a Sami (Saami) hunter and reindeer herder was surveyed as a window into the concepts of health, healing, and disease in early twentieth-century Sapmi (Northern Sweden). The two books of Johan Turi (1854–1936)—An Account of the Sami (1910) and Lappish Texts (1918–19) were examined to determine the varieties of recorded zootherapeutic, mineral, chemical, and ethnobotanical lore, as well as the therapeutic acts, identified conditions, and veterinary knowledge included. Methods Tabulation of the materials and species mentioned in Turi’s descriptions (n = 137) permitted analysis of the relative frequency of differing types of healing in Turi’s overall therapeutic repertoire, his relative attention to chronic vs. acute ailments, and the frequency of magic as a component of healing. A qualitative appraisal was made of the degree to which outside influences affected Sami healing of the period. A further assessment of the possible clinical efficacy of the recorded remedies was undertaken. Results Turi’s remedies consist most often of zootherapeutics (31%), followed by physical acts such as massage, moxibustion, or manipulation (22%). Ethnobotanical cures make up a significantly smaller portion of his repertoire (17%), followed by mineral and chemical cures (12%). Magic rituals (including incantations and ritual acts) make up a significant portion of Turi’s repertoire, and could be used alone (17%) or in conjunction with other types of healing (38%). Turi’s healing aimed primarily at acute ailments (65%), with chronic conditions addressed less often (35%). A literature review revealed that Turi’s remedies held a marked frequency of likely efficacy, at least in cases in which it was possible to ascertain the precise species, conditions, or substances described. Although it is possible at times to recognize foreign sources in Turi’s repertoire, it is clear that Turi understood all his healing methods as distinctively

  10. The expression platform and the aptamer: cooperativity between Mg2+ and ligand in the SAM-I riboswitch

    PubMed Central

    Hennelly, Scott P.; Novikova, Irina V.; Sanbonmatsu, Karissa Y.

    2013-01-01

    Riboswitch operation involves the complex interplay between the aptamer domain and the expression platform. During transcription, these two domains compete against each other for shared sequence. In this study, we explore the cooperative effects of ligand binding and Magnesium interactions in the SAM-I riboswitch in the context of aptamer collapse and anti-terminator formation. Overall, our studies show the apo-aptamer acts as (i) a pre-organized aptamer competent to bind ligand and undergo structural collapse and (ii) a conformation that is more accessible to anti-terminator formation. We show that both Mg2+ ions and SAM are required for a collapse transition to occur. We then use competition between the aptamer and expression platform for shared sequence to characterize the stability of the collapsed aptamer. We find that SAM and Mg2+ interactions in the aptamer are highly cooperative in maintaining switch polarity (i.e. aptamer ‘off-state’ versus anti-terminator ‘on-state’). We further show that the aptamer off-state is preferentially stabilized by Mg2+ and similar divalent ions. Furthermore, the functional switching assay was used to select for phosphorothioate interference, and identifies potential magnesium chelation sites while characterizing their coordinated role with SAM in aptamer stabilization. In addition, we find that Mg2+ interactions with the apo-aptamer are required for the full formation of the anti-terminator structure, and that higher concentrations of Mg2+ (>4 mM) shift the equilibrium toward the anti-terminator on-state even in the presence of SAM. PMID:23258703

  11. The strength and hemispheric asymmetry of Equatorial Ionization Anomaly during two geomagnetic storms in 2013 from Global Ionosphere Map and SAMI2

    NASA Astrophysics Data System (ADS)

    Luo, Weihua; Zhu, Zhengping; Lan, Jiaping

    2016-08-01

    The variations of the strength and the hemispheric asymmetry of EIA were studied by Global Ionosphere Map (GIM) and SAMI2 during two geomagnetic storm periods in March and June 2013. Compared with the 30-days median TEC, the TEC at the two crests of EIA had small variations while the TEC at the trough had a more remarkable variation for the two storms after the SSC. The TEC difference between the two EIA peaks had an increase or decrease several hours after the SSC, the asymmetry between the two crests of EIA represented by the defined asymmetry index has no obvious variations except several hours after the SSC, and EIA strength represented by the Crest-to-Trough Ratio (CTR) had a remarkable increase one day after the SSC day for March storm and decrease several hours after the SSC for June storm. The variations last several hours, with more than 40% variations compared with the value during the quiet period. The EIA peaks were also found to move toward the equator after the SSC during the two storms. The simulation from SAMI2 and HWM07 also shows that EIA crests would move toward the equator during storm time and EIA strength would decrease, which suggests that the disturbed neutral wind and disturbed electric field may be important factors affecting the EIA during the storm periods.

  12. Comparing results of high-resolution palaeoecological analyses with oral histories of land-use of a Sami reindeer herding pen in northern Sweden

    NASA Astrophysics Data System (ADS)

    Kamerling, Ilse M.; Edwards, Kevin J.; Schofield, James E.; Aronsson, Kjell-Åke

    2016-04-01

    Reindeer herding is a key component of Sami culture, but much is still unknown about its development both in the recent and more distant past due to the limited availability of historical and archaeological evidence. Pollen analysis provides a potential tool to supplement this lack of evidence through the detection and evaluation of landscape responses to the impact of reindeer pastoralism. In the boreal forests of northern Fennoscandia, localised forest clearance to create space for dwellings and livestock is presented in the palynological record as a decline in arboreal taxa and an increase in herbaceous taxa favoured by the increased light levels, resistance to soil trampling, and/or the increased soil nutrient levels provided by reindeer dung, domestic waste and ash from smudge fires. Oral histories of 20th century forest Sami reindeer herding at an abandoned reindeer herding pen (renvall) at Akkajävi, northern Sweden (66.9° N, 21.1° E), are integrated here with high-resolution palaeoecological reconstructions of the local vegetation to: (i) assess the sensitivity and value of various palynomorphs to the impacts of reindeer pastoralism; (ii) investigate whether the patterns seen in the palaeoecological record match the timing of activity at and abandonment of the site as understood from these oral histories. A peat monolith collected from within an annexe of the renvall was pollen analysed at a high resolution, supplemented with coprophilous fungal spore (livestock grazing/gathering), microscopic charcoal ([anthropogenic] burning) and sedimentological (loss-on-ignition; soil erosion) records. For the first time, this has allowed for the identification of multi-decadal cycles of use and abandonment of a renvall in the pollen record, but more obviously so in its coprophilous fungal spore archive, with the pattern and timing of changes at the site confirming events previously known only from oral histories. A second, paired profile was collected from the fen

  13. 77 FR 39245 - Sami Arshak Yanikian: Debarment Order

    Federal Register 2010, 2011, 2012, 2013, 2014

    2012-07-02

    ... because they were intended to cure, mitigate, treat, or prevent disease. Mr. Yanikian was informed that... States without FDA approval, and despite his repeated representations to FDA that he was not selling...

  14. The SAMI Galaxy Survey: the link between angular momentum and optical morphology

    NASA Astrophysics Data System (ADS)

    Cortese, L.; Fogarty, L. M. R.; Bekki, K.; van de Sande, J.; Couch, W.; Catinella, B.; Colless, M.; Obreschkow, D.; Taranu, D.; Tescari, E.; Barat, D.; Bland-Hawthorn, J.; Bloom, J.; Bryant, J. J.; Cluver, M.; Croom, S. M.; Drinkwater, M. J.; d'Eugenio, F.; Konstantopoulos, I. S.; Lopez-Sanchez, A.; Mahajan, S.; Scott, N.; Tonini, C.; Wong, O. I.; Allen, J. T.; Brough, S.; Goodwin, M.; Green, A. W.; Ho, I.-T.; Kelvin, L. S.; Lawrence, J. S.; Lorente, N. P. F.; Medling, A. M.; Owers, M. S.; Richards, S.; Sharp, R.; Sweet, S. M.

    2016-11-01

    We investigate the relationship between stellar and gas specific angular momentum j, stellar mass M* and optical morphology for a sample of 488 galaxies extracted from the Sydney-AAO Multi-object Integral field Galaxy Survey. We find that j, measured within one effective radius, monotonically increases with M* and that, for M* > 109.5 M⊙, the scatter in this relation strongly correlates with optical morphology (i.e. visual classification and Sérsic index). These findings confirm that massive galaxies of all types lie on a plane relating mass, angular momentum and stellar-light distribution, and suggest that the large-scale morphology of a galaxy is regulated by its mass and dynamical state. We show that the significant scatter in the M*-j relation is accounted for by the fact that, at fixed stellar mass, the contribution of ordered motions to the dynamical support of galaxies varies by at least a factor of 3. Indeed, the stellar spin parameter (quantified via λR) correlates strongly with Sérsic and concentration indices. This correlation is particularly strong once slow rotators are removed from the sample, showing that late-type galaxies and early-type fast rotators form a continuous class of objects in terms of their kinematic properties.

  15. THE SAMI GALAXY SURVEY: TOWARD A UNIFIED DYNAMICAL SCALING RELATION FOR GALAXIES OF ALL TYPES

    SciTech Connect

    Cortese, L.; Glazebrook, K.; Mould, J.; Fogarty, L. M. R.; Bland-Hawthorn, J.; Croom, S. M.; Scott, N.; Allen, J. T.; Bloom, J.; Bryant, J. J.; Ho, I.-T.; Bekki, K.; Colless, M.; Sharp, R.; Couch, W.; Goodwin, M.; Tonini, C.; Cluver, M.; Davies, R. L.; Drinkwater, M. J.; and others

    2014-11-10

    We take advantage of the first data from the Sydney-AAO Multi-object Integral field Galaxy Survey to investigate the relation between the kinematics of gas and stars, and stellar mass in a comprehensive sample of nearby galaxies. We find that all 235 objects in our sample, regardless of their morphology, lie on a tight relation linking stellar mass (M {sub *}) to internal velocity quantified by the S {sub 0.5} parameter, which combines the contribution of both dispersion (σ) and rotational velocity (V {sub rot}) to the dynamical support of a galaxy (S{sub 0.5}=√(0.5 V{sub rot}{sup 2}+σ{sup 2})). Our results are independent of the baryonic component from which σ and V {sub rot} are estimated, as the S {sub 0.5} of stars and gas agree remarkably well. This represents a significant improvement compared to the canonical M {sub *} versus V {sub rot} and M {sub *} versus σ relations. Not only is no sample pruning necessary, but also stellar and gas kinematics can be used simultaneously, as the effect of asymmetric drift is taken into account once V {sub rot} and σ are combined. Our findings illustrate how the combination of dispersion and rotational velocities for both gas and stars can provide us with a single dynamical scaling relation valid for galaxies of all morphologies across at least the stellar mass range 8.5 

  16. Free state conformational sampling of the SAM-I riboswitch aptamer domain

    PubMed Central

    Stoddard, Colby D; Montange, Rebecca K.; Hennelly, Scott P.; Rambo, Robert P.; Sanbonmatsu, Karissa Y.; Batey, Robert T.

    2010-01-01

    Summary Riboswitches are highly structured elements residing in the 5' untranslated region of messenger RNAs that specifically bind cellular metabolites to alter gene expression. While there are many structures of ligand bound riboswitches that reveal details of bimolecular recognition, their unliganded structures remain poorly characterized. Characterizing the molecular details of the unliganded state is crucial for understanding the riboswitch's mechanism of action because it is this state that actively interrogates the cellular environment and helps direct the regulatory outcome. To develop a detailed description of the ligand free form of an S-adenosylmethionine binding riboswitch at the local and global levels, we have employed a series of biochemical, biophysical, and computational methods. Our data reveals that the ligand binding domain adopts an ensemble of states that minimizes the energy barrier between the free and bound states to establish an efficient decision making brachpoint in the regulatory process. PMID:20637415

  17. "Survivance" in Sami and First Nations Boarding School Narratives: Reading Novels by Kerttu Vuolab and Shirley Sterling

    ERIC Educational Resources Information Center

    Kuokkanen, Rauna

    2003-01-01

    Educational institutions have played a central role in colonizing Indigenous peoples. The colonial school system has also been a very effective tool in implementing racist theories and indoctrinating them in children (Indigenous and non-Indigenous alike) worldwide. In this paper, the author demonstrates how, despite the vast differences in actual…

  18. Parental Involvement in the Development of a Culture-Based School Curriculum

    ERIC Educational Resources Information Center

    Johansson, Gunilla

    2009-01-01

    This study focuses on parental involvement in Sami schools when developing a culturally sensitive school curriculum. The research recognizes a number of competing and complementary interests that play a role when constructing structures and policies in curriculum development. Two Sami schools in Sweden with 115 pupils, their parents and 27…

  19. Reindeer Diode

    ERIC Educational Resources Information Center

    Mattila, Jukka O.

    2013-01-01

    In Finnish Lapland, like in other Northern European regions by the Arctic Sea, aboriginal Sami people still base much of their daily income on reindeer. Earlier the Sami people followed their reindeer herds more or less all the year round, in nomadic fashion. Moving to fixed dwellings has created a problem in herding and guarding the property of…

  20. Listening for the Reindeer's Heartbeat: An Interview with Harald Gaski.

    ERIC Educational Resources Information Center

    Palmer, Paula

    1998-01-01

    In this interview, Professor Harald Gaski, a Sami from Arctic Norway, notes similarities and differences in Sami and American-Indian cultures related to forced boarding schools for assimilation purposes, traditional education, religion, "yoiking" (singing) and music, connection to nature, and tribal schools. He advocates the international…

  1. The Development of a Substance Abuse Treatment Program for Forensic Patients with Cognitive Impairment

    ERIC Educational Resources Information Center

    Glassmire, David M.; Welsh, Robert K.; Clevenger, Jeanne K.

    2007-01-01

    The Substance Abuse and Mental Illness (SAMI) program combines cognitive rehabilitation and dual-diagnosis substance abuse treatment within a stages of change context. This article describes the development, implementation, and preliminary outcome analysis of the SAMI program in a forensic hospital.

  2. Preliminary measurements of the edge magnetic field pitch from 2-D Doppler backscattering in MAST and NSTX-U (invited)

    NASA Astrophysics Data System (ADS)

    Vann, R. G. L.; Brunner, K. J.; Ellis, R.; Taylor, G.; Thomas, D. A.

    2016-11-01

    The Synthetic Aperture Microwave Imaging (SAMI) system is a novel diagnostic consisting of an array of 8 independently phased antennas. At any one time, SAMI operates at one of the 16 frequencies in the range 10-34.5 GHz. The imaging beam is steered in software post-shot to create a picture of the entire emission surface. In SAMI's active probing mode of operation, the plasma edge is illuminated with a monochromatic source and SAMI reconstructs an image of the Doppler back-scattered (DBS) signal. By assuming that density fluctuations are extended along magnetic field lines, and knowing that the strongest back-scattered signals are directed perpendicular to the density fluctuations, SAMI's 2-D DBS imaging capability can be used to measure the pitch of the edge magnetic field. In this paper, we present preliminary pitch angle measurements obtained by SAMI on the Mega Amp Spherical Tokamak (MAST) at Culham Centre for Fusion Energy and on the National Spherical Torus Experiment Upgrade at Princeton Plasma Physics Laboratory. The results demonstrate encouraging agreement between SAMI and other independent measurements.

  3. Southern Appalachian Mountains initiative: Regional partnership for air quality management

    SciTech Connect

    Brewer, P.F.

    1999-07-01

    The Southern Appalachian Mountains Initiative (SAMI) is a voluntary partnership of state and federal agencies, industry, environmental groups, academia, and interested public. SAMI was established to identify and recommend air emissions management strategies to remedy existing and prevent future adverse air quality impacts to natural resources in Southern Appalachia, with particular focus on Class I national park and wilderness areas. SAMI's integrated assessment is focusing simultaneously on ozone, visibility impairment, and acid deposition. Computer models are linking emissions, atmospheric transport, exposures, and environmental and socioeconomic effects. The assessment is considering the impacts of existing and newly enacted federal air regulatory requirements and alternative emissions management strategies that SAMI might recommend for regional, state, or community-based actions.

  4. Update on the Improving Access to Psychological Therapies programme in England†

    PubMed Central

    Fonagy, Peter; Clark, David M.

    2015-01-01

    Professor Sami Timimi recently expressed concerns about the Improving Access to Psychological Therapies (IAPT) programme. We argue that the concerns are largely unfounded and provide readers with an update on the programme. PMID:26755970

  5. Reindeer Diode

    NASA Astrophysics Data System (ADS)

    Mattila, Jukka O.

    2013-01-01

    In Finnish Lapland, like in other Northern European regions by the Arctic Sea, aboriginal Sami people still base much of their daily income on reindeer. Earlier the Sami people followed their reindeer herds more or less all the year round, in nomadic fashion. Moving to fixed dwellings has created a problem in herding and guarding the property of the moving wild packs of hundreds or thousands of reindeer, which Sami families usually possess. Already for decades the mobility provided by Ski-Doos—along with herding dogs—has helped with the job. However, the era of limitless wilderness in reindeer herding is over. Nowadays hundreds of kilometers of reindeer fence separate Sami herding districts from each other.

  6. Weld quality evaluation using a high temperature SQUID array

    SciTech Connect

    Clark, D. D.; Espy, M. A.; Kraus, Robert H., Jr.; Matlachov, A. N.; Lamb, J. S.

    2002-01-01

    This paper presents preliminary data for evaluating weld quality using high temperature SQUIDS. The SQUIDS are integrated into an instrument known as the SQUID Array Microscope, or SAMi. The array consists of ll SQUIDs evenly distributed over an 8.25 mm baseline. Welds are detected using SAMi by using an on board coil to induce eddy currents in a conducting sample and measuring the resulting magnetic fields. The concept is that the induced magnetic fields will differ in parts of varying weld quality. The data presented here was collected from three stainless steel parts using SAMi. Each part was either solid, included a good weld, or included a bad weld. The induced magnetic field's magnitude and phase relative to the induction signal were measured. For each sample considered, both the magnitude and phase data were measurably different than the other two samples. These results indicate that it is possible to use SAMi to evaluate weld quality.

  7. Preliminary measurements of the edge magnetic field pitch from 2-D Doppler backscattering in MAST and NSTX-U (invited)

    DOE PAGES

    Vann, R. G. L.; Brunner, K. J.; Ellis, R.; Taylor, G.; Thomas, D. A.

    2016-09-13

    The Synthetic Aperture Microwave Imaging (SAMI) system is a novel diagnostic consisting of an array of 8 independently phased antennas. At any one time, SAMI operates at one of the 16 frequencies in the range 10-34.5 GHz. The imaging beam is steered in software post-shot to create a picture of the entire emission surface. In SAMI’s active probing mode of operation, the plasma edge is illuminated with a monochromatic source and SAMI reconstructs an image of the Doppler back-scattered (DBS) signal. By assuming that density fluctuations are extended along magnetic field lines, and knowing that the strongest back-scattered signals aremore » directed perpendicular to the density fluctuations, SAMI’s 2-D DBS imaging capability can be used to measure the pitch of the edge magnetic field. In this paper, we present preliminary pitch angle measurements obtained by SAMI on the Mega Amp Spherical Tokamak (MAST) at Culham Centre for Fusion Energy and on the National Spherical Torus Experiment Upgrade at Princeton Plasma Physics Laboratory. Lastly, the results demonstrate encouraging agreement between SAMI and other independent measurements.« less

  8. The Influence of the Solar Cycle on Plasmasphere Refilling

    NASA Astrophysics Data System (ADS)

    Krall, J.; Huba, J.

    2015-12-01

    During refilling, ionospheric plasma streams into the inner magnetosphere from both the northern and southern hemispheres. Plasmasphere refilling rates depend on both the ionospheric sources and on the thermalization of streaming ions. We use the NRL SAMI3 ionosphere/plasmasphere code[1] coupled to the NRLMSIS empirical atmosphere model and the HWM14 empirical wind model, to simulate H+, He+ and O+ populations in the plasmasphere. The SAMI3 ionosphere code includes 7 ion species (H+, He+, O+, N+, O2+, N2+, NO+), each treated as a separate fluid, with temperature equations being solved for H+, He+, O+ and e. Measurements show that refilling rates decrease with increasing solar activity, an effect reproduced by SAMI3 and its two-dimensional cousin, SAMI2. We find that the refilling rate and the resulting the plasmasphere electron content are sensitive to the thermospheric composition and temperature, as well as photoelectron heating and photoproduction rates. Depending on conditions, simulations suggest that the plasmaspheric contribution to the total electron content can either increase or decrease with solar activity, as represented by the daily and 81-day-average F10.7 indices. [1] Huba, J. and J. Krall, 2013, ``Modeling the plasmasphere with SAMI3'', Geophys. Res. Lett. 40, 6--10, doi:10.1029/2012GL054300 Research supported by NRL base funds and the NASA HSR program.

  9. Integrated assessment modeling of atmospheric pollutants in the Southern Appalachian Mountains. Part I: hourly and seasonal ozone.

    PubMed

    Boylan, James W; Odman, Mehmet T; Wilkinson, James G; Russell, Armistead G; Doty, Kevin G; Norris, William B; McNider, Richard T

    2005-07-01

    Recently, a comprehensive air quality modeling system was developed as part of the Southern Appalachians Mountains Initiative (SAMI) with the ability to simulate meteorology, emissions, ozone, size- and composition-resolved particulate matter, and pollutant deposition fluxes. As part of SAMI, the RAMS/EMS-95/URM-1ATM modeling system was used to evaluate potential emission control strategies to reduce atmospheric pollutant levels at Class I areas located in the Southern Appalachians Mountains. This article discusses the details of the ozone model performance and the methodology that was used to scale discrete episodic pollutant levels to seasonal and annual averages. The daily mean normalized bias and error for 1-hr and 8-hr ozone were within U.S. Environment Protection Agency guidance criteria for urban-scale modeling. The model typically showed a systematic overestimation for low ozone levels and an underestimation for high levels. Because SAMI was primarily interested in simulating the growing season ozone levels in Class I areas, daily and seasonal cumulative ozone exposure, as characterized by the W126 index, were also evaluated. The daily ozone W126 performance was not as good as the hourly ozone performance; however, the seasonal ozone W126 scaled up from daily values was within 17% of the observations at two typical Class I areas of the SAMI region. The overall ozone performance of the model was deemed acceptable for the purposes of SAMI's assessment. PMID:16111143

  10. Measurement and modeling of the refilling plasmasphere during 2001

    DOE PAGES

    Krall, J.; Huba, J. D.; Jordanova, V. K.; Denton, R. E.; Carranza, T.; Moldwin, M. B.

    2016-03-18

    The Naval Research Laboratory SAMI3 (Sami3 is Also a Model of the Ionosphere) and the RAM-CPL (Ring current Atmosphere interaction Model-Cold PLasma) codes are used to model observed plasmasphere dynamics during 25 November 2001 to 1 December 2001 and 1–5 February 2001. Model results compare well to plasmasphere observations of electron and mass densities. Comparison of model results to refilling data and to each other shows good agreement, generally within a factor of 2. We find that SAMI3 plasmaspheric refilling rates and ion densities are sensitive to the composition and temperature of the thermosphere and exosphere, and to photoelectron heating.more » Furthermore, results also support our previous finding that the wind-driven dynamo significantly impacts both refilling rates and plasmasphere dynamics during quiet periods.« less

  11. Measurement and modeling of the refilling plasmasphere during 2001

    NASA Astrophysics Data System (ADS)

    Krall, J.; Huba, J. D.; Jordanova, V. K.; Denton, R. E.; Carranza, T.; Moldwin, M. B.

    2016-03-01

    The Naval Research Laboratory SAMI3 (Sami3 is Also a Model of the Ionosphere) and the RAM-CPL (Ring current Atmosphere interaction Model-Cold PLasma) codes are used to model observed plasmasphere dynamics during 25 November 2001 to 1 December 2001 and 1-5 February 2001. Model results compare well to plasmasphere observations of electron and mass densities. Comparison of model results to refilling data and to each other shows good agreement, generally within a factor of 2. We find that SAMI3 plasmaspheric refilling rates and ion densities are sensitive to the composition and temperature of the thermosphere and exosphere, and to photoelectron heating. Results also support our previous finding that the wind-driven dynamo significantly impacts both refilling rates and plasmasphere dynamics during quiet periods.

  12. d-Vision: Seeking Excellence through a Hands on Engineering Multi Discipline Global Internship Program

    ERIC Educational Resources Information Center

    Suss, Gavin

    2010-01-01

    The question is, "What can vision do?" (Fritz, 1989) rather than "What is vision?" Keter's Chairman, Mr. Sami Sagol's vision is to establish an internship program that will strengthen the competitive edge of the Israeli industry, within the international arena. The program will set new standards of excellence for product…

  13. Can Schools Save Indigenous Languages? Policy and Practice on Four Continents: Palgrave Studies in Minority Languages and Communities

    ERIC Educational Resources Information Center

    Hornberger, Nancy H., Ed.

    2010-01-01

    This volume offers a close look at four cases of indigenous language revitalization: Maori in Aotearoa/New Zealand, Sami in Scandinavia, Hnahno in Mexico and Quechua and other indigenous languages in Latin America. Essays by experts from each case are in turn discussed in international perspective by four counterpart experts. This book is divided…

  14. Frozen Actions in the Arctic Linguistic Landscape: A Nexus Analysis of Language Processes in Visual Space

    ERIC Educational Resources Information Center

    Pietikainen, Sari; Lane, Pia; Salo, Hanni; Laihiala-Kankainen, Sirkka

    2011-01-01

    This article examines the linguistic landscape (LL) of seven villages above the Arctic Circle, in the region called North Calotte. The area forms a complex nexus of contested and changing multilingualism, particularly as regards to endangered indigenous Sami languages and Kven and Meankieli minority languages. Viewing LL as a discursively…

  15. 78 FR 3042 - J.P. Morgan Securities LLC, et al.; Notice of Application and Temporary Order

    Federal Register 2010, 2011, 2012, 2013, 2014

    2013-01-15

    ... COMMISSION J.P. Morgan Securities LLC, et al.; Notice of Application and Temporary Order January 9, 2013... Act, with respect to an injunction entered against J.P. Morgan Securities LLC (``JPMS''), EMC Mortgage... Investments II, Inc. (``SAMI''), SACO I Inc. (``SACO'') and J.P. Morgan Acceptance Corporation I...

  16. 77 FR 66084 - Quarterly Publication of Individuals, Who Have Chosen To Expatriate, as Required by Section 6039G

    Federal Register 2010, 2011, 2012, 2013, 2014

    2012-11-01

    ... MARY ADRIANOPOULOS GENIE IRENE ALBARRAK SAMI MANSOUR ANDERSON MARIE GABRIELLE APONTE ERICK ELVIS ARBENZ...- MARCI ANN BURG DEAN STEVEN DON DOUGLAS MARCELLE-LATRISE DRUCK JACOB ALEXANDER DUNN PETER WALLACE EWALD... GISI-TOLLE KERSTIN SANDRA GOEBEL GARY ROBERT GOLAN DANIEL SAM GRAF KAROLINE MADELEINE GUNTHARDT...

  17. Educating Nomads for Self-Actualization and Development. Literacy Lessons.

    ERIC Educational Resources Information Center

    Ezeomah, Chimah

    Nomadism is a worldwide phenomenon and its practitioners fall into three categories: (1) hunter/food gatherers, such as the Hadzabe in the United Republic of Tanzania; (2) itinerant workers, including the gypsies in North America; and (3) pastoralists, such as the Masai and Shuaw Arabs in Africa, the Sami in Finland, Norway, and Sweden, and the…

  18. What Are We Seeking to Sustain through Culturally Sustaining Pedagogy? A Loving Critique Forward

    ERIC Educational Resources Information Center

    Paris, Django; Alim, H. Samy

    2014-01-01

    In this article, Django Paris and H. Samy Alim use the emergence of Paris's concept of culturally sustaining pedagogy (CSP) as the foundation for a respectful and productive critique of previous formulations of asset pedagogies. Paying particular attention to asset pedagogy's failures to remain dynamic and critical in a constantly…

  19. Development of a data-verified ionospheric model with an ionosonde network

    NASA Astrophysics Data System (ADS)

    Kim, Jeong-Heon; Kim, Yong Ha; Oh, Seung-June

    2016-06-01

    As a base model for space weather application, we develop an ionospheric model (SAMI2-CNU) by revising the open source SAMI2 model. The revision includes the photoionization of X-rays in the range below 50 Å and photoelectron impact ionization. As a solar flux input to the model, we utilize the real-time solar extreme ultraviolet (EUV) and X-ray (1 ~ 105.0 nm) fluxes of the FISM (flare irradiance spectral model). In order to verify the SAMI2-CNU model, we compare the peak densities of the E and the F2 layers with those from the GIRO (Global Ionospheric Radio Observatory) network for 110 days with the F10.7 range of 70 - 280 in the last solar cycle. The model provides larger values of NmF2 by 30 - 40%, but the NmE values are reasonably close to the ionosonde values. By carrying out a linear correlation analysis between the model and the ionosonde values, we derived scale factors of 0.67 and 0.41 for the photoionization rates in the F2 and the E regions, respectively. With these scale factors, the SAMI2-CNU model allows us to match the ionosonde NmF2 and NmE values within 7% on the average. We also simulated ionospheric changes during eight solar flare events and found averaged 20% and 46% enhancements of NmF2 and NmE, respectively, over the pre-flare values. Although the SAMI2-CNU model has the same problem with matching the NmF2 enhancement as the original SAMI2, it provides reasonable estimates of the NmE increase, as well as reasonable matches of the NmF2 and the NmE values with the ionosonde values. Thus, the SAMI2-CNU model can be used as a physics model in the data-assimilated model that is being developed for the regional ionosphere around the Korea peninsula.

  20. Synthetic aperture microwave imaging with active probing for fusion plasma diagnostics

    SciTech Connect

    Shevchenko, Vladimir F.; Freethy, Simon J.; Huang, Billy K.

    2014-08-21

    A Synthetic Aperture Microwave Imaging (SAMI) system has been designed and built to obtain 2-D images at several frequencies from fusion plasmas. SAMI uses a phased array of linearly polarised antennas. The array configuration has been optimised to achieve maximum synthetic aperture beam efficiency. The signals received by antennas are down-converted to the intermediate frequency range and then recorded in a full vector form. Full vector signals allow beam focusing and image reconstruction in both real time and a post-processing mode. SAMI can scan over 16 pre-programmed frequencies in the range of 10-35GHz with a switching time of 300ns. The system operates in 2 different modes simultaneously: both a 'passive' imaging of plasma emission and also an 'active' imaging of the back-scattered signal of the radiation launched by one of the antennas from the same array. This second mode is similar to so-called Doppler backscattering (DBS) reflectometry with 2-D resolution of the propagation velocity of turbulent structures. Both modes of operation show good performance in fusion plasma experiments on Mega Amp Spherical Tokamak (MAST). We have obtained the first ever 2-D images of BXO mode conversion windows. With active probing, first ever turbulence velocity maps have been obtained. We present an overview of the diagnostic and discuss recent results. In contrast to quasi-optical microwave imaging systems SAMI requires neither big aperture viewing ports nor large 2-D detector arrays to achieve the desired imaging resolution. The number of effective 'pixels' of the synthesized image is proportional to the number of receiving antennas squared. Thus only a small number of optimised antennas is sufficient for the majority of applications. Possible implementation of SAMI on ITERand DEMO is discussed.

  1. Tracking the Footprints of the People without History - Insect Assemblages and Environmental Change in Northern Scandinavia

    NASA Astrophysics Data System (ADS)

    Panagiotakopulu, E.

    2014-12-01

    Using palaeocology and in particular palaeoentomology to understand climate, environmental change and impacts by indigenous groups in the North Atlantic Arctic fringe provides the opportunity to obtain refined details about both the rates of impact and the timing of the change from hunting and gathering to farming. In northern Norway and Sweden the Sami coastal fisher-hunters and inland reindeer herders shared the landscape with incoming agriculturalists and were often assimilated or marginalised. While inside their settled areas there is a palaeoentomological record for the Sami and often information about resource use and seasonality is evident from the fossil insect record, their footprint on the wider landscape tends to be slight and difficult to discern. The diverse and often intermittent nature of Sami activities, which may range from reindeer herding, fishing and even some agricultural activities, makes the task of firmly identifying impacts and differentiating these from climate change a complex task. On the other hand, the transition from a diverse subsistence to intensified pastoralism leaves a clear record in the fossil insect assemblages, both from midden deposits and natural profiles. To add to the complexities of the interpretation, farmers in northern Norway for example, were actively involved in fishing and the fur trade, and introduced grain faunas found in the farm mounds attest to the returns on this, but there is no way to be certain whether the occupiers of the farms were Sami or Norse, or a mixture of both. For a group where both archaeological and historical evidence is sparse, the insect record may unfold the poorly known ecological impact of the Sami.

  2. Modeling Ionospheric Electrodynamics (Invited)

    NASA Astrophysics Data System (ADS)

    Huba, J. D.

    2009-12-01

    We present modeling results of ionospheric electrodynamics using the 3D NRL ionosphere model SAMI3. Recently, SAMI3 has been upgraded to solve the potential equation that determines the electrostatic potential from the ionospheric conductances (Pedersen and Hall) and drivers: neutral wind, gravity, and parallel current systems. We present results showing the impact of different neutral wind models (e.g., HWM93, HWM07, TIMEGCM) on the dynamics of the low- to mid-latitude ionosphere, as well as the Region 1 and 2 current systems. We point out issues and concerns with obtaining an accurate specification of the global electric field within the context of existing models.(with J. Krall, G. Joyce, S. Slinker, and G. Crowley). Research supported by NASA and ONR

  3. Hector - Next Generation Multi-Object IFU for the Anglo-Australian Telescope

    NASA Astrophysics Data System (ADS)

    Bryant, J. J.; Bland-Hawthorn, J.

    2016-10-01

    Hector will be the new massively-multiplexed IFU spectrograph for the Anglo-Australian Observatory in Australia and the next main dark-time instrument for the observatory. Based on the success of the SAMI instrument, which is undergoing the largest galaxy survey done to-date, the hexabundle technology underpinning SAMI is being improved to a new innovative design and scaled up in numbers to give 50-100 IFU imaging bundles across a 2 or 3-degree field. 'Starbug' robots will position the hexabundles across the field plate and several thousand fibers will then be fed into new replicable spectrographs. First prototypes will be on-sky in mid-2016, with full instrument build expected to take ˜5 years. Hector will allow a survey of 100,000 nearby galaxies, sufficient to disentangle intertwined processes in order to investigate the buildup of angular momentum in galaxies and how gas gets into and out of galaxies.

  4. Dayside Ionospheric Superfountain

    NASA Technical Reports Server (NTRS)

    Tsurutani, Bruce T.; Verkhoglyadova, Olga P.; Mannucci, Anthony J.

    2010-01-01

    The Dayside Ionospheric Super-fountain modified SAMI2 code predicts the uplift, given storm-time electric fields, of the dayside near-equatorial ionosphere to heights of over 800 kilometers during magnetic storm intervals. This software is a simple 2D code developed over many years at the Naval Research Laboratory, and has importance relating to accuracy of GPS positioning, and for satellite drag.

  5. 2dfdr: Data reduction software

    NASA Astrophysics Data System (ADS)

    AAO software Team

    2015-05-01

    2dfdr is an automatic data reduction pipeline dedicated to reducing multi-fibre spectroscopy data, with current implementations for AAOmega (fed by the 2dF, KOALA-IFU, SAMI Multi-IFU or older SPIRAL front-ends), HERMES, 2dF (spectrograph), 6dF, and FMOS. A graphical user interface is provided to control data reduction and allow inspection of the reduced spectra.

  6. IPEG- IMPROVED PRICE ESTIMATION GUIDELINES (IBM 370 VERSION)

    NASA Technical Reports Server (NTRS)

    Chamberlain, R. G.

    1994-01-01

    The Improved Price Estimation Guidelines, IPEG, program provides a simple yet accurate estimate of the price of a manufactured product. IPEG facilitates sensitivity studies of price estimates at considerably less expense than would be incurred by using the Standard Assembly-line Manufacturing Industry Simulation, SAMIS, program (COSMIC program NPO-16032). A difference of less than one percent between the IPEG and SAMIS price estimates has been observed with realistic test cases. However, the IPEG simplification of SAMIS allows the analyst with limited time and computing resources to perform a greater number of sensitivity studies than with SAMIS. Although IPEG was developed for the photovoltaics industry, it is readily adaptable to any standard assembly line type of manufacturing industry. IPEG estimates the annual production price per unit. The input data includes cost of equipment, space, labor, materials, supplies, and utilities. Production on an industry wide basis or a process wide basis can be simulated. Once the IPEG input file is prepared, the original price is estimated and sensitivity studies may be performed. The IPEG user selects a sensitivity variable and a set of values. IPEG will compute a price estimate and a variety of other cost parameters for every specified value of the sensitivity variable. IPEG is designed as an interactive system and prompts the user for all required information and offers a variety of output options. The IPEG/PC program is written in TURBO PASCAL for interactive execution on an IBM PC computer under DOS 2.0 or above with at least 64K of memory. The IBM PC color display and color graphics adapter are needed to use the plotting capabilities in IPEG/PC. IPEG/PC was developed in 1984. The original IPEG program is written in SIMSCRIPT II.5 for interactive execution and has been implemented on an IBM 370 series computer with a central memory requirement of approximately 300K of 8 bit bytes. The original IPEG was developed in 1980.

  7. Estimating Prices of Products

    NASA Technical Reports Server (NTRS)

    Aster, R. W.; Chamberlain, R. G.; Zendejas, S. C.; Lee, T. S.; Malhotra, S.

    1986-01-01

    Company-wide or process-wide production simulated. Price Estimation Guidelines (IPEG) program provides simple, accurate estimates of prices of manufactured products. Simplification of SAMIS allows analyst with limited time and computing resources to perform greater number of sensitivity studies. Although developed for photovoltaic industry, readily adaptable to standard assembly-line type of manufacturing industry. IPEG program estimates annual production price per unit. IPEG/PC program written in TURBO PASCAL.

  8. IPEG- IMPROVED PRICE ESTIMATION GUIDELINES (IBM PC VERSION)

    NASA Technical Reports Server (NTRS)

    Aster, R. W.

    1994-01-01

    The Improved Price Estimation Guidelines, IPEG, program provides a simple yet accurate estimate of the price of a manufactured product. IPEG facilitates sensitivity studies of price estimates at considerably less expense than would be incurred by using the Standard Assembly-line Manufacturing Industry Simulation, SAMIS, program (COSMIC program NPO-16032). A difference of less than one percent between the IPEG and SAMIS price estimates has been observed with realistic test cases. However, the IPEG simplification of SAMIS allows the analyst with limited time and computing resources to perform a greater number of sensitivity studies than with SAMIS. Although IPEG was developed for the photovoltaics industry, it is readily adaptable to any standard assembly line type of manufacturing industry. IPEG estimates the annual production price per unit. The input data includes cost of equipment, space, labor, materials, supplies, and utilities. Production on an industry wide basis or a process wide basis can be simulated. Once the IPEG input file is prepared, the original price is estimated and sensitivity studies may be performed. The IPEG user selects a sensitivity variable and a set of values. IPEG will compute a price estimate and a variety of other cost parameters for every specified value of the sensitivity variable. IPEG is designed as an interactive system and prompts the user for all required information and offers a variety of output options. The IPEG/PC program is written in TURBO PASCAL for interactive execution on an IBM PC computer under DOS 2.0 or above with at least 64K of memory. The IBM PC color display and color graphics adapter are needed to use the plotting capabilities in IPEG/PC. IPEG/PC was developed in 1984. The original IPEG program is written in SIMSCRIPT II.5 for interactive execution and has been implemented on an IBM 370 series computer with a central memory requirement of approximately 300K of 8 bit bytes. The original IPEG was developed in 1980.

  9. LZIFU: IDL emission line fitting pipeline for integral field spectroscopy data

    NASA Astrophysics Data System (ADS)

    Ho, I.-Ting

    2016-07-01

    LZIFU (LaZy-IFU) is an emission line fitting pipeline for integral field spectroscopy (IFS) data. Written in IDL, the pipeline turns IFS data to 2D emission line flux and kinematic maps for further analysis. LZIFU has been applied and tested extensively to various IFS data, including the SAMI Galaxy Survey, the Wide-Field Spectrograph (WiFeS), the CALIFA survey, the S7 survey and the MUSE instrument on the VLT.

  10. Simulation of low-latitude ionospheric response to 2015 St. Patrick's Day super geomagnetic storm using ionosonde-derived PRE vertical drifts over Indian region

    NASA Astrophysics Data System (ADS)

    Joshi, L. M.; Sripathi, S.; Singh, Ram

    2016-03-01

    In this paper, we present low-latitude ionospheric response over Indian longitude to the recent super geomagnetic storm of 17 March 2015, using the Sami2 is Another Model of the Ionosphere (SAMI2) model which incorporates ionosonde-derived vertical drift impacted by prompt penetration eastward electric field occurring during the evening prereversal enhancement (PRE) in the vertical drift. The importance of this storm is that (1) Dst reaches as low as -228 nT and (2) prompt penetration of eastward electric field coincided with evening hours PRE. The daytime vertical E × B drifts in the SAMI2 model are, however, considered based on Scherliess-Fejer model. The simulations indicate a significant enhancement in F layer height and equatorial ionization anomaly (EIA) in the post sunset hours on 17 March 2015 vis-a-vis quiet day. The model simulations during recovery phase, considering disturbance dynamo vertical E × B drift along with equatorward disturbance wind, indicate suppression of the daytime EIA. SAMI2 simulations considering the disturbance wind during the recovery phase suggest that equatorward wind enhances the ionospheric density in the low latitude; however, its role in the formation of the EIA depends on the polarity of the zonal electric field. Comparison of model derived total electron content (TEC) with the TEC from ground GPS receivers indicates that model does reproduce enhancement of the EIA during the main phase and suppression of the EIA during the recovery phase of the superstorm. However, peculiarities pertaining to the ionospheric response to prompt penetration electric field in the Indian sector vis-a-vis earlier reports from American sector have been discussed.

  11. 2D Doppler backscattering using synthetic aperture microwave imaging of MAST edge plasmas

    NASA Astrophysics Data System (ADS)

    Thomas, D. A.; Brunner, K. J.; Freethy, S. J.; Huang, B. K.; Shevchenko, V. F.; Vann, R. G. L.

    2016-02-01

    Doppler backscattering (DBS) is already established as a powerful diagnostic; its extension to 2D enables imaging of turbulence characteristics from an extended region of the cut-off surface. The Synthetic Aperture Microwave Imaging (SAMI) diagnostic has conducted proof-of-principle 2D DBS experiments of MAST edge plasma. SAMI actively probes the plasma edge using a wide (±40° vertical and horizontal) and tuneable (10-34.5 GHz) beam. The Doppler backscattered signal is digitised in vector form using an array of eight Vivaldi PCB antennas. This allows the receiving array to be focused in any direction within the field of view simultaneously to an angular range of 6-24° FWHM at 10-34.5 GHz. This capability is unique to SAMI and is a novel way of conducting DBS experiments. In this paper the feasibility of conducting 2D DBS experiments is explored. Initial observations of phenomena previously measured by conventional DBS experiments are presented; such as momentum injection from neutral beams and an abrupt change in power and turbulence velocity coinciding with the onset of H-mode. In addition, being able to carry out 2D DBS imaging allows a measurement of magnetic pitch angle to be made; preliminary results are presented. Capabilities gained through steering a beam using a phased array and the limitations of this technique are discussed.

  12. Observations and Modeling of the Nighttime Electron Density Enhancement in the Mid-latitude Ionosphere

    NASA Astrophysics Data System (ADS)

    Chen, C.; Saito, A.; Lin, C.; Huba, J. D.; Liu, J. G.

    2010-12-01

    In this study, we compare the observational data from FORMOSAT-3/COSMIC and theoretical model results performed by SAMI2 (Sami2 is Another Model of the Ionosphere) for studying the longitudinal structure of the Mid-latitude Summer Nighttime Anomaly (MSNA). In order to study the occurrence of the nighttime electron density enhancement, we defined MSNA index by the ratio of the difference of the nighttime and daytime electron densities. The observational results by the FORMOSAT-3/COSMIC satellites show that there are three obvious nighttime electron density enhancement areas around South American, European, and Northeast Asian regions during local summer. The SAMI2 model can also successfully reproduce the ionospheric MSNA structure during local summer on both hemispheres, except for Northeast Asian region. This difference between observation and model simulation may be caused by the difference between the neutral wind model and the real winds. The physical mechanisms for the longitudinal structure of the MSNA are investigated in the different model conditions. Results show that the equatorward meridional neutral winds can drive the electron density up to a higher altitude along the magnetic field lines and the longer plasma production rate by solar EUV at higher latitudes in the summer time can provide the electron density source in the nighttime ionosphere. We concluded that the combination effect by the neutral wind and the plasma production rate play the important role of the MSNA longitudinal structure.

  13. Cancer among circumpolar populations: an emerging public health concern

    PubMed Central

    Young, T. Kue; Kelly, Janet J.; Friborg, Jeppe; Soininen, Leena; Wong, Kai O.

    2016-01-01

    Objectives To determine and compare the incidence of cancer among the 8 Arctic States and their northern regions, with special focus on 3 cross-national indigenous groups – Inuit, Athabaskan Indians and Sami. Methods Data were extracted from national and regional statistical agencies and cancer registries, with direct age-standardization of rates to the world standard population. For comparison, the “world average” rates as reported in the GLOBOCAN database were used. Findings Age-standardized incidence rates by cancer sites were computed for the 8 Arctic States and 20 of their northern regions, averaged over the decade 2000–2009. Cancer of the lung and colon/rectum in both sexes are the commonest in most populations. We combined the Inuit from Alaska, Northwest Territories, Nunavut and Greenland into a “Circumpolar Inuit” group and tracked cancer trends over four 5-year periods from 1989 to 2008. There has been marked increase in lung, colorectal and female breast cancers, while cervical cancer has declined. Compared to the GLOBOCAN world average, Inuit are at extreme high risk for lung and colorectal cancer, and also certain rare cancers such as nasopharyngeal cancer. Athabaskans (from Alaska and Northwest Territories) share some similarities with the Inuit but they are at higher risk for prostate and breast cancer relative to the world average. Among the Sami, published data from 3 cohorts in Norway, Sweden and Finland show generally lower risk of cancer than non-Sami. Conclusions Cancer among certain indigenous people in the Arctic is an increasing public health concern, especially lung and colorectal cancer. PMID:26765259

  14. Simulation of low latitude ionospheric response to 2015 St. Patrick's Day super geomagnetic storm over Indian longitude sector

    NASA Astrophysics Data System (ADS)

    Mohan Joshi, Lalit; Sripathi, Samireddipelle; Singh, Ram

    2016-07-01

    We present low latitude ionospheric response over Indian longitude to the recent super geomagnetic storm of 17 March 2015, using the SAMI2 model which incorporates ionosonde derived vertical drift impacted by prompt penetration eastward electric field occurring during the evening Prereversal Enhancement (PRE) in the vertical drift. The importance of this storm is that (a) Dst reaches as low as -228 nT and (b) prompt penetration of eastward electric field coincided with evening hours PRE. The daytime vertical EXB drifts in the SAMI2 model are, however, considered based on Scherliess-Fejer model. The simulations indicate a significant enhancement in F layer height and equatorial ionization anomaly (EIA) in the post sunset hours on 17 March 2015 vis-a-vis quiet day. The model simulations during recovery phase, considering disturbance dynamo vertical EXB drift along with equatorward disturbance wind, indicates suppression of the daytime EIA. SAMI2 simulations considering the disturbance wind during the recovery phase suggests that equatorward wind enhances the ionospheric density in the low latitude, however, its role in the formation of the EIA depends on the polarity of the zonal electric field. Comparison of model derived total electron content (TEC) with the TEC from ground GPS receivers indicate that model does reproduce enhancement of the EIA during the main phase and suppression of the EIA during the recovery phase of the super storm. However, peculiarities pertaining to the ionospheric response to prompt penetration electric field in the Indian sector vis-a-vis earlier reports from American sector will be discussed.

  15. Photovoltaic-system costing-methodology development. Final report

    SciTech Connect

    Not Available

    1982-07-01

    Presented are the results of a study to expand the use of standardized costing methodologies in the National Photovoltaics Program. The costing standards, which include SAMIS for manufacturing costs and M and D for marketing and distribution costs, have been applied to concentrator collectors and power-conditioning units. The M and D model was also computerized. Finally, a uniform construction cost-accounting structure was developed for use in photovoltaic test and application projects. The appendices contain example cases which demonstrate the use of the models.

  16. FIT3D: Fitting optical spectra

    NASA Astrophysics Data System (ADS)

    Sánchez, S. F.; Pérez, E.; Sánchez-Blázquez, P.; González, J. J.; Rosales-Ortega, F. F.; Cano-Díaz, M.; López-Cobá, C.; Marino, R. A.; Gil de Paz, A.; Mollá, M.; López-Sánchez, A. R.; Ascasibar, Y.; Barrera-Ballesteros, J.

    2016-09-01

    FIT3D fits optical spectra to deblend the underlying stellar population and the ionized gas, and extract physical information from each component. FIT3D is focused on the analysis of Integral Field Spectroscopy data, but is not restricted to it, and is the basis of Pipe3D, a pipeline used in the analysis of datasets like CALIFA, MaNGA, and SAMI. It can run iteratively or in an automatic way to derive the parameters of a large set of spectra.

  17. Assembly-line Simulation Program

    NASA Technical Reports Server (NTRS)

    Chamberlain, Robert G.; Zendejas, Silvino; Malhotra, Shan

    1987-01-01

    Costs and profits estimated for models based on user inputs. Standard Assembly-line Manufacturing Industry Simulation (SAMIS) program generalized so useful for production-line manufacturing companies. Provides accurate and reliable means of comparing alternative manufacturing processes. Used to assess impact of changes in financial parameters as cost of resources and services, inflation rates, interest rates, tax policies, and required rate of return of equity. Most important capability is ability to estimate prices manufacturer would have to receive for its products to recover all of costs of production and make specified profit. Written in TURBO PASCAL.

  18. Investigation of the spatial structure and developmental dynamics of near-Earth plasma perturbations under the action of powerful HF radio waves

    SciTech Connect

    Belov, A. S.

    2015-10-15

    Results of numerical simulations of the near-Earth plasma perturbations induced by powerful HF radio waves from the SURA heating facility are presented. The simulations were performed using a modified version of the SAMI2 ionospheric model for the input parameters corresponding to the series of in-situ SURA–DEMETER experiments. The spatial structure and developmental dynamics of large-scale plasma temperature and density perturbations have been investigated. The characteristic formation and relaxation times of the induced large-scale plasma perturbations at the altitudes of the Earth’s outer ionosphere have been determined.

  19. Propagation in 3D of microwaves through density perturbations

    NASA Astrophysics Data System (ADS)

    Williams, T. R. N.; Köhn, A.; O'Brien, M. R.; Vann, R. G. L.

    2014-07-01

    Simulations using 3D and 2D full-wave codes have shown that edge filaments in tokamak plasmas can significantly affect the propagation of microwaves across a broad frequency spectrum, resulting in scattering angles of up to 46°. Parameter scans were carried out for density perturbations comparable in width and amplitude to MAST filaments and the effect on the measured emission was calculated. 3D effects were discovered in the case of an obliquely incident beam. In general, the problem of electromagnetic propagation past wavelength-sized 3D inhomogeneities is not well understood, yet is of importance for both heating and diagnostic applications in the electron cyclotron frequency range for tokamaks, as well as atmospheric physics. To improve this understanding, a new cold-plasma code, EMIT-3D, was written to extend full-wave microwave simulations in magnetized plasmas to 3D, and make comparisons to the existing 2D code IPF-FDMC. This work supports MAST experiments using the SAMI diagnostic to image microwave emission from the plasma edge due to mode conversion from electron Bernstein waves. Significant fluctuations in the SAMI data mean that detailed modelling is required to improve its interpretation.

  20. On the utility of the ionosonde Doppler derived EXB drift during the daytime

    NASA Astrophysics Data System (ADS)

    Mohan Joshi, Lalit; Sripathi, Samireddipelle

    2016-07-01

    Vertical EXB drift measured using the ionosonde Doppler sounding during the daytime suffers from an underestimation of the actual EXB drift. This is due to the photochemistry that determines the height of the F layer during the daytime, in addition to the zonal electric field. Systematic investigations have indicated a fair/good correlation to exist between the C/NOFS and ionosonde Doppler measured vertical EXB drift during the daytime over magnetic equator. A detailed analysis, however, indicated that the linear relation between the ionosonde Doppler drift and C/NOFS EXB drift varied with seasons. Thus, solar, seasonal and also geomagnetic variables were included in the Doppler drift correction, using the artificial neural network based approach. The RMS error in the neural network was found to be lesser than that in the linear regression analysis. Daytime EXB drift was derived using the neural network which was also used to model the ionospheic redistribution in the SAMI2 model. SAMI2 model reproduced strong (/weak) equatorial ionization anomaly (EIA) for cases when neural network corrected daytime vertical EXB drift was high (/low). Similar features were also observed in GIM TEC maps. Thus, the results indicate that the neural network can be utilized to derive the vertical EXB drift from its proxies, like the ionosonde Doppler drift. These results indicate that the daytime ionosonde measured vertical EXB drift can be relied upon, provided adequate corrections are applied to it.

  1. Autonomous in situ measurements of seawater alkalinity.

    PubMed

    Spaulding, Reggie S; DeGrandpre, Michael D; Beck, James C; Hart, Robert D; Peterson, Brittany; De Carlo, Eric H; Drupp, Patrick S; Hammar, Terry R

    2014-08-19

    Total alkalinity (AT) is an important parameter for describing the marine inorganic carbon system and understanding the effects of atmospheric CO2 on the oceans. Measurements of AT are limited, however, because of the laborious process of collecting and analyzing samples. In this work we evaluate the performance of an autonomous instrument for high temporal resolution measurements of seawater AT. The Submersible Autonomous Moored Instrument for alkalinity (SAMI-alk) uses a novel tracer monitored titration method where a colorimetric pH indicator quantifies both pH and relative volumes of sample and titrant, circumventing the need for gravimetric or volumetric measurements. The SAMI-alk performance was validated in the laboratory and in situ during two field studies. Overall in situ accuracy was -2.2 ± 13.1 μmol kg(-1) (n = 86), on the basis of comparison to discrete samples. Precision on duplicate analyses of a carbonate standard was ±4.7 μmol kg(-1) (n = 22). This prototype instrument can measure in situ AT hourly for one month, limited by consumption of reagent and standard solutions.

  2. Sense of coherence and self-reported health among Roma people in Sweden – a pilot study

    PubMed Central

    Hassler, Sven; Eklund, Leena

    2012-01-01

    Objectives The Roma people have been known in Europe for a 1000 years, during which they have usually been the subject of discrimination and oppression leading to isolation, powerlessness and poor health. The objective of this study is to investigate the sense of coherence (SOC) in relation to self-reported health among a group of Roma people in southwest Sweden. Study design A cross-sectional, quantitative pilot study. Methods A questionnaire was constructed based on the Short-Form Health Survey (SF-12) and Antonovsky's Sense of Coherence Scale (SOC-13) and was distributed among Roma people in southwest Sweden (n = 102). Self-reported health was summarised in a physical score (PCS) and a mental score (MCS). Comparisons were made with a general Swedish majority population and a Sami population. Results The health scores were significantly lower among the Roma people compared to Swedes – PCS: Roma 46.0 (Swedes 52.0) and MCS: Roma 47.5 (Swedes 52.6). The SOC score for the Roma people (54.4) was significantly lower than that of the Swedes (65.2) and Sami (65.0). Conclusions The low SOC with the Swedish majority society is a strong indication of the marginalisation and exclusion of the Roma people from mainstream society. Low scores in self-reported health among the Roma people also establishes the serious health risks the Roma people are experiencing through their present life situation. PMID:22584516

  3. High-Quality Perovskite Films Grown with a Fast Solvent-Assisted Molecule Inserting Strategy for Highly Efficient and Stable Solar Cells.

    PubMed

    Yuan, Shuai; Qiu, Zhiwen; Gao, Chaomin; Zhang, Hailiang; Jiang, Yanan; Li, Cuncheng; Yu, Jinghua; Cao, Bingqiang

    2016-08-31

    The performance of organolead halide perovskites based solar cells has been enhanced dramatically due to the morphology control of the perovskite films. In this paper, we present a fast solvent-assisted molecule inserting (S-AMI) strategy to grow high-quality perovskite film, in which the methylammonium iodide/2-propanol (MAI/IPA) solution is spin-coated onto a dimethylformamide (DMF) wetted mixed lead halide (PbX2) precursor film. The DMF can help the inserting of MAI molecules into the PbX2 precursor film and provide a solvent environment to help the grain growth of the perovskite film. The perovskite film grown by the S-AMI approach shows large and well-oriented grains and long carrier lifetime due to the reduced grain boundary. Solar cells constructed with these perovskite films yield an average efficiency over 17% along with a high average fill factor of 80%. Moreover, these unsealed solar cell devices exhibit good stability in an ambient atmosphere. PMID:27526617

  4. High-Quality Perovskite Films Grown with a Fast Solvent-Assisted Molecule Inserting Strategy for Highly Efficient and Stable Solar Cells.

    PubMed

    Yuan, Shuai; Qiu, Zhiwen; Gao, Chaomin; Zhang, Hailiang; Jiang, Yanan; Li, Cuncheng; Yu, Jinghua; Cao, Bingqiang

    2016-08-31

    The performance of organolead halide perovskites based solar cells has been enhanced dramatically due to the morphology control of the perovskite films. In this paper, we present a fast solvent-assisted molecule inserting (S-AMI) strategy to grow high-quality perovskite film, in which the methylammonium iodide/2-propanol (MAI/IPA) solution is spin-coated onto a dimethylformamide (DMF) wetted mixed lead halide (PbX2) precursor film. The DMF can help the inserting of MAI molecules into the PbX2 precursor film and provide a solvent environment to help the grain growth of the perovskite film. The perovskite film grown by the S-AMI approach shows large and well-oriented grains and long carrier lifetime due to the reduced grain boundary. Solar cells constructed with these perovskite films yield an average efficiency over 17% along with a high average fill factor of 80%. Moreover, these unsealed solar cell devices exhibit good stability in an ambient atmosphere.

  5. A new Skyrme energy density functional for a better description of spin-isospin resonances

    NASA Astrophysics Data System (ADS)

    Roca-Maza, X.; Colò, G.; Cao, Li-Gang; Sagawa, H.

    2015-10-01

    A correct determination of the isospin and spin-isospin properties of the nuclear effective interaction should lead to an accurate description of the Gamow-Teller resonance (GT), the Spin Dipole Resonance (SDR), the Giant Dipole Resonance (GDR) or the Antianalog Giant Dipole Resonance (AGDR), among others. A new Skyrme energy density functional named SAMi is introduced with the aim of going a step forward in setting the bases for a more precise description of spin-isospin resonances [1, 2]. In addition, we will discuss some new features of our analysis on the AGDR in 208Pb [3] as compared with available experimental data on this resonance [4, 5, 6], and on the GDR [7]. Such study, guided by a simple yet physical pocket formula, has been developed by employing the so called SAMi-J family of systematically varied interactions. This set of interactions is compatible with experimental data for values of the symmetry energy at saturation J and slope parameter L falling in the ranges 31-33 MeV and 75-95 MeV, respectively.

  6. A new Skyrme energy density functional for a better description of spin-isospin resonances

    SciTech Connect

    Roca-Maza, X.; Colò, G.; Cao, Li-Gang; Sagawa, H.

    2015-10-15

    A correct determination of the isospin and spin-isospin properties of the nuclear effective interaction should lead to an accurate description of the Gamow-Teller resonance (GT), the Spin Dipole Resonance (SDR), the Giant Dipole Resonance (GDR) or the Antianalog Giant Dipole Resonance (AGDR), among others. A new Skyrme energy density functional named SAMi is introduced with the aim of going a step forward in setting the bases for a more precise description of spin-isospin resonances [1, 2]. In addition, we will discuss some new features of our analysis on the AGDR in {sup 208}Pb [3] as compared with available experimental data on this resonance [4, 5, 6], and on the GDR [7]. Such study, guided by a simple yet physical pocket formula, has been developed by employing the so called SAMi-J family of systematically varied interactions. This set of interactions is compatible with experimental data for values of the symmetry energy at saturation J and slope parameter L falling in the ranges 31−33 MeV and 75−95 MeV, respectively.

  7. Evolutionary demography of agricultural expansion in preindustrial northern Finland.

    PubMed

    Helle, Samuli; Brommer, Jon E; Pettay, Jenni E; Lummaa, Virpi; Enbuske, Matti; Jokela, Jukka

    2014-11-01

    A shift from nomadic foraging to sedentary agriculture was a major turning point in human evolutionary history, increasing our population size and eventually leading to the development of modern societies. We however lack understanding of the changes in life histories that contributed to the increased population growth rate of agriculturalists, because comparable individual-based reproductive records of sympatric populations of agriculturalists and foragers are rarely found. Here, we compared key life-history traits and population growth rate using comprehensive data from the seventieth to nineteenth century Northern Finland: indigenous Sami were nomadic hunter-fishers and reindeer herders, whereas sympatric agricultural Finns relied predominantly on animal husbandry. We found that agriculture-based families had higher lifetime fecundity, faster birth spacing and lower maternal mortality. Furthermore, agricultural Finns had 6.2% higher annual population growth rate than traditional Sami, which was accounted by differences between the subsistence modes in age-specific fecundity but not in mortality. Our results provide, to our knowledge, the most detailed demonstration yet of the demographic changes and evolutionary benefits that resulted from agricultural revolution. PMID:25232134

  8. Risk perception related to depletion of the ozone layer and UV-B radiation in the arctic.

    PubMed

    Kolstad, A

    1998-01-01

    Increase in UV-B radiation, due to stratospheric ozone depletion, is an environmental threat to arctic ecosystems and the health of their inhabitants. The aims of this longitudinal study are to provide basic population risk perception data related to UV-B and ozone depletion, and to compare the UV-B risk perception over time and with risk perception related to other objects and occurrences. A survey questionnaire, calling for a total of 118 judgments, measures risk perception, worries, and anticipated consequences. In the 1996 study, 143 persons completed the questionnaire, 34 of whom belong to the indigenous Sami population. Risk perception and the possibility of protecting oneself against 13 risks were measured on 7-point scales. The mean risk rating for depletion of the ozone layer and UV-B radiation was moderate to high. The possibility of protection was rated relatively low. Women, the youngest, and respondents in the North were most worried and perceived the highest risks. The Sami respondents are less worried and perceive a lower risk, a realistic short-term evaluation due to their protection by pigment in the skin and their clothing habits.

  9. Autonomous in situ measurements of seawater alkalinity.

    PubMed

    Spaulding, Reggie S; DeGrandpre, Michael D; Beck, James C; Hart, Robert D; Peterson, Brittany; De Carlo, Eric H; Drupp, Patrick S; Hammar, Terry R

    2014-08-19

    Total alkalinity (AT) is an important parameter for describing the marine inorganic carbon system and understanding the effects of atmospheric CO2 on the oceans. Measurements of AT are limited, however, because of the laborious process of collecting and analyzing samples. In this work we evaluate the performance of an autonomous instrument for high temporal resolution measurements of seawater AT. The Submersible Autonomous Moored Instrument for alkalinity (SAMI-alk) uses a novel tracer monitored titration method where a colorimetric pH indicator quantifies both pH and relative volumes of sample and titrant, circumventing the need for gravimetric or volumetric measurements. The SAMI-alk performance was validated in the laboratory and in situ during two field studies. Overall in situ accuracy was -2.2 ± 13.1 μmol kg(-1) (n = 86), on the basis of comparison to discrete samples. Precision on duplicate analyses of a carbonate standard was ±4.7 μmol kg(-1) (n = 22). This prototype instrument can measure in situ AT hourly for one month, limited by consumption of reagent and standard solutions. PMID:25051401

  10. Roads not taken: A narrative positioning analysis of older adults' stories about missed opportunities.

    PubMed

    Blix, Bodil Hansen; Hamran, Torunn; Normann, Hans Ketil

    2015-12-01

    The point of departure for this article is narrative gerontology's conceptualization of life as storied and the assumption that identity development and meaning making do not cease at any age, but rather continue throughout life. We suggest that if identity construction is considered to be a lifelong project, narrative gerontology would benefit from applying analytical perspectives focused on the situated activity of narration. In this article, we apply a three-level positioning analysis to segments of interviews with two elderly Sami women concerning missed opportunities or roads not taken and, more specifically, to narrations about missed opportunities for education. We argue that such narrations should not necessarily be considered expressions of regret or processes of reconciliation but rather as pivotal in here-and-now identity constructions. Narrations about missed opportunities demonstrate that what narrators choose to insert into their life stories is chosen for a purpose and for an audience in a specific interpersonal and discursive context. We suggest that narrative gerontology would benefit from a broader focus on the diversity of sites of engagement in which older adults perform identity constructions. This shift implies moving beyond traditional studies of older adults' life stories and biographical narratives as related in the context of qualitative research interviews (of which the present study of Sami older adults' life stories is indeed an example). PMID:26568226

  11. LZIFU: an emission-line fitting toolkit for integral field spectroscopy data

    NASA Astrophysics Data System (ADS)

    Ho, I.-Ting; Medling, Anne M.; Groves, Brent; Rich, Jeffrey A.; Rupke, David S. N.; Hampton, Elise; Kewley, Lisa J.; Bland-Hawthorn, Joss; Croom, Scott M.; Richards, Samuel; Schaefer, Adam L.; Sharp, Rob; Sweet, Sarah M.

    2016-09-01

    We present lzifu (LaZy-IFU), an idl toolkit for fitting multiple emission lines simultaneously in integral field spectroscopy (IFS) data. lzifu is useful for the investigation of the dynamical, physical and chemical properties of gas in galaxies. lzifu has already been applied to many world-class IFS instruments and large IFS surveys, including the Wide Field Spectrograph, the new Multi Unit Spectroscopic Explorer (MUSE), the Calar Alto Legacy Integral Field Area (CALIFA) survey, the Sydney-Australian-astronomical-observatory Multi-object Integral-field spectrograph (SAMI) Galaxy Survey. Here we describe in detail the structure of the toolkit, and how the line fluxes and flux uncertainties are determined, including the possibility of having multiple distinct kinematic components. We quantify the performance of lzifu, demonstrating its accuracy and robustness. We also show examples of applying lzifu to CALIFA and SAMI data to construct emission line and kinematic maps, and investigate complex, skewed line profiles presented in IFS data. The code is made available to the astronomy community through github. lzifu will be further developed over time to other IFS instruments, and to provide even more accurate line and uncertainty estimates.

  12. A mechanism for S-adenosyl methionine assisted formation of a riboswitch conformation: a small molecule with a strong arm

    PubMed Central

    Huang, Wei; Kim, Joohyun; Jha, Shantenu; Aboul-ela, Fareed

    2009-01-01

    The S-adenosylmethionine-1 (SAM-I) riboswitch mediates expression of proteins involved in sulfur metabolism via formation of alternative conformations in response to binding by SAM. Models for kinetic trapping of the RNA in the bound conformation require annealing of nonadjacent mRNA segments during a transcriptional pause. The entropic cost required to bring nonadjacent segments together should slow the folding process. To address this paradox, we performed molecular dynamics simulations on the SAM-I riboswitch aptamer domain with and without SAM, starting with the X-ray coordinates of the SAM-bound RNA. Individual trajectories are 200 ns, among the longest reported for an RNA of this size. We applied principle component analysis (PCA) to explore the global dynamics differences between these two trajectories. We observed a conformational switch between a stacked and nonstacked state of a nonadjacent dinucleotide in the presence of SAM. In the absence of SAM the coordination between a bound magnesium ion and the phosphate of A9, one of the nucleotides involved in the dinucleotide stack, is destabilized. An electrostatic potential map reveals a ‘hot spot’ at the Mg binding site in the presence of SAM. These results suggest that SAM binding helps to position J1/2 in a manner that is favorable for P1 helix formation. PMID:19720737

  13. Low-latitude midnight brightness in 630.0 nm limb observations by FORMOSAT-2/ISUAL

    NASA Astrophysics Data System (ADS)

    Rajesh, P. K.; Chen, C. H.; Lin, C. H.; Liu, J. Y.; Huba, J. D.; Chen, A. B.; Hsu, R. R.; Chen, Y. T.

    2014-06-01

    This paper investigates the intense airglow brightness often observed in the 630.0 nm limb images taken using Imager of Sprites and Upper Atmospheric Lightnings (ISUAL), onboard FORMOSAT-2 satellite, where the tangent plane of the measurement falls in the local midnight sector. Most of the images show only single brightness, but in some cases there could be multiple peaks, which sometimes appears to be centered on geographic equator and in some cases falls on either sides of the magnetic equator. In order to understand such intense emission in the near-midnight hours, the observations are simulated using SAMI2 (SAMI2 is Another Model of the Ionosphere) model parameters based on the ISUAL viewing geometry. The simulations reproduced the measured airglow intensity pattern quite remarkably and suggested that the meridional neutral wind and the resulting plasma distribution are closely related with the observed brightness. The intensity and locations of the airglow brightness peaks could potentially be utilized to infer the strength of meridional neutral wind.

  14. ["Thank you, doctor". Knowledge of intercultural communication is necessary in health care for refugees].

    PubMed

    Hetta, O M

    1992-03-20

    Up to now, the Norwegian population has been homogeneous as regards language and culture, the only exception being the 30,000 indigenous Sami people. With the recent increase of the number of immigrants, particularly refugees and asylum seekers, Norwegian health care workers are faced with a new challenge: communication barriers due to differences in culture. This article lists 12 signal systems and shows how messages can be transmitted, interpreted and misinterpreted, depending on cultural background. Our world view and socio-cultural reference is important for how we interpret messages conveyed in the form of words and nonverbal signals. Ten commandments regarding refugee/intercultural health care are formulated as practical guidelines. PMID:1553731

  15. Dip-coating process: Silicon sheet growth development for the large-area silicon sheet task of the low-cost silicon solar array project

    NASA Technical Reports Server (NTRS)

    Zook, J. D.; Heaps, J. D.; Maciolek, R. B.; Koepke, B. G.; Gutter, C. D.; Schuldt, S. B.

    1977-01-01

    The objective of this research program is to investigate the technical and economic feasibility of producing solar-cell-quality sheet silicon by coating one surface of carbonized ceramic substrates with a thin layer of large-grain polycrystalline silicon from the melt. The past quarter demonstrated significant progress in several areas. Seeded growth of silicon-on-ceramic (SOC) with an EFG ribbon seed was demonstrated. Different types of mullite were successfully coated with silicon. A new method of deriving minority carrier diffusion length, L sub n from spectral response measurements was evaluated. ECOMOD cost projections were found to be in good agreement with the interim SAMIS method proposed by JPL. On the less positive side, there was a decrease in cell performance which we believe to be due to an unidentified source of impurities.

  16. HAARP-Induced Ionospheric Ducts

    SciTech Connect

    Milikh, Gennady; Vartanyan, Aram

    2011-01-04

    It is well known that strong electron heating by a powerful HF-facility can lead to the formation of electron and ion density perturbations that stretch along the magnetic field line. Those density perturbations can serve as ducts for ELF waves, both of natural and artificial origin. This paper presents observations of the plasma density perturbations caused by the HF-heating of the ionosphere by the HAARP facility. The low orbit satellite DEMETER was used as a diagnostic tool to measure the electron and ion temperature and density along the satellite orbit overflying close to the magnetic zenith of the HF-heater. Those observations will be then checked against the theoretical model of duct formation due to HF-heating of the ionosphere. The model is based on the modified SAMI2 code, and is validated by comparison with well documented experiments.

  17. The starfish diagram: Visualising data within the context of survey samples

    NASA Astrophysics Data System (ADS)

    Konstantopoulos, I. S.

    2015-04-01

    As astronomy becomes increasingly invested in large surveys the ample representation of an individual target becomes a significant challenge. Tabulations of basic properties can convey the message in an absolute sense but not within the context of the sample from which the individual is drawn. We present a novel but simple plot that simultaneously visualises the properties of the sample and the individual. Numbers and characters are kept at an absolute minimum to enable the stacking of such plots without introducing too much verbal information. Once the user becomes accustomed to their appearance, a set of starfish diagrams provides a direct representation of the individual within a sample, or between various samples. The utility and versatility of the plot is demonstrated through its application to astrophysical data (SAMI Galaxy Survey) and sports statistics. We provide a brief description of the concept and the source code, which is simple to adapt to any statistical dataset, be it descriptive of physics, demographics, finance, and more.

  18. Assessment of the Potential to Reduce Emissions from Road Transportation, Notably NOx, Through the Use of Alternative Vehicles and Fuels in the Great Smoky Mountains Region

    SciTech Connect

    Sheffield, J.

    2001-08-30

    Air pollution is a serious problem in the region of the Great Smoky Mountains. The U.S. Environmental Protection Agency (EPA) may designate non-attainment areas by 2003 for ozone. Pollutants include nitrogen oxides (NO{sub x}), sulfur dioxide (SO{sub 2}), carbon monoxide (CO), volatile organic compounds (VOCs), lead, and particulate matter (PM), which are health hazards, damage the environment, and limit visibility. The main contributors to this pollution are industry, transportation, and utilities. Reductions from all contributors are needed to correct this problem. While improvements are projected in each sector over the next decades, the May 2000 Interim Report issued by the Southern Appalachian Mountains Initiative (SAMI) suggests that the percentage of NO{sub x} emissions from transportation may increase.

  19. On the decline of ground lichen forests in the Swedish boreal landscape: Implications for reindeer husbandry and sustainable forest management.

    PubMed

    Sandström, Per; Cory, Neil; Svensson, Johan; Hedenås, Henrik; Jougda, Leif; Borchert, Nanna

    2016-05-01

    Lichens are a bottleneck resource for circumpolar populations of reindeer, and as such, for reindeer husbandry as an indigenous Sami land-use tradition in northern Sweden. This study uses ground lichen data and forest information collected within the Swedish National Forest Inventory since 1953, on the scale of northern Sweden. We found a 71 % decline in the area of lichen-abundant forests over the last 60 years. A decline was observed in all regions and age classes and especially coincided with a decrease of >60 year old, open pine forests, which was the primary explanatory factor in our model. The effects of reindeer numbers were inconclusive in explaining the decrease in lichen-abundant forest. The role that forestry has played in causing this decline can be debated, but forestry can have a significant role in reversing the trend and improving ground lichen conditions.

  20. Pipe3D, a pipeline to analyze Integral Field Spectroscopy Data: I. New fitting philosophy of FIT3D

    NASA Astrophysics Data System (ADS)

    Sánchez, S. F.; Pérez, E.; Sánchez-Blázquez, P.; González, J. J.; Rosález-Ortega, F. F.; Cano-Dí az, M.; López-Cobá, C.; Marino, R. A.; Gil de Paz, A.; Mollá, M.; López-Sánchez, A. R.; Ascasibar, Y.; Barrera-Ballesteros, J.

    2016-04-01

    We present an improved version of FIT3D, a fitting tool for the analysis of the spectroscopic properties of the stellar populations and the ionized gas derived from moderate resolution spectra of galaxies. This tool was developed to analyze integral field spectroscopy data and it is the basis of Pipe3D, a pipeline used in the analysis of CALIFA, MaNGA, and SAMI data. We describe the philosophy and each step of the fitting procedure. We present an extensive set of simulations in order to estimate the precision and accuracy of the derived parameters for the stellar populations and the ionized gas. We report on the results of those simulations. Finally, we compare the results of the analysis using FIT3D with those provided by other widely used packages, and we find that the parameters derived by FIT3D are fully compatible with those derived using these other tools.

  1. MCMC Analysis of biases in the interpretation of disk galaxy kinematics

    NASA Astrophysics Data System (ADS)

    Aquino-Ortíz, E.; Valenzuela, O.; Cano-Díaz, M.; Sánchez-Sánchez, S. F.; Hernández-Toledo, H.

    2016-06-01

    The new generation of galaxy surveys like SAMI, CALIFA and MaNGA opens up the possibility of studying simultaneously properties of galaxies such as spiral arms, bars, disk geometry and orientation, stellar and gas mass distribution, 2D kinematics, etc. The previous task involves exploring a complicated multi-dimensional parameter space. Puglielli et al. (2010) introduced Bayesian statistics and MCMC (Monte Carlo Markov Chain) techniques to construct dynamical models of spiral galaxies. In our study we used synthetic velocity fields that include non-circular motions and assume different disk orientations in order to produce mock observations. We apply popular reconstruction techniques in order to estimate the geometrical disk parameters, systemic velocities, rotation curve shape and maximum circular velocity which are crucial to construct the scaling relations. We conclude that a detailed analysis of kinematics in galaxies using MCMC technique will be reflected in accurate estimations of galaxy properties and more robust scalings relations, otherwise physical conclusions may be importantly biased.

  2. A coupled ionosphere-raytrace model for high-power HF heating

    NASA Astrophysics Data System (ADS)

    Zawdie, K. A.; Huba, J. D.; Drob, D. P.; Bernhardt, P. A.

    2015-11-01

    The first 3-D model of artificial HF ionospheric heating to self-consistently calculate the modification in heating location due to evolving ionospheric gradients has been developed. The model combines the ionosphere model SAMI3/ESF and the HF propagation code MoJo-15. At each time step, the simulated path of the HF wave through the ionosphere is used to determine the HF heating location. These calculations have been used to explain the physical mechanism responsible for the snapback effect observed in an Arecibo HF heating experiment described by Bernhardt et al. (1988). The heater wave is refracted by the density cavity, which causes the heating location to drift in longitude. Eventually, the density cavity convects into the path of the refracted ray, such that only a small portion of the ray is above the threshold for HF heating and the heating location snaps back even though the ray itself is still refracted in longitude.

  3. Data and Information Exchange System for the "Reindeer Mapper" Project

    NASA Technical Reports Server (NTRS)

    Maynard, Nancy; Yurchak, Boris

    2005-01-01

    During this past year, the Reindeer Mapper Intranet system has been set up on the NASA system, 8 team members have been established, a Reindeer Mapper reference list containing 696 items has been entered, 6 power point presentations have been put on line for review among team members, 304 satellite images have been catalogued (including 16 Landsat images, 288 NDVI 10-day composited images and an anomaly series- May 1998 to December 2002, and 56 SAR CEOS S A R format files), schedules and meeting dates are being shared, students at the Nordic Sami Institute are experimenting with the system for reindeer herder indigenous knowledge sharing, and an "address book" is being developed. Several documents and presentations have been translated and made available in Russian for our Russian colleagues. This has enabled our Russian partners to utilize documents and presentations for use in their research (e.g., SAR imagery comparisons with Russian GIS of specific study areas) and discussion with local colleagues.

  4. Can HF heating generate ESF bubbles?

    NASA Astrophysics Data System (ADS)

    Zawdie, K. A.; Huba, J. D.

    2014-12-01

    The injection of powerful HF waves into the ionosphere can lead to strong electron heating followed by a pressure perturbation which can locally reduce the plasma density. In the postsunset equatorial ionosphere, density perturbations can provide the seed to generate equatorial spread F (ESF) bubbles. In this paper, a modified version of the SAMI3/ESF ionosphere code is used to model the density depletions created by HF heating and to determine if ESF bubbles can be artificially generated. It is found that HF heating primarily redistributes plasma along the geomagnetic field and does not significantly perturb the flux tube integrated conductivities. Thus, HF heating does not appear to be a viable method to seed or generate ESF bubbles.

  5. Global signatures and seasonal variations of 630.0 nm nightglow

    NASA Astrophysics Data System (ADS)

    Chiang, J. C.; Chang, T.; Tam, S. W.; Huang, T.; Lin, C.; Chen, A. B.; Hsu, R.

    2010-12-01

    This report investigates the global midnight brightness distribution around 23:00 local time through FORMOSAT-2/ISUAL Satellite imaging observations. We focus on the OI 630.0 nm nightglow emission at ~250 km altitudes near the equator. The database used in this study includes data from 2007 to 2008. The data statistics are separated by the four seasons. The results show that the midnight brightness often occurs near the geographic equator. And the seasonal variations of the brightening locations are observed in a tendency to show up in the summer hemisphere. But the weaker nightglow brightness tends to appear from May to July. The observations presented here are also compared with modeled electron density based on the SAMI2 model. We suggest that the midnight brightness is contributed from not only pre-reversal enhancement but also from thermospheric midnight temperature maximum (MTM) effect.

  6. Understanding consistencies and gaps between desired forest futures: An analysis of visions from stakeholder groups in Sweden.

    PubMed

    Sandström, Camilla; Carlsson-Kanyama, Annika; Lindahl, Karin Beland; Sonnek, Karin Mossberg; Mossing, Annika; Nordin, Annika; Nordström, Eva-Maria; Räty, Riitta

    2016-02-01

    Conflicting perspectives on forests has for a long time challenged forest policy development in Sweden. Disagreements about forest futures create intractable deadlocks when stakeholders talk past each other. The purpose of this study is to move beyond this situation through the application of participatory backcasting. By comparing visions of the future forest among stakeholder groups, we highlight contemporary trajectories and identify changes that were conceived as desirable. We worked with four groups: the Biomass and Bioenergy group, the Conservation group, the Sami Livelihood group and the Recreation and Rural Development group; in total representatives from 40 organizations participated in workshops articulating the groups' visions. Our results show well-known tensions such as intrinsic versus instrumental values but also new ones concerning forests' social values. Identified synergies include prioritization of rural development, new valued-added forest products and diversified forest management. The results may feed directly into forest policy processes facilitating the process and break current deadlocks. PMID:26744046

  7. On the decline of ground lichen forests in the Swedish boreal landscape: Implications for reindeer husbandry and sustainable forest management.

    PubMed

    Sandström, Per; Cory, Neil; Svensson, Johan; Hedenås, Henrik; Jougda, Leif; Borchert, Nanna

    2016-05-01

    Lichens are a bottleneck resource for circumpolar populations of reindeer, and as such, for reindeer husbandry as an indigenous Sami land-use tradition in northern Sweden. This study uses ground lichen data and forest information collected within the Swedish National Forest Inventory since 1953, on the scale of northern Sweden. We found a 71 % decline in the area of lichen-abundant forests over the last 60 years. A decline was observed in all regions and age classes and especially coincided with a decrease of >60 year old, open pine forests, which was the primary explanatory factor in our model. The effects of reindeer numbers were inconclusive in explaining the decrease in lichen-abundant forest. The role that forestry has played in causing this decline can be debated, but forestry can have a significant role in reversing the trend and improving ground lichen conditions. PMID:26754169

  8. Modulational Instability of Cylindrical and Spherical NLS Equations. Statistical Approach

    SciTech Connect

    Grecu, A. T.; Grecu, D.; Visinescu, Anca; De Nicola, S.; Fedele, R.

    2010-01-21

    The modulational (Benjamin-Feir) instability for cylindrical and spherical NLS equations (c/s NLS equations) is studied using a statistical approach (SAMI). A kinetic equation for a two-point correlation function is written and analyzed using the Wigner-Moyal transform. The linear stability of the Fourier transform of the two-point correlation function is studied and an implicit integral form for the dispersion relation is found. This is solved for different expressions of the initial spectrum (delta-spectrum, Lorentzian, Gaussian), and in the case of a Lorentzian spectrum the total growth of the instability is calculated. The similarities and differences with the usual one-dimensional NLS equation are emphasized.

  9. Time-series records of pCO{sub 2} and NO{sub 3} during the OMP Field Program: a final report for DOE Grant DE-FG03-96ER62224

    SciTech Connect

    Michael D. DeGrandpre

    2000-04-01

    The specific goals of this research are to (1) determine daily and seasonal variability of seawater pCO{sub 2} partial pressure of CO{sub 2} and NO{sub 3} in Middle Atlantic Bight (MAB) waters; (2) estimate seasonal CO{sub 2} fluxes between the MAB shelf and the atmosphere; and (3) determine the primary controls of surface seawater pCO{sub 2} in this coastal system. During the first phase of the DOE-OMP (1992-1995) we developed the Submersible Autonomous Moored Instrument for CO{sub 2} (SAMI-CO{sub 2}) which is designed to measure seawater CO{sub 2} on ocean moorings for extended periods.

  10. Cone of Darkness: Finding Blank-sky Positions for Multi-object Wide-field Observations

    NASA Astrophysics Data System (ADS)

    Lorente, N. P. F.

    2014-05-01

    We present the Cone of Darkness, an application to automatically configure blank-sky positions for a series of stacked, wide-field observations, such as those carried out by the SAMI instrument on the Anglo-Australian Telescope (AAT). The Sydney-AAO Multi-object Integral field spectrograph (SAMI) uses a plug-plate to mount its 13×61 core imaging fibre bundles (hexabundles) in the optical plane at the telescope's prime focus. To make the most efficient use of each plug-plate, several observing fields are typically stacked to produce a single plate. When choosing blank-sky positions for the observations it is most effective to select these such that one set of 26 holes gives valid sky positions for all fields on the plate. However, when carried out manually this selection process is tedious and includes a significant risk of error. The Cone of Darkness software aims to provide uniform blank-sky position coverage over the field of observation, within the limits set by the distribution of target positions and the chosen input catalogs. This will then facilitate the production of the best representative median sky spectrum for use in sky subtraction. The application, written in C++, is configurable, making it usable for a range of instruments. Given the plate characteristics and the positions of target holes, the software segments the unallocated space on the plate and determines the position which best fits the uniform distribution requirement. This position is checked, for each field, against the selected catalog using a TAP ADQL search. The process is then repeated until the desired number of sky positions is attained.

  11. Low latitude Ionospheric response to the recent super storm of 17 March 2015: Modeling perspectives and recent findings

    NASA Astrophysics Data System (ADS)

    Joshi, L. M.; Sripathi, S.; Singh, R.

    2015-12-01

    In this paper, simulation of low latitude ionospheric response to the recent super geomagnetic storm of 17 March 2015 at Indian longitude, utilizing SAMI2 codes by incorporating Doppler EXB drift, relevant to the storm period, is being presented. Intense enhancement in the EXB drift of 60 to 70 m/s over magnetic equator was observed in the evening hours of 17 March due to the prompt penetration of the high latitude electric field. This remarkable intensification of EXB drift transported the F layer to beyond 550 km altitude, quite unusual in the Indian sector. Model EXB drift in the day time during the recovery phase of the super storm was slightly westward, unlike the eastward EXB drift during the quiet day. This has been found to be linked with the disturbance dynamo during the recovery phase. SAMI2 model, utilizing the Doppler EXB drift during the evening hours and model EXB drift during the rest of the period, could simulate the intense F layer height rise and latitudinal expansion of EIA during storm main phase. Equator ward disturbance thermospheric winds during the recovery phase have also been incorporated in the simulation. Simulation results also indicated a complete suppression of the equatorial ionization anomaly (EIA) during the recovery phase, linked with the westward disturbance dynamo electric field. Model simulations indicate the role of the disturbance neutral winds during the recovery phase in enhancing the plasma density, however, the development of the EIA has been found to be controlled by the zonal electric field. The model results have been compared with the ground observations of the total electron content (TEC). TEC map over the Indian region shows a remarkable suppression of the EIA during the recovery phase of the geomagnetic storm. Peculiarities of this super storm will also be discussed in the light of the current understanding of the space weather impact on the low latitude ionosphere.

  12. Design and methods in a survey of living conditions in the Arctic – the SLiCA study

    PubMed Central

    Eliassen, Bent-Martin; Melhus, Marita; Kruse, Jack; Poppel, Birger; Broderstad, Ann Ragnhild

    2012-01-01

    Objectives The main objective of this study is to describe the methods and design of the survey of living conditions in the Arctic (SLiCA), relevant participation rates and the distribution of participants, as applicable to the survey data in Alaska, Greenland and Norway. This article briefly addresses possible selection bias in the data and also the ways to tackle it in future studies. Study design Population-based cross-sectional survey. Methods Indigenous individuals aged 16 years and older, living in Greenland, Alaska and in traditional settlement areas in Norway, were invited to participate. Random sampling methods were applied in Alaska and Greenland, while non-probability sampling methods were applied in Norway. Data were collected in 3 periods: in Alaska, from January 2002 to February 2003; in Greenland, from December 2003 to August 2006; and in Norway, in 2003 and from June 2006 to June 2008. The principal method in SLiCA was standardised face-to-face interviews using a questionnaire. Results A total of 663, 1,197 and 445 individuals were interviewed in Alaska, Greenland and Norway, respectively. Very high overall participation rates of 83% were obtained in Greenland and Alaska, while a more conventional rate of 57% was achieved in Norway. A predominance of female respondents was obtained in Alaska. Overall, the Sami cohort is older than the cohorts from Greenland and Alaska. Conclusions Preliminary assessments suggest that selection bias in the Sami sample is plausible but not a major threat. Few or no threats to validity are detected in the data from Alaska and Greenland. Despite different sampling and recruitment methods, and sociocultural differences, a unique database has been generated, which shall be used to explore relationships between health and other living conditions variables. PMID:22456042

  13. Analysis of the enhanced negative correlation between electron density and electron temperature related to earthquakes

    NASA Astrophysics Data System (ADS)

    Shen, X. H.; Zhang, X.; Liu, J.; Zhao, S. F.; Yuan, G. P.

    2015-04-01

    Ionospheric perturbations in plasma parameters have been observed before large earthquakes, but the correlation between different parameters has been less studied in previous research. The present study is focused on the relationship between electron density (Ne) and temperature (Te) observed by the DEMETER (Detection of Electro-Magnetic Emissions Transmitted from Earthquake Regions) satellite during local nighttime, in which a positive correlation has been revealed near the equator and a weak correlation at mid- and low latitudes over both hemispheres. Based on this normal background analysis, the negative correlation with the lowest percent in all Ne and Te points is studied before and after large earthquakes at mid- and low latitudes. The multiparameter observations exhibited typical synchronous disturbances before the Chile M8.8 earthquake in 2010 and the Pu'er M6.4 in 2007, and Te varied inversely with Ne over the epicentral areas. Moreover, statistical analysis has been done by selecting the orbits at a distance of 1000 km and ±7 days before and after the global earthquakes. Enhanced negative correlation coefficients lower than -0.5 between Ne and Te are found in 42% of points to be connected with earthquakes. The correlation median values at different seismic levels show a clear decrease with earthquakes larger than 7. Finally, the electric-field-coupling model is discussed; furthermore, a digital simulation has been carried out by SAMI2 (Sami2 is Another Model of the Ionosphere), which illustrates that the external electric field in the ionosphere can strengthen the negative correlation in Ne and Te at a lower latitude relative to the disturbed source due to the effects of the geomagnetic field. Although seismic activity is not the only source to cause the inverse Ne-Te variations, the present results demonstrate one possibly useful tool in seismo-electromagnetic anomaly differentiation, and a comprehensive analysis with multiple parameters helps to

  14. Exploring the role of ionospheric drivers during the extreme solar minimum of 2008

    NASA Astrophysics Data System (ADS)

    Klenzing, J.; Burrell, A. G.; Heelis, R. A.; Huba, J. D.; Pfaff, R.; Simões, F.

    2013-12-01

    During the recent solar minimum, solar activity reached the lowest levels observed during the space age, resulting in a contracted atmosphere. This extremely low solar activity provides an unprecedented opportunity to understand the variability of the Earth's ambient ionosphere. The average E × B drifts measured by the Vector Electric Field Instrument (VEFI) on the Communications/Navigation Outage Forecasting System (C/NOFS) satellite during this period are found to have several differences from the expected climatology based on previous solar minima, including downward drifts in the early afternoon and a weak to non-existent pre-reversal enhancement. Using SAMI2 (Sami2 is Another Model of the Ionosphere) as a computational engine, we investigate the effects of these electrodynamical changes as well as the contraction of the thermosphere and reduced EUV ionization on the ionosphere. The sensitivity of the simulations to wind models is also discussed. These modeled ionospheres are compared to the C/NOFS average topside ion density and composition and Formosa Satellite-3/Constellation Observing System for Meteorology, Ionosphere, and Climate average NmF2 and hmF2. In all cases, incorporating the VEFI drift data significantly improves the model results when compared to both the C/NOFS density data and the F3/C GOX data. Changing the MSIS and EUVAC models produced changes in magnitude, but not morphology with respect to local time. The choice of wind model modulates the resulting topside density and composition, but only the use of the VEFI E × B drifts produces the observed post-sunset drop in the F peak.

  15. Nonmigrating tidal signature in the distributions of equatorial plasma bubbles and prereversal enhancement

    NASA Astrophysics Data System (ADS)

    Kil, Hyosub; Kwak, Young-Sil; Lee, Woo Kyoung; Krall, Jonathan; Huba, Joseph D.; Oh, Seung-Jun

    2015-04-01

    Some wave-like features in the longitudinal distribution of equatorial plasma bubbles understood in association with diurnal eastward propagating zonal wave number 3 nonmigrating tide (DE3) in the dayside. However, whether or not the wave features are the daytime DE3 signature has not yet been rigorously investigated. This study investigates (1) the existence of the DE3 signature in the longitudinal distribution of bubbles by analyzing the first Republic of China (ROCSAT-1) satellite data acquired in 2000-2002 and (2) the role of daytime DE3 in the creation of bubbles by examining the linear growth rate of the generalized Rayleigh-Taylor (R-T) instability. The linear growth rate is derived from the "Sami2 is Another Model of the Ionosphere" model simulation results. In the longitudinal distribution of bubbles derived from ROCSAT-1 observations, the wave number 4 component, the representative characteristic of DE3, is a weak feature. In addition, the amplitude and phase of the wave number 4 component do not show a consistent behavior in comparison with those of DE3. Our numerical calculation results show that the linear growth rate of the R-T instability is not sensitive to the variation of the daytime vertical plasma drift. These results indicate that the DE3 signature in the occurrence rate of bubbles is not obvious and the effect of daytime DE3 on the creation of bubbles is negligible.

  16. Dipole response in neutron-rich nuclei with new Skyrme interactions

    NASA Astrophysics Data System (ADS)

    Zheng, H.; Burrello, S.; Colonna, M.; Baran, V.

    2016-07-01

    We investigate the isoscalar and isovector E 1 response of neutron-rich nuclei, within a semiclassical transport model employing effective interactions for the nuclear mean field. In particular, we adopt the recently introduced SAMi-J Skyrme interactions, whose parameters are specifically tuned to improve the description of spin-isospin properties of nuclei. Our analysis evidences a relevant degree of isoscalar-isovector mixing of the collective excitations developing in neutron-rich systems. Focusing on the low-lying strength emerging in the isovector response, we show that this energy region essentially corresponds to the excitation of isoscalar-like modes, which also contribute to the isovector response owing to their mixed character. Considering effective interactions which mostly differ in the isovector channels, we observe that these mixing effects increase with the slope L of the symmetry energy at saturation density, leading to a larger strength in the low-energy region of the isovector response. This result appears connected to the increase, with L , of the neutron-proton asymmetry at the surface of the considered nuclei, i.e., to the neutron skin thickness.

  17. Maskevarri Ráhppát in Finnmark, northern Norway - is it an earthquake-induced landform complex?

    NASA Astrophysics Data System (ADS)

    Sutinen, R.; Aro, I.; Närhi, P.; Piekkari, M.; Middleton, M.

    2014-07-01

    The Sami word ráhppát means rough bouldery/stony terrain with sharp-relief topography in Finnmark, northern Norway. Ráhppát is a common name in the region of the Younger Dryas landforms, yet the origin of ráhppát has remained obscure. The timing of the Younger Dryas is concomitant with the maximum neotectonic fault instability in Fennoscandia. Hence, earthquake activity may have been one of the contributing factors for the Younger Dryas morphologies. Ráhppát on the Maskevarri fell, classified as a part of Tromsø-Lyngen sub-stage of the Younger Dryas, was studied by means of geomorphology and measurements of electrical-sedimentary anisotropy. Ráhppát was found to be built up of an anastomosing network of stony esker-like ridges and mounds bordered with arch-shaped and sinusoidal ridges. These bordering ridges exhibit sedimentary (azimuthal soil electrical conductivity) anisotropy parallel-to-ridge trends and were interconnected to meltwater gullies suggesting generation through short-lived conduit infills. We did not find electrical-sedimentary evidence to support the concept of englacial thrusting and/or compression, often described for Younger Dryas moraines. Maskevarri Ráhppát is typified by ~ 500 ponds and small lakes on three different elevations descending in an up-ice direction. These may have generated through late glacial earthquake(s) also contributing to subglacial deformation of Maskevarri Ráhppát.

  18. Summertime pCO2 in the Cumberland Sound in the eastern Arctic

    NASA Astrophysics Data System (ADS)

    Turk, D.; Vagle, S.; Thomas, H.; Bedard, J.; Burt, W.; Manizza, M.; McGillis, W. R.; Wallace, D.

    2012-12-01

    The Arctic Ocean is estimated to contribute roughly 10% of the global annual uptake of CO2 in the ocean. Studies show this appears to be particularly sensitive to environmental changes. However this estimate as well as the impact of environmental conditions on the sources and sinks of carbon dioxide is based on limited data currently available in the Arctic. Here, we present the first measurements of water pCO2 in the Cumberland Sound during the summer of 2011. Cumberland Sound is a major inlet, 300 km long, with an average width of 65 km, in the east coast of Baffin Island connected the Labrador Sea and affected by multiple freshwater sources. Measurements were performed during the ice-free season using the a SAMI-pCO2 and collecting profiles of discrete water samples in the upper 40m. The pCO2 measurements are combined with physical observations and satellite chlorophyll estimates, and compared to biogeochemical model results.

  19. Prompt Ion Outflows and Artificial Ducts during High-Power HF Heating at HAARP: Effect of Suprathermal Electrons?

    NASA Astrophysics Data System (ADS)

    Mishin, E. V.; Milikh, G. M.

    2014-12-01

    In situ observations from the DMSP and Demeter satellites established that high-power HF heating of the ionosphere F-region results in significant ion outflows associated with 10-30% density enhancements in the topside ionosphere magnetically-conjugate to the heated region. As follows from the SAMI2 two-fluid model calculations, their formation time should exceed 5-7 minutes. However, specially designed DMSP-HAARP experiments have shown that artificial ducts and ion outflows appear on the topside within 2 minutes. We describe the results of these observations and present a semi-quantitative explanation of the fast timescale due to suprathermal electrons accelerated by HF-induced plasma turbulence. There are two possible effects of suprathermal electrons: (1) the increase of the ambipolar electric field over the usual thermal ambipolar diffusion and (2) excitation of heat flux-driven plasma instability resulting in an anomalous electron-ion momentum exchange. Both effects result in faster upward ion flows.

  20. Dynamics of Subauroral Polarization Stream (SAPS) Structures

    NASA Astrophysics Data System (ADS)

    Sazykin, S. Y.; Coster, A. J.; Huba, J.; Ridley, A. J.; Erickson, P. J.; Foster, J. C.; Baker, J. B. H.; Wolf, R.

    2015-12-01

    The Subauroral Polarization Stream (SAPS) flow structures are narrow ionospheric channels of fast (in excess of 100 m/s) westward drift just outside the equatorward edge of the diffuse aurora in the dusk-to-midnight local time sector. Other terms for this phenomenon include subauroral Ion Drift (SAID) events and Polarization Jets. SAPS structures represent a striking departure from the commonly-used two-cell convection pattern. They are thought to arise from the displacement of the downward region-2 Birkeland currents on the dusk side equatorward of the low-latitude boundary of the auroral oval during times of changing high-latitude convection. In this paper, we will use several event simulations with the SAMI3-RCM numerical model (a self-consistent ionosphere-inner magnetosphere model) and RCM-GITM (a self-consistent model of the ionosphere-thermosphere-inner magnetosphere) to analyze the relative roles of changes in the IMF Bz component, ionospheric electron density depletions, and thermospheric modifications in controlling the dynamics of SAPS. Simulation results will be compared to multi-instrument ionospheric observations.

  1. Hypoalbuminemia and Malnutrition Associated With Cow’s Milk Allergy: A Case Report

    PubMed Central

    Altinel Acoglu, Esma; Akcaboy, Meltem; Melek Oguz, Melahat; Kilic, Mustafa; Zorlu, Pelin; Senel, Saliha

    2016-01-01

    Introduction Cow’s milk allergy is the most common food allergy in children. Symptoms usually involve the skin and the gastrointestinal and respiratory tracts. Gastrointestinal tract manifestations of cow’s milk allergy are nonspecific, and are the only type that can be diagnosed in all age groups. Here, we report a rare case of cow's milk allergy in an infant with hypoalbuminemia and malnutrition. Case Presentation A nine-month-old girl was admitted to Dr. Sami Ulus maternity and children’s health and diseases training and research hospital, Ankara, Turkey, in September 2013, for weakness and swelling of the legs that had endured for two days. She had bilateral pretibial pitting (+2) edema. Laboratory data revealed albumin at 1.7 g/dL; serum Na, K, urea, creatinin, and alanine-aspartate aminotransferase levels were normal. Her urinary analysis did not reveal proteinuria. Stool samples were normal, and stool steatocrite was negative. Anti-gliadin, anti-endomysium, and anti-tissue transglutaminase antibodies were negative. Cow’s milk allergy was diagnosed due to cow’s milk-specific IgE and skin prick test results. Conclusions On rare occasions, cow’s milk allergy presents with hypoalbuminemia. When diagnosis is delayed, this allergy may impair the growth and quality of life and may even be life-threatening.

  2. Enhancing Drought Early Warning System for Sustainable Water Resources and Agricultural Management through Apllication of Space Science - Nigeria in Perspective

    NASA Astrophysics Data System (ADS)

    Okpara, J. N.; Akeh, L. E.; Anuforom, A. C.; Aribo, P. B.; Olayanju, S. O.

    Enhancing Drought Early Warning System for Sustainable Water Resources and Agriculture Management through Application of Space Science - Nigeria in Perspective BY J N Okpara L E Akeh Anuforom P B Aribo and S O Olayanju Directorate of Applied Meteorological Services Nigerian Meteorological Agency NIMET P M B 615 Garki Abuja Nigeria e-mail underline Juddy Okpara yahoo co uk and underline tonycanuforom yahoo com underline Abstract This paper attempts to highlight the importance of drought early warning system in water resources and agricultural management in Nigeria Various studies have shown that the negative impacts of droughts and other forms of extreme weather phenomena can be substantially reduced by providing early warning on any impending weather extremes X-rayed in this study are the various techniques presently used by the Nigerian Meteorological Agency NIMET in generating information for meteorological Early Warning System EWS which are based on models that make use of ground-based raingauge data and sea surface temperatures SST Komuscu standardized precipitation index SPI inclusive These methods are often limited by such factors as network density of stations limited communication infrastructure human inefficiency etc NIMET is therefore embarking on the development of a new Satellite Agrometeorological Information System SAMIS-Nigeria for famine and drought early warning The system combines satellite data with raingauge data to give a range of

  3. The Hector Survey: integral field spectroscopy of 100,000 galaxies

    NASA Astrophysics Data System (ADS)

    Bland-Hawthorn, J.

    2015-02-01

    In March 2013, the Sydney-AAO Multi-object Integral field spectrograph (SAMI) began a major survey of 3400 galaxies at the AAT, the largest of its kind to date. At the time of writing, over a third of the targets have been observed and the scientific impact has been immediate. The Manga galaxy survey has now started at the SDSS telescope and will target an even larger sample of nearby galaxies. In Australia, the community is now gearing up to deliver a major new facility called Hector that will allow integral field spectroscopy of 100 galaxies observed simultaneously. By the close of the decade, it will be possible to obtain integral field spectroscopy of 100,000 galaxies over 3000 square degrees of sky down to r=17 (median). Many of these objects will have HI imaging from the new ASKAP radio surveys. We discuss the motivation for such a survey and the use of new cosmological simulations that are properly matched to the integral field observations. The Hector survey will open up a new and unique parameter space for galaxy evolution studies.

  4. Pipe3D, a pipeline to analyze Integral Field Spectroscopy Data: II. Analysis sequence and CALIFA dataproducts

    NASA Astrophysics Data System (ADS)

    Sánchez, S. F.; Pérez, E.; Sánchez-Blázquez, P.; García-Benito, R.; Ibarra-Mede, H. J.; González, J. J.; Rosales-Ortega, F. F.; Sánchez-Menguiano, L.; Ascasibar, Y.; Bitsakis, T.; Law, D.; Cano-Díaz, M.; López-Cobá, C.; Marino, R. A.; Gil de Paz, A.; López-Sánchez, A. R.; Barrera-Ballesteros, J.; Galbany, L.; Mast, D.; Abril-Melgarejo, V.; Roman-Lopes, A.

    2016-04-01

    We present Pipe3D, an analysis pipeline based on the FIT3D fitting tool, developed to explore the properties of the stellar populations and ionized gas of integral field spectroscopy (IFS) data. Pipe3D was created to provide coherent, simple to distribute, and comparable dataproducts, independently of the origin of the data, focused on the data of the most recent IFU surveys (e.g., CALIFA, MaNGA, and SAMI), and the last generation IFS instruments (e.g., MUSE). In this article we describe the different steps involved in the analysis of the data, illustrating them by showing the dataproducts derived for NGC 2916, observed by CALIFA and P-MaNGA. As a practical example of the pipeline we present the complete set of dataproducts derived for the 200 datacubes that comprises the V500 setup of the CALIFA Data Release 2 (DR2), making them freely available through the network. Finally, we explore the hypothesis that the properties of the stellar populations and ionized gas of galaxies at the effective radius are representative of the overall average ones, finding that this is indeed the case.

  5. The global warming of group satellite galaxies

    NASA Astrophysics Data System (ADS)

    Yozin, C.; Bekki, K.

    2016-08-01

    Recent studies adopting λRe, a proxy for specific angular momentum, have highlighted how early-type galaxies (ETGs) are composed of two kinematical classes for which distinct formation mechanisms can be inferred. With upcoming surveys expected to obtain λRe from a broad range of environments (e.g. SAMI, MaNGA), we investigate in this numerical study how the λRe-ɛe distribution of fast-rotating dwarf satellite galaxies reflects their evolutionary state. By combining N-body/SPH simulations of progenitor disc galaxies (stellar mass ≃109 M⊙), their cosmologically-motivated sub-halo infall history and a characteristic group orbit/potential, we demonstrate the evolution of a satellite ETG population driven by tidal interactions (e.g. harassment). As a general result, these satellites remain intrinsically fast-rotating oblate stellar systems since their infall as early as z = 2; mis-identifications as slow rotators often arise due to a bar/spiral lifecycle which plays an integral role in their evolution. Despite the idealistic nature of its construction, our mock λRe-ɛe distribution at z < 0.1 reproduces its observational counterpart from the ATLAS3D/SAURON projects. We predict therefore how the observed λRe-ɛe distribution of a group evolves according to these ensemble tidal interactions.

  6. Scaling relations for galaxies of all types with CALIFA and MaNGA surveys.

    NASA Astrophysics Data System (ADS)

    Aquino-Ortíz, E.; Sánchez-Sánchez, S. F.; Valenzuela, O.; Cano-Díaz, M.; Hernández-Toledo, H.

    2016-06-01

    We used gas and stellar kinematics for the final Data Release of 667 spatially resolved galaxies publicly available from Calar Alto Legacy Integral Field Area survey (CALIFA) with the aim of study dynamical scaling relations as Tully & Fisher for rotation velocity, Faber & Jackson for velocity dispersion and also a combination of them through the S_{K} parameter defined as S_{K}^2 = KV_{rot}^2 + σ^2. We found a offset between gas and stellar kinematics in Tully & Fisher and Faber & Jackson relations, however when we used the S_{K} parameter all galaxies regardless of the morphological type lie in this M_{*} vs S_{k} scaling relation with a significant improvement compared with the M_{*} vs V_{rot} and M_{*} vs σ relations, in agreement with previous studies with SAMI survey, however the slope ant zero-point are different with them. We also explored different values of the K parameter, as well as different proxys to estimate V_{rot} in order to understand and characterize the physical source of scatter, slope and zero-point.

  7. Wide Integral Field Infrared Spectroscopic Survey of Nearby Galaxies

    NASA Astrophysics Data System (ADS)

    Sivanandam, Suresh; Moon, Dae-Sik; Zaritsky, Dennis F.; Chou, Richard; Meyer, Elliot; Ma, Ke; Jarvis, Miranda; Eisner, Joshua A.

    2015-01-01

    We are constructing a novel infrared integral field spectrograph with a large field of view (~50'x20') that will be available on the Kitt Peak 90' Bok telescope this spring. This wide integral field infrared spectrograph (WIFIS) operates over two wavelength ranges, zJ-band (0.9-1.35 microns) and H-band (1.5-1.8 microns), and has moderate spectral resolving power, 3,000 in zJ-band and 2,200 in H-band, respectively. WIFIS' field-of-view is comparable to current optical integral field spectrographs that are carrying out large galaxy surveys, e.g. SAMI, CALIFA, and MaNGA. We are designing a large nearby galaxy survey to complement the data already been taken by these optical integral field spectroscopic surveys. The near-infrared window provides a sensitive probe of the initial mass functions of stellar populations, the OB stellar fractions in massive star forming regions, and the kinematics of and obscured star formation within merging systems. This will be the first large scale infrared integral field spectroscopic survey of nearby galaxies.

  8. Reexamining X-mode suppression and fine structure in artificial E region field-aligned plasma density irregularities

    NASA Astrophysics Data System (ADS)

    Miceli, R. J.; Hysell, D. L.; Munk, J.; McCarrick, M.; Huba, J. D.

    2013-09-01

    Artificial field-aligned plasma density irregularities (FAIs) were generated in the E region of the ionosphere above the High Frequency Active Auroral Research Program facility during campaigns in May and August of 2012 and observed using a 30 MHz coherent scatter radar imager in Homer, Alaska. The purpose of this ionospheric modification experiment was to measure the threshold pump power required to excite thermal parametric instabilities by O-mode heating and to investigate the suppression of the FAIs by simultaneous X-mode heating. We find that the threshold pump power for irregularity excitation was consistent with theoretical predictions and increased by approximately a factor of 2 when X-mode heating was present. A modified version of the Another Model of the Ionosphere (SAMI2) ionospheric model was used to simulate the threshold experiments and suggested that the increase was entirely due to enhanced D region absorption associated with X-mode heating. Additionally, a remarkable degree of fine structure possibly caused by natural gradient drift instability in the heater-modified volume was observed in experiments performed during geomagnetically active conditions.

  9. Farley Buneman wave heating: Confirming heuristics with radar observations

    NASA Astrophysics Data System (ADS)

    Miceli, R. J.; Hysell, D. L.; Munk, J.; Huba, J. D.

    2013-12-01

    Combined observations from the Poker Flat incoherent scatter radar (PFISR) and a 30 MHz coherent scatter radar in Homer, Alaska were made during geomagnetic storms in November 2012 and March 2013. Enhanced electron temperature and density in the E region were measured by the PFISR and strong echoes from field aligned irregularities were measured by the coherent scatter radar. We compare these observations with a heuristic model of Farley Buneman waves based on the formulations of Milikh and Dimant (2002) and the SAMI2 global model of the ionosphere. The model predicts phase speed and magnetic aspect width profiles, as well as profiles of ionospheric state variables as functions of the convective electric field. By accounting for the thickness of the region where Farley Buneman waves exist and weighting the profiles accordingly, the model is capable of estimating the phase velocity and magnetic aspect width that would be observed by a coherent scatter radar. We then use the comparison to assess the empirical relationships of coherent scatter radar observations of Farley Buneman waves.

  10. Improving small-angle X-ray scattering data for structural analyses of the RNA world

    PubMed Central

    Rambo, Robert P.; Tainer, John A.

    2010-01-01

    Defining the shape, conformation, or assembly state of an RNA in solution often requires multiple investigative tools ranging from nucleotide analog interference mapping to X-ray crystallography. A key addition to this toolbox is small-angle X-ray scattering (SAXS). SAXS provides direct structural information regarding the size, shape, and flexibility of the particle in solution and has proven powerful for analyses of RNA structures with minimal requirements for sample concentration and volumes. In principle, SAXS can provide reliable data on small and large RNA molecules. In practice, SAXS investigations of RNA samples can show inconsistencies that suggest limitations in the SAXS experimental analyses or problems with the samples. Here, we show through investigations on the SAM-I riboswitch, the Group I intron P4-P6 domain, 30S ribosomal subunit from Sulfolobus solfataricus (30S), brome mosaic virus tRNA-like structure (BMV TLS), Thermotoga maritima asd lysine riboswitch, the recombinant tRNAval, and yeast tRNAphe that many problems with SAXS experiments on RNA samples derive from heterogeneity of the folded RNA. Furthermore, we propose and test a general approach to reducing these sample limitations for accurate SAXS analyses of RNA. Together our method and results show that SAXS with synchrotron radiation has great potential to provide accurate RNA shapes, conformations, and assembly states in solution that inform RNA biological functions in fundamental ways. PMID:20106957

  11. A Coupled Ionosphere-Raytrace Model for Artificial HF Heating

    NASA Astrophysics Data System (ADS)

    Zawdie, K.; Huba, J. D.; Drob, D. P.; Bernhardt, P. A.

    2015-12-01

    The first self-consistent 3D model of artificial HF ionospheric heating has been developed. The model combines the first principles ionosphere model SAMI3/ESF and the ray trace code MoJo-15. The location of HF heating is calculated by simulating the ray path through the ionosphere and determining the average heating location. This new model has been used to successfully simulate the snapback effect discovered in a Arecibo HF heating experiment described by Bernhardt et al. [1988]. The simulations provide new insight into the physical mechanism for snapback. As Bernhardt et al. [1988] hypothesized, the heater wave is refracted by the density cavity, thus causing the location of heating to drift in longitude. The cause of snapback, however, is not that the ray snaps back to its original configuration once the density cavity has convected out of range. Instead, the density cavity convects into the path of the refracted ray such that only a small portion of the ray near the original heating location is above the threshold for HF heating. The heating location thus suddenly snaps back to the original location but the ray itself is still refracted in longitude.

  12. ISM and dynamical scaling relations in the local Universe

    NASA Astrophysics Data System (ADS)

    Cortese, L.

    2016-06-01

    In the last decade we have seen a tremendous progress in our understanding of the life cycle of galaxies. Particularly powerful has been the synergy between representative surveys of cold gas, dust and metals and improved theoretical models able to follow the evolution of the different phases of the ISM in a self-consistent way. At the same time, the advent of optical integral field spectroscopic surveys is finally allowing us to quantify how the kinematical properties of gas and stars vary across the Hubble sequence. In this talk, I will review recent observational work aimed at providing a local benchmark for the study of the star formation cycle in galaxies and dynamical scaling relations in galaxies. By combining observations obtained as part the Herschel Reference Survey, the GALEX Arecibo SDSS survey, the ALFALFA survey and the SAMI Galaxy Survey, I will discuss what nearby galaxies can teach us about the interplay between kinematics, star formation, chemical enrichment and environmental effects in our neighbourhoods.

  13. Hypoalbuminemia and Malnutrition Associated With Cow’s Milk Allergy: A Case Report

    PubMed Central

    Altinel Acoglu, Esma; Akcaboy, Meltem; Melek Oguz, Melahat; Kilic, Mustafa; Zorlu, Pelin; Senel, Saliha

    2016-01-01

    Introduction Cow’s milk allergy is the most common food allergy in children. Symptoms usually involve the skin and the gastrointestinal and respiratory tracts. Gastrointestinal tract manifestations of cow’s milk allergy are nonspecific, and are the only type that can be diagnosed in all age groups. Here, we report a rare case of cow's milk allergy in an infant with hypoalbuminemia and malnutrition. Case Presentation A nine-month-old girl was admitted to Dr. Sami Ulus maternity and children’s health and diseases training and research hospital, Ankara, Turkey, in September 2013, for weakness and swelling of the legs that had endured for two days. She had bilateral pretibial pitting (+2) edema. Laboratory data revealed albumin at 1.7 g/dL; serum Na, K, urea, creatinin, and alanine-aspartate aminotransferase levels were normal. Her urinary analysis did not reveal proteinuria. Stool samples were normal, and stool steatocrite was negative. Anti-gliadin, anti-endomysium, and anti-tissue transglutaminase antibodies were negative. Cow’s milk allergy was diagnosed due to cow’s milk-specific IgE and skin prick test results. Conclusions On rare occasions, cow’s milk allergy presents with hypoalbuminemia. When diagnosis is delayed, this allergy may impair the growth and quality of life and may even be life-threatening. PMID:27621935

  14. Transcriptional and epigenetic networks of helper T and innate lymphoid cells.

    PubMed

    Shih, Han-Yu; Sciumè, Giuseppe; Poholek, Amanda C; Vahedi, Golnaz; Hirahara, Kiyoshi; Villarino, Alejandro V; Bonelli, Michael; Bosselut, Remy; Kanno, Yuka; Muljo, Stefan A; O'Shea, John J

    2014-09-01

    The discovery of the specification of CD4(+) helper T cells to discrete effector 'lineages' represented a watershed event in conceptualizing mechanisms of host defense and immunoregulation. However, our appreciation for the actual complexity of helper T-cell subsets continues unabated. Just as the Sami language of Scandinavia has 1000 different words for reindeer, immunologists recognize the range of fates available for a CD4(+) T cell is numerous and may be underestimated. Added to the crowded scene for helper T-cell subsets is the continuously growing family of innate lymphoid cells (ILCs), endowed with common effector responses and the previously defined 'master regulators' for CD4(+) helper T-cell subsets are also shared by ILC subsets. Within the context of this extraordinary complexity are concomitant advances in the understanding of transcriptomes and epigenomes. So what do terms like 'lineage commitment' and helper T-cell 'specification' mean in the early 21st century? How do we put all of this together in a coherent conceptual framework? It would be arrogant to assume that we have a sophisticated enough understanding to seriously answer these questions. Instead, we review the current status of the flexibility of helper T-cell responses in relation to their genetic regulatory networks and epigenetic landscapes. Recent data have provided major surprises as to what master regulators can or cannot do, how they interact with other transcription factors and impact global genome-wide changes, and how all these factors come together to influence helper cell function. PMID:25123275

  15. Analysis of the dynamics of thin primary mirrors for large astronomical telescopes

    NASA Technical Reports Server (NTRS)

    Ostroff, A. J.; Mccann, M.

    1973-01-01

    The NASTRAN structural analysis program was used to investigate the dynamic properties of thin primary mirrors suitable for use in large orbiting astronomical telescopes. An analysis is included of the mode shapes and modal frequencies for several thin, homogeneous, isotropic mirrors. Typical cases include two different mirror diameters, two different diameter-to-thickness ratios, and both a mirror without and a mirror with a central hole that is 22 percent of the mirror diameter. The finite-element structural model is evaluated by comparing the NASTRAN generated results with theoretical values for a simply supported, flat, circular mirror. The same model is then used for evaluating the spherical mirrors. The mode shapes and frequencies of a 0.762-meter-diameter mirror with a 60-to-1 diameter-to-thickness ratio and a three-point rigid kinematic (not overconstrained) mount are calculated and plotted for comparison with results obtained previously from the SAMIS structural analysis program for this same mirror. A static analysis is also shown for comparison with experimentally obtained influence coefficients.

  16. Systemic Manifestation of Rotavirus Infection in Children: A Report of Three Cases

    PubMed Central

    Akcaboy, Meltem; Melek Oguz, Melahat; Altınel Acoglu, Esma; Acar, Mehtap; Zorlu, Pelin; Ozbay Hosnut, Ferda; Senel, Saliha

    2016-01-01

    Introduction Rotavirus is a leading cause of acute gastroenteritis in children. Although the clinical complaints associated with rotavirus are generally gastrointestinal, including vomiting and diarrhea, data suggest that it can also cause symptoms that extend beyond the gastrointestinal tract. Case Presentations We report three pediatric cases of rotavirus infection: one accompanied by encephalopathy and two with elevated hepatic transaminase activity. The patients were admitted to Dr. Sami Ulus maternity and children’s health and diseases training and research hospital, Ankara, Turkey, from 2012 - 2014. The presented patients’ aspartate aminotransferase (AST) (1765-2614 IU L-1) and alanine aminotransferase (ALT) (1448-3558 IU L-1) levels are, to date, the highest reported levels associated with rotavirus infections, and suggest that the rotavirus can cause severe hepatic transaminase elevation. Conclusions This report aimed to increase awareness of the occurrence of extra-intestinal systemic manifestations of rotavirus infection. Although such cases may be rare, they still suggest that that rotavirus is a systemic viral infection. PMID:27781124

  17. Uplift of Ionospheric Oxygen Ions During Extreme Magnetic Storms

    NASA Technical Reports Server (NTRS)

    Tsurutani, Bruce T.; Mannucci, Anthony J.; Verkhoglyadova, Olga P.; Huba, Joseph; Lakhina, Gurbax S.

    2013-01-01

    Research reported earlier in literature was conducted relating to estimation of the ionospheric electrical field, which may have occurred during the September 1859 Carrington geomagnetic storm event, with regard to modern-day consequences. In this research, the NRL SAMI2 ionospheric code has been modified and applied the estimated electric field to the dayside ionosphere. The modeling was done at 15-minute time increments to track the general ionospheric changes. Although it has been known that magnetospheric electric fields get down into the ionosphere, it has been only in the last ten years that scientists have discovered that intense magnetic storm electric fields do also. On the dayside, these dawn-to-dusk directed electric fields lift the plasma (electrons and ions) up to higher altitudes and latitudes. As plasma is removed from lower altitudes, solar UV creates new plasma, so the total plasma in the ionosphere is increased several-fold. Thus, this complex process creates super-dense plasmas at high altitudes (from 700 to 1,000 km and higher).

  18. Stochastic evolution of rotations of early type galaxies

    NASA Astrophysics Data System (ADS)

    Choi, Hoseung; Yi, Sukyoung

    2016-01-01

    Recent Integral-Field Spectrograph surveys (SAURON, ATLAS 3D, and SAMI project, for example) have revealed that early type galaxies have wide range of rotational properties even though they share similar photometric properties. High resolution numerical studies have shown that galaxy-galaxy interactions have significant effect on the rotation of early type galaxies, however, with limited number of sample galaxies.We present kinematic analysis of thousands of galaxies in 20 clusters from a set of cosmological hydrodynamic zoom-in simulations. Although galaxy mergers play an important role, the direction of change in the amount of rotation depends on many merger parameters such as mass ratio, orbital parameters, and relative direction of galaxy rotations. Furthermore, all their merger parameters themselves are results of non-linear galaxy formation and evolution processes. By compiling numerous galaxy merger events, we discuss statistical properties of the evolution of early type galaxy rotation. We present the impacts of various interactions: major and minor mergers, multiple mergers, and flybys.

  19. An advanced technique for speciation of organic nitrogen in atmospheric aerosols

    NASA Astrophysics Data System (ADS)

    Samy, S.; Robinson, J.; Hays, M. D.

    2011-12-01

    The chemical composition of organic nitrogen (ON) in the environment is a research topic of broad significance. The topic intersects the branches of atmospheric, aquatic, and ecological science; thus, a variety of instrumentation, analytical methods, and data interpretation tools have evolved for determination of ON. Recent studies that focus on atmospheric particulate nitrogen (N) suggest a significant fraction (20-80%) of total N is bound in organic compounds. The sources, bioavailability and transport mechanisms of these N-containing compounds can differ, producing a variety of environmental consequences. Amino acids (AA) are a key class of atmospheric ON compounds that can contribute to secondary organic aerosol (SOA) formation and potentially influence water cycles, air pollutant scavenging, and the radiation balance. AA are water-soluble organic compounds (WSOC) that can significantly alter the acid-base chemistry of aerosols, and may explain the buffering capacity that impacts heterogeneous atmospheric chemistry. The chemical transformations that N-containing organic compounds (including AA) undergo can increase the light-absorbing capacity of atmospheric carbon via formation of 'brown carbon'. Suggested sources of atmospheric AA include: marine surface layer transport from bursting sea bubbles, the suspension of bacteria, fungi, algae, pollen, spores, or biomass burning. Methodology for detection of native (underivatized) amino acids (AA) in atmospheric aerosols has been developed and validated (Samy et al., 2011). This presentation describes the use of LC-MS (Q-TOF) and microwave-assisted gas phase hydrolysis for detection of free and combined amino acids in aerosols collected in a Southeastern U.S. forest environment. Accurate mass detection and the addition of isotopically labeled surrogates prior to sample preparation allows for sensitive quantitation of target AA in a complex aerosol matrix. A total of 16 native AA were detected above the reporting

  20. "On the gate of Arctic": Doors open to foreign schools

    NASA Astrophysics Data System (ADS)

    Pecchiar, Irene

    2015-04-01

    With the increased attention to the changing of the Arctic Region as a consequence of global climate changes, effective science education, outreach and communication need to be higher priorities within the scientific communities. In order to encourage the dissemination of polar research at educational levels Slovene high school students in Trieste were first engaged at school and at the National Museum of Antarctica of Trieste using conferences and laboratory activities to introduce the main polar climate change topics. Then together with three teachers they visited Tromso University (North Norway) for a week. The first aim of this project was to increase awareness of foreign schools on major topics concerning the Arctic issues (from the economic/social to the environmental/climatic point of view). Forty-three high school students were involved in the laboratory activities running at the University of Tromso and participated in seminars. The topics focused on were Ocean Acidification, Global Warming and the combined effects with other anthropogenic stressors. During their stay, students interviewed several scientists in order to allow them to edit a »visiting report«, that was updated every day in their blog and to elaborate all the material collected (photos, videos, data of laboratory work, reports). In Tromso, they were also introduced to the culture and tradition of the Scandinavian indigenous people at the Center of Sami Study. Back in Italy, they published some articles in local newspapers, and then they presented their results at the National Museum of Antarctica of Trieste about all the data elaboration in an open day exhibition with posters, short movies and PowerPoint presentations. All this work was made in order to pass their experience into the world. This was a pilot project, highlighting the role of universities as links between research and outreach. The next step should be to enlarge these kinds of activities to many Schools, Universities and

  1. Politicians, Patriots and Plotters: Unlikely Debates Occasioned by Maximilian Hell's Venus Transit Expedition of 1769

    NASA Astrophysics Data System (ADS)

    Kontler, Laszlo

    2013-05-01

    This paper discusses the cultural and political contexts and reception of the most important by-product of Maximilian Hell's famous Venus transit expedition of 1768-69, the Demonstratio. Idioma Ungarorum et Lapponum idem esse (1770) by Hell's associate Janos Sajnovics. Now considered a landmark in Finno-Ugrian linguistics, the Demonstratio addressed an academic subject that was at that time almost destined to be caught up in an ideological battlefield defined by the shifting relationship between the Habsburg government, the Society of Jesus, and the Hungarian nobility. The "enlightened absolutist" policies of the former aimed at consolidating the Habsburg monarchy as an empire, at the expense of privileged groups, including religious orders as well as the noble estates. In the situation created by the 1773 suppression of the Jesuit order (a signal of declining patronage from the dynasty), the growing preoccupation on the part of ex-Jesuits like Hell and Sajnovics with "things Hungarian" could have been part of an attempt to re-situate themselves on the Central European map of learning. At the same time, the founding document of this interest, the Demonstratio, evoked violent protests from the other target of Habsburg policies, the Hungarian nobility, because its basic assumptions - the kinship of the Hungarian and the Sami (Lappian) language - potentially undermined the noble ideology of social exclusiveness, established on the alleged "Scythian" ancestry of Hungarians. By exploring the complex motives, intentions, reactions and responses of the chief agents in this story, it is possible to highlight the extra-scientific constraints and facilitators for the practice of knowledge in late eighteenth century Central Europe.

  2. Exploring the influence of surface waves in the carbon dioxide transfer velocity between the ocean and atmosphere in the coastal region

    NASA Astrophysics Data System (ADS)

    Ocampo-Torres, Francisco Javier; Francisco Herrera, Carlos; Gutiérrez-Loza, Lucía; Osuna, Pedro

    2016-04-01

    Field measurements have been carried out in order to better understand the possible influence of ocean surface waves in the transfer of carbon dioxide between the ocean and atmosphere in the coastal zone. The CO2 fluxes are being analysed and results are shown in a contribution by Gutiérrez-Loza et al., in this session. Here we try to highlight the findings regarding the transfer velocity (kCO2) once we have incorporated direct measurements of carbon dioxide concentration in the water side. In this study direct measurements of CO2 fluxes were obtained with an eddy covariance tower located in the shoreline equipped with an infrared open-path gas analyzer (LI-7500, LI-COR) and a sonic anemometer (R3-100 Professional Anemometer, Gill Instruments), both at about 13 m above the mean sea level, and sampling at 20 Hz. For some period of time simultaneous information of waves was recorded with a sampling rate of 2 Hz using an Acoustic Doppler Current Profiler (Workhorse Sentinel, Teledyne RD Instruments) at 10 m depth and 350 m away from the tower. Besides, recently the concentration of CO2 in water has also been recorded making use of a SAMI-CO2 instrument. A subtle effect of the wave field is detected in the estimated kCO2. Looking into details of the surface currents being detected very near the air-sea interface through an ADPC, a certain association can be found with the gas transfer velocity. Furthermore, some of the possible effects of breaking wave induced turbulence in the coastal zone is to be addressed. This work represents a RugDiSMar Project (CONACYT 155793) contribution. The support from CB-2011-01-168173 CONACYT project is greatly acknowledged.

  3. The Mitchell Spectrograph: Studying Nearby Galaxies with the VIRUS Prototype

    NASA Astrophysics Data System (ADS)

    Blanc, Guillermo A.

    The Mitchell Spectrograph (a.k.a. VIRUS-P) on the 2.7m Harlan J. Smith telescope at McDonald Observatory is currently the largest field of view (FOV) integral field unit (IFU) spectrograph in the world (1.7'x1.7'). It was designed as a prototype for the highly replicable VIRUS spectrograph which consists of a mosaic of IFUs spread over a 16' diameter FOV feeding 150 spectrographs similar to the Mitchell. VIRUS will be deployed on the 9.2 meter Hobby-Eberly Telescope (HET) and will be used to conduct the HET Dark Energy Experiment (HETDEX). Since seeing first light in 2007 the Mitchell Spectrograph has been widely used, among other things, to study nearby galaxies in the local universe where their internal structure and the spatial distribution of different physical parameters can be studied in great detail. These observations have provided important insight into many aspects of the physics behind the formation and evolution of galaxies and have boosted the scientific impact of the 2.7 meter telescope enormously. Here I review the contributions of the Mitchell Spectrograph to the study of nearby galaxies, from the investigation of the spatial distribution of dark matter and the properties of supermassive black holes, to the studies of the process of star formation and the chemical composition of stars and gas in the ISM, which provide important information regarding the formation and evolution of these systems. I highlight the fact that wide field integral field spectrographs on small and medium size telescopes can be powerful cost effective tools to study the astrophysics of galaxies. Finally I briefly discuss the potential of HETDEX for conducting studies on nearby galaxies. The survey parameters make it complimentary and competitive to ongoing and future surveys like SAMI and MANGA.

  4. Sulfur Solubility In Silicate Melts: A Thermochemical Model

    NASA Astrophysics Data System (ADS)

    Moretti, R.; Ottonello, G.

    A termochemical model for calculating sulfur solubility of simple and complex silicate melts has been developed in the framework of the Toop-Samis polymeric approach combined with a Flood - Grjotheim theoretical treatment of silicate slags [1,2]. The model allows one to compute sulfide and sulfate content of silicate melts whenever fugacity of gaseous sulphur is provided. "Electrically equivalent ion fractions" are needed to weigh the contribution of the various disproportion reactions of the type: MOmelt + 1/2S2 ,gas MSmelt+1/2O2 ,gas (1) MOmelt + 1/2S2 ,gas + 3/2O2 ,gas MSO4 ,melt (2) Eqs. 1 and 2 account for the oxide-sulfide and the oxide-sulfate disproportiona- tion in silicate melt. Electrically equivalent ion fractions are computed, in a fused salt Temkin notation, over the appropriate matrixes (anionic and cationic). The extension of such matrixes is calculated in the framework of a polymeric model previously developed [1,2,3] and based on a parameterization of acid-base properties of melts. No adjustable parameters are used and model activities follow the raoultian behavior implicit in the ion matrix solution of the Temkin notation. The model is based on a huge amount of data available in literature and displays a high heuristic capability with virtually no compositional limits, as long as the structural role assigned to each oxide holds. REFERENCES: [1] Ottonello G., Moretti R., Marini L. and Vetuschi Zuccolini M. (2001), Chem. Geol., 174, 157-179. [2] Moretti R. (2002) PhD Thesis, University of Pisa. [3] Ottonello G. (2001) J. Non-Cryst. Solids, 282, 72-85.

  5. Quantitative comparisons of various air pollutant emission sources of ozone precursors in East Tennessee - a study evaluated from the emission inventory development

    SciTech Connect

    Bandyopadhyay, N.

    1996-12-31

    The United States Department of the Interior has raised concerns regarding air pollution impacts in the Great Smoky Mountains National Park (GSMNP). The formation of the Southern Appalachian Mountains Initiative (SAMI) is regional effort to understand the air quality impacts of emission sources upon the Appalachian Mountains. The Tennessee Division of Air Pollution Control (TDAPC) has recently committed additional resources for the analyses of proposals for increased emissions of air pollutants in East Tennessee. The TDAPC has planned to assess these effects by conducting an air quality modeling project. The United States Environmental Protection Agency`s (US EPA`s) Urban Airshed Model (UAM) has been used as the primary air quality model for this purpose. The purpose of this project will be to evaluate the expected impact of any major new or modified air pollution source located in Tennessee on ozone in the GSMNP. An accurate emission inventory is essential to any air quality modeling analysis. A modeling inventory has been developed by the TDAPC for the base year 1993. The modeling area includes 40 counties in East and Middle Tennessee and 42 counties in neighboring states. For the counties in Tennessee, a detailed inventory of the point sources was prepared. For the other states inside the modeling domain, the EPA`s Aerometric Information Retrieval System (AIRS)-AIRS Facility Subsystem (AFS) was used to obtain point source data, The accuracy of the AFS data for the other states was not addressed, A detailed quantitative analysis has been conducted with the emission inventory developed for Tennessee counties. The purpose of this study is to quantify the relative contributions of the emissions of Volatile Organic Compounds (VOCs) and Nitrogen Oxides (NO{sub x}) from different point, area, mobile and biogenic sources to ozone formation in the vicinity of the GSMNP.

  6. QUENCHING DEPENDS ON MORPHOLOGIES: IMPLICATIONS FROM THE ULTRAVIOLET-OPTICAL RADIAL COLOR DISTRIBUTIONS IN GREEN VALLEY GALAXIES

    SciTech Connect

    Pan, Zhizheng; Lin, Weipeng; Li, Jinrong; Kong, Xu; Wang, Jing E-mail: linwp@shao.ac.cn

    2014-09-01

    In this Letter, we analyze the radial ultraviolet-optical color distributions in a sample of low redshift green valley galaxies, with the Galaxy Evolution Explorer (GALEX)+Sloan Digital Sky Survey (SDSS) images, to investigate how the residual recent star formation is distributed in these galaxies. We find that the dust-corrected u – r colors of early-type galaxies (ETGs) are flat out to R {sub 90}, while the colors monotonously turn blue when r > 0.5 R {sub 50} for late-type galaxies (LTGs). More than half of the ETGs are blue-cored and have remarkable positive NUV – r color gradients, suggesting that their star formations are centrally concentrated. The rest have flat color distributions out to R {sub 90}. The centrally concentrated star formation activity in a large portion of ETGs is confirmed by the SDSS spectroscopy, showing that ∼50% of the ETGs have EW(Hα) >6.0 Å. Of the LTGs, 95% show uniform radial color profiles, which can be interpreted as a red bulge plus an extended blue disk. The links between the two kinds of ETGs, e.g., those objects having remarkable ''blue-cores'' and those having flat color gradients, are less known and require future investigations. It is suggested that the LTGs follow a general model by which quenching first occurs in the core regions, and then finally extend to the rest of the galaxy. Our results can be re-examined and have important implications for the IFU surveys, such as MaNGA and SAMI.

  7. Characteristics of VLF wave propagation in the Earth's magnetosphere in the presence of an artificial density duct

    NASA Astrophysics Data System (ADS)

    Pasmanik, Dmitry; Demekhov, Andrei

    We study the propagation of VLF waves in the Earth's ionosphere and magnetosphere in the presence of large-scale artificial plasma inhomogeneities which can be created by HF heating facilities like HAARP and ``Sura''. A region with enhanced cold plasma density can be formed due to the action of HF heating. This region is extended along geomagnetic field (up to altitudes of several thousand km) and has rather small size across magnetic field (about 1 degree). The geometric-optical approximation is used to study wave propagation. The plasma density and ion composition are calculated with the use of SAMI2 model, which was modified to take the effect of HF heating into account. We calculate ray trajectories of waves with different initial frequency and wave-normal angles and originating at altitudes of about 100 km in the region near the heating area. The source of such waves could be the lightning discharges, modulated HF heating of the ionosphere, or VLF transmitters. Variation of the wave amplitude along the ray trajectories due to refraction is considered and spatial distribution of wave intensity in the magnetosphere is analyzed. We show that the presence of such a density disturbances can lead to significant changes of wave propagation trajectories, in particular, to efficient guiding of VLF waves in this region. This can result in a drastic increase of the VLF-wave intensity in the density duct. The dependence of wave propagation properties on parameters of heating facility operation regime is considered. We study the variation of the spatial distribution of VLF wave intensity related to the slow evolution of the artificial inhomogeneity during the heating.

  8. Norway.

    PubMed

    1992-08-01

    Norway with a territory of 386,000 sq. km or 150,000 sq. miles is slightly larger than New Mexico. In 1991 the population was estimated at 4.3 million with an annual growth rate of .5% and a literacy rate of 100%. The infant mortality rate is 7/1000 live births, and lie expectancy is 73 years for men and 80 years for women. Norway's government is a hereditary constitutional monarchy since independence n 1905. Ethnically, Norwegians are predominantly Germanic, but there are indigenous communities of Sami (Lapps) in the north, and in recent years almost 150,000 immigrants, foreign workers, and asylum-seekers have settled there. Norway's health system includes free hospital care, physicians compensation, cash benefits during illness and pregnancy, and other medical and dental plans. Until the 1981 election, Norway has been governed by Labor Party governments since 1935, except for 3 periods (1963, 1965-71, and 1972-73). Gro Harlem Brundtland is again the prime minister after forming her 3rd government in 10 years. Norway holds national elections in September 1993. Norway's large shipping fleet is modern; metals, pulp and paper products, chemicals, shipbuilding, and fishing are traditional industries, and major oil and gas discoveries in the mid-1970s transformed the economy. High oil prices in the 1983-85 period raised consumer spending, wages, and inflation. Norway is aspiring to restructure its nonoil economy in favor of efficient, nontraditional industry. The prime minister has indicated that Norway may apply for European Community (EC) membership before the end of 1992. Its main trading partners are the EC countries and its Scandinavian neighbors with the US in 5th place. PMID:12178045

  9. Transcriptional and epigenetic networks that drive helper T cell identities

    PubMed Central

    Shih, Han-Yu; Sciumè, Giuseppe; Poholek, Amanda C; Vahedi, Golnaz; Hirahara, Kiyoshi; Villarino, Alejandro V; Bonelli, Michael; Bosselut, Remy; Kanno, Yuka; Muljo, Stefan A; O’Shea, John J.

    2014-01-01

    The discovery of the specification of CD4+ helper T cells to discrete effector “lineages” represented a watershed event in conceptualizing mechanisms of host defense and immunoregulation. However, our appreciation for the actual complexity of helper T cell subsets continues unabated. Just as the Sami language of Scandinavia has 1000 different words for reindeer, the range of fates available for a CD4+ T cell is numerous and may be underestimated. Added to the crowded scene for helper T cell subsets is the continuously growing family of innate lymphoid cells (ILCs), endowed with common effector responses and the previously defined “master regulators” for CD4+ helper T cell subsets are also shared by ILC subsets. Within the context of this extraordinary complexity are concomitant advances in the understanding of transcriptomes and epigenomes. So what do terms like “lineage commitment” and helper T cell “specification” mean in the early 21st century? How do we put all of this together in a coherent conceptual framework? It would be arrogant to assume that we have a sophisticated enough understanding to seriously answer these questions. Instead, we will review the current status of the flexibility of helper T cell responses in relation to their genetic regulatory networks and epigenetic landscapes. Recent data have provided major surprises as to what master regulators can or cannot do, how they interact with other transcription factors and impact global genome-wide changes and how all these factors come together to influence helper cell function. PMID:25123275

  10. The effects of spatial resolution on integral field spectrograph surveys at different redshifts - The CALIFA perspective

    NASA Astrophysics Data System (ADS)

    Mast, D.; Rosales-Ortega, F. F.; Sánchez, S. F.; Vílchez, J. M.; Iglesias-Paramo, J.; Walcher, C. J.; Husemann, B.; Márquez, I.; Marino, R. A.; Kennicutt, R. C.; Monreal-Ibero, A.; Galbany, L.; de Lorenzo-Cáceres, A.; Mendez-Abreu, J.; Kehrig, C.; del Olmo, A.; Relaño, M.; Wisotzki, L.; Mármol-Queraltó, E.; Bekeraitè, S.; Papaderos, P.; Wild, V.; Aguerri, J. A. L.; Falcón-Barroso, J.; Bomans, D. J.; Ziegler, B.; García-Lorenzo, B.; Bland-Hawthorn, J.; López-Sánchez, Á. R.; van de Ven, G.

    2014-01-01

    Context. Over the past decade, 3D optical spectroscopy has become the preferred tool for understanding the properties of galaxies and is now increasingly used to carry out galaxy surveys. Low redshift surveys include SAURON, DiskMass, ATLAS3D, PINGS, and VENGA. At redshifts above 0.7, surveys such as MASSIV, SINS, GLACE, and IMAGES have targeted the most luminous galaxies to study mainly their kinematic properties. The on-going CALIFA survey (z ~ 0.02) is the first of a series of upcoming integral field spectroscopy (IFS) surveys with large samples representative of the entire population of galaxies. Others include SAMI and MaNGA at lower redshift and the upcoming KMOS surveys at higher redshift. Given the importance of spatial scales in IFS surveys, the study of the effects of spatial resolution on the recovered parameters becomes important. Aims: We explore the capability of the CALIFA survey and a hypothetical higher redshift survey to reproduce the properties of a sample of objects observed with better spatial resolution at lower redshift. Methods: Using a sample of PINGS galaxies, we simulated observations at different redshifts. We then studied the behaviour of different parameters as the spatial resolution degrades with increasing redshift. Results: We show that at the CALIFA resolution, we are able to measure and map common observables in a galaxy study: the number and distribution of H ii regions (Hα flux structure), the gas metallicity (using the O3N2 method), the gas ionization properties (through the [N ii]/Hα and [O iii]/Hβ line ratios), and the age of the underlying stellar population (using the D4000 index). This supports the aim of the survey to characterise the observable properties of galaxies in the Local Universe. Our analysis of simulated IFS data cubes at higher redshifts highlights the importance of the projected spatial scale per spaxel as the most important figure of merit in the design of an integral field survey.

  11. From Outside-in to Inside-out: Galaxy Assembly Mode Depends on Stellar Mass

    NASA Astrophysics Data System (ADS)

    Pan, Zhizheng; Li, Jinrong; Lin, Weipeng; Wang, Jing; Fan, Lulu; Kong, Xu

    2015-05-01

    In this Letter, we investigate how galaxy mass assembly mode depends on stellar mass M* using a large sample of ˜10,000 low-redshift galaxies. Our galaxy sample is selected to have SDSS {{R}90}\\gt 5\\buildrel{\\prime\\prime}\\over{.} 0, which allows the measures of both the integrated and the central NUV-r color indices. We find that in the {{M}*}-(NUV-r) green valley (GV), the {{M}*}\\lt {{10}10} {{M}⊙ } galaxies mostly have positive or flat color gradients, while most of the {{M}*}\\gt {{10}10.5} {{M}⊙ } galaxies have negative color gradients. When their central Dn4000 index values exceed 1.6, the {{M}*}\\lt {{10}10.0} {{M}⊙ } galaxies have moved to the UV red sequence, whereas a large fraction of the {{M}*}\\gt {{10}10.5} {{M}⊙ } galaxies still lie on the UV blue cloud or the GV region. We conclude that the main galaxy assembly mode is transiting from “the outside-in” mode to “the inside-out” mode at {{M}*}\\lt {{10}10} {{M}⊙ } and at {{M}*}\\gt {{10}10.5} {{M}⊙ }. We argue that the physical origin of this is the compromise between the internal and the external processes that drive the star formation quenching in galaxies. These results can be checked with the upcoming large data produced by the ongoing integral field spectroscopic survey projects, such as CALIFA, MaNGA, and SAMI in the near future.

  12. Quenching Depends on Morphologies: Implications from the Ultraviolet-Optical Radial Color Distributions in Green Valley Galaxies

    NASA Astrophysics Data System (ADS)

    Pan, Zhizheng; Li, Jinrong; Lin, Weipeng; Wang, Jing; Kong, Xu

    2014-09-01

    In this Letter, we analyze the radial ultraviolet-optical color distributions in a sample of low redshift green valley galaxies, with the Galaxy Evolution Explorer (GALEX)+Sloan Digital Sky Survey (SDSS) images, to investigate how the residual recent star formation is distributed in these galaxies. We find that the dust-corrected u - r colors of early-type galaxies (ETGs) are flat out to R 90, while the colors monotonously turn blue when r > 0.5 R 50 for late-type galaxies (LTGs). More than half of the ETGs are blue-cored and have remarkable positive NUV - r color gradients, suggesting that their star formations are centrally concentrated. The rest have flat color distributions out to R 90. The centrally concentrated star formation activity in a large portion of ETGs is confirmed by the SDSS spectroscopy, showing that ~50% of the ETGs have EW(Hα) >6.0 Å. Of the LTGs, 95% show uniform radial color profiles, which can be interpreted as a red bulge plus an extended blue disk. The links between the two kinds of ETGs, e.g., those objects having remarkable "blue-cores" and those having flat color gradients, are less known and require future investigations. It is suggested that the LTGs follow a general model by which quenching first occurs in the core regions, and then finally extend to the rest of the galaxy. Our results can be re-examined and have important implications for the IFU surveys, such as MaNGA and SAMI.

  13. Mechanisms for quenching star formation activities in green valley galaxies and its depends on morphologies

    NASA Astrophysics Data System (ADS)

    Kong, Xu; Pan, Zhizheng; Lian, Jianhui

    2015-08-01

    Galaxies are categorized into two main populations, red quiescent galaxies and blue star-forming galaxies. One of the key questions is which physical mechanisms are responsible for quenching star formation activities in blue galaxies and the resulting transformation? In this talk, we present research on the morphologies, spectra, and environments of "green valley" galaxies in the COSMOS field and low redshift "green valley" galaxies in SDSS. Our findings suggest that environmental conditions, most likely starvation and harassment, significantly affect the transformation of M* < 10^10.0 Msun blue galaxies into red galaxies, especially at z < 0.5. Using image from SDSS and GALEX, we analyze the radial ultraviolet-optical color distributions in a sample of low redshift green valley galaxies, and investigate how quenching is processing in a galaxy. The early-type "green valley" galaxies (ETGs) have dramatically different radial NUV-r color distributions compared to late-type "green valley" galaxies (LTGs), most of ETGs have blue cores, nearly all LTGs have uniform color profiles that can be well-interpreted as red bulges plus blue disk components. These results suggest that the LTGs follow a general model by which quenching first occurs in the core regions, and then finally extend to the rest of the galaxy; for ETGs, their star formations are centrally concentrated. Our results can be re-examined and have important implications for the IFU surveys, such as MaNGA and SAMI (2013ApJ...776...14P, 2014ApJ...792L...4P, 2015MNRAS.446.1449L).

  14. Evaluation of Iodine Deficiency in Children with Attention Deficit/Hyperactivity Disorder

    PubMed Central

    Kanık Yüksek, Saliha; Aycan, Zehra; Öner, Özgür

    2016-01-01

    Objective: To investigate the incidence of iodine deficiency (ID) and its effects on mental function in children referred to the Dr. Sami Ulus Maternity and Children’s Training and Research Hospital with a prospective diagnosis of attention deficit/hyperactivity disorder (ADHD). Methods: The study was conducted on 89 children referred in the period from September 2009 to June 2010 with a diagnosis of ADHD. A questionnaire was given to all parents. Conners’ rating scales were applied to the parents (CPRS) and teachers (CTRS), and revised Wechsler intelligence scale for children (WISC-R) to the children. Serum thyroid-stimulating hormone, free triiodothyronine and free thyroxine, thyroglobulin, anti-thyroid peroxidase, anti-thyroglobulin, and urinary iodine levels were measured in all children. Results: Median age was 9.41±1.95 years, and 83.1% of subjects were male. The mean urinary iodine level of the children was 92.56±22.25 μg/L. ID was detected in 71.9% of subjects and all were mild ID. There was no significant relationship between urinary iodine levels with WISC-R subtest scores and CPRS. However, a significant association was found between urinary iodine levels and hyperactivity section of CTRS (p<0.05). Likewise, a significant relationship was found between learning disorder/mental retardation diagnosis and freedom subtest of WISC-R (p<0.05). Conclusion: This study highlights the effects of ID on comprehension, perception, attention, and learning. However, the results need to be supported by new randomized controlled trials. PMID:26758811

  15. Native predators reduce harvest of reindeer by Sámi pastoralists.

    PubMed

    Hobbs, N Thompson; Andrén, Henrik; Persson, Jens; Aronsson, Malin; Chapron, Guillaume

    2012-07-01

    Contemporary efforts to protect biological diversity recognize the importance of sustaining traditional human livelihoods, particularly uses of the land that are compatible with intact landscapes and ecologically complete food webs. However, these efforts often confront conflicting goals. For example, conserving native predators may harm pastoralist economies because predators consume domestic livestock that sustain people. This potential conflict must be reconciled by policy, but such reconciliation requires a firm understanding of the effects of predators on the prey used by people. We used a long-term, large-scale database and Bayesian models to estimate the impacts of lynx (Lynx lynx), wolverine (Gulo gulo), and brown bear (Ursus arctos) on harvest of semi-domesticated reindeer (Rangifer tarandus) by Sami pastoralists in Sweden. The average annual harvest of reindeer averaged 25% of the population (95% credible interval = 19, 31). Annual harvest declined by 96.6 (31, 155) reindeer for each lynx family group (the surveyed segment of the lynx population) in a management unit and by 94.3 (20, 160) for each wolverine reproduction (the surveyed segment of the wolverine population). We failed to detect effects of predation by brown bear. The mechanism for effects of predation on harvest was reduced population growth rate. The rate of increase of reindeer populations declined with increasing abundance of lynx and wolverine. The density of reindeer, latitude, and weather indexed by the North Atlantic Oscillation also influenced reindeer population growth rate. We conclude that there is a biological basis for compensating the Sámi reindeer herders for predation on reindeer.

  16. Pestivirus and alphaherpesvirus infections in Swedish reindeer (Rangifer tarandus tarandus L.).

    PubMed

    Kautto, Arja H; Alenius, Stefan; Mossing, Torgny; Becher, Paul; Belák, Sándor; Larska, Magdalena

    2012-04-23

    Herding semi-domesticated reindeer has economic and social value for Sami people in the northern territories of Fennoscandia. However, with the intensification of reindeer husbandry, interspecies transmission of pathogens between reindeer and domestic animals may become a problem, especially for countries such as Sweden, Norway, and Finland where pestivirus and alphaherpesvirus have been eradicated in domestic ruminants. This study, which included 1158 Swedish reindeer, showed relatively high prevalence of antibodies against bovine viral diarrhoea virus (BVDV) (32%) and bovine herpesvirus-1 (BoHV-1) (53%). Adult animals were more often seropositive for BVDV and BoHV-1 (50% and 78%, respectively) than were calves (18 and 11%, respectively). While the seroprevalence of alphaherpesvirus was similar in different herding districts, pestivirus seropositivity was highest in the South and diminished towards the North of the Swedish reindeer herding area. High correlation of the seropositivity against both pathogens at both individual and herd levels may indicate possible mutual synergetic effects and may be explained by the immunosuppressive nature of the viruses. While alphaherpesvirus seroprevalence was probably related to putative cervid herpesvirus 2 (CvHV-2), the pestivirus infecting reindeer remains undefined. The virus neutralisation test of reindeer sera using different pestivirus strains, revealed higher titres against Border disease virus strains like 137/4 (BDV-1) and Reindeer-1 (BDV-2) than against BVDV-1. However, the virus was not identified by real time RT-PCR in any of the samples (n=276) from seronegative reindeers. The study showed that pestivirus and alphaherpesvirus infections are endemic in the Swedish reindeer population.

  17. Artificial Aurora and Irregularity Generation at Low- and Mid-Latitude HF Heating Facilities: Past, Present, and Future

    NASA Astrophysics Data System (ADS)

    Bernhardt, Paul

    From the 1970's to the present, artificial aurora and field aligned irregularities have been produced at the mid-latitude HF facilities in Platteville, Colorado; Arecibo, Puerto Rico; and SURA, Russia. The artificial optical displays were produced by high power HF radio waves with effective radiated powers in the 80 to 250 Megawatt range. The high power electromagnetic waves excite Langmuir cavitons near the HF wave reflection altitude. Suprathermal electrons are released during the caviton collapse and collisions with atomic oxygen and other neutral atoms produce the artificial aurora. Ground based images of the optical emissions have been used to (1) show artificial and natural irregularities in the E- and F-region, (2) provide remote sensing of neutral winds and plasma drifts, and (3) yield estimates of the composition of the upper atmosphere in the HF interaction region. Currently, the Arecibo HF facility which was destroyed in 1999 by Hurricane Floyd is being reconstituted over the Arecibo dish using crossed-dipoles coupled to a secondary reflector. This new facility should be completed by 2011 for operation near 5 and 8 MHz. In addition, the feasibility of putting a heating facility near the equator is being studied. Numerical simulations using high power electromagnetic waves coupled to the NRL SAMI3 physics based ionosphere model is providing insight to use of these new facilities. Using the Arecibo HF facility, the geomagnetic conjugate region in Argentina should be able to measure artificial aurora as well as both electron density and electron temperature perturbations. A suite of ionospheric sensors comprised of a low-light-level imager, an incoherent scatter radar, and a digital ionosonde would be needed for these observations. An equatorial HF facility would be able to produce symmetric patches of artificial aurora as well as trigger equatorial bubbles by seeding localized density reductions in the plasma.

  18. Post-midnight occurrence of equatorial plasma bubbles

    NASA Astrophysics Data System (ADS)

    Ajith, K. K.; Otsuka, Yuichi; Yamamoto, Mamoru; Yokoyama, Tatsuhiro; Tulasiram, S.

    2016-07-01

    The equatorial plasma bubbles (EPBs)/equatorial spread F (ESF) irregularities are an important topic of space weather interest because of their impact on transionospheric radio communications, satellite-based navigation and augmentation systems. This local plasma depleted structures develop at the bottom side F layer through Rayleigh-Taylor instability and rapidly grow to topside ionosphere via polarization electric fields within them. The steep vertical gradients due to quick loss of bottom side ionization and rapid uplift of equatorial F layer via prereversal enhancement (PRE) of zonal electric field makes the post-sunset hours as the most preferred local time for the formation of EPBs. However, there is a different class of irregularities that occurs during the post-midnight hours of June solstice reported by the previous studies. The occurrence of these post-midnight EPBs maximize during the low solar activity periods. The growth characteristics and the responsible mechanism for the formation of these post-midnight EPBs are not yet understood. Using the rapid beam steering ability of 47 MHz Equatorial Atmosphere Radar (EAR) at Kototabang (0.2°S geographic latitude, 100.3°E geographic longitude, and 10.4°S geomagnetic latitude), Indonesia, the spatial and temporal evolution of equatorial plasma bubbles (EPBs) were examined to classify the evolutionary-type EPBs from those which formed elsewhere and drifted into the field of view of radar. The responsible mechanism for the genesis of summer time post-midnight EPBs were discussed in light of growth rate of Rayleigh-Taylor instability using SAMI2 model.

  19. Termochemical Models For Slags and Silicate Melts, Review and Perspectives

    NASA Astrophysics Data System (ADS)

    Ottonello, G.

    Thermochemical models devoted to the comprehension of reactive and mixing properties of silicate melts and slags may be roughly grouped into four main classes: 1) fictive chemical; 2) quasi chemical; 3) fictive structural; 4) polymeric. In the first class we may group the fictive regular mixture approach of Ghiorso and Carmichael [1,2]and its extensions [3-5]and the subregular model of Berman and Brown [6]. To the second class belong the modified quasi chemical approach of Pelton and coworkers [7,8] , and the Kapoor - Froberg cellular model and its extensions [9-11]. The third class has much to share with the second one (and indeed the cellular model could be ascribed to this class as well). To this class belong the "central surround model" of Sastri and Lahiri [12] , the associated solution models of Bjorkman [13], Hastie and coworkers [14]and Goel and coworkers [15], the two sublattice model of Hillert and coworkers [16]and the polynomial expansions of Hoch and Arpshofen [17] . The fourth class encompasses the models of Masson[18-20] , Toop-Samis [21,22]and its extensions [23-25] . The phylosophy beyond each one of the four classes is basically different. Benefits and drawbacks are present in any of them, and applications are often limited to simple systems (or to sufficiently complex systems, in the case of arbitrary deconvolutions of type 1) and to limited P-T ranges. The crucial aspects of the various models will be outlined to some extent. It will be shown that, often, model conflictuality is only appartent and that, in some cases, model failure is unperceived by acritical utilizers. New perspectives in the future research devoted to the comprehension of melt reactivity in compositionally complex systems, with special enphasis on the solubility of gaseous components and unmixing, will be finally discussed. References: [1] Ghiorso M.S. and Carmichael I.S.E. (1980) Contrib. Mineral. Petrol., 71, 323-342. [2] Ghiorso M.S., Carmichael I.S.E., Rivers M.L. and Sack

  20. Variation of Plasmaspheric (90-4000 km) Field-aligned Electron Density and Ion Composition as a Function of Geomagnetic Storm Activity

    NASA Astrophysics Data System (ADS)

    Reddy, A.; Sonwalkar, V. S.

    2015-12-01

    Whistler mode (WM) radio sounding from IMAGE has led to the first measurements of plasmaspheric field-aligned electron density and ion composition as a function of geomagnetic storm activity during Aug-Sep 2005, a period that included several successive geomagnetic storms of varying strength. The plasmapause was located at L~2.4 during the onset and main phases of the storms. On the dayside, as a function of storm activity we found in general the following results: (1) The electron density, relative ion concentrations, and O+/H+ transition height had different temporal behavior. (2) Electron density in the first 1-2 days of the storm increased followed by a decrease in the recovery phase. (3) αH+ decreased during the onset, main and early recovery phase, and then it increased; αO+ increased in the early recovery phase, and then it decreased; αHe+ in general increased in the onset or main phase and decreased in the recovery phase. (4) O+/H+ transition height increased by ~200-300 km during the onset, main and early recovery phase. (5) When successive storms occurred in less than a day's span, the latter storms had little or no effect on the electron density and ion composition. On the nightside, WM sounding data was sparse. In the case of one moderate storm, we found that 3 days after the storm, electron density at F2 peak and relative ion concentrations (at all altitudes) were comparable to those before the storm, whereas electron density above O+/H+ transition height decreased. WM sounding results for the dayside and nightside were in agreement with measurements from CHAMP (350 km) and DMSP (850 km). WM sounding measurements coupled with physics-based models (e.g. SAMI2) will allow: (a) investigation of the role of thermospheric winds, dynamo and storm time electric fields in causing the variations in electron and ion densities, and (b) testing of current theories and validating physics-based models of the thermosphere-ionosphere-magnetosphere coupling.

  1. 50 years of snow stratigraphy observations

    NASA Astrophysics Data System (ADS)

    Johansson, C.; Pohjola, V.; Jonasson, C.; Challagan, T. V.

    2012-04-01

    With start in autumn 1961 the Abisko Scientific Research Station (ASRS) located in the Swedish sub Arctic has performed snow stratigraphy observations, resulting in a unique 50 year long time series of data. The data set contains grain size, snow layer hardness, grain compactness and snow layer dryness, observed every second week during the winter season. In general snow and snow cover are important factors for the global radiation budget, and the earth's climate. On a more local scale the layered snowpack creates a relatively mild microclimate for Arctic plants and animals, and it also determines the water content of the snowpack (snow water equivalent) important for e.g. hydrological applications. Analysis of the snow stratigraphy data, divided into three consecutive time periods, show that there has been a change in the last time period. The variable most affected is the snow layer hardness, which shows an increase in hardness of the snowpack. The number of observations with a very hard snow layer/ice at ground level increased three-fold between the first two time periods and the last time period. The thickness of the bottom layer in the snowpack is also highly affected. There has been a 60% increase in layers thinner than 10 cm in the last time period, resulting in a mean reduction in the thickness of the bottom layer from 14 cm to 11 cm. Hence the living conditions for plants and animals at the ground surface have been highly changed. The changes in the snowpack are correlated to an increased mean winter air temperature. Thus, continued increasing, or temperatures within the same ranges as in the last time period, is likely to create harder snow condition in the future. These changes are likely to affect animals that live under the snow such as lemmings and voles or animals that graze sub-Arctic vegetation in winter (e.g. reindeer that would potentially require increased supplementary feeding that incurs financial costs to Sami reindeer herders). Any decrease

  2. New York City International Polar Weekend at the American Museum of Natural History

    NASA Astrophysics Data System (ADS)

    Pfirman, S.; Turrin, M.; Macphee, R.

    2008-12-01

    The American Museum of Natural History, in partnership with Lamont-Doherty Earth Observatory and the Earth Institute of Columbia University and Barnard College, is featuring the International Polar Year through a New York City International Polar Weekend (NYC-IPW) in 2007, 2008 and 2009. The event showcases current polar research, polar environmental changes, history and culture during two days of family programs and activities, performances, and lectures. The goal of the NYC-IPW is to engage diverse audiences and enhance the public understanding of polar science, in particular IPY research, through close interactions with polar experts. Activities for the public include many disciplines, ranging from the physical sciences and cultural anthropology to music and art, and are presented in many forms, from lectures, panels and films to posters and play. Highlights of the NYC-IPW include: 1) A polar fair for youth and adults, showcasing scientists, artists, and educators who have worked at one or both poles and including many interactive exhibits featuring such topics as life in New York at the end of the last Ice Age, how Arctic sea ice is changing, and life on and under the ice. 2) Performances and presentations oriented towards children and families, including Inuit Throat Singers, Central Park Zoo Theater Group, and a northern lights show. 3) Lectures showcasing current IPY research and addressing such issues as the possible effects of climate change on the poles and the rest of the world, as well as polar poetry, art and film. 4) A partnership with New York City Urban Advantage program for Middle School students in the city to meet with scientists, teachers and students who had participated in polar research and travel. 5) Norwegian Consulate sponsorship of science presenters and Sami performers. The March 2007 event involved 85 presenters and volunteers from 22 institutions, and attracted ca. 3,500 visitors. Approximately 5,000 visitors attended the February 2008

  3. InXy and SeXy, compact heterologous reporter proteins for mammalian cells.

    PubMed

    Fluri, David A; Kelm, Jens M; Lesage, Guillaume; Baba, Marie Daoud-El; Fussenegger, Martin

    2007-10-15

    Mammalian reporter proteins are essential for gene-function analysis, drugscreening initiatives and as model product proteins for biopharmaceutical manufacturing. Bacillus subtilis can maintain its metabolism by secreting Xylanase A (XynA), which converts xylan into shorter xylose oligosaccharides. XynA is a family 11 xylanase monospecific for D-xylose containing substrates. Mammalian cells transgenic for constitutive expression of wild-type xynA showed substantial secretion of this prokaryotic enzyme. Deletion analysis confirmed that a prokaryotic signal sequence encoded within the first 81 nucleotides was compatible with the secretory pathway of mammalian cells. Codon optimization combined with elimination of the prokaryotic signal sequence resulted in an exclusively intracellular mammalian Xylanase A variant (InXy) while replacement by an immunoglobulin-derived secretion signal created an optimal secreted Xylanase A derivative (SeXy). A variety of chromogenic and fluorescence-based assays adapted for use with mammalian cells detected InXy and SeXy with high sensitivity and showed that both reporter proteins resisted repeated freeze/thaw cycles, remained active over wide temperature and pH ranges, were extremely stable in human serum stored at room temperature and could independently be quantified in samples also containing other prominent reporter proteins such as the human placental alkaline phosphatase (SEAP) and the Bacillus stearothermophilus-derived secreted alpha-amylase (SAMY). Glycoprofiling revealed that SeXy produced in mammalian cells was N- glycosylated at four different sites, mutation of which resulted in impaired secretion. SeXy was successfully expressed in a variety of mammalian cell lines and primary cells following transient transfection and transduction with adeno-associated virus particles (AAV) engineered for constitutive SeXy expression. Intramuscular injection of transgenic AAVs into mice showed significant SeXy levels in the bloodstream

  4. On the Formation of Elliptical Galaxies via Mergers in Galaxy Groups

    NASA Astrophysics Data System (ADS)

    Taranu, Dan; Dubinski, John; Yee, Howard K. C.

    2015-08-01

    gas-rich disks and compact spheroids) and cosmological merger trees, and discuss prospects for comparisons with data from the new generation of IFU surveys like SAMI.

  5. Topside Ionosphere Plasma Bubbles Seen in He+ Density: Results and Problems

    NASA Astrophysics Data System (ADS)

    Sidorova, Larisa; Filippov, Sergey

    He (+) density depletions, considered as fossil equatorial plasma bubble signatures, were involved in this study. They are usually detected in the topside ionosphere (approx. 1000 km) deeply inside the plasmasphere (L=1.3-3). a) The question about an opportunity to detect the topside plasma bubbles of equatorial origin in their separate plasma component (He (+) ) is investigated. There are the indications [Sidorova, ASR, 2004, 2007; Sidorova and Filippov, JASTP, 2012] that there is genetic connection between the He (+) density depletions and the equatorial plasma bubbles. For validation of this idea the characteristic times of the main photochemical and electro-dynamical processes, in which the plasma bubbles and their minor ion component (He (+) ) are involved, have been calculated and compared. The model estimations, obtained in SAMIS3 (3D model of equatorial spread F) and kindly presented by J. Huba (USA), are also used for the investigation. It was revealed that the plasma bubbles, reaching the “ceiling” heights, can exist within 2-3 days and that there is principal opportunity to observe them in the separate plasma component (He (+) ). (b) The longitudinal statistics of the He (+) density depletions (P), calculated for all seasons and both hemispheres (20-50(°) INVLAT), were obtained. It was revealed that the most of the P plots have “wave-like” structure with well-defining four peaks. The peaks are the most pronounced in the NH during March equinox/December solstice and in the SH during March equinox/June solstice. Similar wave number 4 longitudinal structure has recently been found in the low-latitude ionosphere density distribution [Immel et al., GRL, 2006; England et al., GRL, 2006; Jin et al., JGR, 2008]. It is assumed that the longitudinal plasma density variations appear due to the modulated vertical Е×В drift. It is supposed that solar thermal tides excited in the troposphere induce zonal perturbation electric fields, which are added to the

  6. Selected papers from the 23rd MicroMechanics and Microsystems Europe Workshop (MME 2012) (Ilmenau, Germany, September 9-12, 2012)

    NASA Astrophysics Data System (ADS)

    Hoffmann, Martin

    2013-07-01

    In September 2012, the 23rd MicroMechanics Europe Workshop (MME) took place in Ilmenau, Germany. With about 120 participants from 20 countries and 76 accepted presentations, the workshop series turned out to be a successful platform for young scientists to present their work to our scientific community. Traditionally, the interaction is an important aspect of this workshop: while short presentations introduce the posters, an extended poster session allows intensive discussion which is quite useful to the participants. The discussion very often extends into the breaks and the evening events. It is also encouraging for them that the best presentations are selected and invited to submit a full paper to this journal. Thanks to the support of IOP Publishing, this next logical step to present work to the scientific world is made possible. In this issue, you can find the best papers that have been selected by a committee during the workshop taking the written workshop contribution, the poster and the presentation into account. Again, all areas of micromechanics from new technology developments up to systems integration were presented at the workshop at different levels of completion. The selected papers present those results which are almost complete. Nevertheless, it is nice to see that in some cases topics grow over the years from 'nice ideas' to realized system concepts. And although this is the 23rd workshop, it is clear that micromechanics is a topic that is not running short of new ideas. First, I would like to thank the authors of the selected papers for each of their individual excellent contributions. My gratitude also goes to my fellow members in the programme committee (Per Ohlckers, Martin Hill and Sami Franssila) for their cooperation in the selection of invited speakers and submitted papers, as well as the anonymous Journal of Micromechanics and Microengineering (JMM) reviewers for their careful selection of the final papers presented here. Last, but not

  7. Hour-Scale Variability in NGC 663 and NGC 1960

    NASA Astrophysics Data System (ADS)

    Souza, Steven P.; Garcia Soto, Aylin; Wong, Hallee

    2016-06-01

    Since 2010 we have been monitoring massive emission-line (mainly Be) stars in young open clusters using narrowband imaging at Hα (656nm) and the nearby continuum (645nm) (Souza, Davis, and Teich 2013, BAAS. 45, PM354.22; Souza, Beltz-Mohrmann, and Sami 2014. JAAVSO, 42, 154). To supplement longer-timescale data taken at Williams College we obtained high-cadence observations, in both filters, of NGC 663 on the night of 12/10/15, and of NGC 1960 on the nights of 12/10/14, 1/23/15, 1/25/15, 11/11/15, and 12/13/15 at the 0.5m ARCSAT at Apache Point Observatory. After raw magnitude extraction using Aperture Photometry Tool (Laher et al. 2012, PASP, 124, 737), we used inhomogeneous ensemble photometry (Bhatti et al., 2010, ApJ Supp., 186, 233) to correct for transparency and seeing variations. The NGC 663 field is crowded; of 29 known Be stars in the observed field, 10 have nearby interferers. None of the remaining 19 Be stars showed significant variation during ~5.5 hours of observation. 1σ uncertainty estimates range from 0.02mag at R~10 to 0.15mag at R~14. To verify the observing and reduction procedure, we recovered hour-scale variability in known variables BY Cas (δ Cephei type, ~0.05mag decline) and V1155 Cas (β Cephei type, ~0.04mag amplitude). In NGC 1960, of 5 known and suspect Be stars observed, two not previously reported as variable (BD+34 1110 and USNOB1.0 1241-0103450) showed irregular variation on timescales of hours. In NGC 1960 we also report the incidental discovery of two non-Be suspect variables: a likely eclipsing binary (0.07mag), and a possible δ Scuti star (maximum amplitude ~0.02mag). We gratefully acknowledge support for student research from NSF grant AST-1005024 to the Keck Northeast Astronomy Consortium, and the Office of the Dean of Faculty and the DIII Research Funding Committee of Williams College. Based on observations obtained with Apache Point Observatory's 0.5-m Astrophysical Research Consortium Small Aperture Telescope.

  8. A study of 3D structure of nighttime electron density enhancement in the mid-latitude ionosphere by GPS tomography

    NASA Astrophysics Data System (ADS)

    Chen, C.; Saito, A.

    2011-12-01

    The mid-latitude summer nighttime anomaly (MSNA) is a feature that the nighttime electron density larger than that in the daytime mid-latitude ionosphere. This anomaly was first detected in the southern hemisphere five decades ago and observed in the northern hemisphere recently by ionosondes and satellites. Previous studies presented the electron density structure of MSNA by using COSMIC occultation data and found that MSNA is clearly seen around 300 km altitude during local summer. However, due to lack of observation, the day-to-day variation of MSNA was not investigated. A GPS tomography method by SPEL of Kyoto University using the total electron content (TEC) data measured by the ground-based GPS receiver network is employed in this study. The wide coverage and continuous observation of GPS receivers are suitable for investigating the spatial and day-to-day variations of ionospheric electron densities. The algorithm of the GPS tomography developed by SPEL of Kyoto University use a constraint condition that the gradient of election density tends to be smooth in the horizontal direction and steep in the vicinity of the F2 peak, instead of inputting the initial conditions. Therefore, the algorithm is independent of any ionospheric and plasmaspheric electron density distribution models. The dense ground-based GPS receiver network around European region is used to study the three dimensional (3D) structure of MSNA with GPS tomography. Results show that the MSNA usually appear around the geomagnetic mid-latitude region during local summer nighttime. The feature of MSNA is most obvious at the ionospheric F2-peak altitudes. The result also shows a day-to-day variation in the formation of MSNA, in terms of the occurrence time, intensity, and spatial extent. The tomographic results are compared with the ionosondes, satellites, and radar measurements. A theoretical model simulation, SAMI2, is also used to further discuss the mechanism of MSNA. The comparison with other

  9. Crystal structures of human 108V and 108M catechol O-methyltransferase

    SciTech Connect

    Rutherford, K.; Le Trong, I.; Stenkamp, R.E.; Parson, W.W.

    2008-08-01

    Catechol O-methyltransferase (COMT) plays important roles in the metabolism of catecholamine neurotransmitters and catechol estrogens. The development of COMT inhibitors for use in the treatment of Parkinson's disease has been aided by crystallographic structures of the rat enzyme. However, the human and rat proteins have significantly different substrate specificities. Additionally, human COMT contains a common valine-methionine polymorphism at position 108. The methionine protein is less stable than the valine polymorph, resulting in decreased enzyme activity and protein levels in vivo. Here we describe the crystal structures of the 108V and 108M variants of the soluble form of human COMT bound with S-adenosylmethionine (SAM) and a substrate analog, 3,5-dinitrocatechol. The polymorphic residue 108 is located in the {alpha}5-{beta}3 loop, buried in a hydrophobic pocket {approx}16 {angstrom} from the SAM-binding site. The 108V and 108M structures are very similar overall [RMSD of C{sup {alpha}} atoms between two structures (C{sup {alpha}} RMSD) = 0.2 {angstrom}], and the active-site residues are superposable, in accord with the observation that SAM stabilizes 108M COMT. However, the methionine side chain is packed more tightly within the polymorphic site and, consequently, interacts more closely with residues A22 ({alpha}2) and R78 ({alpha}4) than does valine. These interactions of the larger methionine result in a 0.7-{angstrom} displacement in the backbone structure near residue 108, which propagates along {alpha}1 and {alpha}5 toward the SAM-binding site. Although the overall secondary structures of the human and rat proteins are very similar (C{sup {alpha}} RMSD = 0.4 {angstrom}), several nonconserved residues are present in the SAM-(I89M, I91M, C95Y) and catechol- (C173V, R201M, E202K) binding sites. The human protein also contains three additional solvent-exposed cysteine residues (C95, C173, C188) that may contribute to intermolecular disulfide bond

  10. [Evaluation of 44 pediatric measles cases detected in Ankara, Turkey during 2012-2013 epidemic and molecular characterization of the viruses obtained from two cases].

    PubMed

    Metin, Ozge; Tanir, Gönül; Oz, Fatma Nur; Kalaycioglu, Atila Taner; Yolbakan, Sultan; Tuygun, Nilden; Bayhan, Gülsüm Iclal; Aydin Teke, Türkan; Korukluoglu, Gülay

    2014-04-01

    Elimination of measles and rubella until the end of 2015 in parallel with the "World Health Organization (WHO) Europe Region's Measles Elimination" work-up has been targetted and "Measles Elimination Program'' has been carried out since 2002 in Turkey. Due to the routine vaccination programmes the number of the vaccinated children have increased and epidemic incidences have been falling. However, imported measles cases from Europe and other neighboring countries have been observed in Turkey in the recent two years. Patients who applied to Dr. Sami Ulus Maternity and Children's Training and Research Hospital with a pre-diagnosis of measles between December 2012 and April 2013 were screened in this study. Seventy-eight patients who match the clinical definition of the disease (> 38°C fever and maculopapular rash and cough or nasal discharge or conjunctivitis) were evaluated. Forty-four children (25 male, 19 female; age range: 4-191 months, mean age: 58.6 ± 59.5 months) with a positive measles IgM test result were taken into consideration and the epidemiological and clinical features of these children were evaluated. In addition to fever and rash, cough, nasal discharge and conjunctivitis were seen in 36 (82%), 24 (55%), and 18 (41%) patients, respectively. Thirty five (80%) patients were diagnosed in December, 6 (14%) in January, 2 (4%) in February, and 1 (2%) in March. All patients included in the study were unvaccinated or too young to be vaccinated according to the routine vaccination calendar. The index case was a three-year old unvaccinated girl who had a history of contact with the Syrian neighborhoods. During the study period; following contact with the index case, two doctors (born in 1986 with a history of single dose of vaccination at ninth month) and three children (without vaccination) were also diagnosed as measles. Eight (18%) patients were hospitalized because of complications. Four (50%) of them had pneumonia and the other four (50%) had lack of

  11. FOREWORD: HELAS II International Conference

    NASA Astrophysics Data System (ADS)

    Gizon, Laurent; Roth, Markus

    2008-07-01

    . Also available in the online edition are (i) an interactive conference picture, (ii) the abstract book, and (iii) material on the special session `Waves, Waves and Waves'. Additional articles related to both the HELAS II and the SOHO 19/GONG 2007 conferences can be found in a topical issue of Solar Physics, volume 251, nos 1-2. Financial support was provided by the HELAS Network, the Max Planck Institute for Solar System Research (through Ulrich Christensen and Sami Solanki) and the University of Göttingen (through Stefan Dreizler). We thank the local organizers, and in particular Sabine Deutsch, for their outstanding efforts in making the conference a success. We are also grateful to Graham Douglas and Jacky Mucklow of IoP Publishing for their help in the production of this volume. Laurent Gizon and Markus Roth Editors Katlenburg-Lindau, Germany

  12. Preface: phys. stat. sol. (c) 1/7

    NASA Astrophysics Data System (ADS)

    Cheikhrouhou, Abdelwaheb

    2004-05-01

    Physics Laboratory, Sciences Faculty of Sfax (Tunisia) and the Co-Chairmen were Professor Sami Mahmood, Dean of Sciences at Yarmouk University (Jordan) and Professor Mohamed Akhavan from the Sharif University of Technology (Iran). The four-day conference consisted of several oral and poster sessions, followed by social programs in the evenings. The success of the event could be measured during the closing session on the last day, when several delegates emphasized the high-quality science that had been evident at the conference. A post conference three-day tour to the south of Tunisia (Matmata, Douz City: the gate of desert and the mountains oasis: Tamerza, Mides and Chebika) was also arranged. The conference was generously sponsored by: - The Tunisian Ministry of High Education, Scientific Research and Technology - The Tunisian Secretary of State for Scientific Research and Technology - The Tunisian National Office of Tourism - The Abdus Salam International Centre for Theoretical Physics (ICTP) - French Institute for Cooperation in Tunisia - Tunisian-Italian Scientific Partnership - British Gas - Tunisian Society for Electricity and Gas - Imex Olive Oil -Confiserie TRIKI Le Moulin The next MSM conference in 2005 will be held in Morocco.

  13. Optimizing Communications Between Arctic Residents and IPY Scientific Researchers

    NASA Astrophysics Data System (ADS)

    Stapleton, M.; Carpenter, L.

    2007-12-01

    in San Francisco on December 10 to 14, 2007. One component of this conference is entitled « Education, Outreach and Communications During IPY and Beyond ». ACIC proposes to present a discussion paper, « Optimizing Communications Between Arctic Residents and IPY Scientific Researchers », describing the status of IPY outreach and communications in the Arctic at this time. The paper will be complemented by photographs which illustrate the context of communication activity in these regions. ACIC has an existing international network of indigenous northern communicators. The IPY Northern Coordination Offices in Canada, and key informants in Alaska, RAIPON in the Russian Federation, and the Association of Sami Journalists, will be interviewed to determine involvement in IPY activities planned and/or undertaken. The level of community and professional awareness will be surveyed through interviews with community radio personnel. Aspirations and expectations for further cooperation with IPY reseearchers will be determined. Barriers and shortfalls will be identified. The usability and potential of current communications will be assessed. Endorsed IPY projects will be contacted to determine their Arctic communication plans and activities, barriers and opportunities. Information gained from the Joint Committee Assessment in October will be considered in the context of northern informant input. Conclusions and recommendations will reported, with the goal of optimizing opportunities to connect indigenous Arctic residents and IPY scientific research centres.

  14. PREFACE: The Eighth Liquid Matter Conference The Eighth Liquid Matter Conference

    NASA Astrophysics Data System (ADS)

    Dellago, Christoph; Kahl, Gerhard; Likos, Christos N.

    2012-07-01

    interface tension of flat and curved interfaces from Monte Carlo simulationsA Tröster and K Binder Phase diagrams of particles with dissimilar patches: X-junctions and Y-junctionsJ M Tavares and P I C Teixeira The unbearable heaviness of colloids: facts, surprises, and puzzles in sedimentationRoberto Piazza, Stefano Buzzaccaro and Eleonora Secchi Exploring water and other liquids at negative pressureFrédéric Caupin, Arnaud Arvengas, Kristina Davitt, Mouna El Mekki Azouzi, Kirill I Shmulovich, Claire Ramboz, David A Sessoms and Abraham D Stroock The configurational space of colloidal patchy polymers with heterogeneous sequencesIvan Coluzza and Christoph Dellago Repeated sorption of water in SBA-15 investigated by means of in situ small-angle x-ray scatteringM Erko, D Wallacher, G H Findenegg and O Paris Transition of the hydration state of a surfactant accompanying structural transitions of self-assembled aggregatesM Hishida and K Tanaka The effects of topology on the structural, dynamic and mechanical properties of network-forming materialsMark Wilson Surface tension of an electrolyte-air interface: a Monte Carlo studyAlexandre Diehl, Alexandre P dos Santos and Yan Levin Water and other tetrahedral liquids: order, anomalies and solvationB Shadrack Jabes, Divya Nayar, Debdas Dhabal, Valeria Molinero and Charusita Chakravarty Diffusion coefficient and shear viscosity of rigid water modelsSami Tazi, Alexandru Boţan, Mathieu Salanne, Virginie Marry, Pierre Turq and Benjamin Rotenberg Phase behaviour of colloidal assemblies on 2D corrugated substratesSamir El Shawish, Emmanuel Trizac and Jure Dobnikar Structural properties of dendrimer-colloid mixturesDominic A Lenz, Ronald Blaak and Christos N Likos Fluid-fluid demixing of off-critical colloid-polymer systems confined between parallel platesE A G Jamie, R P A Dullens and D G A L Aarts Simulations of nematic homopolymer melts using particle-based models with interactions expressed through collective variablesKostas Ch

  15. PREFACE: International Conference on the Use of X-ray (and related) Techniques in Arts and Cultural Heritage (XTACH 11)

    NASA Astrophysics Data System (ADS)

    Hamdan, Nasser; El-Khatib, Sami

    2012-07-01

    ), Raman measurements, as well as other sample preparation techniques. The training course concluded with a series of presentations of the results by the participants, attended by the NXFL team and experts from the IAEA. This training course was organized as part of the activities of the IAEA technical cooperation RAS1011 Project: Using Ion Beam Analysis and Complementary Nuclear Techniques for Material Characterization in ARASIA State Parties. The course was attended by participants from Iraq, Jordan, Lebanon, Qatar, Syria, the United Arab Emirates and Yemen. We would like to thank the conference sponsors: Tashkeel, Sharjah Museums, and Sharjah Department of Culture and Information (Directorate on Antiquities). We would also like to thank our invited speakers, the international advisory committee, the referees and the participants. It has been a pleasure working with them all. Organizing Committee Nasser Hamdan AUS, NXFL Members Pia Anderson AUS Hussain Al-Awadhi UoS & NXFL Sami El Khatib AUS Attaelmanan Gaffar UoS & NXFL Johannes Giesen AUS Sabah Jasim Directory of Antiquities Sharjah Najeh Jisrawi UoS & NXFL Adil Tamimi AUS International Advisory Committee Zaki Aslan ATHAR, ICCROM, Italy Mark Beech Abu Dhabi Culture & Heritage, UAE Rene Van Grieken University of Antwerp, Belgium Gene Hall Rutgers, The State University of N.J. Peter Jackson Office of the Ruler of Sharjah Andreas Karydas IAEA Laboratories, Seiberdorf, Austria Giacinto Porco The Italian Association of Non-Destructive Testing, Italy Mohammad Roumie (CNRS) Lebanese Atomic Energy, Commission, Lebanon Acknowledgments The organizers gratefuly acknowledge the support received from the College of Arts and Sciences and the Provosts office at the American University of Sharjah. The support of the Physics Section, Division of Physical and Chemical Sciences at the IAEA is greatly appreciated. We would like to give special thanks to Dr Francoise Muelhauser from the IAEA. We would like also to thank the conference

  16. The Eighth Liquid Matter Conference.

    PubMed

    Dellago, Christoph; Kahl, Gerhard; Likos, Christos N

    2012-06-27

    interface tension of flat and curved interfaces from Monte Carlo simulationsA Tröster and K Binder Phase diagrams of particles with dissimilar patches: X-junctions and Y-junctionsJ M Tavares and P I C Teixeira The unbearable heaviness of colloids: facts, surprises, and puzzles in sedimentationRoberto Piazza, Stefano Buzzaccaro and Eleonora Secchi Exploring water and other liquids at negative pressureFrédéric Caupin, Arnaud Arvengas, Kristina Davitt, Mouna El Mekki Azouzi, Kirill I Shmulovich, Claire Ramboz, David A Sessoms and Abraham D Stroock The configurational space of colloidal patchy polymers with heterogeneous sequencesIvan Coluzza and Christoph Dellago Repeated sorption of water in SBA-15 investigated by means of in situ small-angle x-ray scatteringM Erko, D Wallacher, G H Findenegg and O Paris Transition of the hydration state of a surfactant accompanying structural transitions of self-assembled aggregatesM Hishida and K Tanaka The effects of topology on the structural, dynamic and mechanical properties of network-forming materialsMark Wilson Surface tension of an electrolyte-air interface: a Monte Carlo studyAlexandre Diehl, Alexandre P dos Santos and Yan Levin Water and other tetrahedral liquids: order, anomalies and solvationB Shadrack Jabes, Divya Nayar, Debdas Dhabal, Valeria Molinero and Charusita Chakravarty Diffusion coefficient and shear viscosity of rigid water modelsSami Tazi, Alexandru Boţan, Mathieu Salanne, Virginie Marry, Pierre Turq and Benjamin Rotenberg Phase behaviour of colloidal assemblies on 2D corrugated substratesSamir El Shawish, Emmanuel Trizac and Jure Dobnikar Structural properties of dendrimer-colloid mixturesDominic A Lenz, Ronald Blaak and Christos N Likos Fluid-fluid demixing of off-critical colloid-polymer systems confined between parallel platesE A G Jamie, R P A Dullens and D G A L Aarts Simulations of nematic homopolymer melts using particle-based models with interactions expressed through collective variablesKostas Ch

  17. Radio Telescopes Will Add to Cassini-Huygens Discoveries

    NASA Astrophysics Data System (ADS)

    2004-12-01

    accuracy. They expect to measure the probe's position within two-thirds of a mile (1 kilometer) at a distance of nearly 750 million miles. "That's like being able to sit in your back yard and watch the ball in a ping-pong game being played on the Moon," said Leonid Gurvits of JIVE. Both the JPL and JIVE teams will record the data collected by the radio telescopes and process it later. In the case of the Doppler measurements, some real-time information may be available, depending on the strength of the signal, but the scientists on this team also plan to do their detailed analysis on recorded data. The JPL team is utilizing special instrumentation from the Deep Space Network called Radio Science Receivers. One will be loaned to the GBT and another to the Parkes radio observatory. "This is the same instrument that allowed us to support the challenging communications during the landing of the Spirit and Opportunity Mars rovers as well as the Cassini Saturn Orbit Insertion when the received radio signal was very weak," said Sami Asmar, the JPL scientist responsible for the data recording. When the Galileo spacecraft's probe entered Jupiter's atmosphere in 1995, a JPL team used the NSF's Very Large Array (VLA) radio telescope in New Mexico to directly track the probe's signal. Adding the data from the VLA to that experiment dramatically improved the accuracy of the wind-speed measurements. "The Galileo probe gave us a surprise. Contrary to some predictions, we learned that Jupiter's winds got stronger as we went deeper into its atmosphere. That tells us that those deeper winds are not driven entirely by sunlight, but also by heat coming up from the planet's core. If we get lucky at Titan, we'll get surprises there, too," said Robert Preston, another JPL scientist. The Huygens probe is a spacecraft built by the European Space Agency (ESA). In addition to the NRAO telescopes, the JPL Doppler Wind Experiment will use the Australia Telescope National Facility and other radio

  18. Welcome to the 2014 volume of Smart Materials and Structures

    NASA Astrophysics Data System (ADS)

    Garcia, Ephrahim

    2014-01-01

    time, the energy harvesting symposium. (2) A special issue called 'Electromechanically active polymer (EAP) transducers: research in Europe', a collection of articles from the European Scientific Network for Artificial Muscles—ESNAM group. This year, look out for focus issues put together by the editorial board on 'fluidic artificial muscles' and 'active materials and structures for origami engineering'. We will also continue to run a busy program of Topical Reviews, which are often among the most cited and most downloaded articles in the journal. Congratulations to Ganesh Raghunath and his team (University of Maryland) who won the Smart Materials and Structures prize for the best paper at SMASIS 2013, and to Kyle Mulligan and his team (University of Sherbrooke) who won our best student paper prize at Cansmart 2013. We were delighted with the news last year that ASME awarded two of its prestigious annual best paper awards to articles published in SMS: the 2013 ASME 'Adaptive Structures and Material Systems Best Paper Award in Adaptive Materials and Material Systems' went to Donghyeon Ryu and Kenneth J Loh for their article 'Strain sensing using photocurrent generated by photoactive P3HT-based nanocomposites'. The 2013 ASME 'Adaptive Structures and Material Systems Best Paper Award in Structural Dynamics and Control' went to Julianna Abel, Jonathan Luntz and Diann Brei for their article 'A two-dimensional analytical model and experimental validation of garter stitch knitted shape memory alloy actuator architecture'. Finally, may I take this opportunity to thank our fantastic Editorial board of Associate Editors who tirelessly oversee the review of each submitted article and give their invaluable advice, helping to develop and shape the journal. Welcome to Professor Alper Erturk who has recently joined us. We also acknowledge and thank Professor Andrea Del Grosso, Professor Sami Masri, Professor Seung Jo Kim and Professor Christian Boller who retired from the Board