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Sample records for sedimento marino proveniente

  1. San Marino.

    PubMed

    1985-02-01

    San Marino, an independent republic located in north central Italy, in 1983 had a population of 22,206 growing at an annual rate of .9%. The literacy rate is 97% and the infant mortality rate is 9.6/1000. The terrain is mountainous and the climate is moderate. According to local tradition, San Marino was founded by a Christian stonecutter in the 4th century A.D. as a refuge against religious persecution. Its recorded history began in the 9th century, and it has survived assaults on its independence by the papacy, the Malatesta lords of Rimini, Cesare Borgia, Napoleon, and Mussolini. An 1862 treaty with the newly formed Kingdom of Italy has been periodically renewed and amended. The present government is an alliance between the socialists and communists. San Marino has had its own statutes and governmental institutions since the 11th century. Legislative authority at present is vested in a 60-member unicameral parliament. Executive authority is exercised by the 11-member Congress of State, the members of which head the various administrative departments of the goverment. The posts are divided among the parties which form the coalition government. Judicial authority is partly exercised by Italian magistrates in civil and criminal cases. San Marino's policies are tied to Italy's and political organizations and labor unions active in Italy are also active in San Marino. Since World War II, there has been intense rivalry between 2 political coalitions, the Popular Alliance composed of the Christian Democratic Party and the Independent Social Democratic Party, and the Liberty Committee, coalition of the Communist Party and the Socialist Party. San Marino's gross domestic product was $137 million and its per capita income was $6290 in 1980. The principal economic activities are farming and livestock raising, along with some light manufacturing. Foreign transactions are dominated by tourism. The government derives most of its revenue from the sale of postage stamps to collectors around the world and from payment of an annual budget subsidy by the Italian government. Despite its close ties with Italy, San Marino has maintained its distinctive status for centuries. PMID:12178101

  2. Dan Marino Helping Those with Autism Spectrum Disorders | NIH MedlinePlus the Magazine

    MedlinePLUS

    ... Marino Foundation. Photo: Dan Marino Foundation Former NFL star quarterback Dan Marino and his wife Claire experienced ... to succeed in life,'" says the former NFL star. "That's where the focus for The Dan Marino ...

  3. Epidemiology of headache in the Republic of San Marino.

    PubMed Central

    D'Alessandro, R; Benassi, G; Lenzi, P L; Gamberini, G; Sacquegna, T; De Carolis, P; Lugaresi, E

    1988-01-01

    An epidemiological survey on headache was performed in the Republic of San Marino, which is the smallest independent State in the world, located near the Adriatic Coast, within Italy. Among a random sample of 1500 inhabitants over 7 years of age the frequency of headache, severe headache and migraine in the previous year was 35.3%, 12.2%, 9.3% respectively for men, and 46.2%, 20.6%, 18% for women. The most common factors reported to provoke headache were emotional stress, physical strain, lack of sleep, particular foods or drinks and for women menstruation. Migraine patients differed from people without headache in that they had a higher consumption of coffee, more frequently reported bad sleep, allergic disease and previous appendectomy. Furthermore, migraine patients and severe headache sufferers had a higher diastolic blood pressure than non headache subjects. PMID:3258357

  4. VizieR Online Data Catalog: NGC 2808 HB stars abundances (Marino+, 2014)

    NASA Astrophysics Data System (ADS)

    Marino, A. F.; Milone, A. P.; Przybilla, N.; Bergemann, M.; Lind, K.; Asplund, M.; Cassisi, S.; Catelan, M.; Casagrande, L.; Valcarce, A. A. R.; Bedin, L. R.; Cortes, C.; D'Antona, F.; Jerjen, H.; Piotto, G.; Schlesinger, K.; Zoccali, M.; Angeloni, R.

    2014-11-01

    To identify our stellar sample, we use the photometric catalogue of Momany et al. (2004), which has been obtained from U, B and V images collected with the Wide-Field Imager (WFI) mounted at the 2.2m ESO-MPI (Max-Planck-Institut) telescope at La Silla observatory, Chile. Our spectroscopic data consist of FLAMES/GIRAFFE and FLAMES/UVES data collected under the ESO programme 086.D-0141 (PI: Marino). The GIRAFFE fibres were used with the HR12 setup, covering the spectral range from ~5820 to ~6140Å with a resolution of ~18700. (6 data files).

  5. Karst and mixing-zone porosity in the Amposta Marino field, offshore Spain

    SciTech Connect

    Wigley, P.L.; Bouvier, J.D.; Dawans, J.M. )

    1988-08-01

    The offshore Amposta Marino field, located southeast of the Ebro delta, produces from the karstified Lower Cretaceous Montsia Limestone. The field is a buried-hill structure overlain by marine clastic sediments. During drowning, the buried hill was surrounded by sea water and thus represents the typical setting in which mixing-zone corrosion is a major porosity-creating process in modern carbonates (e.g., Yucatan Peninsula, Bahamas). Mixing-zone corrosion in a clastal setting differs from freshwater karstification in that it creates an essentially horizontal zone of well-connected matrix and cave porosity. This high-porosity zone is best developed on the flanks of a structure and, ideally, has a rim-like distribution. On 3-D seismic, the authors recognize a subhorizontal reflector that cuts across the gently dipping Amposta structure. This reflector was proven by seismic-to-well matching to represent a highly porous interval. Mapping of this reflector showed that it occurs somewhat discontinuously around the western margin of the structure and fairly continuously around the eastern margin, forming a clear rim feature around the flanks of the buried hill.

  6. Mass population screening for celiac disease in children: the experience in Republic of San Marino from 1993 to 2009

    PubMed Central

    2013-01-01

    Background Prevalence of celiac disease in developed countries is assessed about 1:100–1:150. The real prevalence is unknown because mass screenings are expensive and difficult to organize. Moreover celiac disease can affect people at every age and studies on asymptomatic subjects at different ages are not comparable. In this study we wanted to know the real prevalence of celiac disease in children in the Republic of San Marino. We also analysed concordance of different tests used and costs of mass screening. Methods The study started in 1993. From 1993 to 1997 children aged 6, 10 and 14 were screened. Since 1997 only children aged 6 were monitored, in order to have a homogeneous population. In fact, every child born since 1980 was taken into account. Children were recruited by classroom lists of students for general paediatric examination. Until 2005 the screening test was based on dosage of antibodies anti-gliadin (AGA) IgA and IgG on venous blood. Since 2006 these tests were replaced by anti-transglutaminase IgA antibodies (ATTG). Anti-endomysial antibodies (EMA) were performed if result of any between either AGA or ATTG tests was positive or borderline; if EMA was positive, then an endoscopy with histological examination was performed to confirm the final diagnosis. Results Attendance to paediatric examination was 96%, submission to blood test was 87%. 42 on 5092 (0,8%; 1:125) children resulted affected by celiac disease. Histology always confirmed diagnosis by serology except for two cases. AGA test (until 2005) yielded 28 on 4304 (0,7% 1:143); ATTG test (since 2006) revealed 14 positive cases on 788 (1,8%; 1:55) leading to a larger percentage of diagnosis. EMA antibodies always confirmed positivity of ATTG. Conclusions Prevalence of celiac disease in children of Republic of San Marino is comparable to other North-European Countries. Sensitivity of ATTG proved much higher than that of anti-gliadin antibodies. Concordance between ATTG and EMA was 100%. Concordance between serology and histology was approximately 100%. Cost of screening was yearly about 5000 euros (250 children screened every year). PMID:24152602

  7. The restart of meteorological observations in the 19th century in Lisbon: the contribution of Marino Miguel FRANZINI (1779-1861)

    NASA Astrophysics Data System (ADS)

    Alcoforado, Maria-Joao; Nunes, Fatima

    2013-04-01

    After the early meteorological observations of the 1770s to the 1790s in continental Portugal (including a 5 year daily series by J. Velho), there were hardly any until 1815. In December 1815, a meteorological station was set up in Lisbon by Marino Miguel Franzini (1779-1861), an engineer who was also actively involved in Politics (liberal party). Following the tradition of the 18th century enlightenment movement, he took a keen interest in Nature and Sciences, particularly in the "influence" of weather and climate on health and agriculture. Franzini started his observations by request of a physician who sought to understand the reasons why the maximum mortality occurred on the summer months, unlike in northern countries of Europe where maximum mortality occurred in winter (as it happens nowadays in Portugal). The deterministic background of the two scientists is clear. Franzini was a member of the Lisbon Academy of Sciences (founded in 1799) and had contact with foreign Academies and foreign scientists. His instruments were carefully constructed and described, including graduation scales, and stations' location was indicated. Data from two years observations (several meteorological variables) was published in the Academy of Sciences Memoirs. From 1818 until 1826 and from 1835 until 1856 data was divulged in journals and newspapers, such as the "Journal of Medical Sciences", together with data on necrology in some of Lisbon parishes (illustrating the interest of physicians on weather); meteorological data and information about agriculture was also published in the "Lisbon Gazette". Unfortunately, there are hardly any daily data, as Franzini grouped his records according to weather types, as will be explained. Franzini's series will be presented in our talk. The gap between 1826 and 1835 was due to the political activities in which Franzini was involved: the civil war (liberals against absolutist) disruptedscientific research in Portugal. Official meteorological observations began in Lisbon,in December 1854, in a site not far away from Franzini's station. The long series of Lisbon includes the 1835-54 Franzini's series.

  8. VizieR Online Data Catalog: Photometry and abundances of NGC1851 stars (Marino+, 2014)

    NASA Astrophysics Data System (ADS)

    Marino, A. F.; Milone, A. P.; Yong, D.; Dotter, A.; da Costa, G.; Asplund, M.; Jerjen, H.; Mackey, D.; Norris, J.; Cassisi, S.; Sbordone, L.; Stetson, P. B.; Weiss, A.; Aparicio, A.; Bedin, L. R.; Lind, K.; Monelli, M.; Piotto, G.; Angeloni, R.; Buonanno, R.

    2015-03-01

    In this paper, we used four distinct photometric data sets. First, we used Stetson (2000PASP..112..925S) ground-based B, V, R and I photometry. This photometric catalogue has been established from about 550 images taken at different telescopes, i.e. the Max Planck 2.2m, the Cerro Tololo Inter-American Observatory (CTIO) 4, 1.5 and 0.9m telescopes, and the Dutch 0.9m telescope in La Silla. In the present work, we have complemented the Stetson catalogue with images collected with the Wide Field Imager (WFI) of the Max Planck 2.2m telescope at La Silla (WFI@2.2m) through the U filter under the SUrvey of Multiple pOpulations (SUMO) campaign. Secondly, to study stars in the halo of NGC 1851, we collected BVI images with WFI@2.2m of a field between ~10 and 35 arcmin to the south of the cluster centre. Photometry and astrometry for this data set have been obtained by using the program img2xym_WFI and the procedure described by Anderson et al. (2006A&A...454.1029A). Third and finally, to investigate the most crowded central regions, we use Hubble Space Telescope (HST) F606W and F814W photometry obtained with the Wide Field Channel of the Advanced Camera for Survey (WFC/ACS) and F275W photometry collected with the Ultraviolet and Visual Channel of the Wide Field Camera 3 (UVIS/WFC3). (2 data files).

  9. 22 CFR 228.03 - Identification of principal geographic code numbers.

    Code of Federal Regulations, 2010 CFR

    2010-04-01

    ... § 228.03 Identification of principal geographic code numbers. The USAID Geographic Code Book sets forth... Marino, Saudi Arabia, Serbia*, Singapore, Slovak Republic, Slovenia, South Africa, Spain,...

  10. Numerical analysis of the hydrogeologic controls in a layered coastal aquifer system, Oahu, Hawaii, USA

    NASA Astrophysics Data System (ADS)

    Oki, Delwyn S.; Souza, William R.; Bolke, Edward L.; Bauer, Glenn R.

    The coastal aquifer system of southern Oahu, Hawaii, USA, consists of highly permeable volcanic aquifers overlain by weathered volcanic rocks and interbedded marine and terrestrial sediments of both high and low permeability. The weathered volcanic rocks and sediments are collectively known as caprock, because they impede the free discharge of groundwater from the underlying volcanic aquifers. A cross-sectional groundwater flow and transport model was used to evaluate the hydrogeologic controls on the regional flow system in southwestern Oahu. Controls considered were: (a) overall caprock hydraulic conductivity; and (b) stratigraphic variations of hydraulic conductivity in the caprock. Within the caprock, variations in hydraulic conductivity, caused by stratigraphy or discontinuities of the stratigraphic units, are a major control on the direction of groundwater flow and the distribution of water levels and salinity. Results of cross-sectional modeling confirm the general groundwater flow pattern that would be expected in a layered coastal system. Groundwater flow is: (a) predominantly upward in the low-permeability sedimentary units; and (b) predominantly horizontal in the high-permeability sedimentary units. Résumé Le système aquifère littoral du sud d'Oahu (Hawaii, États-Unis) est constitué par des aquifères de terrains volcaniques très perméables, recouverts par des roches volcaniques altérées, et interstratifiés avec des sédiments marins et continentaux de perméabilité aussi bien forte que faible. Les roches volcaniques altérées et les sédiments sont globalement considérés comme une couverture, parce qu'ils s'opposent à l'écoulement de l'eau souterraine provenant des aquifères volcaniques sous-jacents. Les contrôles hydrogéologiques sur le système aquifère régional du sud-ouest d'Oahu ont étéévaluées au moyen d'un modèle d'écoulement et de transport sur une section transversale. Ces contrôles prennent en compte la conductivité hydraulique de la couverture dans son ensemble et les variations de la conductivité hydraulique liées à la stratigraphie de la couverture. A l'intérieur de la couverture, les variations de la conductivité hydraulique, dues à la stratigraphie ou à des discontinuités entre les unités stratigraphiques, sont le contrôle principal de la direction d'écoulement et de la répartition des niveaux et de la salinité de l'eau. La modélisation sur une section transversale a donné des résultats qui confirment l'organisation générale des directions d'écoulement, telle qu'elle pouvait être envisagée dans un aquifère littoral multicouche. L'écoulement souterrain est essentiellement vertical vers le haut dans les unités sédimentaires à faible perméabilité, et essentiellement horizontal dans les unités sédimentaires à forte perméabilité. Resumen El sistema acuífero costero de la zona sur de Oahu, en Hawaii, está formado por acuíferos volcánicos de alta permeabilidad, subyacentes a rocas volcánicas alteradas, con inclusiones de sedimentos marinos y terrestres, tanto de alta como de baja permeabilidad. Al conjunto de rocas volcánicas alteradas y sedimentos se le conoce por "tapón de roca", ya que impide la descarga libre de las aguas subterráneas del acuífero volcánico subyacente. Se usó un modelo de flujo de agua subterránea y transporte de solutos en sección vertical para evaluar los aspectos hidrogeológicos que controlan el flujo regional en la zona sudoeste de Oahu. Se consideraron: (a) la conductividad hidráulica global del tapón y (b) las variaciones estratigráficas de la conductividad hidráulica. En el tapón de roca, las variaciones de la conductividad hidráulica, causadas por la estratigrafía o por discontinuidades en las unidades estratigráficas, son las que controlan la dirección del flujo subterráneo y la distribución de niveles piezométricos y salinidad. Los resultados del modelo en sección transversal confirman la distribución del flujo subterráneo que cabría esperar en un sistema costero estratificado. El flujo de aguas subterráneas es: (a) predominantemente vertical hacia arriba en las unidades sedimentarias de baja permeabilidad; y (b) predominantemente horizontal en las unidades sedimentarias de alta permeabilidad.

  11. Operación IceBridge: Explorando la Antártida - Duration: 3 minutes, 4 seconds.

    NASA Video Gallery

    Operación IceBridge es una misión aérea de la NASA dedicada a estudiar cambios en el hielo marino y terrestre en ambos polos del planeta. En octubre y noviembre de 2012, IceBridge completó su cuart...

  12. 78 FR 86 - In the Matter of:

    Federal Register 2010, 2011, 2012, 2013, 2014

    2013-01-02

    ... Notices, the most recent being that of August 12, 2012 (77 FR 49699, August 16, 2012), has continued the... From the Federal Register Online via the Government Publishing Office DEPARTMENT OF COMMERCE Bureau of Industry and Security In the Matter of: Henson Chua, 2945 Somerset Place, San Marino, CA...

  13. 78 FR 63978 - Proposed CERCLA Settlements Relating to the Truckers Warehouse Site in Passaic, Passaic County...

    Federal Register 2010, 2011, 2012, 2013, 2014

    2013-10-25

    ... AGENCY Proposed CERCLA Settlements Relating to the Truckers Warehouse Site in Passaic, Passaic County... Comprehensive Environmental Response, Compensation, and Liability Act of 1980, as amended (``CERCLA''), notice...(h)(1) of CERCLA, with (1) RJS Corp.; (2) Your Factory Warehouse, Inc., Douglas Marino and...

  14. OPERACIÓN IceBridge: Explorando cambios en el hielo de Groenlandia - Duration: 2 minutes, 29 seconds.

    NASA Video Gallery

    Operación IceBridge es una misión aérea de la NASA dedicada a estudiar cambios en la capa de hielo y el hielo marino en ambos polos del planeta. En la primavera de 2012, IceBridge llevó a cabo ...

  15. Concepts & Procedures. [SITE 2002 Section].

    ERIC Educational Resources Information Center

    Sarner, Ronald, Ed.; Mullick, Rosemary J., Ed.; Bauder, Deborah Y., Ed.

    This document contains the following full and short papers on concepts and procedures from the SITE (Society for Information Technology & Teacher Education) 2002 conference: "Exploring Minds Network" (Marino C. Alvarez and others); "Learning Communities: A Kaleidoscope of Ecological Designs" (Alain Breuleux and others); "PDA's and Research: A…

  16. Beautiful Science: Worth a Visit

    ERIC Educational Resources Information Center

    Bingham, Frederick M.

    2013-01-01

    For those in the profession of teaching physics who reside in or plan to visit the Los Angeles area, I would highly recommend a trip to the Huntington Library in San Marino, specifically to a permanent exhibit entitled "Beautiful Science: Ideas that Changed the World" in the Dibner Hall of the History of Science. The exhibit contains original

  17. Care and Feeding of the Library Researcher.

    ERIC Educational Resources Information Center

    Woodward, Daniel

    1987-01-01

    Describes the patrons of and typical research projects conducted at the Huntington Library in San Marino, California, as well as the role of the library, including research services and grants, library collections, and assistance to researchers beyond the library setting. (CLB)

  18. Beautiful Science: Worth a Visit

    ERIC Educational Resources Information Center

    Bingham, Frederick M.

    2013-01-01

    For those in the profession of teaching physics who reside in or plan to visit the Los Angeles area, I would highly recommend a trip to the Huntington Library in San Marino, specifically to a permanent exhibit entitled "Beautiful Science: Ideas that Changed the World" in the Dibner Hall of the History of Science. The exhibit contains original…

  19. Literacy and Community. The Twentieth Yearbook: A Peer Reviewed Publication of the College Reading Association, 1998. [Papers from the College Reading Association Conference, 1997].

    ERIC Educational Resources Information Center

    Sturtevant, Elizabeth G., Ed.; Dugan, JoAnn, Ed.; Linder, Patricia, Ed.; Linek, Wayne M., Ed.

    This 20th Yearbook of the College Reading Association reflects the theme of "community" again and again, in diverse ways. First in the yearbook are the Presidential Address by Marino C. Alvarez, "Adolescent Literacy: Are We in Contact?" and the three Keynote Addresses: "My Life in Reading" (J. Chall); "A Social-Constructivist View of Family…

  20. ON THE HYDRAULICS OF STREAM FLOW ROUTING WITH BANK STORAGE: JOURNAL ARTICLE

    EPA Science Inventory

    NRMRL-ADA-00232 Hantush*, M.M., Harada, M., and Marino, M.A. On the Hydraulics of Stream Flow Routing with Bank Storage. Journal of Hydrologic Engineering 7 (1):76-89 (2002). EPA/600/J-02/173. Bank storage is a process in which volumes o...

  1. SCREENING MODEL FOR VOLATILE POLLUTANTS IN DUEL POROSITY SOILS: JOURNAL ARTICLE

    EPA Science Inventory

    NRMRL-ADA-00230 Hantush*, M.M., Govindaraju, R.S., and Marino, M.A. Screening Model for Volatile Pollutants in Duel Porosity Soils. Journal of Hydrology 260:58-74 (2000). EPA/600/J-02/172. This paper develops mass fraction models for transport and fate of volatile organic chemi...

  2. 20 CFR 404.463 - Nonpayment of benefits of aliens outside the United States; “foreign social insurance system...

    Code of Federal Regulations, 2011 CFR

    2011-04-01

    ... the duration of their absence therefrom and must make the payments without restriction or... States may be paid benefits regardless of the duration of their absence from the United States unless for... (effective March 1957) Portugal (effective May 1968) San Marino (effective January 1965) Spain (effective...

  3. 20 CFR 404.463 - Nonpayment of benefits of aliens outside the United States; “foreign social insurance system...

    Code of Federal Regulations, 2010 CFR

    2010-04-01

    ... the duration of their absence therefrom and must make the payments without restriction or... States may be paid benefits regardless of the duration of their absence from the United States unless for... (effective March 1957) Portugal (effective May 1968) San Marino (effective January 1965) Spain (effective...

  4. Why Should Community College Faculty Write Grant Proposals?

    ERIC Educational Resources Information Center

    Renninger, Phyl; Meilof, Anne; Pitts, Todd; Smalley, Janie

    2007-01-01

    Community colleges have seen dramatic enrollment increases (Kasper, 2002), and some are now offering 4-year degrees (Evelyn, 2003). They are eligible for more grants than in the past, and community college funding from state and federal appropriations is shrinking (Lawrence & Marino, 2003). For these reasons, it is imperative that community

  5. Exploration of an alluvial aquifer in Oman by time-domain electromagnetic sounding

    NASA Astrophysics Data System (ADS)

    Young, M. E.; de Bruijn, R. G. M.; Al-Ismaily, A. Salim

    One-third of the population of Oman depends upon groundwater extracted from the alluvium of the Batinah Plain, on the coast of the Gulf of Oman. Deep geophysical exploration techniques were used to determine the depth and nature of the alluvium and the boundaries of the aquifer. The base and structural controls of the alluvial basin at its contact with Tertiary marine sediments and Cretaceous ophiolite were mapped with seismic reflection data, recorded originally for oil exploration. The base of the alluvium dips northward from the foothills of the Northern Oman Mountains, reaching a maximum depth of 2000m at the coast. The varying facies of the alluvium are grossly characterised by different, overlapping ranges of electrical resistivity, depending largely on the clay content and degree of cementation. Resistivities near the coast are reduced by saline intrusion. These variations of resistivity were mapped with time-domain electromagnetic sounding along 400km of profile, to distinguish among the three zones of the alluvial aquifer. The wedge of saline intrusion was also delineated, up to 10km from the coast. The thickness of the saturated gravel aquifer ranges from 20-160m in an area greater than 600km2. Rsum Un tiers de la population d'Oman est aliment par de l'eau souterraine pompe dans les alluvions de la plaine de Batinah, sur la cte du golfe d'Oman. Des techniques d'exploration gophysique profonde ont t mises en oeuvre pour dterminer la profondeur et la nature des alluvions et les limites de l'aquifre. La base et les contrles structuraux du bassin alluvial au contact des sdiments marins tertiaires et des ophiolites crtaces ont t cartographis partir des donnes de sismique rflexion obtenues l'origine pour la recherche ptrolire. La base des alluvions plonge vers le nord partir du pimont du massif septentrional d'Oman, pour atteindre une profondeur maximale de 2000m sur la cte. Les divers facis alluviaux sont grossirement caractriss par des diffrentes gammes de rsistivitlectrique se recouvrant, dpendant surtout de la teneur en argiles et du degr de cimentation. Les rsistivits prs de la cte diminuent du fait de l'intrusion marine. Ces variations de rsistivit ont t cartographies partir de 400km de profils lectromagntiques, dans le domaine temporel ; trois zones ont t distingues dans l'aquifre alluvial. Le biseau sal a aussi t dlimit, jusqu' 10km de la cte. L'paisseur de la partie sature des graviers va de 20-160m sur une tendue suprieure 600km2. Resumen Un tercio de la poblacin de Omn depende de las aguas subterrneas extradas del aluvial de la Llanura de Batinah, en la costa del Golfo de Omn. Para determinar la profundidad y naturaleza del aluvial, as como los lmites del acufero, se han usado tcnicas de exploracin geofsica profunda. El basamento y los lmites estructurales del aluvial en su contacto con los sedimentos marinos del Terciario y la ofiolita cretcica se obtuvieron mediante ssmica de reflexin, registrada previamente en campaas de exploracin petrolfera. La base del aluvial buza hacia el norte desde el pie de las Montaas del Norte de Omn, alcanzando una profundidad mxima de 2000m en la costa. Las distintas facies del aluvial estn caracterizadas por rangos distintos, pero superpuestos, de resistividad elctrica, dependiendo del contenido en arcillas y del grado de cementacin. Las resistividades cerca de la costa se reducen por la intrusin salina. Estas variaciones de resistividad se obtuvieron con registros electromagnticos a lo largo de un perfil de 400km, con el objetivo de distinguir las tres zonas del acufero aluvial. Tambin se pudo obtener la geometra de la cua de intrusin, que llega hasta 10km de la costa. El espesor de las gravas saturadas que forman el acufero oscila entre los 20-160m en un rea superior a 600km2.

  6. Beautiful Science: Worth a Visit

    NASA Astrophysics Data System (ADS)

    Bingham, Frederick M.

    2013-03-01

    For those in the profession of teaching physics who reside in or plan to visit the Los Angeles area, I would highly recommend a trip to the Huntington Library in San Marino, specifically to a permanent exhibit entitled "Beautiful Science: Ideas that Changed the World" in the Dibner Hall of the History of Science. The exhibit contains original books and manuscripts from the library's own collections. The sheer magnitude of human achievement represented here and the amount of effort and money that must have been required to amass these books boggles the mind.

  7. Talking about Life

    NASA Astrophysics Data System (ADS)

    Impey, Chris

    2010-08-01

    Preface; Part I. Introduction Timothy Ferris, Iris Fry, Steven Dick, Ann Druyan, Pinky Nelson, Neil Tyson, Steve Benner and William Bains; Part II. Earth Roger Buick, Lynn Rothschild, John Baross, Joe Kirschvink, Andrew Knoll, Simon Conway Morris, Roger Hanlon and Lori Marino; Part III. Solar System Chris McKay, David Grinspoon, Jonathan Lunine, Carolyn Porco, Laurie Leshin, Guy Consolmagno and Peter Smith; Part IV. Exoplanets Alan Boss, Geoff Marcy, Debra Fischer, Sara Seager, David Charbonneau and Vikki Meadows; Part V. Frontiers Jill Tarter, Seth Shostak, Ray Kurzweil, Nick Bostrom, Paul Davies, Martin Rees, Ben Bova and Jennifer Michael Hecht; Reading list; Glossary; Index.

  8. Cambios histricos en el aporte terrgeno de la cuenca del Ro de la Plata sobre la plataforma interna Uruguaya

    NASA Astrophysics Data System (ADS)

    Marrero, Anala; Tudur, Adriana; Prez, Laura; Cua, Caroline; Muniz, Pablo

    2014-12-01

    El Ro de la Plata (RdlP) presenta significativas variaciones naturales (hidrodinmicas y oceanogrficas) asociadas a diferentes condiciones climticas. El propsito de este trabajo es inferir los cambios de aportes continentales de sedimentos y su relacin con las variaciones hidrolgicas del Ro de la Plata, a travs del anlisis de proxies sedimentolgicos y geoqumicos en testigos de sedimentos de la plataforma interna uruguaya que registran los ltimos 100 aos, aproximadamente. A partir de la datacin por 210Pb de dos testigos de sedimentos (GeoB 13813-4 y BAR1) se reconstruy la geocronologa del ambiente, y se relacion con datos de las forzantes climticas Pacific Decadal Oscillation, El Nio/La Nia Southern Oscillation, Atlantic Multidecadal Oscillation, y las anomalas hidrolgicas de los ros Paran y Uruguay. Los valores ms positivos y estables del Southern Oscillation Index, los cuales corresponden a fases La Nia, se observan en el periodo correspondiente entre 1910-1970, respecto al resto de la serie, donde se aprecia una mayor variabilidad y una tendencia hacia valores ms negativos (eventos El Nio). Se hicieron dendrogramas (clustering) jerrquicos para ambos testigos. Para el testigo GeoB 13813-4, se utiliz la relacin Ca/Ti y la granulometra, mientras que para BAR1 se recurri a variables granulomtricas y la tasa de sedimentacin. El mayor aporte continental hacia la regin de la plataforma adyacente al Ro de la Plata registrado a partir del ao 1970, podra ser el factor principal de los agrupamientos observados en los clusters para ambos testigos. Las agrupaciones mostraron una diferenciacin en la dcada de 1970, lo que estara asociado al aumento de los caudales de los ros Paran y Uruguay, durante las ltimas tres dcadas del siglo XX. Por otra parte se observa que la granulometra del testigo BAR1 present un mayor tamao de grano y ms variabilidad que en el caso del testigo GeoB 13813-4. Tambin se determin una mayor acumulacin de sedimentos a travs del tiempo en el cinturn de barro del Ro de la Plata (plataforma continental adyacente), comparado con aquel registrado en la Barra del Indio (lmite entre zona intermedia y externa del estuario). Estas diferencias podran estar relacionadas con la influencia del Ro de la Plata, el cual genera un ambiente altamente dinmico sobre la Barra del Indio y un ambiente ms estable sobre el cinturn de barro en la plataforma continental.

  9. A note on instanton effects in ABJM theory

    NASA Astrophysics Data System (ADS)

    Wang, Xian-fu; Wang, Xin; Huang, Min-xin

    2014-11-01

    We consider the quantum spectral problem appearing the Fermi gas formulation of the ABJM (Aharony-Bergman-Jafferis-Maldacena) matrix model. This is known to related to the refined topological string on local ℙ1 × ℙ1 Calabi-Yau geometry. In the ABJM setting the problem is formulated by an integral equation, and is somewhat different from the one formulated directly in terms of the Calabi-Yau geometry and studied in our earlier paper. We use the similar method in our earlier paper to determine the non-perturbative contributions to the quantum phase volume in the ABJM case from the Bohr-Sommerfeld quantization condition. As in our earlier paper, the non-perturbative contributions contain higher order smooth corrections beyond those required by singularity cancellations with the perturbative contributions proposed by Kallen and Marino. Our results imply possible new contributions to the grand potential of the ABJM matrix model.

  10. The mysterious fate of la Bibliothque de Louis Pasteur (1822-1895).

    PubMed

    Oertling, Sarita B; Marlin, Robert O; Goldman, Armond S

    2014-11-01

    In addition to the holdings at Bibliothque Nationale de France and Muse du Pasteur Institut Paris, major parts of la Bibliothque de Louis Pasteur are in four institutions in the United States - Reynolds Historical Library at the University of Alabama at Birmingham, Alabama; Burndy Library on the History of Science and Technology at Huntington Library in San Marino, California; Harry Ransom Humanities Research Center at University of Texas in Austin, Texas; and Truman G Blocker History of Medicine Collections, The Moody Medical Library, University of Texas Medical Branch, Galveston, Texas. The circuitous paths that led each part of la Bibliothque de Louis Pasteur to their present locations were traced and the lives of key individuals in medicine, science and the humanities who obtained these valuable documents were recounted. The documents in each institution were discussed and a plan was considered to make them accessible to scholars who wish to further explore the life of Louis Pasteur. PMID:24585594

  11. The Upper Neoproterozoic glacial complex in central areas of the Siberian platform

    NASA Astrophysics Data System (ADS)

    Kochnev, B. B.; Pokrovskii, B. G.; Proshenkin, A. I.

    2015-10-01

    A stratum of glacial diamictites with thickness of up to 160 m at the basement of the sedimentary cover, overlain by a series of cap carbonates up to 40 m thick is described for several boreholes in the central regions of the Siberian platform. The isotope composition of carbon in carbonates is identical to the Ediacaran cap carbonates from the Patom upland. The series of detrital zircons from diamictites (60 grains) contains three young grains aged 740-690 Ma, which restricts the time of formation of the glacial deposits to the late Neoproterozoic. Thus, the glaciations that were synchronous to the Stert and/or Marino glacial stages on the Siberian platform had a cap character.

  12. Exact slope and interpolating functions in N=6 supersymmetric Chern-Simons theory.

    PubMed

    Gromov, Nikolay; Sizov, Grigory

    2014-09-19

    Using the quantum spectral curve approach we compute, exactly, an observable (called slope function) in the planar Aharony-Bergman-Jafferis-Maldacena theory in terms of an unknown interpolating function h(?) which plays the role of the coupling in any integrability based calculation in this theory. We verified our results with known weak coupling expansion in the gauge theory and with the results of semiclassical string calculations. Quite surprisingly at strong coupling the result is given by an explicit rational function of h(?) to all orders. By comparing the structure of our result with that of an exact localization based calculation for a similar observable in Marino and Putrov [J. High Energy Phys. 06 (2010) 011], we conjecture an exact expression for h(?). PMID:25279619

  13. Survival and movements of Magellanic penguins rehabilitated from oil fouling along the coast of South America, 2000-2010.

    PubMed

    Ruoppolo, Valeria; Vanstreels, Ralph Eric Thijl; Woehler, Eric J; Heredia, Sergio Andres Rodrguez; Adornes, Andra Corrado; da Silva-Filho, Rodolfo Pinho; Matus, Ricardo; Poleschi, Carla; Griot, Karen; Kolesnikovas, Cristiane K Miyaji; Serafini, Patrcia

    2012-07-01

    Oil pollution is a significant conservation concern. We examined data from six institutions along the coast of South America: Emergency Relief Team of the International Fund for Animal Welfare, Fundacin Mundo Marino, Centro de Recuperao de Animais Marinhos, Natura Patagonia, Associao R3 Animal, and Mar del Plata Aquarium and data from resightings in Argentina, Brazil, Chile and Falkland/Malvinas Islands. From 2000 to 2010, 2183 oiled Magellanic penguins were rehabilitated as part of the routine activities of these institutions or during emergency responses to eight oil spills in which they were involved; all rehabilitated penguins were flipper banded and released. Since their release, 41 penguins were resighted until 31 December 2011. The results demonstrate that, when combined with other prevention strategies, the rehabilitation of Magellanic penguins is a strategy that contributes to the mitigation of adverse effects of oil spills and chronic pollution to the species. PMID:22683106

  14. Biosphere 2 anew

    NASA Astrophysics Data System (ADS)

    The seven scientists who volunteered to live in Biosphere 2 for the past 6.5 months will be reentering the real world this Saturday, September 17, as Biosphere's new management team shifts into high gear to revitalize the $150 million sealed ecosystem's science plan. The new management team stepped in April 1 after a court order obtained by the project's owner Ed Bass kicked out its then prevailing management team. In mid-August, Biosphere 2 announced that it had joined forces with Columbia University's Lamont-Doherty Earth Observatory in a nonprofit venture to set a new research agenda for the reportedly troubled 3.2-acre facility. Biosphere has commissioned about a dozen white papers to be written during the next 7 months to help articulate the optimum science program. The past really isn't the issue, says biogeochemist Bruno Marino, Biosphere's new research director.

  15. Peer review of RELAP5/MOD3 documentation

    SciTech Connect

    Craddick, W.G.

    1993-12-31

    A peer review was performed on a portion of the documentation of the RELAP5/MOD3 computer code. The review was performed in two phases. The first phase was a review of Volume 3, Developmental Assessment problems, and Volume 4, Models and Correlations. The reviewers for this phase were Dr. Peter Griffith, Dr. Yassin Hassan, Dr. Gerald S. Lellouche, Dr. Marino di Marzo and Mr. Mark Wendel. The reviewers recommended a number of improvements, including using a frozen version of the code for assessment guided by a validation plan, better justification for flow regime maps and extension of models beyond their data base. The second phase was a review of Volume 6, Quality Assurance of Numerical Techniques in RELAP5/MOD3. The reviewers for the second phase were Mr. Mark Wendel and Dr. Paul T. Williams. Recommendations included correction of numerous grammatical and typographical errors and better justification for the use of Lax`s Equivalence Theorem.

  16. Assessing ecological correlates of marine bird declines to inform marine conservation

    PubMed Central

    Vilchis, L Ignacio; Johnson, Christine K; Evenson, Joseph R; Pearson, Scott F; Barry, Karen L; Davidson, Peter; Raphael, Martin G; Gaydos, Joseph K

    2015-01-01

    Identifying drivers of ecosystem change in large marine ecosystems is central for their effective management and conservation. This is a sizable challenge, particularly in ecosystems transcending international borders, where monitoring and conservation of long-range migratory species and their habitats are logistically and financially problematic. Here, using tools borrowed from epidemiology, we elucidated common drivers underlying species declines within a marine ecosystem, much in the way epidemiological analyses evaluate risk factors for negative health outcomes to better inform decisions. Thus, we identified ecological traits and dietary specializations associated with species declines in a community of marine predators that could be reflective of ecosystem change. To do so, we integrated count data from winter surveys collected in long-term marine bird monitoring programs conducted throughout the Salish Sea—a transboundary large marine ecosystem in North America's Pacific Northwest. We found that decadal declines in winter counts were most prevalent among pursuit divers such as alcids (Alcidae) and grebes (Podicipedidae) that have specialized diets based on forage fish, and that wide-ranging species without local breeding colonies were more prone to these declines. Although a combination of factors is most likely driving declines of diving forage fish specialists, we propose that changes in the availability of low-trophic prey may be forcing wintering range shifts of diving birds in the Salish Sea. Such a synthesis of long-term trends in a marine predator community not only provides unique insights into the types of species that are at risk of extirpation and why, but may also inform proactive conservation measures to counteract threats—information that is paramount for species-specific and ecosystem-wide conservation. Evaluación de las Correlaciones Ecológicas de las Declinaciones de Aves Marinas para Informar a la Conservación Marina Resumen La identificación de los conductores del cambio ambiental en los grandes ecosistemas marinos es esencial para su conservación y manejo efectivo. Esto es un reto bastante grande, particularmente en los ecosistemas que trascienden fronteras internacionales, cuando el monitoreo y la conservación de especies migratorias de amplio rango y sus hábitats son logística y financieramente problemáticos. En este caso, usando herramientas tomadas de la epidemiología, elucidamos conductores comunes subyacentes en la declinación de especies dentro de un ecosistema marino, muy similar a cómo los análisis epidemiológicos evalúan los factores de riesgo para los resultados de salud negativos e informar mejor sus decisiones. Con esto, identificamos los rasgos ecológicos y las especializaciones de dieta asociados con la declinación de especies en una comunidad de depredadores marinos que podría ser un reflejo de cambios ambientales. Para lograr esto, integramos datos de conteo de programas de censos de invierno recolectados a lo largo de monitoreos a largo plazo de aves marinas llevados a cabo en el mar Salish – un gran ecosistema marino que trasciende fronteras en el noroeste del Océano Pacífico. Encontramos que las declinaciones por década en los conteos de invierno fueron más prevalentes entre los pescadores de persecución, como los álcidos (Alcidae) y los zambullidores (Podicipedidae), que tienen dietas especializadas basadas en peces forrajeros y que las especies con distribución amplia y sin colonias reproductivas locales estaban más predispuestas a estas declinaciones. Mientras que una combinación de factores posiblemente esté causando las declinaciones de especialistas de peces forrajeros, proponemos que los cambios en la disponibilidad de presas de niveles tróficos bajos pueden estar forzando cambios en la extensión invernal de aves pescadoras en el mar Salish. Dicha síntesis de tendencias a largo plazo en una comunidad de depredadores marinos no sólo proporciona percepciones únicas de este tipo de especies que están en riesgo de ser extirpadas y el por qué de esto, sino también puede informar a las medidas de conservación proactivas para contrarrestar amenazas – información que es primordial para la conservación específica de especies y del ecosistema en su totalidad. PMID:25195954

  17. Carbohydrates as indicators of biogeochemical processes

    NASA Astrophysics Data System (ADS)

    Lazareva, E. V.; Romankevich, E. A.

    2012-05-01

    A method is presented to study the carbohydrate composition of marine objects involved into sedimento- and diagenesis (plankton, particulate matter, benthos, and bottom sediments). The analysis of the carbohydrates is based upon the consecutive separation of their fractions with different solvents (water, alkali, and acid). The ratio of the carbohydrate fractions allows one to evaluate the lability of the carbohydrate complex. It is also usable as an indicator of the biogeochemical processes in the ocean, as well of the genesis and the degree of conversion of organic matter in the bottom sediments and nodules. The similarity in the monosaccharide composition is shown for dissolved organic matter and aqueous and alkaline fractions of seston and particulate matter.

  18. Seventy-One Important Questions for the Conservation of Marine Biodiversity

    PubMed Central

    PARSONS, E C M; FAVARO, BRETT; AGUIRRE, A ALONSO; BAUER, AMY L; BLIGHT, LOUISE K; CIGLIANO, JOHN A; COLEMAN, MELINDA A; CÔTÉ, ISABELLE M; DRAHEIM, MEGAN; FLETCHER, STEPHEN; FOLEY, MELISSA M; JEFFERSON, REBECCA; JONES, MIRANDA C; KELAHER, BRENDAN P; LUNDQUIST, CAROLYN J; MCCARTHY, JULIE-BETH; NELSON, ANNE; PATTERSON, KATHERYN; WALSH, LESLIE; WRIGHT, ANDREW J; SUTHERLAND, WILLIAM J

    2014-01-01

    The ocean provides food, economic activity, and cultural value for a large proportion of humanity. Our knowledge of marine ecosystems lags behind that of terrestrial ecosystems, limiting effective protection of marine resources. We describe the outcome of 2 workshops in 2011 and 2012 to establish a list of important questions, which, if answered, would substantially improve our ability to conserve and manage the world’s marine resources. Participants included individuals from academia, government, and nongovernment organizations with broad experience across disciplines, marine ecosystems, and countries that vary in levels of development. Contributors from the fields of science, conservation, industry, and government submitted questions to our workshops, which we distilled into a list of priority research questions. Through this process, we identified 71 key questions. We grouped these into 8 subject categories, each pertaining to a broad component of marine conservation: fisheries, climate change, other anthropogenic threats, ecosystems, marine citizenship, policy, societal and cultural considerations, and scientific enterprise. Our questions address many issues that are specific to marine conservation, and will serve as a road map to funders and researchers to develop programs that can greatly benefit marine conservation. Setenta y Un Preguntas Importantes para la Conservación de la Biodiversidad Marina Resumen Los océanos proporcionan alimento, actividad económica y valor cultural para una gran porción de la humanidad. Nuestro conocimiento de los ecosistemas marinos está atrasado con respecto al que tenemos de los ecosistemas terrestres, lo que limita la protección efectiva de los recursos naturales. Describimos el resultado de dos talleres en 2011 y 2012 para establecer una lista de preguntas importantes, las cuales al ser respondidas, mejorarían sustancialmente nuestra habilidad de conservar y manejar los recursos marinos del mundo. Entre los participantes se incluyeron a individuos de la docencia, el gobierno y organizaciones no-gubernamentales, con una amplia experiencia que atraviesa disciplinas, ecosistemas marinos y países que varían en el nivel de desarrollo. Los contribuyentes de los campos de la ciencia, la conservación, la industria y el gobierno, presentaron preguntas a nuestros talleres, las cuales separamos en una lista de preguntas de investigación prioritarias. Por medio de este proceso, identificamos 71 preguntas clave. Las agrupamos en ocho categorías temáticas, cada una perteneciente a un componente amplio de la conservación marina: pesquerías, cambio climático, otras amenazas antropogénicas, ecosistemas, ciudadanía marina, política, consideraciones sociales y culturales, y la iniciativa científica. Nuestras preguntas se dirigen a muchas cuestiones que son específicas de la conservación marina, y servirán como una ruta a seguir para patrocinadores e investigadores que busquen desarrollar programas que puedan beneficiar ampliamente a la conservación marina. PMID:24779474

  19. Tracing the evolution within nearby galaxy groups: a multi-wavelength approach

    NASA Astrophysics Data System (ADS)

    Bettoni, Daniela; Marino, Antonina; Rampazzo, Roberto; Plana, Henri; Rosado, Margarita; Galletta, Giuseppe; Mazzei, Paola; Bianchi, Luciana; Buson, Lucio M.; Ambrocio-Cruz, Patricia; Gabbasov, Ruslan

    2015-03-01

    Evolutionary scenarios suggest that several mechanisms (from inner secular evolution to accretion/merging) may transform galaxy members, driving groups from an active star forming phase to a more passive, typical of dense environments. We are investigating this transition in a nearby group sample, designed to cover a wide range of properties (see also Marino et al. (2010), Bettoni et al. (2011) and Marino et al. (2012)). We study two groups, USGC U268 and USGC U376 located in different regions of the Leo cloud, through a photometric and kinematic characterization of their member galaxies. We revisit the group membership, using results from recent red-shift surveys, and we investigate their substructures. U268, composed of 10 catalogued members and 11 new added members, has a small fraction (~24%) of early-type galaxies (ETGs). U376 has 16 plus 8 new added members, with ~38% of ETGs. We find the significant substructuring in both groups suggesting that they are likely accreting galaxies. U268 is located in a more loose environment than U376. For each member galaxy, broad band integrated and surface photometry have been obtained in far-UV (FUV) and near-UV (NUV) with GALEX, and in u, g, r, i, z (SDSS) bands. H? imaging and 2D high resolution kinematical data have been obtained using PUMA Scanning Fabry-Perot interferometer at the 2.12 m telescope in San Pedro Mrtir (Baja California, Mxico). We improved the galaxy classification and we detected morphological and kinematical distortions that may be connected to either on-going and/or past interaction/accretion events or environmental induced secular evolution. U268 appears more active than U376, with a large fraction of galaxies showing interaction signatures (60% vs. 13%). The presence of bars among late-type galaxies is ~10% in U268 and 29% in U376. The cumulative distribution of (FUV - NUV) colors of galaxies in U268 is significantly different (bluer) than that of U376's galaxies. Most (80%) of the early-type members in U376 inhabits the red sequence, a large fraction of galaxies, of different morphological types, are located in the green valley, while the blue sequence is under-populated with respect to U268.

  20. Characterization of a Bacillus thuringiensis strain collection isolated from diverse Costa Rican natural ecosystems.

    PubMed

    Arrieta, Glen; Espinoza, Ana M

    2006-03-01

    Costa Rican natural ecosystems are among the most diverse in the world. For this reason, we isolated strains of the entomopathogenic bacteria Bacillus thuringiensis (Bt) to determine their diversity, distribution and abundance. A total of 146 Bt strains were obtained from environmental samples collected from diverse natural ecosystems and life zones of Costa Rica. We recovered Bt strains from 71%, 63%, 61% and 54% of soil samples, fresh leaves, other substrates and leaf litter respectively. Bt was isolated in 65% of the samples collected in the humid tropical forest in national parks (Braulio Carrillo, Gandoca Manzanillo, Sierpe, Hitoy Cerere, and Cahuita), and in 59% of the samples collected in the dry tropical forest (Parque Nacional Marino las Baulas, Palo Verde and Santa Rosa). In the very humid tropical forest (Tortuguero) Bt was isolated in 75% of the samples and in the very humid tropical forest transition perhumid (Carara) it was found in 69% of the samples. The strains exhibit a diverse number, size and morphology of parasporal inclusion bodies: irregular (47%), oval (20%), bipyramidal (3%), bipyramidal and cubic (1%), bipyramidal, oval and irregular (5%) and bipyramidal, oval and cubic crystals (2%). Strains isolated from Braulio Carrillo, Tortuguero and Cahuita, presented predominantly irregular crystals. On the other hand, more than 60% of the isolates from Trraba-Sierpe and Hitoy-Cerere had medium oval crystals. Strains from Gandoca-Manzanillo, Palo Verde and Carara presented mainly combinations of oval and irregular crystals. Nevertheless, the greatest diversity in crystal morphology was observed in those from Santa Rosa, Llanos del Rio Medio Queso and Parque Marino las Baulas. Protein analyses of the crystal-spore preparations showed delta-endotoxin with diverse electrophoretic patterns, with molecular weights in the range of 20 to 160 kDa. Fifty six percent of the strains amplified with the cry2 primer, 54% with vip3, 20% with cry1, 9% with cry3-cry7 and 8% with cry8. The cry11 and cyt genes were found in 8% and 7% of the strains, respectively. When analyzed with specific primers for the cryl subfamily, 13 different genetic profiles were obtained. In addition, twenty-four strains did not amplify with any of the primers used, suggesting they contain novel cry genes. The diversity of Bt genes found in this collection indicates it could have great potential for the control of different species of insect pests. The toxicological characterization of the strains by bioassays against important insect pests will provide useful information about their potential use for the formulation of biological insecticides and their respective cry and vip genes for the transformation of crops to confer resistance to insects. PMID:18457170

  1. In vitro susceptibility testing of Mycobacterium tuberculosis complex strains isolated from seals to antituberculosis drugs.

    PubMed

    Bernardelli, Amelia; Morcillo, Nora; Loureiro, Julio; Quse, Viviana; Davenport, Silvana

    2004-06-01

    Mycobacteria strains belonging to the Mycobacterium tuberculosis complex were isolated from seals found in the South Atlantic. The animals were received in Mundo Marino installations and treated for Mycobacterium tuberculosis complex by conventional therapy of intensive care and enriched food supply; however, in all cases treatment failed. Necropsies of all animals revealed extensive lesions compatible with tuberculosis involving lungs, liver, spleen and lymphatic nodes. Classical biochemical methods as well as molecular techniques using the IS6110 probes were performed for mycobacterial identification. Furthermore, the LCx M. tuberculosis assay (Abbott Laboratories) identified all strains as Mycobacterium tuberculosis complex members. The in vitro susceptibility pattern was examined in mycobacterial strains isolated from seven seals and in 3 reference strains--BCG, H37Rv (M. tuberculosis) and AN5 (Mycobacterium bovis)--to 4 medications--isoniazid, rifampin, streptomycin and ethambutol. Minimal inhibitory drug concentrations were determined by the Mycobacterial Growth Indicator Tube (BD Argentina) method and a microdilution and colorimetric assay using 3-(4-5 dimethyltiazol-2)-2,5 diphenyltetrazolium bromide. All the isolates and the reference strains BCG and AN5 were inhibited by MIC values similar to those of H37Rv with good agreement obtained by both techniques. These findings suggest that a therapeutic regimen aimed to seals diagnosed with tuberculosis play an important role in the prevention of tuberculosis transmission from infected animals to humans that are in routine contact with them. PMID:15495576

  2. Cerebellum development and medulloblastoma.

    PubMed

    Roussel, Martine F; Hatten, Mary E

    2011-01-01

    In the last 20 years, it has become clear that developmental genes and their regulators, noncoding RNAs including microRNAs and long-noncoding RNAs, within signaling pathways play a critical role in the pathogenesis of cancer. Many of these pathways were first identified in genetic screens in Drosophila and other lower organisms. Mammalian orthologs were subsequently identified and genes within the pathways cloned and found to regulate cell growth. Genes and pathways expressed during embryonic development, including the Notch, Wnt/?-Catenin, TGF-?/BMP, Shh/Patched, and Hippo pathways are mutated, lost, or aberrantly regulated in a wide variety of human cancers, including skin, breast, blood, and brain cancers, including medulloblastoma. These biochemical pathways affect cell fate determination, axis formation, and patterning during development and regulate tissue homeostasis and regeneration in adults. Medulloblastoma, the most common malignant nervous system tumor in childhood, are thought to arise from disruptions in cerebellar development [reviewed by Marino, S. (2005)]. Defining the extracellular cues and intracellular signaling pathways that control cerebellar neurogenesis, especially granule cell progenitor (GCP) proliferation and differentiation has been useful for developing models to unravel the mechanisms underlying medulloblastoma formation and growth. In this chapter, we will review the development of the cerebellar cortex, highlighting signaling pathways of potential relevance to tumorigenesis. PMID:21295689

  3. Population Models for Massive Globular Clusters

    NASA Astrophysics Data System (ADS)

    Lee, Young-Wook; Joo, Seok-Joo; Han, Sang-Il; Na, Chongsam; Lim, Dongwook; Roh, Dong-Goo

    2015-03-01

    Increasing number of massive globular clusters (GCs) in the Milky Way are now turned out to host multiple stellar populations having different heavy element abundances enriched by supernovae. Recent observations have further shown that [CNO/Fe] is also enhanced in metal-rich subpopulations in most of these GCs, including ω Cen and M22 (Marino et al. 2011, 2012). In order to reflect this in our population modeling, we have expanded the parameter space of Y 2 isochrones and horizontal-branch (HB) evolutionary tracks to include the cases of normal and enhanced nitrogen abundances ([N/Fe] = 0.0, 0.8, and 1.6). The observed variations in the total CNO content were reproduced by interpolating these nitrogen enhanced stellar models. Our test simulations with varying N and O abundances show that, once the total CNO sum ([CNO/Fe]) is held constant, both N and O have almost identical effects on the HR diagram (see Fig. 1).

  4. The leatherback turtle, Dermochelys coriacea, exhibits both polyandry and polygyny.

    PubMed

    Crim, J L; Spotila, L D; Spotila, J R; O'Connor, M; Reina, R; Williams, C J; Paladino, F V

    2002-10-01

    The leatherback turtle (Dermochelys coriacea) is an endangered species, and world-wide populations are declining. To understand better the mating structure of this pelagic and fragile species, we investigated paternity in nearly 1000 hatchlings from Playa Grande in Parque Marino Nacional Las Baulas, Costa Rica. We collected DNA samples from 36 adult female leatherbacks and assessed allele frequency distributions for three microsatellite loci. For 20 of these 36 females, we examined DNA from hatchlings representing multiple clutches, and in some cases assessed up to four successive clutches from the same female. We inferred paternal alleles by comparing maternal and hatchling genotypes. We could not reject the null hypothesis of single paternity in 12 of 20 families (31 of 50 clutches), but we did reject the null hypothesis in two families (eight of 50 clutches). In the remaining six families, the null hypothesis could not be accepted or rejected with certainty because the number of hatchlings exhibiting extra nonmaternal alleles was small, and could thus be a result of mutation or sample error. Successive clutches laid by the same female had the same paternal allelic contribution, indicating sperm storage or possibly monogamy. None of 20 females shared the same three-locus genotype whereas there were two instances of shared genotypes among 17 inferred paternal three-locus genotypes. We conclude that both polyandry and polygyny are part of the mating structure of this leatherback sea turtle population. PMID:12296951

  5. The Telescope: Outline of a Poetic History

    NASA Astrophysics Data System (ADS)

    Stocchi, M. P.

    2011-06-01

    Amongst the first editions of Galileo's books, only the Saggiatore has on its frontispiece the image of the telescope. Indeed, the telescope is not pictured on the very emphatic frontispieces of the other books in which Galileo was presenting and defending the results achieved by his celestial observations, such as the Sidereus Nuncius. Many contemporary scientists denied the reliability of the telescope, and some even refused to look into the eyepiece. In the 16th and 17th century, the lenses, mirrors, and optical devices of extraordinary complexity did not have the main task of leading to the objective truth but obtaining the deformation of the reality by means of amazing effects of illusion. The Baroque art and literature had the aim of surprising, and the artists gave an enthusiastic support to the telescope. The poems in praise of Galileo's telescopic findings were quite numerous, including Adone composed by Giovanni Battista Marino, one of the most renowned poets of the time. The Galilean discoveries were actually accepted by the poets as ideologically neutral contributions to the "wonder" in spite they were rejected or even condemned by the scientists, philosophers, and theologians.

  6. Impact of cross-polarization isolation on polarimetric target decomposition and target detection

    NASA Astrophysics Data System (ADS)

    Xu, Feng; Wang, Haipeng; Jin, Ya-Qiu; Liu, Xiuqing; Wang, Robert; Deng, Yunkai

    2015-04-01

    Cross-polarization isolation is one of the key engineering parameters for a polarimetric radar system. Previous studies focused more on the calibration of cross-talk contamination. This paper presents a numerical evaluation of the requirement for cross-polarization isolation from the data users' perspective, i.e., the quantitative impact of polarization cross talk on polarimetric target decomposition and the associated applications such as classification and detection. Sensitivity analyses of several commonly used target decomposition parameters suggest that a theoretical lower bound of -32 dB isolation level is preferred to avoid any significant impact on these parameters. Our analyses with both simulated and real synthetic aperture radar (SAR) data show that a level of -25 dB would be acceptable for general terrain surface classification. This requirement is also true for man-made target detection application. Using simulated SAR images of man-made targets in natural environment, sensitivity analyses on two polarimetric detectors, Yang and Marino, both suggest that target detection performance would break down rapidly if isolation deteriorates from -25 dB to -20 dB.

  7. Feasibility study of a layer-oriented wavefront sensor for solar telescopes: comment.

    PubMed

    Kellerer, Agla

    2014-11-10

    The future generation of telescopes will be equipped with multi-conjugate adaptive-optics (MCAO) systems in order to obtain high angular resolution over large fields of view. MCAO comes in two flavors: star- and layer-oriented. Existing solar MCAO systems rely exclusively on the star-oriented approach. Earlier we suggested a method to implement the layer-oriented approach, and in view of recent concerns by Marino and Wger [Appl. Opt.53, 685 (2014)10.1364/AO.53.000685APOPAI1559-128X], we now explain the proposed scheme in further detail. We note that in any layer-oriented system one sensor is conjugated to the pupil and the others are conjugated to higher altitudes. For the latter, not all the sensing surface is illuminated by the entire field of view. The successful implementation of nighttime layer-oriented systems shows that the field reduction is no crucial limitation. In the solar approach the field reduction is directly noticeable because it causes vignetting of the Shack-Hartmann subaperture images. It can be accounted for by a suitable adjustment of the algorithms to calculate the local wavefront slopes. We discuss a further concern related to the optical layout of a layer-oriented solar system. PMID:25402984

  8. An oceanographic context for the foraging ecology of eastern Pacific leatherback turtles: Consequences of ENSO

    NASA Astrophysics Data System (ADS)

    Saba, Vincent S.; Shillinger, George L.; Swithenbank, Alan M.; Block, Barbara A.; Spotila, James R.; Musick, John A.; Paladino, Frank V.

    2008-05-01

    We analyzed some of the primary biological and physical dynamics within the eastern Pacific leatherback turtle ( Dermochelys coriacea) migration area in relation to ENSO and leatherback nesting ecology at Parque Nacional Marino Las Baulas (PNMB), Costa Rica. We used data from remote sensing to calculate resource availability via a net primary production (NPP) model, and to analyze the physical dynamics of the migration area via sea surface temperature fronts. Within the migration area, NPP north of 15°S was highly governed by interannual variability as indicated by the Multivariate ENSO Index while south of 15°S, production had a more seasonal signal. Nesting peaks of leatherbacks at PNMB were associated with cool, highly productive La Niña events and with large-scale equatorial phytoplankton blooms encompassing 110°W that were induced by iron enrichment following the termination of El Niño events. Resource availability in the northern migration area (eastern equatorial Pacific) appeared to determine the nesting response for the population at PNMB, Costa Rica. We suggest that ENSO significantly influences the nesting ecology of leatherbacks at PNMB because the majority of the population consists of pelagic foragers that strictly rely on the eastern equatorial Pacific for prey consumption prior to the nesting season. Coastal foragers may be a minority in the population because of high mortality rates associated with coastal gillnet fisheries along Central and South America.

  9. Cerebellum: Development and Medulloblastoma

    PubMed Central

    Roussel, Martine F.; Hatten, Mary E.

    2011-01-01

    In the last 20 years, it has become clear that developmental genes and their regulators, noncoding RNAs including microRNAs and long-noncoding RNAs, within signaling pathways play a critical role in the pathogenesis of cancer. Many of these pathways were first identified in genetic screens in Drosophila and other lower organisms. Mammalian orthologs were subsequently identified and genes within the pathways cloned and found to regulate cell growth. The GENES and pathways expressed during embryonic development, including the Notch, Wnt/β-Catenin, TGF-β/BMP, Shh/Patched, and Hippo pathways are mutated, lost, or aberrantly regulated in a wide variety of human cancers, including skin, breast, blood, and brain cancers, including medulloblastoma. These biochemical pathways affect cell fate determination, axis formation, and patterning during development and regulate tissue homeostasis and regeneration in adults. Medulloblastoma, the most common malignant nervous system tumor in childhood, are thought to arise from disruptions in cerebellar development [reviewed by Marino, S. (2005). Medulloblastoma: Developmental mechanisms out of control. Trends Mol. Med. 11, 17–22]. Defining the extracellular cues and intracellular signaling pathways that control cerebellar neurogenesis, especially granule cell progenitor (GCP) proliferation and differentiation has been useful for developing models to unravel the mechanisms underlying medulloblastoma formation and growth. In this chapter, we will review the development of the cerebellar cortex, highlighting signaling pathways of potential relevance to tumorigenesis. PMID:21295689

  10. The western coast of Africa in Ptolemy's Geography and the location of his prime meridian

    NASA Astrophysics Data System (ADS)

    Marx, Christian

    2016-03-01

    A controversial question concerning ancient geography is the location of the prime meridian which underlies the position data in Ptolemy's Geography and runs through the Fortunate Islands. An answer to this question is derived by means of a localisation of the places given by Ptolemy at the African western coast, i.e. in Mauritania Tingitana and Libya Interior, whose modern identifications are often uncertain or unknown. The origination of Ptolemy's positions from the distance data of seafarings is considered. A comparison of his data with distances reported by Pliny yields a satisfactory agreement. The localisation of Ptolemy's places is based on distances derived from Ptolemy's coordinates and partly on further information by ancient authors. Through it previous identifications are confirmed and new identifications are found. It shows that the Fortunate Islands correspond to several eastern islands of the Canary Islands. Explanations are given for the errors of Ptolemy's position data. A likely error by Ptolemy barely considered is his repetition of a part of Mauritania Tingitana in his description of Libya Interior. The existence of this repetition is confirmed by an adjustment of a transformation between the positions of the duplicated places and a statistical test of the arranged model. A comparison of longitudinal distances in different ancient sources reveals that the position of Ptolemy's prime meridian is based on distances given by Marinos and Eratosthenes.

  11. The bottom quartile for health indices in America vs Europe.

    PubMed

    Shandera, Wayne Xavier

    2014-01-01

    The inequities in health outcomes in different parts of the developed world merit further analysis. An index comprising mortality and morbidity factors was composed for American states and European nations. Multiple factors and bottom quartile status were analyzed by regression methodology. The 51 American states (and District of Columbia) showed a "Health Index" value based on life expectancy at birth and morbidity determined by rates of cardiac disease and cancer that ranged from 63 (Mississippi and West Virginia) to 94 (Utah). The 48 of 51 European states with assessable data showed a Health Index based on life expectancy at birth and quality adjusted life years that ranged from 53 (Russia) to 98 (San Marino). American states with the lowest quartile values were clustered in the American South and Appalachian areas. European states ranking in the bottom quartile were typically from Eastern Europe and showed a history of a Communism and recognized governmental corruption. Because American poor health rankings are the result of controllable factors (smoking, adult onset diabetes, obesity), Americans can improve their bottom quartile status more readily than Europeans whose ranking status is a function of history (Communism, civil conflicts) and poverty (Southeastern and Eastern nations). PMID:25037885

  12. Effects of the 1991-92 El Nio on scleractinian corals of the Costa Rican central Pacific coast.

    PubMed

    Jimnez, C; Corts, J

    2001-12-01

    Coral communities on the central Pacific coast of Costa Rica were affected during the 1991-92 El Nio warming event. More than 57% of all observed colonies at three localities (Parque Nacional Manuel Antonio, Punta Cambutal, and Parque Marino Ballena) were bleached. Mortality during this El Nio was much lower (approximately 9%) than in previous events. Psammocora spp. accounted for approximately 66% of dead corals, while massive (Porites lobota, Pavona spp.) and branching (Pocillopora spp.) for approximately 34%. Our results suggest that the observed bleaching in P. lobata was related to zooxanthellar densities and not to changes in pigment concentrations: only chlorophyll a varied between normally pigmented and bleached colonies at one locality (Ballena). Site differences in zooxanthellar densities or their pigment concentrations, may not be the result of the bleaching event itself, because a percentage of dead corals and zooxanthellar densities of bleached colonies seems to follow a trend with the exposure to tidal regimes and currents at each site. Local oceanographic conditions can be influencing the zooxanthellar densities and their response to the warming, together with intrinsic differences between colonies as well. The impact of this event can be considered serious given the short period of time that elapsed between El Nio related mortalities and the slow reefs recovery, the mode of reproduction of reef building species, and the anthropogenic-originated disturbances which affect the coral communities and reefs of the Costa Rican central Pacific coast. PMID:15264538

  13. Compression-triggered instabilities of multi-layer systems: From thin elastic membranes to lipid bilayers on flexible substrates

    NASA Astrophysics Data System (ADS)

    Stone, Howard A.

    2013-03-01

    Instabilities are triggered when elastic materials are subjected to compression. We explore new features of two distinct systems of this type. First, we describe a two-layer polymeric system under biaxial compressive stress, which exhibits a repetitive wrinkle-to-fold transition that subsequently generates a hierarchical network of folds during reorganization of the stress field. The folds delineate individual domains, and each domain subdivides into smaller ones over multiple generations. By modifying the boundary conditions and geometry, we demonstrate control over the final network morphology. Some analogies to the venation pattern of leaves are indicated. Second, motivated by the confined configurations common to cells, which are wrapped in lipid bilayer membranes, we study a lipid bilayer, coupled to an elastic sheet, and demonstrate that, upon straining, the confined lipid membrane is able to passively regulate its area. In particular, by stretching the elastic support, the bilayer laterally expands without rupture by fusing adhered lipid vesicles; upon compression, lipid tubes grow out of the membrane plane, thus reducing its area. These transformations are reversible, as we show using cycles of expansion and compression, and closely reproduce membrane processes found in cells during area regulation. The two distinct systems illustrate the influence of the substrate on finite amplitude shape changes, for which we describe the time-dependent shape evolution as the stress relaxes. This talk describes joint research with Manouk Abkarian, Marino Arroyo, Pilnam Kim, Mohammad Rahimi and Margarita Staykova.

  14. Relationships between petrophysical, sedimentological and microstructural properties of the Oolithes Blanche formation, a saline aquifer in the Paris Basin.

    NASA Astrophysics Data System (ADS)

    Casteleyn, Lisa; Robion, Philippe; Collin, Pierry-Yves; Menndez, Beatriz; David, Christian; Fernandes, Nathalie; Desaubliaux, Guy; Dreux, Rmi; Rigollet, Christophe; Badinier, Guillaume

    2010-05-01

    The Paris Basin appears to be appropriate in terms of CO2 capture and storage when considering both the amount of CO2 produced and the availability of depleted fields and deep saline aquifers. The purpose of this study is to investigate the petrophysical properties in relation with the sedimento-diagenetic environment of the "Oolithe Blanche" formation (Dogger), a deep saline aquifer considered as a potential candidate for CO2 storage. Regarding the scarcity of the core data in the Paris Basin, our investigation was firstly based on the study of field analogs in the south-east of the Paris Basin. The Oolithe Blanche Formation is composed of very shallow marine oolitic and bioclastic limestones, mainly grainstones. Three main sedimentological fabrics were defined: tide-dominated, wave-dominated (oolitic shoal) and prograding oolitic shoal fabrics. These three fabrics show subtle variations in composition (ooliths vs bioclasts) and in the distribution of the carbonate textures. The Oolithe Blanche Formation (Bathonian) is 70-80 meters thick and water salinity ranges from 1 to 4 g NaCl/l. 18 oriented blocks were collected on outcrops selected for the different sedimentological facies recognised in the formation: 9 blocks in the Bierry Ls Belles Fontaines quarry (Yonne), 5 blocks in the Ravires quarries (Cte d'Or) and 4 blocks in the Massangis quarry (Yonne). On each block, several petrophysical properties were measured on three perpendicular plugs: porosity, pore size distribution derived from mercury injection tests, permeability, capillary imbibition parameters, electrical conductivity and acoustic velocities. The sedimento-diagenetic fabric and microstructural analysis was defined by using optical microscope and scanning electron microscopy, coupled with image analysis on thin sections. The porosity measured using the water saturation triple weight method ranges from 6% to 34%. The permeability values are low, between 0.1 mD and 9 mD. The data from the mercury intrusion porosimetry show that the distribution of the pore-throat diameter is either unimodal (microporosity only) or bimodal (macro- and microporosity). The microporosity is intraparticles (intraoolitic) and macroporosity is interparticles and is related to processes of dolo-dedolomitization. Variations of the capillary imbibition parameters acoustic velocities and electric conductivity can be explained by the microstructure. So, our investigations show a relationship between the sedimento-diagenetic fabrics and the petrophysical fabrics. The variation of reservoir properties are mainly controlled by two microstructural characters : the cement (type, quantity and distribution) and the microporosity distribution inside the oolithe grains. Now, these latter results calibrated by studying field analogs must be extended to bore-hole data and core data to optimize our knowledge of the deep saline aquifer of the Oolithe Blanche. Without these investigations, it will be impossible to estimate the good or poor quality of this deep saline aquifer with respect to CO2 storage.

  15. Resposta do detector de ondas gravitacionais Mario Schenberg ao "ringdown" de buraco negros

    NASA Astrophysics Data System (ADS)

    Costa, C. A.; Aguiar, O. D.; Magalhes, N. S.

    2003-08-01

    Acredita-se que quando duas estrelas de nutrons coalescem, elas, eventualmente, formam um buraco negro com massa igual a soma das massas dos objetos originais. Durante a formao do buraco negro, o espao-tempo em torno do sistema sofre perturbaes que se propagam na forma de radiao gravitacional. A forma de onda associada a radiao gravitacional, durante este estgio, aproxima-se a uma senide exponencialmente amortecida. Este tipo de sinal conhecido como "ringdown", e seu comportamento e parametrizao so muito bem conhecidos. Neste trabalho, simulamos computacionalmente sinais provenientes do "ringdown" de buracos negros, com a finalidade de testar o desempenho do detector de ondas gravitacionais Mario Schenberg em observ-los, quando entrar em funcionamento. Este primeiro teste terico ajudou-nos a criar estratgias de deteco de sinais imersos no rudo instrumental. Calculamos a relao sinal-rudo como uma funo da frequncia, bem como sua integral dentro da faixa de sensibilidade do detector. Os resultados obtidos mostraram que o detector Schenberg ter sensibilidade suficiente para detectar este tipo de sinal, proveniente de fontes astrofsicas localizadas dentro de um raio de ~100kpc.

  16. Vigilando la Calidad del Agua de los Grandes Rios de la Nacion: El Programa NASQAN del Rio Grande (Rio Bravo del Norte)

    USGS Publications Warehouse

    Lurry, Dee L.; Reutter, David C.; Wells, Frank C.; Rivera, M.C., (translator); Munoz, A.

    1998-01-01

    La Oficina del Estudio Geologico de los Estados Unidos (U.S. Geological Survey, 0 USGS) ha monitoreado la calidad del agua de la cuenca del Rio Grande (Rio Bravo del Norte) desde 1995 como parte de la rediseiiada Red Nacional para Contabilizar la Calidad del Agua de los Rios (National Stream Quality Accounting Network, o NASOAN) (Hooper and others, 1997). EI programa NASOAN fue diseiiado para caracterizar las concentraciones y el transporte de sedimento y constituyentes quimicos seleccionados, encontrados en los grandes rios de los Estados Unidos - incluyendo el Misisipi, el Colorado y el Columbia, ademas del Rio Grande. En estas cuatro cuencas, el USGS opera actualmente (1998) una red de 40 puntos de muestreo pertenecientes a NASOAN, con un enfasis en cuantificar el flujo en masa (la cantidad de material que pasa por la estacion, expresado en toneladas por dial para cada constituyente. Aplicacando un enfoque consistente, basado en la cuantificacion de flujos en la cuenca del Rio Grande, el programa NASOAN esta generando la informacion necesaria para identificar fuentes regionales de diversos contaminantes, incluyendo sustancias qui micas agricolas y trazas elementos en la cuenca. EI efecto de las grandes reservas en el Rio Grande se puede observar segun los flujos de constituyentes discurren a 10 largo del rio. EI analisis de los flujos de constituyentes a escala de la cuenca proveera los medios para evaluar la influencia de la actividad humana sobre las condiciones de calidad del agua del Rio Grande.

  17. Causes of sinks near Tucson, Arizona, USA

    NASA Astrophysics Data System (ADS)

    Hoffmann, John P.; Pool, Donald R.; Konieczki, A. D.; Carpenter, Michael C.

    Land subsidence in the form of sinks has occurred on and near farmlands near Tucson, Pima County, Arizona, USA. The sinks occur in alluvial deposits along the flood plain of the Santa Cruz River, and have made farmlands dangerous and unsuitable for farming. More than 1700 sinks are confined to the flood plain of the Santa Cruz River and are grouped along two north-northwestward-trending bands that are approximately parallel to the river and other flood-plain drainages. An estimated 17,000m3 of sediment have been removed in the formation of the sinks. Thirteen trenches were dug to depths of 4-6m to characterize near-surface sediments in sink and nonsink areas. Sediments below about 2m included a large percentage of dispersive clays in sink areas. Sediments in nonsink areas contain a large component of medium- to coarse-grained, moderately to well sorted sand that probably fills a paleochannel. Electromagnetic surveys support the association of silts and clays in sink areas that are highly electrically conductive relative to sand in nonsink areas. Sinks probably are caused by the near-surface process of subsurface erosion of dispersive sediments along pre-existing cracks in predominantly silt and clay sediments. The pre-existing cracks probably result from desiccation or tension that developed during periods of water-table decline and channel incision during the past 100 years or in earlier periods. Résumé Des effondrements en forme d'entonnoir se sont produits sur et près d'exploitations agricoles de Pima (Arizona). Ces entonnoirs apparaissent dans les alluvions le long de la plaine d'inondation de la rivière Santa Cruz ; ils ont rendu ces terrains dangereux et inexploitables pour l'agriculture. Plus de 1700 entonnoirs existent dans la plaine d'inondation de la rivière Santa Cruz et sont groupés en deux bandes orientées nord-nord-ouest, approximativement parallèles à la rivière et aux autres chenaux de la plaine d'inondation. Un volume de sédiments estiméà 17,000m3 a été entraîné lors de la formation de ces entonnoirs. Treize tranchées ont été creusées à des profondeurs de 4 à 6m afin de caractériser les sédiments proches de la surface dans les zones avec et sans entonnoirs. Les sédiments situés à 2m environ sous la surface contiennent un fort pourcentage d'argile dispersée, dans les zones à entonnoirs. Dans les zones sans entonnoirs, la granulométrie des sédiments est constituée en fortes proportions de sables moyens à grossiers, moyennement à bien lités, qui remplissent probablement un ancien chenal. Des levés électromagnétiques montrent que l'association de silts et d'argiles dans les zones à entonnoirs possède une forte conductivitéélectrique, par comparaison avec les sables des zones sans entonnoirs. Les entonnoirs sont dus probablement à des processus, proches de la surface, d'érosion souterraine des sédiments constitués surtout de silts et d'argiles. Les fractures préexistantes résultent sans doute de la dessiccation ou de la tension se produisant lors des périodes d'abaissement de la nappe, liéà l'enfoncement du lit de la rivière au cours des cent dernières années ou même avant.1 Resumen Se ha detectado la formación de dolinas como resultado de la subsidencia que ha tenido lugar en las zonas agrícolas Condado de Pima, Arizona, EEUU. Estos colapsos han aparecido en depósitos aluviales a lo largo de la llanura de inundación del Río Santa Cruz y han hecho que las zonas agrícolas sean peligrosas e inadecuadas para su uso. Las más de 1700 dolinas aparecidas se agrupan a lo largo de dos bandas con dirección nor-noroeste, paralelas al río y a otros ejes de drenaje del llano. Se ha estimado un desplazamiento de 17.000metros cúbicos de sedimentos para formar estas dolinas. Se excavaron trece zanjas de entre 4 y 6metros para caracterizar los sedimentos más superficiales tanto en áreas colapsadas como no colapsadas. Por debajo de los dos metros de profundidad, los sedimentos presentan altos porcentajes de arcillas dispersivas en las zonas de dolinas. En las zonas en que no se han producido colapsos, se aprecian altos contenidos de arena de grano entre mediano y grueso, con una granulometría entre moderada y bastante uniforme, que probablemente rellenan un paleocanal. Las campañas electromagnéticas confirman la asociación entre los materiales arcillosos, eléctricamente conductivos, y la presencia de dolinas, mientras que los materiales arenosos, menos conductivos eléctricamente, se asocian a las zonas no colapsadas. Las dolinas se deben probablemente a procesos de erosión subsuperficial de los sedimentos arcillosos a lo largo de fracturas preexistentes. Estas fracturas se produjeron probablemente como resultado de la desecación del suelo en los periodos de descenso del nivel freático, en los últimos cien años.

  18. Global Analysis of Anthropogenic Debris Ingestion by Sea Turtles

    PubMed Central

    Schuyler, Qamar; Hardesty, Britta Denise; Wilcox, Chris; Townsend, Kathy

    2014-01-01

    Ingestion of marine debris can have lethal and sublethal effects on sea turtles and other wildlife. Although researchers have reported on ingestion of anthropogenic debris by marine turtles and implied incidences of debris ingestion have increased over time, there has not been a global synthesis of the phenomenon since 1985. Thus, we analyzed 37 studies published from 1985 to 2012 that report on data collected from before 1900 through 2011. Specifically, we investigated whether ingestion prevalence has changed over time, what types of debris are most commonly ingested, the geographic distribution of debris ingestion by marine turtles relative to global debris distribution, and which species and life-history stages are most likely to ingest debris. The probability of green (Chelonia mydas) and leatherback turtles (Dermochelys coriacea) ingesting debris increased significantly over time, and plastic was the most commonly ingested debris. Turtles in nearly all regions studied ingest debris, but the probability of ingestion was not related to modeled debris densities. Furthermore, smaller, oceanic-stage turtles were more likely to ingest debris than coastal foragers, whereas carnivorous species were less likely to ingest debris than herbivores or gelatinovores. Our results indicate oceanic leatherback turtles and green turtles are at the greatest risk of both lethal and sublethal effects from ingested marine debris. To reduce this risk, anthropogenic debris must be managed at a global level. Análisis Global de la Ingesta de Residuos Antropogénicos por Tortugas Marinas La ingesta de residuos marinos puede tener efectos letales y subletales sobre las tortugas marinas y otros animales. Aunque hay investigadores que han reportado la ingesta de residuos antropogénicos por tortugas marinas y la incidencia de la ingesta de residuos ha incrementado con el tiempo, no ha habido una síntesis global del fenómeno desde 1985. Por esto analizamos 37 estudios publicados, desde 1985 hasta 2012, que reportan datos colectados desde antes de 1900 y a lo largo del 2011. Investigamos específicamente si el predominio de la ingesta ha cambiado con el tiempo, qué tipos de residuos se ingieren comúnmente, la distribución geográfica de la ingesta de residuos por tortugas marinas en relación a la distribución global de residuos y cuáles especies y etapas de vida tienen más probabilidad de ingerir residuos. La probabilidad de que las tortugas verdes (Chelonia mydas) y laúd (Dermochelys coriacea) ingieran escombros incrementa significativamente con el tiempo; plástico fue el residuo que más se ingirió. Las tortugas en casi todas las regiones estudiadas ingieren residuos, pero la probabilidad de ingesta no estuvo relacionada con las densidades modeladas de residuos. Además de esto, tortugas más pequeñas, en etapa oceánica de vida, tuvieron una mayor probabilidad de ingerir residuos que las tortugas forrajeras terrestres, mientras que las especies carnívoras tuvieron menos probabilidad de ingerir residuos que las herbívoras o las gelatinívoras. Nuestros resultados indican que las tortugas verdes y laúd tienen el mayor riesgo de efectos letales y subletales de la ingesta de residuos marinos. Para reducir el riesgo, los residuos antropogénicos deben manejarse en un nivel global. PMID:23914794

  19. Experimental Constraints on a Dark Matter Origin for the DAMA Annual Modulation Effect

    SciTech Connect

    Aalseth, Craig E.; Barbeau, Phil; Cerdeno, D. G.; Colaresi, J.; Collar, J. I.; de Lurgio, P.; Drake, G.; Fast, James E.; Greenberg, C.; Hossbach, Todd W.; Kephart, Jeremy D.; Marino, Michael G.; Miley, Harry S.; Orrell, John L.; Reyna, D.; Robertson, R. G. H.; Talaga, R. L.; Tench, O.; Van Wechel, T. D.; Wilkerson, J.; Yocum, K. M.

    2008-12-17

    Abstract Follows: C. E. Aalseth,1 P. S. Barbeau,2 D. G. Cerdeo,3 J. Colaresi,4 J. I. Collar,2 P. de Lurgio,5 G. Drake,5 J. E. Fast,1 C. H. Greenberg,2 T. W. Hossbach,1 J. D. Kephart,1 M. G. Marino,7 H. S. Miley,1 J. L. Orrell,1 D. Reyna,6 R. G. H. Robertson,7 R. L. Talaga,5 O. Tench,4 T. D. Van Wechel,7 J. F. Wilkerson,7 and K. M. Yocum4 (CoGeNT Collaboration) 1Pacific Northwest National Laboratory, Richland, Washington 99352, USA 2Kavli Institute for Cosmological Physics and Enrico Fermi Institute, University of Chicago, Chicago, Illinois 60637, USA 3Departamento de Fsica Terica C-XI & Instituto de Fsica Terica UAM-CSIC, Universidad Autnoma de Madrid, Cantoblanco, E-28049 Madrid, Spain 4CANBERRA Industries, Meriden, Connecticut 06450, USA 5Argonne National Laboratory, Argonne, Illinois 60439, USA 6Sandia National Laboratories, Livermore, California 94550, USA 7Center for Experimental Nuclear Physics and Astrophysics, and Department of Physics, University of Washington, Seattle, Washington 98195, USA Received 7 July 2008; revised 6 August 2008; published 17 December 2008 A claim for evidence of dark matter interactions in the DAMA experiment has been recently reinforced. We employ a new type of germanium detector to conclusively rule out a standard isothermal galactic halo of weakly interacting massive particles as the explanation for the annual modulation effect leading to the claim. Bounds are similarly imposed on a suggestion that dark pseudoscalars might lead to the effect. We describe the sensitivity to light dark matter particles achievable with our device, in particular, to next-to-minimal supersymmetric model candidates.

  20. Effects of illegal harvest of eggs on the population decline of leatherback turtles in Las Baulas Marine National Park, Costa Rica.

    PubMed

    Tomillo, Pilar Santidrin; Saba, Vincent S; Piedra, Rotney; Paladino, Frank V; Spotila, James R

    2008-10-01

    Within 19 years the nesting population of leatherback turtles (Dermochelys coriacea) at Parque Nacional Marino Las Baulas declined from 1500 turtles nesting per year to about 100. We analyzed the effects of fishery bycatch and illegal harvesting (poaching) of eggs on this population. We modeled the population response to different levels of egg harvest (90, 75, 50, and 25%) and the effect of eradicating poaching at different times during the population decline. We compared effects of 90% poaching with those of 20% adult mortality because both of these processes were present in the population at Las Baulas. There was a stepwise decline in number of nesting turtles at all levels of egg harvest. Extirpation times for different levels of poaching ranged from 45 to 282 years. The nesting population declined more slowly and survived longer with 20% adult mortality (146 years) than it did with 90% poaching (45 years). Time that elapsed until poaching stopped determined the average population size at which the population stabilized, ranging from 90 to 420 nesting turtles. Our model predicted that saving clutches lost naturally would restore the population when adult mortality rates were low and would contribute more to population recovery when there were short remigration intervals between nesting seasons and a large proportion of natural loss of clutches. Because the model indicated that poaching was the most important cause of the leatherback decline at Las Baulas, protecting nests on the beach and protecting the beach from development are critical for survival of this population. Nevertheless, the model predicted that current high mortality rates of adults will prevent population recovery. Therefore, protection of the beach habitat and nests must be continued and fishery bycatch must be reduced to save this population. PMID:18637915

  1. The game of active search for extra-terrestrial intelligence: breaking the `Great Silence'

    NASA Astrophysics Data System (ADS)

    de Vladar, Harold P.

    2013-01-01

    The search for extra-terrestrial intelligence (SETI) has been performed principally as a one-way survey, listening of radio frequencies across the Milky Way and other galaxies. However, scientists have engaged in an active messaging only rarely. This suggests the simple rationale that if other civilizations exist and take a similar approach to ours, namely listening but not broadcasting, the result is a silent universe. A simple game theoretical model, the prisoner's dilemma, explains this situation: each player (civilization) can passively search (defect), or actively search and broadcast (cooperate). In order to maximize the payoff (or, equivalently, minimize the risks) the best strategy is not to broadcast. In fact, the active search has been opposed on the basis that it might be dangerous to expose ourselves. However, most of these ideas have not been based on objective arguments, and ignore accounting of the possible gains and losses. Thus, the question stands: should we perform an active search? I develop a game-theoretical framework where civilizations can be of different types, and explicitly apply it to a situation where societies are either interested in establishing a two-way communication or belligerent and in urge to exploit ours. The framework gives a quantitative solution (a mixed-strategy), which is how frequent we should perform the active SETI. This frequency is roughly proportional to the inverse of the risk, and can be extremely small. However, given the immense amount of stars being scanned, it supports active SETI. The model is compared with simulations, and the possible actions are evaluated through the San Marino scale, measuring the risks of messaging.

  2. Climate change, marine environments, and the US Endangered species act.

    PubMed

    Seney, Erin E; Rowland, Melanie J; Lowery, Ruth Ann; Griffis, Roger B; McClure, Michelle M

    2013-12-01

    Climate change is expected to be a top driver of global biodiversity loss in the 21st century. It poses new challenges to conserving and managing imperiled species, particularly in marine and estuarine ecosystems. The use of climate-related science in statutorily driven species management, such as under the U.S. Endangered Species Act (ESA), is in its early stages. This article provides an overview of ESA processes, with emphasis on the mandate to the National Marine Fisheries Service (NMFS) to manage listed marine, estuarine, and anadromous species. Although the ESA is specific to the United States, its requirements are broadly relevant to conservation planning. Under the ESA, species, subspecies, and "distinct population segments" may be listed as either endangered or threatened, and taking of most listed species (harassing, harming, pursuing, wounding, killing, or capturing) is prohibited unless specifically authorized via a case-by-case permit process. Government agencies, in addition to avoiding take, must ensure that actions they fund, authorize, or conduct are not likely to jeopardize a listed species' continued existence or adversely affect designated critical habitat. Decisions for which climate change is likely to be a key factor include: determining whether a species should be listed under the ESA, designating critical habitat areas, developing species recovery plans, and predicting whether effects of proposed human activities will be compatible with ESA-listed species' survival and recovery. Scientific analyses that underlie these critical conservation decisions include risk assessment, long-term recovery planning, defining environmental baselines, predicting distribution, and defining appropriate temporal and spatial scales. Although specific guidance is still evolving, it is clear that the unprecedented changes in global ecosystems brought about by climate change necessitate new information and approaches to conservation of imperiled species. El Cambio Climático, los Ecosistemas Marinos y el Acta Estadunidense de Especies en Peligro. PMID:24299080

  3. Polvo en la Regin de los Troyanos

    NASA Astrophysics Data System (ADS)

    Gilhutton, R.; Brunini, A.; Coldwell, G.

    La posible existencia de un anillo de polvo en la resonancia 1:1 con Jpiter formado por partculas provenientes de colisiones de asteroides fue propuesta por Liou and Zook (Icarus 113, 403, 1995) y estudiada extensamente por Vieira Martins and Gomes (VIII Reunin Regional Latinoamericana de Astronoma, Montevideo,1995). Si bien las partculas quedaran atrapadas slo por perodos de algunos miles de aos, el proceso colisional continuo en el cinturn de asteroides mantendra constante la densidad, presentndose una mayor concentracin en la regin de los troyanos. En el presente trabajo se presentan resultados preliminares sobre observaciones polarimtricas realizadas desde CASLEO de la regin de L5 que confirmaran la existencia y variaciones de densidad en el anillo de polvo.

  4. Eventos de Desconexao na Cauda de Plasma do Cometa P/Halley

    NASA Astrophysics Data System (ADS)

    Voelzke, M. R.; Fahr, H. J.

    2001-08-01

    Observacoes cometárias e de vento solar sao comparadas com o propósito de determinar-se as condicoes do vento solar associadas aos eventos de desconexao (DEs) observados em caudas de plasma cometárias. Os dados cometários sao provenientes do The International Halley Watch Atlas of Large-Scale Phenomena. A análise visual sistemática das imagens do atlas revelou, entre outras estruturas morfológicas, 47 DEs ao longo da cauda de plasma do P/Halley. Estes 47 DEs registrados em 47 imagens distintas permitiram a descoberta de 19 origens de DEs, ou seja, o tempo em que as desconexoes iniciaram foi calculado. Os dados do vento solar sao provenientes de medidas feitas in situ pela sonda espacial IMP-8, as quais foram usadas para elaborar a variacao da velocidade do vento solar, densidade e pressao dinâmica durante o intervalo analisado. O presente trabalho compara as atuais teorias conflitantes, baseadas nos mecanismos de formacao, com o intuito de explicar o fenômeno cíclico dos DEs, ou seja, os efeitos de producao iônica, os efeitos de pressao e os efeitos de reconexao magnética sao analisados. Para cada uma das 19 origens de DEs comparou-se a densidade com a respectiva velocidade do vento solar com o intuito de determinar-se uma possível correlacao entre estas origens e os efeitos de pressao dinâmica. Quando da ocorrência de 6 origens de DEs o IMP-8 nao realizou medidas, nos outros 13 casos 10 origens (77%) mostraram uma anticorrelacao entre velocidade e densidade e apenas 3 (23%) revelaram uma tendência similar entre velocidade e densidade. Portanto, a análise inicial demonstra uma fraca correlacao entre as origens dos DEs e os efeitos de pressao.

  5. The Roles of Dopamine Transport Inhibition and Dopamine Release Facilitation in Wake Enhancement and Rebound Hypersomnolence Induced by Dopaminergic Agents

    PubMed Central

    Gruner, John A.; Marcy, Val R.; Lin, Yin-Guo; Bozyczko-Coyne, Donna; Marino, Michael J.; Gasior, Maciej

    2009-01-01

    Study Objective: Rebound hypersomnolence (RHS: increased sleep following increased wake) is a limiting side-effect of many wake-promoting agents. In particular, RHS in the first few hours following wake appears to be associated with dopamine (DA)-releasing agents, e.g., amphetamine, but whether it can also be produced by DA transporter (DAT) inhibition alone is unknown. In these studies, DA-releasing and DAT-inhibiting agents and their interaction were systematically examined for their ability to increase wake and induce RHS. Design: Chronically implanted rats were evaluated in a blinded, pseudo-randomized design. Participants: 237 rats were used in these studies with 1 week between repeat tests. Interventions: Animals were habituated overnight and dosed the next day, 5 h after lights on, with test agents. Measurements and Results: Sleep/wake activity and RHS were evaluated using EEG/EMG recording up to 22 h post dosing. In vitro dopamine release was evaluated in rat synaptosomes. At doses that produced equal increases in wake, DA-releasing (amphetamine, methamphetamine, phentermine) and several DAT-inhibiting agents (cocaine, bupropion, and methylphenidate) produced RHS during the first few hours after the onset of sleep recovery. However, other DAT-inhibiting agents (mazindol, nomifensine, GBR-12909, and GBR-12935) did not produce RHS. Combination treatment with amphetamine and nomifensine produced waking activity greater than the sum of their individual activities alone while ameliorating the amphetamine-like RHS. In rat synaptosomes, nomifensine reduced the potency of amphetamine to induce DA release ?270-fold, potentially explaining its action in ameliorating amphetamine-induced RHS. Conclusions: All DA releasing agents tested, and some DAT-inhibiting agents, produced RHS at equal wake-promoting doses. Thus amphetamine-like DA release appears sufficient for inducing RHS, but additional properties (pharmacologic and/or pharmacokinetic) evidently underlie RHS of other DAT inhibitors. Enhancing wake while mitigating RHS can be achieved by combining DAT-inhibiting and DA-releasing agents. Citation: Gruner JA; Marcy VR; LinYG; Bozyczko-Coyne D; Marino MJ; Gasior M. The roles of dopamine transport inhibition and dopamine release facilitation in wake enhancement and rebound hypersomnolence induced by dopaminergic agents. SLEEP 2009;32(11):1425-1438. PMID:19928382

  6. Mineral Dust Elemental Composition Over the Last 220 Kyr from the EPICA-Dome C ice core (East Antarctica)

    NASA Astrophysics Data System (ADS)

    Marino, F.; Maggi, V.; Delmonte, B.; Ghermandi, G.; Petit, J.; Hinkley, T. K.

    2004-12-01

    Mineral windblown aerosol (dust) represents a small fraction of the total mass of atmospheric aerosols. However, it may play an important role in climate and, in turn, it is itself sensitive to climatic changes. The investigation of the temporal variability of dust flux as well as the changes of its mineralogical composition within different climatic periods offers a unique way of assessing the source-related environmental changes, the variation in atmospheric circulation, and the potential influence of dust on biogeochemical cycles, for several key elements (such as Si and Fe). The mineral composition of dust found in ice cores is still poorly known, because few techniques are able to provide information on the chemical composition of the insoluble aerosol fraction, because of the very low mass of dust usually present in polar ice samples. Total volume of mineral content is provided by Coulter Counter measurements, and the dust record shows higher dust input during glacial periods than during interglacials (Delmonte et al., 2004). Sr and Nd isotopic tracers for identification of dust provenance to East Antarctica suggest southern South America as the dominant common source for dust in glacial periods of the late Pleistocene (Delmonte et al., 2004), whereas dust provenance during interglacials periods is still highly uncertain. Elemental composition of mineral dust from the Dome C ice core (75° 06' S, 123° 21' E) drilled in the framework of the European Project for Ice Coring in Antarctica (EPICA) is presented, showing measurements obtained by the Proton Induced X-ray Emission (PIXE) technique applied on insoluble atmospheric dust in ice cores. Within this work, substantial improvements to the experimental set-up and data processing have been made, compared to previously presented works on the first 2200 m of the EDC ice core, corresponding to about 220 kyr of climatic history (Marino et al., 2004; Ghermandi et al., 2003). The PIXE technique, based on X-ray spectrometry, allows direct measurements on filters of the insoluble dust fraction without sample pre-treatment, with analytical detection limits less than 1 ppb. The minimum required mass density of sample material on the filter is about 0.1 microg cm-2. Improvements made here allowed us to obtain accurate records of 8 major and minor crustal elements (Si, Al, Fe, Ti, K, Ca, Mg, Na). The data for these 8 elements, as well as their proportions as oxides, are shown for different climatic periods. Because O, Si, Al, Fe, Ti, K, Ca, Mg, Na are the principal constituents (99.90 %) of the Earth's Continental Crust, a comparison with literature data can reveal changes in relative elemental abundances, and hence variable composition of dust under different climatic conditions.

  7. Recent Developments of the Local Effect Model (LEM) - Implications of clustered damage on cell transformation

    NASA Astrophysics Data System (ADS)

    Elsässer, Thilo

    Exposure to radiation of high-energy and highly charged ions (HZE) causes a major risk to human beings, since in long term space explorations about 10 protons per month and about one HZE particle per month hit each cell nucleus (1). Despite the larger number of light ions, the high ionisation power of HZE particles and its corresponding more complex damage represents a major hazard for astronauts. Therefore, in order to get a reasonable risk estimate, it is necessary to take into account the entire mixed radiation field. Frequently, neoplastic cell transformation serves as an indicator for the oncogenic potential of radiation exposure. It can be measured for a small number of ion and energy combinations. However, due to the complexity of the radiation field it is necessary to know the contribution to the radiation damage of each ion species for the entire range of energies. Therefore, a model is required which transfers the few experimental data to other particles with different LETs. We use the Local Effect Model (LEM) (2) with its cluster extension (3) to calculate the relative biological effectiveness (RBE) of neoplastic transformation. It was originally developed in the framework of hadrontherapy and is applicable for a large range of ions and energies. The input parameters for the model include the linear-quadratic parameters for the induction of lethal events as well as for the induction of transformation events per surviving cell. Both processes of cell inactivation and neoplastic transformation per viable cell are combined to eventually yield the RBE for cell transformation. We show that the Local Effect Model is capable of predicting the RBE of neoplastic cell transformation for a broad range of ions and energies. The comparison of experimental data (4) with model calculations shows a reasonable agreement. We find that the cluster extension results in a better representation of the measured RBE values. With this model it should be possible to better predict the risk of the complex mixed radiation field occurring in deep space. 1. F. A. Cucinotta and M. Durante, Lancet Oncol. 7, 431-435 (2006). 2. M. Scholz and G. Kraft, Radiat. Prot. Dosim. 52, 29-33 (1994). 3. Th. Els¨sser and M. Scholz, Radiat. Res. 167, 319-329 (2007). a 4. R. C. Miller, S. A. Marino, D. J. Brenner, S. G. Martin, M. Richards, G. Randers-Pehrson, and E. J. Hall, Radiat. Res. 142, 54-60 (1995).

  8. Star Formation History of Early-Type Galaxies with Tidal Debris in the S 4 G

    NASA Astrophysics Data System (ADS)

    Ramos, Beatriz H. F.; Menéndez-Delmestre, Karín; Kim, Taehyun; Sheth, Kartik

    2015-03-01

    Local early-type galaxies (ETGs), despite typically being associated to old stellar populations and passive evolution, have been in some cases observed to present peculiarities in their stellar structure, like disks and shells (e.g., Kormendy et al. 1997, Rix, Carollo & Freeman 1999). Moreover, it has been observed that ETGs with such tidal features may present UV emission (Rampazzo et al. 2007, Salim & Rich 2010). These properties make them relevant constraints to galaxy formation models. We are analysing the structure of nearby ETGs observed in the Spitzer Survey of Stellar Structure in Galaxies (S 4 G; Sheth et al. 2010), which comprises the largest mid-IR survey of galaxies in the local Universe. We perform a 2D GALFIT decomposition of the 3.6μm images of 146 ETGs and examine their residual images. We identify tidal features in 17% of these, suggesting that a non-negligible ETGs fraction may have experienced (after the formation of the bulk of their stellar budget) merger events that have left signatures (Canalizo et al. 2007). For 6 of these peculiar ETGs, we also applied GALFIT decomposition to public GALEX/UV and SDSS/optical images. With measurements in multiple bands, we applied SED fitting techniques to estimate star formation rates (SFR) and stellar masses for the galaxies and their tidal features. We find that these 6 peculiar ETGs present masses in agreement with the population of non-peculiar ETGs. However, SFRs are higher than what has been measured for the average ETG population (Shapiro et al. 2010, SDSS MPA-JHU catalog). Based on the Kaviraj (2010) relation, we find that for these peculiar ETGs the estimated age of the most recent star formation event is less than 3Gyrs. Despite this indication of recent star formation, we have not found evidence of prominent UV emission in the tidal features (Marino et al. 2010). We are currently extending our work to the full sample of peculiar ETGs identified in our sample.

  9. Remote sensing of plant emissions of volatile isoprenoids with PRI. Prospects for upscaling (Invited)

    NASA Astrophysics Data System (ADS)

    Penuelas, J.

    2013-12-01

    Josep Peñuelas*1,2, Giovanni Marino1,2,3,4, Joan LLusia1,2, Catherine Morfopoulos1,2,5, Gerard Farre-Armengol1,2, Shawn Kefauver, Alex Guenther6 , Francesca Rapparini7 , Roger Seco1,2,6, Marc Estiarte1,2, Mónica Mejia-Chang1,2, Romà Ogaya1,2, Jordi Sardans1,2 , Andrew Turnipseed6, Peter Harley6, Osvaldo Facini7, Rita Baraldi7, Jim Greenberg6 , Iolanda Filella1,2 1 CSIC, Global Ecology Unit CREAF-CEAB-UAB, Cerdanyola del Vallés 08193, Catalonia, Spain 2 CREAF, Cerdanyola del Vallés 08193, Catalonia, Spain 3 Dipartimento di Bioscienze e Territorio, Università degli Studi del Molise, Contrada Fonte Lappone, 86090 Pesche (IS), Italy 4 Institute for Plant Protection, National Research Council, Via Madonna del Piano 10, 50019 Sesto Fiorentino (FI), Italy 5 Division of Ecology and Evolution, Imperial College, Silwood Park, Ascot, SL5 7PY, UK 6 Atmospheric Chemistry Division, National Center for Atmospheric Research, P.O. Box 3000, Boulder, CO 80307-3000, USA 7 Biometeorology Institute, IBIMET-CNR, Via P. Gobetti 101, Bologna, Italy Abstract Terrestrial plants re-emit around 1-2% of the carbon they fix as isoprene and monoterpenes. These emissions play major roles in the ecological relationships among living organisms and in atmospheric chemistry and climate, and yet their actual quantification at the ecosystem level in different regions is far from being resolved. Phenomenological models are used to estimate the emission rates, but the limited understanding of the function and regulation of these emissions leads to large uncertainties in such estimations. Many measurements have been made at the foliar but few at the ecosystem level, and those that do exist are limited in space and time. We here provide evidence that a simple remote sensing index, the photochemical reflectance index (PRI), which is indicative of light use efficiency (LUE), is a good indirect estimator of foliar isoprenoid emissions and therefore can be used to sense them remotely. These results open new perspectives for potential use of remote sense techniques of vegetation in order to track isoprenoid emissions at larger scales. At ecosystemic scale, in a field measurement campaign in NE Iberian peninsula, PRI estimations fitted well both with MEGAN modelled data and with satellite data assessing formaldehyde as oxidation product of isoprenoids. On the other hand, our study shows the potential of this PRI technique to validate the availability of photosynthetic reducing power as a factor involved in isoprenoid production.

  10. Experimental simulation of gravity currents in erodible bed

    NASA Astrophysics Data System (ADS)

    Bateman, A.; La Roca, M.; Medina, V.

    2009-04-01

    Gravity currents are commonly met in nature, when a flow of denser fluid moves into a less dense one. A typical example of a gravity current is given by the sea water which flows into the bottom of a river during the summer, in correspondence of the estuary, when the river's discharge attains low values. In this case, dangerous consequences can occur, because of the polluting of the aquifer caused by the salty water. Density currents also occurs in lakes and reservoirs, because of a change in temperature or because a flood, both can produce some environmental impacts that are of interest to the local water Agency of the different countries. Of particular relevance is also the interaction of the gravity current with the movement of the sediments from the bottom of the bed. The international state of the art is particularly concerned with experimental and numerical investigation on gravity currents on fixed and porous bed [1-2-3], while, to the authors' knowledge, the interaction of a gravity current with an erodible bed is still an open field of investigation. In this paper experiments concerning with the propagation of a gravity current over fixed and erodible bed are presented. The experiments, conducted at the laboratory of Hydraulics of the Universitat Politecnica de Catalunya (actually in the Prof. Bateman's blue room), were concerned with a transparent tank 2 m long, 0.2 m wide and 0.3 m deep, partly filled with salty water and partly with fresh water, up to a depth of 0.28 m. The salty water, whose density was in the range 1050Marino, P.F. Linden, Lock-release inertial gravity currents over a thick porous layer, The Journal of Fluid Mechanics, Vol. 503, 2004 [2] John E. Simpson. Gravity Currents [3] J.J. Monaghan, R.A.F. Cas, A.M. Kos, M. Hallworth, Gravity currents descending a ramp in a stratified tank, The Journal of Fluid Mechanics, Vol. 379, 1999

  11. Towards an organic palaeosalinity proxy: the effect of salinity, growth rate and growth phase on the hydrogen isotopic composition of alkenones produced by haptophyte algae

    NASA Astrophysics Data System (ADS)

    Chivall, David; M'Boule, Daniela; Schouten, Stefan; Sinninghe Damst, Jaap S.; van der Meer, Marcel T. J.

    2013-04-01

    Palaeosalinity is one of the most important oceanographic parameters which currently cannot be quantified with reasonable accuracy from sedimentary records. Schouten et al.1 established that the fractionation of hydrogen isotopes between growth water and alkenones produced by the haptophyte algae Emiliania huxleyi and Gephyrocapsa oceanica is salinity dependent. As such, the ?D values of alkenones recovered from sediment cores can be used to reconstruct variations in palaeo- sea surface salinity.2 However, to accurately determine absolute palaeosalinity requires a better constraining of the relationship between this hydrogen fractionation, salinity and other parameters such as growth rate and growth phase. Here, we present results from our ongoing work to constrain the relationship between the fractionation factor ?alkenone-water, salinity, growth rate and growth phase for the major alkenone-producing haptophytes. In batch cultures of different strains of the open-ocean haptophyte E. huxleyi sampled during the exponential growth phase, ?C37alkenone-growthwater increases by between 0.0022 and 0.0033 per unit increase in salinity. A similar relationship is observed in batch cultures of the coastal haptophyte Isochrysis galbana, where ? increases with each unit of salinity by 0.0019 - slightly less than for E. huxleyi. However, absolute ?C37alkenone-growthwater values vary strongly between species suggesting that species composition has a strong impact on the ?D value of alkenones. The fractionation factor for alkenones produced by batch cultures of I. galbana is affected by growth phase: the rate of change of ?C37alkenone-growthwater with each unit of salinity decreases from 0.0019 in the exponential phase to 0.0010 during the stationary phase. We also show the effect of varying growth rate over the range 0.2-0.8 day-1 on the fractionation factor for alkenones produced by E. huxleyi grown in continuous culture. These data show that alkenone ?D can be used to reconstruct relative shifts in palaeosalinity in coastal as well as open ocean environments; however, for absolute salinity reconstructions changes in species composition, growth rate and growth phase effects will have to be constrained. References 1. Schouten, S., Ossebaar, J., Schreiber, K., Kienhuis, M. V. M., Langer, G., Benthien, A., Bijma, J. Biogeosciences 3, 113, 2006 2. van der Meer, M. T. J., Baas, M., Rijpstra, W. I. C., Marino, G., Rohling, E. J., Sinninghe Damst, J S., Schouten, S., Earth and Planetary Science Letters 262, 594, 2007

  12. Marine hydrogeology: recent accomplishments and future opportunities

    NASA Astrophysics Data System (ADS)

    Fisher, A. T.

    2005-03-01

    Marine hydrogeology is a broad-ranging scientific discipline involving the exploration of fluid-rock interactions below the seafloor. Studies have been conducted at seafloor spreading centers, mid-plate locations, and in plate- and continental-margin environments. Although many seafloor locations are remote, there are aspects of marine systems that make them uniquely suited for hydrologic analysis. Newly developed tools and techniques, and the establishment of several multidisciplinary programs for oceanographic exploration, have helped to push marine hydrogeology forward over the last several decades. Most marine hydrogeologic work has focused on measurement or estimation of hydrogeologic properties within the shallow subsurface, but additional work has emphasized measurements of local and global fluxes, fluid source and sink terms, and quantitative links between hydrogeologic, chemical, tectonic, biological, and geophysical processes. In addition to summarizing selected results from a small number of case studies, this paper includes a description of several new experiments and programs that will provide outstanding opportunities to address fundamental hydrogeologic questions within the seafloor during the next 20-30 years. L'hydrogéologie marine est une large discipline scientifique impliquant l' exploration des interactions entre les fluides et les roches sous les fonds marins. Des études ont été menées dans les différents environnements sous-marins (zone abyssale, plaque océanique, marges continentales). Bien que de nombreux fonds marins soient connus, il existe des aspects des systèmes marins qui les rendent inadaptés à l'analyse hydrologique. De nouveaux outils et techniques, et la mise en oeuvre de nombreux programmes multidisciplinaires d'exploration océanographique, ont aidé à pousser en avant l'hydrogéologie marine ces dix dernières années. La plus part des études hydrogéologiques se sont concentrées jusqu'à présent sur la mesure ou l'estimation des propriétés à la sub-surface des fonds marins, et des travaux complémentaires ont mis en valeur les mesures de flux, local ou global, de termes « sources » et « pertes », et des liens quantitatifs entre l'hydrogéologie, la chimie, la tectonique, la biologie, et les processus géophysiques. Cet article vise à résumer des résultats sélectionnés parmi un petit nombre d'études, et à décrire plusieurs nouvelles expériences et programmes, qui sont autant d'opportunités pour répondre aux questions fondamentales relatives aux fonds marins, posées ces dernières 20-30 années. La hidrogeología marina es una disciplina científica de amplios alcances que involucra la exploración de interacciones fluido-roca por debajo del fondo del mar. Se han llevado a cabo estudios en centros de expansión del fondo del mar, lugares en medio de una placa, y en ambientes de placa y margen continental. Aunque muchos sitios en el fondo del mar son remotos, existen aspectos de estos sistemas marinos que los hacen particularmente adaptables para análisis hidrológico. Nuevas técnicas y herramientas desarrolladas, y el establecimiento de varios programas multidisciplinarios para exploración oceanográfica, han ayudado a impulsar la hidrogeología marina hacia delante durante las ultimas décadas. La mayor parte del trabajo hidrogeológico marino se ha enfocado en la medición o estimación de propiedades hidrogeológicas dentro del subsuelo superficial, pero trabajo adicionalha enfatizado mediciones de flujos globales y locales, términos de fuente y sumidero de fluidos, y vínculos cuantitativos entre procesos hidrogeológicos, químicos, tectónicos, biológicos y geofísicos. Además de resumir resultados seleccionados de un número pequeño de estudios de caso, este artículo incluye una descripción de varios programas y experimentos nuevos que aportarán oportunidades excepcionales para dirigir preguntas hidrogeológicas fundamentales dentro del fondo oceánico durante los siguientes 20-30 años.

  13. Microbial communities in the deep subsurface

    NASA Astrophysics Data System (ADS)

    Krumholz, Lee R.

    The diversity of microbial populations and microbial communities within the earth's subsurface is summarized in this review. Scientists are currently exploring the subsurface and addressing questions of microbial diversity, the interactions among microorganisms, and mechanisms for maintenance of subsurface microbial communities. Heterotrophic anaerobic microbial communities exist in relatively permeable sandstone or sandy sediments, located adjacent to organic-rich deposits. These microorganisms appear to be maintained by the consumption of organic compounds derived from adjacent deposits. Sources of organic material serving as electron donors include lignite-rich Eocene sediments beneath the Texas coastal plain, organic-rich Cretaceous shales from the southwestern US, as well as Cretaceous clays containing organic materials and fermentative bacteria from the Atlantic Coastal Plain. Additionally, highly diverse microbial communities occur in regions where a source of organic matter is not apparent but where igneous rock is present. Examples include the basalt-rich subsurface of the Columbia River valley and the granitic subsurface regions of Sweden and Canada. These subsurface microbial communities appear to be maintained by the action of lithotrophic bacteria growing on H2 that is chemically generated within the subsurface. Other deep-dwelling microbial communities exist within the deep sediments of oceans. These systems often rely on anaerobic metabolism and sulfate reduction. Microbial colonization extends to the depths below which high temperatures limit the ability of microbes to survive. Energy sources for the organisms living in the oceanic subsurface may originate as oceanic sedimentary deposits. In this review, each of these microbial communities is discussed in detail with specific reference to their energy sources, their observed growth patterns, and their diverse composition. This information is critical to develop further understanding of subsurface geochemical processes and to develop new approaches to subsurface remediation. Résumé La diversité des populations et des communautés microbiennes dans le sol et le sous-sol est présentée dans cet article. Les chercheurs s'interrogent fréquemment sur la diversité microbienne du sous-sol, sur les interactions entre organismes et sur les mécanismes qui permettent le maintien des communautés microbiennes souterraines. Il existe des communautés microbiennes anérobies hétérotrophes dans des grès ou dans des sédiments sableux relativement perméables, à proximité de dépôts riches en matières organiques. Ces micro-organismes semblent se maintenir grâce à la consommation de composés organiques provenant des dépôts organiques voisins. Les sources de matériel organique jouant le rôle de donneur d'électrons sont constituées par des sédiments éocènes riches en lignite situés sous la plaine littorale du Texas, les schistes riches en matières organiques du Crétacé du sud-ouest des États-Unis, ainsi que les argiles contenant des matériaux organiques et des bactéries de fermentation de la plaine littorale atlantique. En outre, il existe des communautés fortement diversifiées dans des régions où aucune source de matière organique n'existe, mais où sont présentes des roches ignées. Le sous-sol riche en basalte de la vallée de la Columbia au Canada et les régions granitiques de Suède en sont des exemples. Ces communautés microbiennes souterraines semblent se maintenir par l'action de bactéries lithotrophes se développant grâce à l'hydrogène qui est produit par réactions chimiques dans le sous-sol. Il existe d'autres communautés microbiennes de profondeur dans les sédiments profonds des océans. Ces systèmes sont souvent associés à un métabolisme anérobie et à une réduction des sulfates. La colonisation microbienne s'étend jusqu'à des profondeurs où les températures élevées limitent leur capacité de survie. Les sources d'énergie pour ces organismes vivant dans les fonds des océans peuvent être les dépôts sédimentaires océaniques. Dans cette revue, chacune des communautés microbiennes est discutée en détail en se référant spécifiquement à leurs sources d'énergie, au schéma observé de leur développement et à leur composition diversifiée. Cette information est donnée de façon critique dans le but d'améliorer la compréhension des processus géochimiques intervenant dans le sous-sol et de développer de nouvelles approches pour la dépollution souterraine. Resumen En este artículo se resume la diversidad de las poblaciones y comunidades microbianas en el subsuelo. A partir de exploraciones realizadas en el subsuelo, los científicos se están cuestionando en la actualidad aspectos relativos a la diversidad microbiana, las interacciones entre los distintos microorganismos y los mecanismos para el mantenimiento de las comunidades de microbios. Se ha comprobado la presencia de comunidades microbianas anaerobias y heterótrofas en areniscas relativamente permeables y en sedimentos arenosos ubicados cerca de depósitos ricos en materia orgánica, de la cual se alimentan. Algunas fuentes de material orgánico, que actúan como donantes de electrones, son: sedimentos del Eoceno ricos en lignito, bajo la planicie costera de Texas; pizarras del Cretácico ricas en materia orgánica, al sudoeste del país y arcillas cretácicas con materia orgánica y bacterias fermentativas, en la llanura Atlántica. También existen comunidades microbianas de gran diversidad en rocas ígneas, aunque la fuente de materia orgánica no es tan evidente. Algunos ejemplos son la subsuperficie del valle del Río Columbia, rico en basaltos, y las regiones graníticas de Suecia y Canadá. Estas comunidades microbianas subsuperficiales se mantienen por la acción de bacterias litotrópicas, que crecen en ambiente de H2, generado en la subsuperficie. También existen comunidades microbianas a gran profundidad, como por ejemplo en los sedimentos oceánicos. Estos sistemas subsisten con un metabolismo anaerobio en un ambiente sulfato-reductor. La colonización microbiana se extiende hasta profundidades tales que las altas temperaturas limitan su supervivencia. Las fuentes de energía para estos organismos pueden ser los depósitos sedimentarios oceánicos. En este artículo se discute cada una de estas comunidades en detalle, en particular sus fuentes de energía, su esquema de crecimiento y la diversidad de su composición. Esta información es de gran interés para permitir un mayor entendimiento de los procesos geoquímicos en profundidad y para desarrollar nuevos métodos de rehabilitación.

  14. Ambiente e formao estelar em galxias

    NASA Astrophysics Data System (ADS)

    Mateus, A., Jr.; Sodr, L., Jr.

    2003-08-01

    Estudamos o ambiente de galxias com formao estelar inicialmente a partir de uma amostra limitada em volume proveniente do 2dF Galaxy Redshift Survey. Discriminamos as galxias com formao estelar com base em distintas classes espectrais, utilizando para esta classificao as larguras equivalentes das linhas [OII]l3727 e Hd. O ambiente caracterizado pela densidade espacial local de galxias. Mostramos que a frao de galxias com formao estelar bastante reduzida em ambientes densos, enquanto a de galxias passivas aumenta nestas regies. Por outro lado, quando analisamos a frao de galxias que apresentam um surto recente de formao estelar, notamos que ela independe do ambiente, sendo que em regies mais densas alguns destes objetos apresentam distores em sua morfologia. Estes resultados so confrontados com a anlise da dependncia ambiental da taxa de formao estelar, estimada pela emisso em Ha, de uma amostra extrada do Sloan Digital Sky Survey. Um declnio gradual da formao estelar tambm observado nesta anlise, sugerindo que as interaes por efeitos de mar sejam responsveis pela reduo da formao estelar em ambientes densos atravs da remoo do reservatrio de gs das galxias. No entanto, estas interaes tambm podem induzir surtos de formao estelar nas galxias, alm de peculiaridades morfolgicas observadas nos objetos que habitam regies mais densas.

  15. Estudio de eventos dinmicos en ondas milimtricas

    NASA Astrophysics Data System (ADS)

    Cristiani, G.; Martnez, G.; Raulin, J. P.; Gimnez de Castro, G.; Rovira, M.

    El estudio de la actividad solar con el telescopio para ondas submilimtricas (SST), nos permite, por vez primera, trabajar con una resolucin temporal de milisegundos. Este hecho ha permitido observar emisin nunca antes comprobada, pulsos o flashes extremadamente rpidos provenientes de las regiones activas, los cuales parecen preanunciar fulguraciones en dichas regiones. Se muestra, como ejemplo, una fulguracin observada con el telescopio HASTA en H?, y los pulsos rpidos que la preceden observados con el SST. Para cuantificar la influencia de la atmsfera terrestre en los datos registrados, se est estudiando la variabilidad temporal de las opacidades a las frecuecias de trabajo (212 y 405 Ghz), es decir los rangos de tiempo para los cuales la opacidad puede variar apreciablemente. Con este fin se calcula la eficiencia de cada canal multiplicada por la temperatura del Sol a estas frecuencias (estas son conocidas con una incerteza del 20 %). Se muestran los resultados obtenidos para cada canal, en donde se grafica este producto como funcin de la opacidad.

  16. Central radio galaxies in groups: cavities, bubbles and the history of AGN heating

    NASA Astrophysics Data System (ADS)

    Giacintucci, S.; Venturi, T.; Raychaudhury, S.; Vrtilek, J.

    2008-10-01

    E' noto che le regioni centrali degli ammassi e gruppi di galassie costituiscono un ambiente in cui gas caldo e plasma radioemittente proveniente dalle galassie dominanti interagiscono tra loro. In particolare, si pensa che la radioemissione dell'AGN centrale ed i suoi possibili cicli di attivita', siano strettamente legati alla presenza di cavita' e "bubbles" nel gas intergalattico. Si presentera' lo status di un progetto osservativo effettuato con il Giant Metrewave Radio Telescope (GMRT, India) su di un campione di 18 gruppi di galassie, osservati a tre frequenze radio (235 MHz, 325 MHz e 610 MHz). Lo studio della morfologia radio degli AGN centrali e la relativa analisi spettrale permettono di ottenere stime sull'eta' di questi oggetti, e sulla loro energia totale, che a loro volta sono in relazione con le proprieta' X dei gruppi stessi. Per tutti gli oggetti del campione sono disponibili osservazioni Chandra di proprieta'. Per due oggetti del campione, 4C+24.36 (al centro di AWM04) e NGC741 (al centro di RSOG17) verra' presentato uno studio dettagliato.

  17. Intermitncia alfvnica gerada por caos na atmosfera solar e no vento solar

    NASA Astrophysics Data System (ADS)

    Rempel, E. L.; Chian, A. C.-L.; Macau, E. E. N.; Rosa, R. R.

    2003-08-01

    Dados medidos no vento solar rpido proveniente dos buracos coronais revelam que os plasmas no meio interplanetrio so dominados por flutuaes Alfvnicas, caracterizadas por uma alta correlao entre as variaes do campo magntico e da velocidade do plasma. As flutuaes exibem muitas caractersticas esperadas em turbulncia magneto-hidrodinmica totalmente desenvolvida, tais como intermitncia e espectros contnuos. Contudo, os mecanismos responsveis pela evoluo de turbulncia Alfvnica intermitente no so completamente compreendidos. Neste trabalho a teoria de caos usada para explicar como sistemas Alfvnicos, modelados pela equao Schrdinger no-linear derivativa e pela equao Kuramoto-Sivashinsky, podem se tornar fortemente caticos medida em que parmetros do plasma so variados. Pequenas perturbaes no parmetro de dissipao podem fazer com que o sistema mude bruscamente de um regime peridico, ou fracamente catico, para um regime fortemente catico. As sries temporais das flutuaes do campo magntico nos regimes fortemente caticos exibem comportamento intermitente, em que fases laminares ou fracamente caticas so interrompidas por fortes estouros caticos. mostrado que o regime fortemente catico atingido quando as solues peridicas ou fracamente caticas globalmente estveis interagem com solues do sistema que so fortemente caticas, mas globalmente instveis. Estas solues globalmente instveis so conjuntos caticos no-atrativos conhecidos como selas caticas, e so responsveis pelos fortes estouros nos regimes intermitentes. Selas caticas tm sido detectadas experimentalmente em uma grande variedade de sistemas, sendo provvel que elas desempenhem um papel importante na turbulncia intermitente observada em plasmas espaciais.

  18. Aceptabilidad del diagnóstico rápido casero para HIV entre hombres gay y otros hombres que tienen sexo con hombres (G&HSH) de la Ciudad de Buenos Aires.

    PubMed

    Balán, Iván C; Carballo-Diéguez, Alex; Marone, Rubén O; Pando, María A; Barreda, Victoria; Avila, María M

    2011-03-01

    El uso del diagnóstico rápido para HIV en Argentina, así como otros países de Latinoamérica, ha sido limitado hasta el momento. Este trabajo reporta los resultados provenientes de un estudio cualitativo realizado entre hombres gays y otros hombres que tienen sexo con hombres (G&HSH) de la Ciudad de Buenos Aires, Argentina. El objetivo principal del mismo fue conocer las ventajas y desventajas que los hombres G&HSH perciben en relación al diagnóstico rápido casero para HIV. Se realizaron ocho grupos focales con 73 participantes en los cuales se discutió acerca de las ventajas y desventajas del uso de los diagnósticos rápidos. Las respuestas fueron codificadas utilizando un programa para análisis de datos cualitativos (NVivo) y analizadas temáticamente. Los participantes describieron numerosas ventajas sobre el uso del diagnóstico rápido casero, aunque algunos reportaron importantes preocupaciones dentro de las cuales se destaca la posibilidad de impulsos suicidas si alguien recibe un resultado positivo estando solo. En términos generales se observó una gran aceptabilidad para el uso del diagnóstico rápido si el mismo es realizado por personal de salud en lugares acondicionados para este fin. PMID:25284951

  19. Simulaes Numricas de Rotao Nuclear Cometria

    NASA Astrophysics Data System (ADS)

    Voelzke, M. R.; Winter, O. C.

    1999-08-01

    Este trabalho apresenta os resultados iniciais de simulaes numricas da evoluo rotacional, de um ncleo cometrio no esfrico, ao longo de uma passagem perilica, levando-se em conta os torques devido a existncia dos jatos de poeira e de gs. Inicialmente os autores apresentam um modelo simples (primeira aproximao), com somente um nico jato na extremidade do semi-eixo maior, para compreender a variao positiva ou negativa que estas foras no gravitacionais exercem sobre o perodo de rotao cometrio. Posteriormente incrementa-se o nmero de jatos, os quais so distribudos ao longo da superfcie cometria, para observar-se a contribuio dos efeitos provenientes dos torques originrios da liberao da poeira e gs cometrios, que provavelmente violar a suposio da livre precesso. Os estados rotacionais, sob torques induzidos devido sublimao, dependem fortemente da localizao das reas ativas do ncleo. Os cometas P/Schwassmann-Wachmann 1, P/Tempel 2, P/Forbes e C/Meunier-Dupouy sero observados fotometricamente, pelos autores, no Laboratrio Nacional de Astrofsica (LNA) ao longo de algumas noites consecutivas em abril, junho e julho de 1999. Estas observaes sero comparadas com as simulaes numricas de rotao cometria.

  20. Aceptabilidad del diagnóstico rápido casero para HIV entre hombres gay y otros hombres que tienen sexo con hombres (G&HSH) de la Ciudad de Buenos Aires

    PubMed Central

    Balán, Iván C.; Carballo-Diéguez, Alex; Marone, Rubén O.; Pando, María A.; Barreda, Victoria; Ávila, María M.

    2011-01-01

    Resumen El uso del diagnóstico rápido para HIV en Argentina, así como otros países de Latinoamérica, ha sido limitado hasta el momento. Este trabajo reporta los resultados provenientes de un estudio cualitativo realizado entre hombres gays y otros hombres que tienen sexo con hombres (G&HSH) de la Ciudad de Buenos Aires, Argentina. El objetivo principal del mismo fue conocer las ventajas y desventajas que los hombres G&HSH perciben en relación al diagnóstico rápido casero para HIV. Se realizaron ocho grupos focales con 73 participantes en los cuales se discutió acerca de las ventajas y desventajas del uso de los diagnósticos rápidos. Las respuestas fueron codificadas utilizando un programa para análisis de datos cualitativos (NVivo) y analizadas temáticamente. Los participantes describieron numerosas ventajas sobre el uso del diagnóstico rápido casero, aunque algunos reportaron importantes preocupaciones dentro de las cuales se destaca la posibilidad de impulsos suicidas si alguien recibe un resultado positivo estando solo. En términos generales se observó una gran aceptabilidad para el uso del diagnóstico rápido si el mismo es realizado por personal de salud en lugares acondicionados para este fin. PMID:25284951

  1. Sobre el estado evolutivo de ? Pictoris

    NASA Astrophysics Data System (ADS)

    Brunini, A.; Benvenuto, O. G.

    Desde el descubrimiento de fuertes excesos infrarrojos en ? Pictoris, esta estrella ha sido muy estudiada y es considerada candidata a poseer un sistema planetario propio. ? Pic est rodeada de un disco asimtrico de polvo que se observa de canto y que esta vaco a distancias <= 40 AU. Esto se considera una fuerte evidencia en favor de la presencia de (al menos) un planeta gigante. Recientemente se han observado lneas de material circunestelar que se han interpretado como consecuencia de la cada de objetos cometarios sobre esta estrella. Recientemente se ha utilizado la existencia del disco de polvo para atribuir una edad corta (pre - secuencia principal) a ?Pic. Sin embargo, la evaporacin de estos cometas provee suficiente polvo como para explicar la presencia del disco observado sin necesidad de edades cortas. En este trabajo mostramos que la comparacin entre la tasa de impactos cometarios estimada en el Sistema Solar para diferentes etapas de su evolucin y los datos observados en ? Pic indica edades avanzadas para ? Pic. Esta estimacin debe tomarse con cautela ya que depende de la estructura de los sistemas planetarios. Adems mostramos que, desde el punto de vista de la evolucin estelar y con las incertezas presentes en la luminosidad y la temperatura efectiva, existe un continuo de edades posible para ? Pic. Sin embargo, empleando los datos provenientes de los flujos cometarios encontramos que una edad prolongada es consistente con ambos tratamientos.

  2. Aquifer/aquitard interfaces: mixing zones that enhance biogeochemical reactions

    NASA Astrophysics Data System (ADS)

    McMahon, P. B.

    2001-01-01

    Several important biogeochemical reactions are known to occur near the interface between aquifer and aquitard sediments. These reactions include O2 reduction; denitrification; and Fe3+, SO42-, and CO2 (methanogenesis) reduction. In some settings, these reactions occur on the aquitard side of the interface as electron acceptors move from the aquifer into the electron-donor-enriched aquitard. In other settings, these reactions occur on the aquifer side of the interface as electron donors move from the aquitard into the electron-acceptor-enriched, or microorganism-enriched, aquifer. Thus, the aquifer/aquitard interface represents a mixing zone capable of supporting greater microbial activity than either hydrogeologic unit alone. The extent to which biogeochemical reactions proceed in the mixing zone and the width of the mixing zone depend on several factors, including the abundance and solubility of electron acceptors and donors on either side of the interface and the rate at which electron acceptors and donors react and move across the interface. Biogeochemical reactions near the aquifer/aquitard interface can have a substantial influence on the chemistry of water in aquifers and on the chemistry of sediments near the interface. Rsum. Il se produit au voisinage de l'interface entre les aquifres et les impermables plusieurs ractions biogochimiques importantes. Il s'agit des ractions de rduction de l'oxygne, de la dnitrification et de la rduction de Fe3+, SO42- et CO2 (mthanogense). Dans certaines situations, ces ractions se produisent du ct impermable de l'interface, avec des accepteurs d'lectrons qui vont de l'aquifre vers l'impermable riche en donneurs d'lectrons. Dans d'autres situations, ces ractions se produisent du ct aquifre de l'interface, avec des donneurs d'lectrons qui se dplacent de l'impermable vers l'aquifre riche en accepteurs d'lectrons ou en microorganismes. Ainsi, l'interface aquifre/impermable constitue une zone de mlange capable de supporter une plus grande activit microbienne que chacune des deux units hydrogologiques seules. L'extension des ractions biogochimiques dans la zone de mlange et la largeur de cette zone dpendent de plusieurs facteurs, dont l'abondance et la solubilit des accepteurs et des donneurs d'lectrons de chaque ct de l'interface, et le taux de raction et de dplacement des accepteurs et des donneurs d'lectrons au travers de cette interface. Les ractions biogochimiques au voisinage de l'interface aquifre/impermable peuvent avoir une influence apprciable sur le chimisme de l'eau des aquifres et sur celui des sdiments au niveau de l'interface. Resmen. Es conocido que varias reacciones biogeoqumicas de importancia pueden tener lugar cerca de la interfaz entre los sedimentos de un acufero y de un acuitardo. Entre ellas, destaca la reduccin del O2, la denitrificacin, y la reduccin del Fe+3, SO4-2 y CO2 (metanognesis). En algunos casos, estas reacciones se producen en la regin cercana al acuitardo, ya que los dadores de electrones se mueven desde ste hacia el acufero, el cual est enriquecido en aceptores de electrones o en microorganismos. As, la interfaz acufero/acuitardo constituye una zona de mezcla que es capaz de sustentar una actividad microbiana mayor que cualquier unidad hidrogeolgica por s misma. El alcance de las reacciones biogeoqumicas en la zona de mezcla y el ancho de esta zona de mezcla depende de varios factores, como la abundancia y la solubilidad de los aceptores y dadores de electrones en ambas caras de la interfaz y la velocidad a la que los aceptores y dadores de electrones reaccionan y se mueven a travs de la interfaz. Las reacciones biogeoqumicas cerca de la interfaz acufero/acuitardo pueden tener una influencia substancial en la hidroqumica de los acuferos y en la qumica de los sedimentos cerca de la superficie.

  3. Some mathematical aspects of quantum field theory

    NASA Astrophysics Data System (ADS)

    Chen, Qingtao

    In recent years, physics especially Quantum Field Theory has had an enormous impact in mathematics. This thesis mainly contains two different parts of mathematical developments of problems inspired from physics. Firstly, I study Topological Quantum Field Theory and its related topics. Gromov-Witten theory of resolved conifold corresponds to the Chern-Simons theory of unknot. In a series of papers, Labastida, Marino, Ooguri, Vafa, proposed a conjectural description of Chern-Simons theory of special linear quantum group invariants of links. LMOV conjecture could be viewed as a counterpart of Gopakumar-Vafa conjecture. These are actually parts of the big picture, large N Chern-Simons/Topological string duality. In the first chapter of this part, the orthogonal quantum group version of LMOV conjecture is rigorously formulated in mathematics by using the representation of Brauer centralizer algebra. We also obtain formulae of Lichorish-Millet type which could be viewed as the application in knot theory and topology. By using the cabling technique, we obtain a uniform formula of colored Kauffman polynomial for all torus links with all partitions. Combined these together, we are able to prove many interesting cases of this orthogonal LMOV conjecture. In particular we can apply this uniform formula to verify certain case of the conjecture at roots of unity. In fact, these integer coefficients appeared in the original (orthogonal) LMOV conjecture are called the BPS numbers in string theory. In the second chapter of this part, graphic representations of the universal R-matrices has been used to discover the recursion formulae between various quantum group invariants. We study the recursion relations of R-matrices corresponding to the inclusions Uq( sln) ? Uq(sl n+1), Uq(sl k) x Uq(sln--k ) ? Uq(sln), Uq(sln) ? U q(so2n), Uq(so2k) x Uq(sln--k) ? Uq(so2n). As an application, we find the ODE recursion formulae for HOMFLY and Kauffman polynomials. Secondly, I study the Modular Forms in Topology, Elliptic Genera, Loop Space and String Manifolds. In a series of papers, the following results are discovered. By developing modular invariance on certain characteristic forms, several cancellation formulas emerge naturally as the generalization of the original gravity anomaly cancellation formulas obtained by L. Alvarez-Gaume and E. Witten in their celebrated paper [2] studying the string theory. These cancellation formulae directly imply the divisibility and the congruence phenomena of characteristic numbers by Atiyah-Singer Index theorem, which plays important roles both in topology and differential geometry. We recover the Hirzebruch divisibility of twist signature and obtain the twist higher Rokhlin congruence by applying the modular invariance properties on the elliptic forms and also prove that it is best possible by studying examples constructed from K3-surface and Bott manifold. We also obtain the divisibility results for the index of double twist signature operators. By studying the "modular transgression" on elliptic forms, we obtain some modularly invariant secondary characteristic forms on odd dimensional manifolds. Also, by using this method, we heuristically calculate the Chern-Simons forms for flat bundles over free loop space. This direction is pioneered by Witten [94), who heuristically interpreted the Landweber-Stong elliptic genus as the index of the formal signature operator on free loop space as well as introduced the formal equivariant index of the Dirac operator on loop space, known as Witten operator. We call a manifold to be string if its loop space is spin. It's known that a string manifold is a spin manifold with vanishing half first Pontryagin class. Using the arithmetic properties of Jacobi-Theta functions, we prove the vanishing of the Witten genus of certain nonsingular string complete intersections in products of complex projective spaces, which generalizes a known result of Landweber and Stong [54].

  4. Establishing IUCN Red List Criteria for Threatened Ecosystems

    PubMed Central

    Rodrguez, Jon Paul; Rodrguez-Clark, Kathryn M; Baillie, Jonathan E M; Ash, Neville; Benson, John; Boucher, Timothy; Brown, Claire; Burgess, Neil D; Collen, Ben; Jennings, Michael; Keith, David A; Nicholson, Emily; Revenga, Carmen; Reyers, Belinda; Rouget, Mathieu; Smith, Tammy; Spalding, Mark; Taber, Andrew; Walpole, Matt; Zager, Irene; Zamin, Tara

    2011-01-01

    Abstract The potential for conservation of individual species has been greatly advanced by the International Union for Conservation of Nature's (IUCN) development of objective, repeatable, and transparent criteria for assessing extinction risk that explicitly separate risk assessment from priority setting. At the IV World Conservation Congress in 2008, the process began to develop and implement comparable global standards for ecosystems. A working group established by the IUCN has begun formulating a system of quantitative categories and criteria, analogous to those used for species, for assigning levels of threat to ecosystems at local, regional, and global levels. A final system will require definitions of ecosystems; quantification of ecosystem status; identification of the stages of degradation and loss of ecosystems; proxy measures of risk (criteria); classification thresholds for these criteria; and standardized methods for performing assessments. The system will need to reflect the degree and rate of change in an ecosystem's extent, composition, structure, and function, and have its conceptual roots in ecological theory and empirical research. On the basis of these requirements and the hypothesis that ecosystem risk is a function of the risk of its component species, we propose a set of four criteria: recent declines in distribution or ecological function, historical total loss in distribution or ecological function, small distribution combined with decline, or very small distribution. Most work has focused on terrestrial ecosystems, but comparable thresholds and criteria for freshwater and marine ecosystems are also needed. These are the first steps in an international consultation process that will lead to a unified proposal to be presented at the next World Conservation Congress in 2012. Establecimiento de Criterios para la Lista Roja de UICN de Ecosistemas Amenazados Resumen El potencial para la conservacin de muchas especies ha avanzado enormemente porque la Unin Internacional para la Conservacin de la Naturaleza (UICN) ha desarrollado criterios objetivos, repetibles y transparentes para evaluar el riesgo de extincin que explcitamente separa la evaluacin de riesgo de la definicin de prioridades. En el IV Congreso Mundial de Conservacin en 2008, el proceso comenz a desarrollar e implementar estndares globales comparables para ecosistemas. Un grupo de trabajo establecido por la UICN ha formulado un sistema inicial de categoras y criterios cuantitativos, anlogos a los utilizados para especies, para asignar niveles de amenaza a ecosistemas a niveles local, regional y global. Un sistema final requerir de definiciones de ecosistemas; cuantificacin del estatus de ecosistemas; identificacin de las etapas de degradacin y prdida de los ecosistemas; medidas de riesgo (criterios) alternativas; umbrales de clasificacin para esos criterios y mtodos estandarizados para la realizacin de evaluaciones. El sistema deber reflejar el nivel y tasa de cambio en la extensin, composicin, estructura y funcionamiento de un ecosistema, y tener sus races conceptuales en la teora ecolgica y la investigacin emprica. Sobre la base de esos requerimientos y la hiptesis de que el riesgo del ecosistema es una funcin del riesgo de las especies que lo componen, proponemos un conjunto de 4 criterios: declinaciones recientes en la distribucin o funcionamiento ecolgica, prdida total histrica en la distribucin o funcionamiento ecolgico, distribucin pequea combinada con declinacin, o distribucin muy pequea. La mayor parte del trabajo se ha concentrado en ecosistemas terrestres, pero tambin se requieren umbrales y criterios comparables para ecosistemas dulceacucolas y marinos. Estos son los primeros pasos de un proceso de consulta internacional que llevar a una propuesta unificada que ser presentada en el prximo Congreso Mundial de Conservacin en 2012. PMID:21054525

  5. Helicity, geostrophic balance and mixing in rotating stratified turbulence: a multi-scale problem

    NASA Astrophysics Data System (ADS)

    Pouquet, A.; Marino, R.; Mininni, P.; Rorai, C.; Rosenberg, D. L.

    2012-12-01

    Helicity, geostrophic balance and mixing in rotating stratified turbulence: a multi-scale problem A. Pouquet, R. Marino, P. D. Mininni, C. Rorai & D. Rosenberg, NCAR Interactions between winds and waves have important roles in planetary and oceanic boundary layers, affecting momentum, heat and CO2 transport. Within the Abyssal Southern Ocean at Mid latitude, this may result in a mixed layer which is too shallow in climate models thereby affecting the overall evolution because of poor handling of wave breaking as in Kelvin-Helmoltz instabilities: gravity waves couple nonlinearly on slow time scales and undergo steepening through resonant interactions, or due to the presence of shear. In the oceans, sub-mesoscale frontogenesis and significant departure from quasi-geostrophy can be seen as turbulence intensifies. The ensuing anomalous vertical dispersion may not be simply modeled by a random walk, due to intermittent structures, wave propagation and to their interactions. Conversely, the energy and seeds required for such intermittent events to occur, say in the stable planetary boundary layer, may come from the wave field that is perturbed, or from winds and the effect of topography. Under the assumption of stationarity, weak nonlinearities, dissipation and forcing, one obtains large-scale geostrophic balance linking pressure gradient, gravity and Coriolis force. The role of helicity (velocity-vorticity correlations) has not received as much attention, outside the realm of astrophysics when considering the growth of large-scale magnetic fields. However, it is measured routinely in the atmosphere in order to gauge the likelihood of supercell convective storms to strengthen, and it may be a factor to consider in the formation of hurricanes. In this context, we examine the transition from a wave-dominated regime to an isotropic small-scale turbulent one in rotating flows with helical forcing. Using a direct numerical simulation (DNS) on a 3072^3 grid with Rossby and Reynolds numbers of 0.07 and 27000, one can resolve both the Zeman scale at which the inertial and eddy turn-over times equalize, and the dissipation scale. We show that fully helical vertical columns dominate at intermediate scales, presumably self-similar and shrouded by a sea of small-scale vortex filaments as in Kolmogorov turbulence. Helicity has a profound effect on the structures of the flow, and a previously developed model that includes a helical component in its eddy viscosity and eddy noise shows a measurable improvement. Indeed, if dimensionless parameters for inertial and gravity waves are reachable numerically, the Reynolds number is too low in DNS for geophysics unless one uses parametrizations of small scale interactions. For spin-down stably-stratified flows, energy and helicity undergo a substantially slower decay than in the unstratified case, and a type of large-scale cyclostrophic balance is invoked to explain this behavior. The decay rate is similar to that occurring in the unstratified rotating case, as modeled by taking into account the quasi-conservation of helicity. We finally mention helicity production when rotation and stratification are both combined. In conclusion, much remains to be done, e.g. examining transport properties of rotating stratified turbulence, such as the effect of helicity on mixing in geophysical flows that can be studied with high-performance computing allowing multi-scale interactions and intermittency to develop.

  6. Chlorine-36 in groundwater of the United States: empirical data

    NASA Astrophysics Data System (ADS)

    Davis, Stanley; Moysey, Stephen; Cecil, DeWayne; Zreda, Marek

    2002-11-01

    Natural production of the radionuclide chlorine-36 (36Cl) has provided a valuable tracer for groundwater studies. The nuclear industry, especially the testing of thermonuclear weapons, has also produced large amounts of 36Cl that can be detected in many samples of groundwater. In order to be most useful in hydrologic studies, the natural production prior to 1952 should be distinguished from more recent artificial sources. The object of this study was to reconstruct the probable preanthropogenic levels of 36Cl in groundwater in the United States. Although significant local variations exist, they are superimposed on a broad regional pattern of 36Cl/Cl ratios in the United States. Owing to the influence of atmospherically transported ocean salt, natural ratios of 36Cl/total Cl are lowest near the coast and increase to a maximum in the central Rocky Mountains of the United States. Résumé. La production naturelle du radionucléide chlore-36 (36Cl) fournit un intéressant traceur pour l'étude des eaux souterraines. L'industrie nucléaire, en particulier les essais de bombes thermonucléaires, a également produit de grandes quantités de 36Cl qui a pu être détecté dans de nombreux échantillons d'eau souterraine. Afin d'en améliorer l'usage dans les études hydrologiques, la production naturelle avant 1952 doit être distinguée des sources artificielles plus récentes. L'objectif de cette étude a été la reconstruction des niveaux probables de 36Cl dans les eaux souterraines des États-Unis, avant la production anthropique du 36Cl. Bien qu'il existe des variations locales significatives, elles se surimposent à un canevas régional de rapports 36Cl/Cl dans les États-Unis. Du fait de l'influence du sel océanique transporté dans l'atmosphère, les rapports naturels de 36Cl/Cl total sont plus faibles près de la côte et augmentent jusqu'à un maximum dans les Montagnes Rocheuses centrales des États-Unis. Resumen. La producción natural del radionucleido cloro-36 (36Cl) representa un trazador valioso para estudios de hidrogeología. La industria nuclear, sobretodo por los ensayos con armas nucleares, también ha producido grandes cantidades de 36Cl que pueden ser detectadas en muchas muestras de aguas subterráneas. Para que sean lo más útiles posible en estudios hidrológicos, la producción natural anterior al año 1952 debe ser diferenciada de la procedente de fuentes artificiales más recientes. El objeto de este estudio era la reconstrucción de los niveles probables de 36Cl en las aguas subterráneas de los Estados Unidos de América con anterioridad a las aportaciones de origen antrópico. Aunque existen variaciones locales significativas, éstas se superponen a un extenso patrón regional de la relación 36Cl/Cl en el país. Debido a la influencia de la sal transportada en los aerosoles marinos, las proporciones naturales de 36Cl/Cl total son menores cerca de la costa, y alcanzan su máximo en el centro de las Montañas Rocosas.

  7. Measuring change over time: the use of geotagged photographs to evaluate the weathering of monuments

    NASA Astrophysics Data System (ADS)

    Doehne, E.

    2012-04-01

    Evaluating the condition of weathered stone surfaces on a monument, building or sculpture requires information on how those surfaces have evolved. In a number of cases, the documentation related to a site or object is either not readily available or has been lost (due to war, fire, etc.). Exploring the use of geotagged photographs to supplement the evaluation of surface changes to monuments was tested using two sites: the Mausoleum at the Huntington Library, Art Collections, and Botanical Gardens in San Marino, California and the Duomo in Florence, Italy. Increasingly, photographs are being geo-located or geotagged, either automatically via GPS/WiFi or manually. Geolocation tags increase the value of a photograph to researchers by providing the geographic location where the image was taken, often along with the date and time the photograph was acquired. Estimates of the number of geolocated photographs posted to the Internet include 148 million on Flickr.com (as of June 3, 2011) increasing to 172 million as of January 15, 2012. On Panarimo.com five million geolocated images were archived as of October 2007. Tools such as auto-geotag and PhotoOverlay are making it easier for users to locate and exactly position existing photographs and historic photographs on sites such as Google Earth (PhotoOverlays are images that are directly embedded in the Google Earth's landscape). 42 photo sharing websites are listed currently on Wikipedia, with seven having Alexa rankings of less than 200, indicating the popularity of photo sharing and the vast nature of this resource. Preliminary results from the Huntington and the Duomo indicate that geolocated images are indeed a useful tool for aiding in understanding stone weathering patterns and changes over time. However, greater software support and new tools are needed to enable researchers to search, organize and analyze groups of photographs from a single geolocation. Such software would have obvious uses beyond the conservation of monuments. For example, insurance, tourism and real estate companies are also interested in evaluating how buildings and land-use have changed over time. Context: Central to making decisions concerning the preservation of patrimony is the practical issue of monitoring material change over time. Is an intervention effective? Should a sculpture be moved indoors or a structure sheltered? Efficiently measuring changes in heritage materials is a significant scientific and logistical challenge to preserving our cultural legacy in stone. Conservation professionals in charge of the long-term survival of material cultural heritage need to know how fast and why these materials change. With a baseline in place, decisions regarding resource allocation and conservation interventions can more readily be made from a basis of scientific understanding. Lacking a baseline, it can be difficult, if not impossible, to evaluate the effectiveness of a preservation intervention or treatment.

  8. Um supressor de fundo térmico para a câmara infravermelha CamIV

    NASA Astrophysics Data System (ADS)

    Jablonski, F.; Laporte, R.

    2003-08-01

    O ângulo sólido subtendido pelos pixels na câmara infravermelha do NexGal (CamIV) que operamos no OPD/LNA contém contribuições provenientes do sistema de coleta de fluxo propriamente dito - sendo esta a parte que interessa para as medidas astronômicas - e contribuições da obstrução central, sistema de suporte do espelho secundário e região exterior à pupila de entrada do telescópio. Estas últimas contribuições são devi-das à emissão de corpo negro à temperatura ambiente e aumentam exponencialmente para comprimentos de onda maiores que 2 micra (banda K, no infravermelho próximo). Embora a resultante pode ser quantificada e subtraída dos sinais relevantes, sua variância se adiciona à variância do sinal, e pode ser facilmente a contribuição domi-nante para a incerteza final das medidas, tornando ineficiente o processo de extração de informação e degradando a sensibilidade da câmara. A maneira clássica de resolver esse problema em sistemas ópticos que operam no infravermelho, onde os efeitos da emissão térmica do ambiente são importantes, é restringir o ângulo sólido subtendido pelos pixels individuais exclusivamente aos raios provenientes do sistema óptico. Para tanto, projeta-se uma imagem real, bastante reduzida, da pupila de entrada do sistema óptico num anteparo que transmita para o sistema de imageamento só o que interessa, bloqueando as contribuições das bordas externas à pupila de entrada, obstrução central do telescópio e sistema de suporte. Como a projeção é realizada em ambiente criogênico, a contribuição térmica espúria é efetivamente eliminada. Nós optamos por um sistema do tipo Offner para implementar na prática esta função. Trata-se de um sistema baseado em espelhos esféricos, bastante compacto e ajustado por construção. A opção por espelhos do mesmo material que o sistema de suporte (Alumínio) minimiza a dilatação diferencial, crítica nesse tipo de aplicação. Apresentamos as soluções detalhadas do projeto óptico-mecânico, bem como uma análise de flexões e desempenho em termos de qualidade de imagem.

  9. Memories of Astronomy Education in Brazil: Clippings from the Discourses of Interviewed Researchers on the Subject. (Spanish Title: Memorias de la Educación en Astronomía en Brasil: Recortes de los Discursos de Investigadores Entrevistados Acerca del Tema ) Memórias da Educação em Astronomia no Brasil: Recortes a Partir das Falas de Pesquisadores Entrevistados sobre o Tema

    NASA Astrophysics Data System (ADS)

    Iachel, Gustavo; Nardi, Roberto

    2014-12-01

    This paper presents a historical retrospective concerning data from a research in Astronomy Education in Brazil, after 1973. It was organized on the basis of the speech analysis of national researchers considered references in this field by their peers. Furthermore, it was elaborated on the basis of other studies from the areas of Science Education, Physics and Astronomy. This historical overview was developed in order to facilitate understanding of the contexts in which the interviewed researchers have developed professionally. Moreover, we attempted to recover the memory of the growing field of research in Astronomy Education in the country. We believe that the history presented can help those trying to understand the past in an attempt to resolve current and future demands. Se presenta en este artículo una retrospectiva histórica referente a datos provenientes de la investigación en enseñanza de la astronomía en el Brasil, después de 1973, organizada sobre la base del análisis de los discursos de los investigadores nacionales considerados referencias en este campo, y también en la lectura de las publicaciones en las áreas de Enseñanza de las Ciencias, Física y Astronomía. Este repaso histórico se desarrolló con el fin de facilitar la comprensión de los contextos en los que los investigadores entrevistados se han desarrollado profesionalmente. Por otra parte, se intentó recuperar la memoria del creciente campo de la investigación en Educación en Astronomía en el país. Creemos que el relato presentado puede contribuir a quien trata de comprender el pasado, en un intento de resolver las demandas actuales y futuras. Relata-se neste artigo uma retrospectiva histórica referente a dados provenientes de pesquisa em Educação em Astronomia no país, pós 1973, organizada com base na análise das falas de pesquisadores considerados referências nacionais nesse campo, como também na leitura de publicações das áreas de ensino de Ciências, Física e Astronomia. Tal panorama histórico foi desenvolvido com o intuito de favorecer nossa compreensão sobre os contextos nos quais os pesquisadores entrevistados se desenvolveram profissionalmente. Ademais, buscou-se recobrar a memória do crescente campo de pesquisa em Educação em Astronomia no país. Entendemos que o histórico apresentado possa contribuir para com os que buscam entender o passado na tentativa de solucionar demandas atuais e futuras.

  10. Esquizofrenia y trastorno en el consumo de sustancias: prevalencia y characterísticas sociodemográficas en la población Latina

    PubMed Central

    Jiménez-Castro, Lorena; Raventós-Vorst, Henriette; Escamilla, Michael

    2012-01-01

    El interés por comprender la co-morbilidad de la esquizofrenia y el trastorno en el uso de sustancias, ha aumentado debido al incremento de este diagnóstico, a los efectos negativos observados en el sujeto y a los costos en los servicios de salud. Este trastorno dual puede tener efectos dramáticos en el curso clínico del trastorno psicótico tales como: mayores recaídas, re-hospitalizaciones, síntomas más severos, no adherencia al tratamiento antipsicótico, cambios marcados del humor, aumento en el grado de hostilidad e ideación suicida, así como alteraciones en otras áreas del funcionamiento incluyendo violencia, victimización, indigencia y problemas legales. La literatura proveniente en particular de Estados Unidos y Europa sugiere que el rango de prevalencia para este diagnóstico puede oscilar entre el 10% hasta el 70%. En este estudio, revisamos la prevalencia del diagnóstico dual de esquizofrenia y trastorno en el uso sustancias, así como sus características sociodemográficas, con base en la literatura disponible alrededor del mundo dando énfasis en la poblacion latina. A pesar de que este diagnóstico es ampliamente aceptado, se conoce poco sobre su prevalencia en la población latina, sobre los factores ambientales, demográficos, clínicos y otras características de estos individuos. Un mejor conocimiento sobre este diagnóstico permitiría mejorar los métodos para la detección y adecuada valoración del trastorno en el uso de sustancias en personas con trastornos metales severos como la esquizofrenia. PMID:21404151

  11. Coerncia espectroscpica de famlias de asterides

    NASA Astrophysics Data System (ADS)

    Moth Diniz, T.; Roig, F. V.

    2003-08-01

    As Famlias de asterides so caracterizadas como agrupamentos de objetos provenientes da quebra por coliso de corpos precursores. Desta forma, seus membros devem preservar relaes genticas que podem ser traduzidas sob a anlise de suas caractersticas espectrais. Neste trabalho apresentado o primeiro estudo espectroscpico de todas as famlias de asterides do cinturo principal. Para tal, a diviso em famlias foi refeita utilizando-se o mtodo HCM com uma base de elementos prprios analticos (Knezevic e Milani, Jun 2001) e para o estudo espectroscpico foram utilizadas diversas campanhas de observao espectroscpica, tais o S3OS2 e o SMASSII, bem como outros dados disponveis na literatura. A homogeneidade espectroscpica de cada famlia foi avaliada atravs da verificao das classes espectroscpicas presentes, bem como da comparao destes espectros com os de objetos de fundo, localizados na vizinhana da famlia. Vinte e duas famlias foram analisadas (as que possuam mais do que 3 membros com espectro) e, dentre as principais concluses pode-se citar a homogeneidade espectroscpica e, provavelmente mineralgica das famlias de Vesta, Eunomia, Hoffmeister, Dora, Merxia, Agnia, Koronis e Veritas. Esta ltima em particular, foi tida como uma famlia no homognea espectroscopicamente em trabalho anterior (Di Martino et al. 1997). Outro resultado interessante , por um lado, a aparente falta de homogeneidade dos membros da famlia de Eos, e por outro sua forte distino dos objetos de fundo. O oposto ocorre na famlia de Themis, esta apresentando-se espectroscopicamente compatvel com os objetos de fundo, mas com grande homogeneidade taxonmica entre seus membros. Algumas das famlias apresentam asterides "intrusos" (objetos cujas caractersticas fsicas no so compatveis com aquelas dos membros da famlia) que, de modo geral desaparecem ao se considerarem nveis mais baixos de corte para a diviso da famlia no HCM, sem prejuzo para o agrupamento dos demais membros.

  12. Um estudo espectrofotomtrico da varivel cataclsmica V3885 Sgr

    NASA Astrophysics Data System (ADS)

    Ribeiro, F. M. A.; Diaz, M. P.

    2003-08-01

    Variveis Cataclsmicas so sistemas binrios cerrados compostos de uma an vermelha que transfere matria para uma an branca, em sistemas no magnticos ocorre a formao de um disco de acreso em torno da an branca. V3885 Sgr uma varivel cataclsmica classificada como sendo do tipo nova-like. apresentado um estudo espectrofotomtrico de V3885 Sgr de alta resoluo temporal feito na regio do visvel. A regio observada centrada em Ha e abrange tambm a linha de HeI 6678. O primeiro resultado obtido neste estudo a determinao do perodo orbital a partir de medidas da velocidade radial da linha de Ha como sendo 0,20716071(22) dias, resolvendo inconsistncias quanto a esse valor na literatura e definindo uma efemride a longo prazo para o sistema. Com este perodo e as medidas de velocidade radial do perfil de linha de Ha foi construdo um diagrama de massas, atravs do qual restringimos as massas das componentes estelares do sistema e limitamos a inclinao orbital do sistema. Foram construdos diagramas de Greenstein para as linhas de Ha e HeI, onde os espectros mdios em cada intervalo de fase so representados lado a lado em escala de cinza, indicando a existncia de uma emisso intensa proveniente da parte posterior do disco. A partir da tomografia Doppler obtivemos perfis de emissividade radial para o disco tanto para a linha de Ha como para HeI. Os resultados obtidos so comparados com os de outros sistemas estudados com a mesma tcnica. Sero apresentados tambm resultados da tomografia de flickering para o sistema.

  13. Las fulguraciones como manifestacin de reconexin en el campo magntico solar

    NASA Astrophysics Data System (ADS)

    Bagal, L. G.; Mandrini, M. C.; Rovira, M. G.; Dmoulin, P.

    Las fulguraciones solares son fenmenos transitorios de liberacin de energa que se desarrollan en las estructuras magnticas de las regiones activas del Sol. Las fulguraciones pueden llegar a liberar hasta 1032 erg en 100 seg. en todo el rango electromagntico, y acelerar partculas. En este trabajo mostramos que la ubicacin de los abrillantamientos en H? de diversas fulguraciones est relacionado con las propiedades de las conexiones de las lneas del campo magntico de la regin, como se espera por las teoras de reconexin en 3D recientemente desarrolladas (Dmoulin et al, 1996a). El campo magntico coronal se extrapola del campo fotosfrico observado suponiendo una configuracin libre de fuerzas lineal. Por medio de un algoritmo se determinan las regiones donde existe un cambio drstico en la conectividad de las lneas de campo (lmites ``cuasi-discontinuos'', o cuasi-separatrices CS). Las CS son bandas abiertas que identifican zonas donde el campo magntico se reconectar con ms probabilidad y, siempre que las mismas sean lo suficientemente finas, se producir allla liberacin de energa proveniente del campo magntico. Hemos encontrado que en todas las regiones fulgurantes estudiadas (Dmoulin et al, 1996b) existen CS en los mismos lugares donde se observaron los abrillantamientos en H?. Alldonde coinciden los abrillantamientos con las CS, stas tienen un espesor menor que 1 Mm. Las lneas de campo coronales extrapoladas de nuestro modelo tienen sus orgenes fotosfricos a ambos lados de las CS, como se espera dados los recientes estudios de reconexin magntica en 3D. Estos resultados ponen a prueba los modelos presentes sobre fulguraciones solares.

  14. Transferncias orbitais dentro do modelo quase bicircular no sistema Terra-Lua-Sol

    NASA Astrophysics Data System (ADS)

    Corra, A. A.; de Almeida Prado, A. F. B.; Stuchi, T. J.; Beaug, C.

    2003-08-01

    O problema quase bicircular planar consiste na determinao da dinmica de um corpo, de massa desprezvel, que se move sob o campo gravitacional de trs corpos. No caso estudado, o quarto corpo considerado um satlite artificial e os demais so a Terra, a Lua e o Sol, formando o sistema de trs corpos. Este modelo permite a construo de uma hamiltoniana similar a do problema restrito de trs corpos (PRTC), incluindo termos peridicos no autnomos, provenientes da presena do Sol, portanto pode ser entendido como uma perturbao ao PRTC. Suas rbitas peridicas aparecem isoladas e possuem o mesmo perodo solar. Os pontos de equilbrio colineares possuem o mesmo carter de estabilidade linear dos pontos lagrangianos (L1, L2 e L3) do PRTC, sendo do tipo sela x centro x centro, instvel na direo x e estveis nas direes y e z. As rbitas peridicas tridimensionais ao redor do ponto colinear chamada rbita Halo. O objetivo deste trabalho determinar rbitas de transferncias de baixo consumo de combustvel para um veculo espacial partindo de uma rbita de estacionamento ao redor da Terra em direo a uma rbita Halo do ponto L1, situado entre a Terra e Lua. Esta tarefa pode ser transformada no problema de valor de contorno: dado um ponto inicial na rbita de estacionamento, um ponto final na rbita halo e o tempo de transferncia, deseja-se obter a trajetria que liga estes dois pontos e que minimize os incrementos de velocidade do veculo. Essas transferncias so realizadas baseadas no mtodo de Lambert e analisadas de modo a fornecer um baixo consumo. Posteriormente, feita uma comparao de consumo com as rbitas de transferncia equivalentes do PRTC.

  15. Chemists, Access, Statistics

    NASA Astrophysics Data System (ADS)

    Holmes, Jon L.

    2000-06-01

    New JCE Internet Feature at JCE Online Biographical Snapshots of Famous Chemists is a new JCE Internet feature on JCE Online. Edited by Barbara Burke, this feature provides biographical information on leading chemists, especially women and minority chemists, fostering the attitude that the practitioners of chemistry are as human as those who endeavor to learn about it. Currently, the column features biographical "snapshots" of 30 chemists. Each snapshot includes keywords and bibliography and several contain links to additional online information about the chemist. More biographical snapshots will appear in future installments. In addition, a database listing over 140 women and minority chemists is being compiled and will be made available online with the snapshots in the near future. The database includes the years of birth and death, gender and ethnicity, major and minor discipline, keywords to facilitate searching, and references to additional biographical information. We welcome your input into what we think is a very worthwhile resource. If you would like to provide additional biographical snapshots, see additional chemists added to the database, or know of additional references for those that are already in the database, please contact JCE Online or the feature editor. Your feedback is welcome and appreciated. You can find Biographical Snapshots of Famous Chemists starting from the JCE Online home page-- click the Features item under JCE Internet and then the Chemist Bios item. Access JCE Online without Name and Password We have recently been swamped by libraries requesting IP-number access to JCE Online. With the great benefit IP-number authentication gives to librarians (no user names and passwords to administer) and to their patrons (no need to remember and enter valid names and passwords) this is not surprising. If you would like access to JCE Online without the need to remember and enter a user name and password, you should tell your librarian about our IP-number access. Current subscriptions can be upgraded to IP-number access at little additional cost. We are pleased to be able to offer to institutions and libraries this convenient mode of access to subscriber only resources at JCE Online. JCE Online Usage Statistics We are continually amazed by the activity at JCE Online. So far, the year 2000 has shown a marked increase. Given the phenomenal overall growth of the Internet, perhaps our surprise is not warranted. However, during the months of January and February 2000, over 38,000 visitors requested over 275,000 pages. This is a monthly increase of over 33% from the October-December 1999 levels. It is good to know that people are visiting, but we would very much like to know what you would most like to see at JCE Online. Please send your suggestions to JCEOnline@chem.wisc.edu. For those who are interested, JCE Online year-to-date statistics are available. Biographical Snapshots of Famous Chemists: Mission Statement Feature Editor: Barbara Burke Chemistry Department, California State Polytechnic University-Pomona, Pomona, CA 91768 phone: 909/869-3664 fax: 909/869-4616 email: baburke@csupomona.edu The primary goal of this JCE Internet column is to provide information about chemists who have made important contributions to chemistry. For each chemist, there is a short biographical "snapshot" that provides basic information about the person's chemical work, gender, ethnicity, and cultural background. Each snapshot includes links to related websites and to a biobibliographic database. The database provides references for the individual and can be searched through key words listed at the end of each snapshot. All students, not just science majors, need to understand science as it really is: an exciting, challenging, human, and creative way of learning about our natural world. Investigating the life experiences of chemists can provide a means for students to gain a more realistic view of chemistry. In addition students, especially women and minorities, need more scientist role models. When teachers weave biographical information into their conceptual lectures, they are using an effective pedagogical tool that will enhance students' understanding of chemical facts. Linking chemical ideas to real people provides a stronger infrastructure than facts alone: students need more than just the facts--they need to know the stories of the people behind the "magic". Without these stories, our students miss the wonderful, exciting, human side of our chemical sciences. Acknowledgments National Science Foundation, Alliance for Minority Progress Grant (HRD 9353276); Chemical Heritage Foundation, Philadelphia, PA; Huntington Library, San Marino, CA.

  16. Raman spectroscopy of detrital garnet from the (U)HP terrane of eastern Papua New Guinea

    NASA Astrophysics Data System (ADS)

    Andò, Sergio; Baldwin, Suzanne L.; Fitzgerald, Paul G.; Malusà, Marco G.; Aliatis, Irene; Vezzoli, Giovanni; Garzanti, Eduardo

    2013-04-01

    Garnet is one of the most widespread heavy minerals in sediments derived from orogenic systems. Its chemical composition varies systematically with temperature and pressure conditions, and thus provides information on the metamorphic evolution of source areas that is crucial in tectonic and geodynamic reconstructions. Garnet is easily identified in mineral grain mounts and is relatively stable during burial diagenesis. Raman spectroscopy allows rapid determination of garnet compositions in grain mounts or thin sections of sand and sandstone samples, and can be used to assess their density and chemical composition quite accurately ("MIRAGEM" method of Bersani et al., 2009; Andò et al., 2009). In the D'Entrecastreaux Islands of southeastern Papua New Guinea, the world's youngest (U)HP rocks are exposed. There, mafic rocks and their felsic host gneisses were metamorphosed under eclogite facies conditions from late Miocene to Pliocene, before being exhumed from depths of ~90 km (Baldwin et al., 2004, 2008). The eclogite preserves a peak assemblage of garnet, omphacite, rutile, phengite and Si02 (Hill and Baldwin, 1993). A coesite-eclogite has been found in one small island outcrop. In order to sample garnet populations representative of a larger geographical area, we sampled and studied a heavy-mineral-dominated placer sand (HMC 80) from a beach from SE Goodenough Island. Garnet grains in beach sand are associated with blue-green to subordinately green-brown amphibole and minor epidote, omphacitic clinopyroxene, titanite, apatite and rutile. The subordinate low-density fraction is feldspatho-quartzose with high-rank metamorphic rock fragments and biotite (Q62 F35 Lm2; MI 360). Detrital garnets are mostly classified as almandine with relatively high Mg and Ca and lacking Mn, typical of the eclogite facies (Win et al., 2007; type Ci garnets of Mange and Morton 2007; Andò et al., 2013). In well-described stratigraphic sequences within syn-and post-tectonic basins adjacent to orogenic systems, Raman-assisted heavy-mineral studies allow us to detect the first arrival of eclogitic garnet, and thus to assess the minimum age of exhumation and final unroofing of high-pressure rocks (Malusà et al., 2011; Malusà and Garzanti, 2012). However, in the (U)HP terrane of southeastern Papua New Guinea, sediments derived from the actively exhuming D'Entrecasteaux Island core complexes are still being deposited offshore, are rarely preserved sub-aerially, and as such stratigraphic constraints are limited. Raman analysis of detrital garnets from placer sand thus provides invaluable constraints to compare with mineral assemblages preserved in exhumed eclogites. REFERENCES Andò S., Bersani D., Vignola P., Garzanti E. 2009. Raman spectroscopy as an effective tool for high-resolution heavy-mineral analysis: Examples from major Himalayan and Alpine fluvio-deltaic systems. Spectrochim. Acta A73:450-455. Andò S., Morton A., Garzanti E. 2013. Metamorphic grade of source rocks revealed by chemical fingerprints of detrital amphibole and garnet. Geol. Soc. London Spec. Publ. Sediment Provenance Studies in Hydrocarbon Exploration & Production. Baldwin S.L., Monteleone B., Webb L.E., Fitzgerald P.G., Grove M., Hill E.J. 2004. Pliocene eclogite exhumation at plate tectonic rates in eastern Papua New Guinea. Nature 431:263-267. Baldwin S.L., Webb L.E., Monteleone B.D. 2008. Late Miocene coesite-eclogite exhumed in the Woodlark Rift. Geology 36:735-738 Bersani D., Andò S., Vignola P., Moltifiori G., Marino I.G., Lottici P.P., Diella V., 2009. Micro-Raman spectroscopy as a routine tool for garnet analysis. Spectrochim. Acta A73:484-491. Hill E.J., Baldwin S.L. 1993. Exhumation of high-pressure metamorphic rocks during crustal extension in the D'Entrecasteaux region, Papua New Guinea. J. Metam. Geol. 11:261-277. Malusà M.G., Faccenna C., Garzanti E., Polino R. 2011. Divergence in subduction zones and exhumation of high-pressure rocks (Eocene Western Alps). Earth Pl. Sci. Lett. 310:21-32. Malusà M.G., Garzanti E. 2012. Actualistic snapshot of the early Oligocene Alps: the Alps-Apennines knot detangled. Terra Nova 24:1-6. Mange M.A., Morton A.C. 2007. Geochemistry of Heavy Minerals. In: Mange, M.A. & Wright, D.T. (Eds) Heavy Minerals in Use, Developments in Sedimentology 58:345-391. Win K.S., Takeuchi M., Tokiwa T. 2007. Changes in detrital garnet assemblages related to transpressive uplifting associated with strike-slip faulting: an example from the Cretaceous System in Kii Peninsula, southwest Japan. Sedim. Geol. 201:412-431.

  17. Magnetic and ground penetrating radar surveys for the research of Medieval settlements in the inland of the Marche Region (Italy)

    NASA Astrophysics Data System (ADS)

    Bavusi, M.; Giocoli, A.; Balasco, M.; Favulli, G.; Moscatelli, U.; Minguzzi, S.; Gnesi, D.; Virgili, S.

    2009-04-01

    This work was carried out in the framework of the R.I.M.E.M. project (Research on Medieval settlements in the inland of the Marche Region, Italy.) leaded by the Universities of Macerata and Udine and having the aim to produce a significant contribution for the comprehension of the settlement process in the Central and Southern Italy during the Late Roman Period and Early Middle Ages. Then, an extensive gradiometric survey were carried out, by using a vapour caesium magnetometer, in the area included amongst the municipal districts of Caldarola, Cessapalombo and San Ginesio, sited in the area closed to Macerata between the valleys of Chienti and Fiastra rivers. Moreover, in the most interesting areas, a 400 MHz 3D ground penetrating radar (GPR)survey was carried out in order to get the precise overlapping with the magnetic method. The Magnetic method is now a standard practice in the archaeological research taken into great consideration for its non-destructivity and quickness and its capability of mapping wide areas in quite a short lapse of time (Bavusi et al., 2008). Moreover the method provides an information well correlable with remote sensing data (Gallo et al, 2008). The GPR method is extremely useful for archaeologists thanks to its non-destructivity and capability of giving real-time and high-resolution data (Basile et al., 2000). Today the effectiveness of this method was improved by powerful 3D visualisation methods as well as 3D space, time or depth slices and iso-amplitude surfaces, too (Nuzzo et al., 2002). The integrations of several geophysical methods are usual (Sambuelli et al.1999, De Domenico et al., 2001; Chianese et al., 2004) particularly when a simple comparison in cross section along the same profiles can be performed. In this work the overlapping between two kinds of data was complicated by different outputs coming from two methods: maps for the magnetic method and cross sections for the GPR one. The 3D survey design for the GPR survey and a complex processing routine was carried out in order to get both data volumes and time slices, more easily comparable with magnetic maps. Magnetic data processing included spike removal and destripe. Finally, the results revealed the presence of several target of archaeological interest and, where two methods were carried out, the results are consistent. M. Bavusi , A. Giocoli, e. Rizzo, v. Lapenna (2008). Geophysical characterisation of Carlo' s V Castle (Crotone, Italy). Journal of Applied Geophysics. DOI: 10.1016/j.jappgeo.2008.09.002. Basile V., Carrozzo M.T., Negri S., Nuzzo L., Quarta T., Villani A.V., (2000). A ground-penetrating radar survey for archaeological investigations in an urban area - Lecce, Italy. Journal of Applied Geophysics, 44, 15-32. Chianese D., D'Emilio M., Di Salvia S., Lapenna V., Ragosta M., Rizzo E. (2004). Magnetic Mapping, Ground Penetrating Radar Surveys and Magnetic Susceptibility Measurements for the Study of the Archaeological Site of Serra di Vaglio (Southern Italy). Journal of Archaeological Science, 31, 633-643. De Domenico D., Giannino F., Marino A., Nuzzo L., Rizzo E., (2001). Indagini elettriche e radar: integrazione dei metodi nello studio dei resti sepolti del monastero normanno in s. Marco D'Alunzio (Messina). Atti del 21° Convegno Nazionale del GNGTS, 351-353. GalloD., Ciminale M., Beckerb H. and Masini N. (2008). Remote sensing techniques for reconstructing a vast Neolithic settlement in Southern Italy. Journal of Archaeological Science, DOI:10.1016/j.jas.2008.07.002. Nuzzo L., Leucci, G . Negri S., Carrozzo M. T. and Quarta T., (2002). Application of 3D visualization techniques in the analysis of GPR data for archaeology. Annals of Geophysics, 45 (2), 321-337. Sambuelli L., Socco L.V., Brecciaroli L., (1999). Acquisition and processing of electric, magnetic and GPR data on a Roman site(Victimulae, Salussola, Biella), Journal of Applied Geophysics, 41, 189-204

  18. Tanque Loma, a new late-Pleistocene megafaunal tar seep locality from southwest Ecuador

    NASA Astrophysics Data System (ADS)

    Lindsey, Emily L.; Lopez R., Eric X.

    2015-01-01

    Fossil deposits in the petroleum-rich sediments of the Santa Elena Peninsula in southwestern Ecuador contain some of the largest and best-preserved assemblages of Pleistocene megafaunal remains known from the neotropics, and thus represent an opportunity to greatly expand our knowledge of Pleistocene paleoecology and the extinction of Quaternary megafauna in this region. This paper reports data from excavations at Tanque Loma, a late-Pleistocene locality on the Santa Elena Peninsula that preserves a dense assemblage of megafaunal remains in hydrocarbon-saturated sediments along with microfaunal and paleobotanical material. The megafauna bones are concentrated in and just above a ∼0.5 m thick asphaltic layer, but occur sparsely and with poorer preservation up to 1 m above this deposit. Several meters of presumed-Holocene sediments overlying the megafauna-bearing strata are rich in bones of microvertebrates including birds, squamates, and rodents. These are interpreted as raptor assemblages. While over 1000 megafaunal bones have been identified from the Pleistocene strata at Tanque Loma, more than 85% of these remains pertain to a single species, the giant ground sloth Eremotherium laurillardi. Only five other megafauna taxa have been identified from this site, including Glossotherium cf. tropicorum, Holmesina occidentalis, cf. Notiomastodon platensis, Equus (Amerhippus) c.f. santaeelenae, and a cervid tentatively assigned to cf. Odocoileus salinae based on body size and geography. No carnivores have yet been identified from Tanque Loma, and microvertebrate remains are extremely rare in the Pleistocene deposits, although terrestrial snail shells and fragmented remains of marine invertebrates are occasionally encountered. Accelerator Mass Spectrometry radiocarbon dates on Eremotherium and cf. Notiomaston bones from within and just above the asphaltic layer yielded dates of ∼17,000 - 23,500 radiocarbon years BP. Taken together, the taxonomic composition, taphonomy, geologic context, and sedimentology of Tanque Loma suggest that this site represents a bone bed assemblage in a heavily vegetated, low-energy riparian environment with secondary infiltration of asphalt that helped to preserve the bones. The predominance of Eremotherium fossils at this site indicate that it may have been an area where these animals congregated, suggesting possible gregarious behavior in this taxon. The radiocarbon dates so far obtained on extinct taxa at Tanque Loma are consistent with a model positing earlier extinctions of megafauna in tropical South America than of related taxa further south on the continent, although this pattern may be an artifact of low sampling in the region. xml:lang="es" Aunque más de 1.000 huesos de megafauna han sido identificados en los estratos del Pleistoceno en Tanque Loma, más del 85% de esos mismos pertenecen a una sola especie, el perezoso gigante Eremotherium laurillardi. Sin embargo, otros cinco taxones de megafauna han sido recuperados de este sitio, los cuales son: Glossotherium cf. G. tropicorum, Holmesina occidentalis, cf. Notiomastodon platensis, Equus (Amerhippus) c.f. santaelenae y un cérvido identificado tentativamente en base a tamaño y geografía como cf. Odocoileus salinae. Ningún carnívoro ha sido identificado aún en Tanque Loma, y los restos de microvertebrados son muy raros en los estratos del Pleistoceno, aunque las conchas de caracol terrestre y los restos fragmentados de invertebrados marinos son encontrados ocasionalmente dentro de esas capas. Los fechados de radiocarbono por espectrómetro de acelerador de masas (AMS) en huesos de Eremotherium y cf. Notiomastodon de la capa de asfalto y por encima de esta resultaron en ∼17,000-23,500 años radiocarbónicos AP. En conjunto, la tafonomía, la composición taxonómica, el contexto geológico, y la sedimentolgía del sitio Tanque Loma surgieren que esta localidad representa un yacimiento depositado en un ambiente ribereño con bajo flujo y vegetación densa, con infiltraciones secundarias de asfalto lo que ayudó a preservar los huesos. El predominio de fósiles de Eremotherium indican que esta podría haber sido una área donde estos animales se congregaban, sugiriendo un posible comportamiento gregario de este taxón. Las fechas radiocarbónicas obtenidas hasta ahora en taxones extinguidos de Tanque Loma son consistente con el modelo postulado sobre la extinción de la megafauna, la cual habría sido más temprana en las regiones tropicales de Sudamérica que al sur del continente. Sin embargo, este patrón podría ser un artefacto del bajo muestreo en la región.

  19. A preliminary inventory of the catfishes of the lower Rio Nhamundá, Brazil (Ostariophysi, Siluriformes)

    PubMed Central

    Duarte Ribeiro, Emanuell; Nogueira Machado, Valéria; Hrbek, Tomas; Farias, Izeni Pires

    2015-01-01

    Abstract The Rio Nhamundá is a poorly-known clearwater river draining the southern Guiana Shield of Brazil. In this study we report the findings of a preliminary ichthyological survey, focusing on catfishes (Siluriformes). We identify a total of 36 species (31 genera, seven families) from the Nhamundá, including 11 species already recorded from the river. Overall, our survey results show that even rapid surveys can provide important information on Amazon fish biodiversity, suggesting potential new species, providing range extensions for nominal species, and additionally highlighting taxa in need of taxonomic revision and genetic study. As well as the traditional forms of data collected on biodiversity surveys (i.e. preserved specimen vouchers), our study also provides "new" types of data in the form of DNA barcodes and images of fishes exhibiting colouration in life, information that will be invaluable in future work addressing difficult groups. O Rio Nhamundá é um rio de água clara, pouco conhecido, que drena parte do Escudo das Guianas em território brasileiro. Nesse estudo, nós reportamos os resultados de um levantamento ictiofaunístico preliminar dessa área, tendo como foco os bagres (Siluriformes). Nós identificamos um total de 36 espécies (31 gêneros, sete famílias) provenientes de nossa coleta, e adicionamos 11 espécies já conhecidas para o rio. De maneira geral, os resultados de nossa pesquisa mostram que mesmo levantamentos rápidos podem gerar informações importantes sobre a biodiversidade de peixes amazônicos, sugerindo potenciais espécies novas, ampliando a área de distribuição de espécies, além de apontar a necessidade de revisões taxonômicas e estudos genéticos para alguns taxa. Para além das formas tradicionais de dados coletados em pesquisas de biodiversidade (i.e. espécimes preservados), nosso estudo fornece "novas" formas de dados, como DNA barcodes e imagens com o padrão de coloração dos espécimes vivos, informações essas que serão de valor inestimável para futuros estudos que abordem grupos taxonômicos difíceis. PMID:25977611

  20. A preliminary inventory of the catfishes of the lower Rio Nhamundá, Brazil (Ostariophysi, Siluriformes).

    PubMed

    Collins, Rupert A; Duarte Ribeiro, Emanuell; Nogueira Machado, Valéria; Hrbek, Tomas; Farias, Izeni Pires

    2015-01-01

    The Rio Nhamundá is a poorly-known clearwater river draining the southern Guiana Shield of Brazil. In this study we report the findings of a preliminary ichthyological survey, focusing on catfishes (Siluriformes). We identify a total of 36 species (31 genera, seven families) from the Nhamundá, including 11 species already recorded from the river. Overall, our survey results show that even rapid surveys can provide important information on Amazon fish biodiversity, suggesting potential new species, providing range extensions for nominal species, and additionally highlighting taxa in need of taxonomic revision and genetic study. As well as the traditional forms of data collected on biodiversity surveys (i.e. preserved specimen vouchers), our study also provides "new" types of data in the form of DNA barcodes and images of fishes exhibiting colouration in life, information that will be invaluable in future work addressing difficult groups. O Rio Nhamundá é um rio de água clara, pouco conhecido, que drena parte do Escudo das Guianas em território brasileiro. Nesse estudo, nós reportamos os resultados de um levantamento ictiofaunístico preliminar dessa área, tendo como foco os bagres (Siluriformes). Nós identificamos um total de 36 espécies (31 gêneros, sete famílias) provenientes de nossa coleta, e adicionamos 11 espécies já conhecidas para o rio. De maneira geral, os resultados de nossa pesquisa mostram que mesmo levantamentos rápidos podem gerar informações importantes sobre a biodiversidade de peixes amazônicos, sugerindo potenciais espécies novas, ampliando a área de distribuição de espécies, além de apontar a necessidade de revisões taxonômicas e estudos genéticos para alguns taxa. Para além das formas tradicionais de dados coletados em pesquisas de biodiversidade (i.e. espécimes preservados), nosso estudo fornece "novas" formas de dados, como DNA barcodes e imagens com o padrão de coloração dos espécimes vivos, informações essas que serão de valor inestimável para futuros estudos que abordem grupos taxonômicos difíceis. PMID:25977611

  1. Astronomy Teaching and Teachers Continuing Education: the Interdisciplinarity during a Total Lunar Eclipse. (Spanish Title: Enseñanza de la Astronomía y la Formación Continua de Profesores: la Interdisciplinariedad Durante un Eclipse Total de Luna.) Educação EM Astronomia E Formação Continuada de Professores: a Interdisciplinaridade Durante um Eclipse Lunar TOTAL

    NASA Astrophysics Data System (ADS)

    Langhi, Rodolfo

    2009-07-01

    This paper describes how 67 teachers from 23 cities, could awaken, in students, the scientific interest, using a natural astronomical phenomenon: a total lunar eclipse. Before and after of eclipse, meetings for continuing education were characterized by interdisciplinarity of astronomy and the importance of these observations. Working groups were formed by teachers and students, who organized the survey data, mobilizing the people in their cities. The results point ways about how to provide the scientific culture and the motivation to learn science in students, using approaches between the following communities: scientific, amateur and school. En este artículo se describe cómo 67 profesores de 23 ciudades, despertó el interés científico en los estudiantes mediante un fenómeno astronómico: un eclipse total de Luna. Antes y después del eclipse, reuniones para la formación continua se centraron en la interdisciplinariedad de la astronomía, y la importancia de las observaciones de este tipo de fenómeno. Profesores y estudiantes formaron grupos de trabajo para investigar datos durante el eclipse, con el participación de la comunidad en sus ciudades. Los resultados apuntan a las opciones que conducen a la cultura científica y la motivación para aprender la ciencia, utilizando las relaciones de los siguientes grupos: científicos, aficionados y la escuela. Este texto relata como 67 professores, provenientes de 23 cidades, puderam despertar, nos alunos, o interesse científico utilizando um fenômeno natural astronômico: um eclipse lunar total. O evento foi precedido e procedido por encontros de formação continuada, onde se caracterizou a interdisciplinaridade da astronomia e a importância das observações de fenômenos como estes. Grupos de trabalho foram formados por professores e alunos, que se organizaram para o levantamento conjunto de dados durante o fenômeno, além do envolvimento da comunidade em suas respectivas cidades. Os resultados apontam para caminhos que podem proporcionar a motivação e a cultura científica, através de aproximações entre as comunidades científica, amadora e escolar.

  2. Correlação de longo alcance em sistemas binários de raios-x usando remoção de flutuações

    NASA Astrophysics Data System (ADS)

    Pereira, M. G.; Moret, M. A.; Zebende, G. F.; Nogueira, E., Jr.

    2003-08-01

    Neste trabalho é proposta uma metodologia de analise de series temporais de fontes astrofísicas, baseada no método proposto por Peng et al. (1994) e Liu et al. (1999), o qual consiste na idéia de que uma série temporal correlacionada pode ser mapeada por um processo de busca de auto-similaridades em diversas escalas de tempo n. Removendo as eventuais tendências e integrando o sinal observado, é obtida uma medida do desvio médio quadrático das flutuações do sinal integrado F(n)~na, onde a representa o fator de escala associado com a auto-similaridade da correlação de longo alcance do sinal. Baseado nos valores obtidos de a, é possível distinguir entre os casos de sinais não-correlacionados, tipo ruído branco (a = 0,5), sinal anti-persistentes (a < 0,5) e sinal persistente (a > 0,5). Usando esta metodologia, foram analisadas 129 curvas de luz de sistemas binários de raios-X, provenientes do banco de dados públicos de observações feitas pelo instrumento All Sky Monitor, a bordo do satélite Rossi X-Ray Timing Explorer (ASM-RXTE). Foram identificadas a presença de a'0,5 em mais de 90% dos sistemas estudados, implicando em dizer que as flutuações de intensidade observadas apresentam correlação de auto-similaridade, sem entretanto, indícios de apresentarem uma escala de tempo característica das flutuações de intensidade. Sistemas onde são observadas erupções (flares), apresentam sistematicamente a > 0,5, característica esta, possivelmente associada com persistência das flutuações de densidade de disco ou taxa de acréscimo de massa. Os sistemas com curvas de luz onde nao são observadas as erupções apresentam uma distribuição normal centrada em a~0,62+/-0,10. Referências ¾ Peng, C.-K., Buldyrev, S.V., Havlin, S., Simons, M., Stanley, H.E., e Goldberg, A.L., Phys. Rev. E, (49), 1685 (1994). ¾ Liu, Y., Gopikrishnan, P., Cizeau, P., Meyer, M., Peng,C.-K., e Stanley, H.E., Phys. Rev. E, (60), 1390 (1999).

  3. Courtship behavior of different wild strains of Ceratitis Capitata (Diptera: Tephritidae)

    SciTech Connect

    Briceno, D.; Eberhard, W.; Vilardi, J.; Cayol, J.-P.; Shelly, T.

    2007-03-15

    This study documents differences in the courtship behavior of wild strains of Ceratitis capitata (Wiedemann) from Madeira (Portugal), Hawaii (U.S.A.), Costa Rica, and Patagonia (Argentina). Some traits showed large variations and others substantial overlaps. The angle at which the male faced toward the female at the moment of transition from continuous wing vibration and intermittent buzzing changed very little during the course of courtship in all strains, but males from Madeira tended to face more directly toward the female than other males. Females tended to look more, and more directly, toward the males as courtship progressed in all strains. The distance between male and female tended to decrease as courtship proceeded in all strains, but the distances at which males initiated continuous vibration, intermittent buzzing, and jumped onto the female were relatively less variable between strains, except for the strain from Costa Rica. Flies of Madeira courted for longer and the male moved his head and buzzed his wings longer than the other strains. (author) [Spanish] Este estudio documenta diferencias en el comportamiento de cortejo de cepas silvestres de Ceratitis capitata (Wied.) provenientes de Madeira (Portugal), Hawaii (Estados Unidos de Norte America), Costa Rica y Patagonia (Argentina). Algunas caracteristicas mostraron grandes variaciones y traslape substancial. Los angulos a los cuales los machos miraron hacia las hembras cambiaron muy poco en el momento de la transicion de la vibracion continua al zumbido intermitente durante el curso del cortejo en todo las cepas, pero los machos de Madeira tendieron a enfrentar mas directamente a la hembra que otros machos. Los angulos de las hembras disminuyeron claramente durante el cortejo en todas las cepas. La distancia entre el macho y la hembra tendio a disminuir conforme el cortejo continuaba en todas las cepas, pero las distancias a las cuales los machos iniciaron la vibracion continua, el zumbido intermitente, y el salto sobre la hembra eran relativamente menos variables entre cepas excepto la cepa de Costa Rica. Moscas de Madeira cortejaron mas tiempo y el macho moviosu cabeza y zumbaba sus alas mas prolongadamente que las otras cepas. (author)

  4. Maize x Teosinte Hybrid Cobs Do Not Prevent Crop Gene Introgression.

    PubMed

    Chavez, Nancy B; Flores, Jose J; Martin, Joseph; Ellstrand, Norman C; Guadagnuolo, Roberto; Heredia, Sylvia; Welles, Shana R

    2012-06-01

    Maize x Teosinte Hybrid Cobs Do Not Prevent Crop Gene Introgression. Whether introgression from crops to wild relatives can occur is an important component of transgene risk assessment. In the case of maize, which co-occurs with its wild relative teosinte in Mexico, the possibility of introgression has been controversial. Maize is cross-compatible with teosinte, and spontaneous hybridization is known to occur. Some scientists have hypothesized that the maize x teosinte cob infructescence will prevent progeny dispersal, thus preventing introgression. Motivated by a prior study where we found maize x teosinte hybrid fruits naturally dispersed under field conditions, we tested whether hybrid cobs hold their fruits as tightly as maize cobs. We found the force required to detach hybrid fruits was substantially and significantly less than that for maize. Consequently, we expect that introgression of transgenes from maize into teosinte in Mexico should occur largely unimpeded by the hybrid cob.La mazorca o elote hbrido de maz x teocintle no impide la introgresin de genes transgnicos provenientes del cultivo. La introgresin entre el maz cultivado y el maz silvestre, o teocintle, es un componente importante en la evaluacin ambiental relacionada con los riesgos de la introduccin de genes transgnicos. La posibilidad de introgresin entre el maz domesticado y el teocintle ha sido un tema controversial, en particular en Mxico, donde maz y teocintle coexisten. El maz es compatible con el teocintle y la hibridizacin espontnea ocurre entre ellos. Algunos cientficos han planteado como hiptesis que al cruzar el maz con teocintle, la estructura interna de la infrutescencia que sujeta los frutos conocida como la mazorca de maz o el elote, impide la dispersin de la progenie evitando que la introgresin ocurra. Los resultados de un estudio previo evidencian la dispersin de los frutos hbridos del maz x teocintle en condiciones naturales. Motivados por estos resultados, hemos decidido investigar si la mazorca o el elote de las infrutescencias del hbrido sujetan los frutos con una fuerza comparable o mayor a la del maz. Nuestras mediciones implican que la fuerza necesaria para liberar los frutos hbridos son substancial y significativamente menores que aquellas necesarias para desprender los frutos del maz. Como conclusin sugerimos que en Mxico, la mazorca o el elote no representan una barrera que impida la introgresin de los genes transgnicos del maz al teocintle. PMID:22707759

  5. Accuracy of CFC groundwater dating in a crystalline bedrock aquifer: Data from a site in southern Sweden

    NASA Astrophysics Data System (ADS)

    Bockgrd, Niclas; Rodhe, Allan; Olsson, K. A.

    The concentrations of chlorofluorocarbons (CFC-11, CFC-12, and CFC-113) and tritium were determined in groundwater in fractured crystalline bedrock at Finnsjn, Sweden. The specific goal was to investigate the accuracy of CFC dating in such an environment, taking potential degradation and mixing of water into consideration. The water was sampled to a depth of 42 m in three boreholes along an 800-m transect, from a recharge area to a local discharge area. The CFC-113 concentration was at the detection limit in most samples. The apparent recharge date obtained from CFC-11 was earlier than from CFC-12 for all samples, with a difference of over 20 years for some samples. The difference was probably caused by degradation of CFC-11. The CFC-12 dating of the samples ranged from before 1945 to 1975, with the exception of a sample from the water table, which had a present-day concentration. Conclusions about flow paths or groundwater velocity could not be drawn from the CFCs. The comparison between CFC-12 and tritium concentrations showed that most samples could be unmixed or mixtures of waters with different ages, and the binary mixtures that matched the measured concentrations were determined. The mixing model approach can be extended with additional tracers. Prcision de la datation au CFC dans un aquifre rocheux-fractur: donnes d'un site du sud de la Sude. Les concentrations en chlorofluorocarbones (CFC-11, CFC-12, CFC-113) et entritium ont t dtermines dans l'eau souterraine d'un massif fractur Finnsjn en Sude. Le but de cette tude est de mieux cerner la prcision de la mthode de datation au CFC dans ce type d'environnement hydrogologique, tout en considrant d'ventuels phnomnes de dgradation et de mlange d'eaux. L'eau a t chantillonne une profondeur de 42 mtres dans trois forages aligns sur 800 mtres entre une zone de recharge et une zone de dversement. Les concentrations en CFC-113 sont dans la plupart des chantillons la limite de dtection. Pour tous les chantillons, la date de la recharge tablie avec le CFC-11 est antrieure la date tablie avec le CFC-12. La diffrence entre les deux dates peut dpasser 20 ans et s'explique-probablement-par la dgradation du CFC-11. Les dates de recharge de la nappe mesures au CFC-12 sont comprises entre 1945 et 1975, except pour un chantillon qui possde une concentration actuelle. Il n'est pas possible de tirer des conclusions concernant la direction des coulements et la vitesse de l'eau souterraine. La comparaison entre CFC-12 et tritium montre que des chantillons pourraient tre soit le rsultat du mlange d'eaux d'ges diffrents, soit des chantillons non-mlangs. Dans le cas d'un mlange binaire, les rapports du mlange composant la concentration mesure sont dtermins. L'approche par modle de mlange peut tre tendue des traceurs additionnels. Precisin en la datacin de aguas subterrneas utilizando CFC en un acufero de rocas cristalinas: datos provenientes de un sitio al sur de Suecia. Se determinaron las concentraciones de clorofluorucarbonos (CFC-11, CFC-12, y CFC-113) y de tritio en aguas subterrneas alojadas en rocas cristalinas fracturadas de Finnsjn, Suecia. El objetivo especfico consisti en investigar la precisin de la datacin de aguas subterrneas con CFC en este tipo de ambiente, tomando en consideracin la degradacin potencial y la mezcla de agua. Las muestras de agua se tomaron a una profundidad de 42 m en tres pozos ubicados a lo largo de una lnea de 800 m transversal a una zona de recarga y de zona de descarga local. En la mayora de las muestras se encontr que la concentracin de CFC-113 estuvo en el lmite de deteccin. La edad que se estim en todas las muestras para la recarga aparente en base a CFC-11 fue ms joven que la edad proveniente de CFC-12, con una diferencia de ms de 20 aos para algunas muestras. Esta diferencia fue causada probablemente por la degradacin del CFC-11. La datacin CFC-12 de las muestras vari de antes de 1945 a 1975, con la excepcin de una muestra tomada en el nivel fretico, la cual present concentracin actual. No fue posible obtener conclusiones acerca de las trayectorias de flujo o la velocidad de agua subterrnea a partir de los CFCs. La comparacin entre las concentraciones de CFC-12 y tritio mostr que la mayora de las muestras pueden tener composicin sencilla o bien consistir de mezclas de aguas de diferentes edades. Esta comparacin tambin permiti determinar las mezclas binarias que corresponden a las concentraciones medidas. Pueden utilizarse trazadores adicionales para ampliar el modelo de mezclas propuesto.

  6. Microbial degradation of chloroethenes in groundwater systems

    NASA Astrophysics Data System (ADS)

    Bradley, Paul M.

    The chloroethenes, tetrachloroethene (PCE) and trichloroethene (TCE) are among the most common contaminants detected in groundwater systems. As recently as 1980, the consensus was that chloroethene compounds were not significantly biodegradable in groundwater. Consequently, efforts to remediate chloroethene-contaminated groundwater were limited to largely unsuccessful pump-and-treat attempts. Subsequent investigation revealed that under reducing conditions, aquifer microorganisms can reductively dechlorinate PCE and TCE to the less chlorinated daughter products dichloroethene (DCE) and vinyl chloride (VC). Although recent laboratory studies conducted with halorespiring microorganisms suggest that complete reduction to ethene is possible, in the majority of groundwater systems reductive dechlorination apparently stops at DCE or VC. However, recent investigations conducted with aquifer and stream-bed sediments have demonstrated that microbial oxidation of these reduced daughter products can be significant under anaerobic redox conditions. The combination of reductive dechlorination of PCE and TCE under anaerobic conditions followed by anaerobic microbial oxidation of DCE and VC provides a possible microbial pathway for complete degradation of chloroethene contaminants in groundwater systems. Résumé Les chloroéthanes, tétrachloroéthane (PCE) et trichloroéthane (TCE) sont parmi les polluants les plus communs trouvés dans les aquifères. Depuis les années 1980, on considère que les chloroéthanes ne sont pas significativement biodégradables dans les aquifères. Par conséquent, les efforts pour dépolluer les nappes contaminées par des chloroéthanes se sont limités à des tentatives de pompage-traitement globalement sans succès. Des travaux ultérieurs ont montré que dans des conditions réductrices, des micro-organismes présents dans les aquifères peuvent, par réduction, dégrader les PCE et TCE en composés moins chlorés, comme le dichloréthane (DCE) et le chlorure de vinyl (VC). Bien que des études de laboratoire réalisées avec des micro-organismes adaptés aux composés halogénés montrent que la réduction complète en éthane est possible, dans la plupart des nappes la réaction de déchloration par réduction s'arrête apparemment au DCE et au VC. Cependant, des recherches récentes menées sur des sédiments d'un aquifère et d'alluvions ont démontré que l'oxydation microbienne de ces descendants réduits peut se produire de manière significative dans des conditions de redox anérobies. La déchloration par réduction de PCE et de TCE dans des conditions anérobies suivie par une oxydation microbienne anérobie des DCE et VC fournit une piste microbienne possible pour obtenir une dégradation complète des chloroéthanes polluants dans les aquifères. Resumen Los cloroetanos (tetracloroetano PCE y tricloroetano TCE) son contaminantes muy habituales en los acuíferos. Hasta 1980 se consideraba que los cloroetanos no eran biodegradables y, por tanto, los métodos de rehabilitación en acuíferos contaminados con cloroetanos se limitaban al pump-and-treat, generalmente con poco éxito. Posteriormente se vio que, en condiciones reductoras, algunos microorganismos pueden reducir PCE y TCE a unos subproductos menos clorados, como el dicloroetano (DCE) y el cloruro de vinilo (VC). Aunque estudios de laboratorio recientes sugieren que la reducción completa a etano es posible, en la mayoría de los sistemas acuíferos la decloración suele detenerse en los DCE o VC. Sin embargo, investigaciones más recientes en acuíferos y sedimentos fluviales demuestran que la oxidación microbiana de estos subproductos puede ser importante bajo condiciones redox anaerobias. La combinación de la reducción de PCE y TCE en condiciones anaerobias seguida de la oxidación microbiana anaerobia de DCE y VC proporciona un método potencial para la degradación total de los cloroetanos en los sistemas acuíferos.

  7. A thick lens of fresh groundwater in the southern Lihue Basin, Kauai, Hawaii, USA

    NASA Astrophysics Data System (ADS)

    Izuka, Scot; Gingerich, Stephen

    2002-11-01

    A thick lens of fresh groundwater exists in a large region of low permeability in the southern Lihue Basin, Kauai, Hawaii, USA. The conventional conceptual model for groundwater occurrence in Hawaii and other shield-volcano islands does not account for such a thick freshwater lens. In the conventional conceptual model, the lava-flow accumulations of which most shield volcanoes are built form large regions of relatively high permeability and thin freshwater lenses. In the southern Lihue Basin, basin-filling lavas and sediments form a large region of low regional hydraulic conductivity, which, in the moist climate of the basin, is saturated nearly to the land surface and water tables are hundreds of meters above sea level within a few kilometers from the coast. Such high water levels in shield-volcano islands were previously thought to exist only under perched or dike-impounded conditions, but in the southern Lihue Basin, high water levels exist in an apparently dike-free, fully saturated aquifer. A new conceptual model of groundwater occurrence in shield-volcano islands is needed to explain conditions in the southern Lihue Basin. Rsum. Dans le sud du bassin de Lihue (Kauai, Hawaii, USA), il existe une paisse lentille d'eau souterraine douce dans une vaste rgion faible permabilit. Le modle conceptuel conventionnel pour la prsence d'eau souterraine Hawaii et dans les autres les de volcans en bouclier ne rend pas compte d'une lentille d'eau douce si paisse. Dans ce modle conceptuel, les accumulations de lave dont sont forms la plupart des volcans en bouclier couvrent de vastes rgions relativement forte permabilit, avec des lentilles d'eau douce peu paisses. Dans le sud du bassin de Lihue, les laves remplissant le bassin et les sdiments constituent une rgion tendue faible conductivit hydraulique rgionale, qui, sous le climat humide du bassin, est sature presque jusqu' sa surface; les surfaces pizomtriques sont plusieurs centaines de mtres au-dessus du niveau de la mer quelques kilomtres de la cte. On pensait jusqu' prsent que des niveaux pizomtriques aussi levs dans des les de volcans en bouclier n'existaient que dans le cas de nappes perches ou de blocage par un dyke, mais dans le sud du bassin de Lihue, des niveaux pizomtriques levs existent dans un aquifre apparemment sans dyke et compltement satur. Un nouveau modle conceptuel de prsence d'eau souterraine dans les les de volcans en bouclier est ncessaire pour expliquer les conditions observes dans le sud du bassin de Lihue. Resumen. Se ha determinado la existencia de un espeso lentejn de aguas subterrneas dulces en una extensa regin de baja permeabilidad situada al sur de la cuenca de Lihue, en Kauai (Hawaii, Estados Unidos de Amrica). El modelo conceptual convencional de las aguas subterrneas en Hawai y en otros cinturones de islas volcnicas no considera la existencia de lentejones tan gruesos de agua dulce. En dicho modelo, las acumulaciones de flujos de lava que constituyen la mayora de los cinturones volcnicos se desarrollan en grandes reas de permeabilidad relativamente baja y con pequeos lentejones de agua dulce. En el sur de la cuenca de Lihue, las lavas de relleno y los sedimentos forman una regin extensa de baja conductividad hidrulica regional que, con el clima hmedo de la zona, est saturada hasta prcticamente la superficie del terreno, mientras que el nivel fretico se encuentra centenares de metros por encima del nivel del mar a pocos kilmetros de la lnea de costa. Se crea hasta ahora que, en los cinturones de islas volcnicas, tales niveles slo tenan lugar en acuferos colgados o en condiciones de confinamiento por diques, pero, al sur de la cuenca de Lihue, se dan en acuferos completamente saturados que no estn limitados por diques. Se necesita un nuevo modelo conceptual de las aguas subterrneas en cinturones de islas volcnicas para explicar las condiciones halladas en la cuenca meridional de Lihue.

  8. Spatial characteristics of groundwater temperature in the Ishikari Lowland, Hokkaido, northern Japan: analytical and numerical applications

    NASA Astrophysics Data System (ADS)

    Dim, J. R.; Sakura, Y.; Fukami, H.; Miyakoshi, A.

    2002-03-01

    In porous sediments of the Ishikari Lowland, there is a gradual increase in the background geothermal gradient from the Ishikari River (3-4 °C 100 m-1) to the southwest highland area (10 °C 100 m-1). However, the geothermal gradient at shallow depths differs in detail from the background distribution. In spite of convective heat-flow loss generally associated with groundwater flow, heat flow remains high (100 mW m-2) in the recharge area in the southwestern part of the Ishikari basin, which is part of an active geothermal field. In the northeastern part of the lowland, heat flow locally reaches 140 mW m-2, probably due to upward water flow from the deep geothermal field. Between the two areas the heat flow is much lower. To examine the role of hydraulic flow in the distortion of the isotherms in this area, thermal gradient vs. temperature analyses were made, and they helped to define the major components of the groundwater-flow system of the region. Two-dimensional simulation modeling aided in understanding not only the cause of horizontal heat-flow variations in this field but also the contrast between thermal properties of shallow and deep groundwater reservoirs. Résumé. Dans les sédiments poreux des basses terres d'Ishikari, on observe une augmentation graduelle du gradient géothermal général depuis la rivière Ishikari (3-4 °C 100 m-1) vers la zone élevée située au sud-ouest (10 °C 100 m-1). Toutefois, le gradient géothermal aux faibles profondeurs diffère dans le détail de la distribution générale. Malgré la perte de flux de chaleur par convection, généralement associée aux écoulements souterrains, le flux de chaleur reste élevé (100 mW m-2) dans la zone de recharge de la partie sud-ouest du bassin de l'Ishikari, qui appartient à un champ géothermal actif. Dans la partie nord-est des basses terres, le flux de chaleur atteint localement 140 mW m-2, probablement à cause d'un écoulement souterrain ascendant depuis le champ géothermal profond. Entre les deux zones, le flux de chaleur est beaucoup plus faible. Afin de déterminer le rôle du flux d'eau souterraine dans la distorsion des isothermes dans cette zone, des analyses du gradient thermal en fonction de la température ont été réalisées elles ont permis de définir les composantes majeures du système aquifère régional. Une modélisation deux-dimensionnelle pour la simulation a ensuite contribué à la compréhension non seulement de la cause des variations horizontales du flux de chaleur dans cette région, mais également du contraste entre les propriétés des réservoirs superficiel et profond. Resumen. En los sedimentos porosos de las tierras bajas de Ishikari, hay un incremento gradual en el gradiente geotérmico desde el río Ishikari (3-4 °C 100 m-1) hacia la zona elevada del sudoeste (10 °C 100 m-1). Sin embargo, el gradiente geotérmico a profundidades someras difiere de la distribución de fondo. A pesar de las pérdidas por el flujo convectivo de calor asociadas generalmente al flujo de aguas subterráneas, el flujo de calor permanece elevado (100 mW m-2) en el área de recarga, hacia el sudoeste de la cuenca del Ishikari, la cual pertenece a un campo geotérmico activo. Al nordeste de las tierras bajas, el flujo de calor alcanza 140 mW m-2, probablemente por el flujo ascendente de agua procedente del campo geotérmico profundo. Entre ambas áreas, el flujo de calor es mucho menor. Para examinar el papel del flujo hidráulico en la distorsión de las isotermas de esta región, se ha comparado el gradiente térmico con la temperatura, con lo cual se ha podido definir los componentes mayoritarios del sistema de flujo de las aguas subterráneas. El uso de modelos bidimensionales ha servido para comprender no sólo del origen de las variaciones horizontales del flujo de calor en este campo, sino también el contraste entre las propiedades térmicas de los reservorios someros y profundos de aguas subterráneas.

  9. The migration, dissolution, and fate of chlorinated solvents in the urbanized alluvial valleys of the southwestern USA

    NASA Astrophysics Data System (ADS)

    Jackson, R. E.

    The migration, dissolution, and subsequent fate of spilled chlorinated solvents in the urban alluvial valleys of the southwestern U.S. appear to be governed by a unique set of hydrogeologic and geochemical processes occurring within terrigeneous clastic depositional systems. The alluvial and lacustrine fill of the basins, the trapping of solvents in fine-grained sediments beneath the urbanized valley centers, the oxic conditions typical of the deeper alluvium, and the contaminant-transport patterns produced by large-scale basin pumping combine to produce long aqueous-phase plumes derived from the dissolution of trapped chlorinated solvents. Although of limited aqueous solubility, these dense solvents are sufficiently mobile and soluble in the southwestern alluvial valleys to have produced aqueous plumes that have migrated several kilometers through the deeper alluvium and have contaminated valuable water-supply well fields in California, Arizona, and New Mexico. The typical length of these plumes and the presence of oxic groundwater indicate that it is unlikely that natural attenuation will be a practical remedial option in the southwestern alluvial valleys or in other alluvial systems in which similar hydrogeologic and geochemical conditions exist. Résumé La migration, la dissolution et l'évolution consécutive des rejets de solvants chlorés dans les vallées alluviales du sud-ouest des États-Unis paraissent déterminées par un même ensemble de processus hydrogéologiques et géochimiques intervenant dans des formations de dépôts clastiques terrigènes. Les remplissages alluviaux et lacustres des bassins, le piégeage des solvants par des sédiments fins sous les centres des vallées urbanisées, les conditions oxiques typiques des alluvions plus profondes et les types de transport de contaminants provoqués par le pompage à l'échelle du bassin se combinent pour produire des panaches, étendus dans la phase aqueuse, provenant de la dissolution de solvants chlorés piégés. Malgré leur faible solubilité dans l'eau, ces solvants denses sont suffisamment mobiles et solubles pour avoir produit, dans le sud-ouest des vallées alluviales, des panaches aqueux qui ont migré de plusieurs kilomètres dans les alluvions plus profondes et ont contaminé des champs captants pour l'eau potable en Californie, en Arizona et au Nouveau-Mexique. La longueur de ces panaches et la présence d'eau souterraine en conditions oxiques indiquent qu'il est peu probable que la décroissance naturelle soit un recours pratique de décontamination dans les vallées alluviales du sud-ouest ou dans d'autres systèmes alluviaux dans lesquels existent des conditions hydrogéologiques et géochimiques semblables. Resumen La migración, disolución y transporte de compuestos clorados en valles aluviales urbanos del sudoeste de los Estados Unidos de América parecen estar gobernados por un conjunto único de procesos hidrogeológicos y geoquímicos que tienen lugar en los depósitos clásticos. El relleno aluvial y lacustre de las cuencas, la inmovilización de los solutos en sedimentos de grano fino bajo las zonas urbanizadas, los condiciones óxicas típicas del aluvial profundo y las direcciones de transporte regidas por los fuertes bombeos en las cuencas se combinan para producir grandes penachos en fase acuosa procedentes de la disolución de los compuestos clorados atrapados en el medio. Aunque la solubilidad de estos compuestos clorados densos es pequeña, es suficiente para producir penachos que en algunos casos se han desplazado varios kilómetros a través del aluvial profundo y han llegado a contaminar zonas de extracción muy productivas en California, Arizona y Nuevo México. La longitud de estos penachos y la presencia de agua subterránea oxidante indican que es improbable que la degradación natural sea un buen método de limpieza de estos acuíferos o de otros sistemas aluviales que presenten características hidrogeológicas y geoquímicas semejantes.

  10. PREFACE: Dynamics of low-dimensional systems Dynamics of low-dimensional systems

    NASA Astrophysics Data System (ADS)

    Bernasconi, M.; Miret-Arts, S.; Toennies, J. P.

    2012-03-01

    With the development of techniques for high-resolution inelastic helium atom scattering (HAS), electron scattering (EELS) and neutron spin echo spectroscopy, it has become possible, within approximately the last thirty years, to measure the dispersion curves of surface phonons in insulators, semiconductors and metals. In recent years, the advent of new experimental techniques such as 3He spin-echo spectroscopy, scanning inelastic electron tunnel spectroscopy, inelastic x-ray scattering spectroscopy and inelastic photoemission have extended surface phonon spectroscopy to a variety of systems. These include ultra-thin metal films, adsorbates at surface and elementary processes where surface phonons play an important role. Other important directions have been actively pursued in the past decade: the dynamics of stepped surfaces and clusters grown on metal surfaces, due to their relevance in many dynamical and chemical processes at surfaces, including heterogeneous catalysis; clusters; diffusion etc. The role of surface effects in these processes has been conjectured since the early days of surface dynamics, although only now is the availability of ab initio approaches providing those conjectures with a microscopic basis. Last but not least, the investigation of non-adiabatic effects, originating for instance from the hybridization (avoided crossing) of the surface phonons branches with the quasi 1D electron-hole excitation branch, is also a challenging new direction. Furthermore, other elementary oscillations such as surface plasmons are being actively investigated. The aforementioned experimental breakthroughs have been accompanied by advances in the theoretical study of atom-surface interaction. In particular, in the past decade first principles calculations based on density functional perturbation theory have boosted the theoretical study of the dynamics of low-dimensional systems. Phonon dispersion relations of clean surfaces, the dynamics of adsorbates, and the vibrational spectra of clusters and carbon-based nanostructures, just to name a few of the low-dimensional systems addressed in this special issue, can be both accurately computed from first principles and measured experimentally. Even less computationally demanding semi-empirical simulations based on tight-binding or continuum models play a crucial role in assessing, for instance, the interplay between morphology, defects and the elastic properties of low-dimensional systems. The impressive amount of work and progress achieved in the past decade within the general theory and spectroscopy of the dynamics of low-dimensional systems is marked by several relevant trends that are exemplified by the contributions gathered together in this special issue. They span a wide spectrum of experimental and theoretical methods applied to the study of the dynamical properties of low-dimensional systems and new emerging phenomena at the nanoscale, such as the peculiar optical properties of ring shaped quantum dots, plasmon dynamics in metallic nanoclusters and the relaxation dynamics of nanomagnets. This issue is dedicated to our esteemed colleague Giorgio Benedek on the occasion of his 70th birthday. It collects together a number of papers written by authors from all over the world with a recognized reputation in the above mentioned fields where Giorgio Benedek has made important and fundamental contributions. Dynamics of low-dimensional systems contents Narratives Giorgio Benedek: an extraordinary universal scientist M Bernasconi, S Miret-Arts and J P Toennies Helium and carbon: two friends for life Giorgio Benedek Special Issue Papers Temperature dependence in atom-surface scattering Eli Pollak and J R Manson Density functional study of the decomposition pathways of SiH3 and GeH3 at the Si(100) and Ge(100) surfaces M Ceriotti, F Montalenti and M Bernasconi Comparative study of vibrations in submonolayer structures of potassium on Pt(111) G G Rusina, S V Eremeev, S D Borisova and E V Chulkov Surface phonons on Pb(111) I Yu Sklyadneva, R Heid, K-P Bohnen, P M Echenique and E V Chulkov Using evidence from nanocavities to assess the vibrational properties of external surfaces G F Cerofolini, F Corni, S Frabboni, G Ottaviani, E Romano, R Tonini and D Narducci Magnetic properties and relaxation dynamics of a frustrated Ni7 molecular nanomagnet E Garlatti, S Carretta, M Affronte, E C Saudo, G Amoretti and P Santini A theoretical study of rotational and translational diffusion dynamics of molecules with a six-fold point symmetry adsorbed on a hexagonal lattice by neutron scattering I Calvo-Almazn, S Miret-Arts and P Fouquet Vibrational dynamics and surface structure of Bi(111) from helium atom scattering measurements M Mayrhofer-Reinhartshuber, A Tamtgl, P Kraus, K H Rieder and W E Ernst Double and triple ionization of silver clusters by electron impactAvik Halder, Anthony Liang, Chunrong Yin and Vitaly V Kresin Scattering of O2 from a graphite surface W W Hayes, Junepyo Oh, Takahiro Kondo, Keitaro Arakawa, Yoshihiko Saito, Junji Nakamura and J R Manson Zero-phonon lines of systems with different dimensions and unconventional vibronic interactions V Hizhnyakov A kinetic Monte Carlo approach to investigate antibiotic translocation through bacterial porins Matteo Ceccarelli, Attilio V Vargiu and Paolo Ruggerone Quantum Zeno and anti-Zeno effects in surface diffusion of interacting adsorbates H C Peate-Rodrguez, R Martnez-Casado, G Rojas-Lorenzo, A S Sanz and S Miret-Arts Weakly bound finite systems: (4He)N-Rb2(3?u), clustering structures from a quantum Monte Carlo approach D Lpez-Durn, R Rodrguez-Cantano, T Gonzlez-Lezana, G Delgado-Barrio, P Villarreal, E Yurtsever and F A Gianturco Multiphonon atom-surface scattering from corrugated surfaces: derivation of the inelastic scattering spectrum for diffraction statesBranko Gumhalter Probing the non-pairwise interactions between CO molecules moving on a Cu(111) surfacePepijn R Kole, Holly Hedgeland, Andrew P Jardine, William Allison, John Ellis and Gil Alexandrowicz Fast emission dynamics in droplet epitaxy GaAs ring-disk nanostructures integrated on SiL Cavigli, S Bietti, M Abbarchi, C Somaschini, A Vinattieri, M Gurioli, A Fedorov, G Isella, E Grilli and S Sanguinetti Assessing the composition of hetero-epitaxial islands via morphological analysis: an analytical model matching GeSi/Si(001) dataR Gatti, F Pezzoli, F Boioli, F Montalenti and Leo Miglio Carbon sp chains in graphene nanoholesIvano E Castelli, Nicola Ferri, Giovanni Onida and Nicola Manini Elastic fields and moduli in defected grapheneRiccardo Dettori, Emiliano Cadelano and Luciano Colombo Tuning the plasmon energy of palladium-hydrogen systems by varying the hydrogen concentrationV M Silkin, R Dez Muio, I P Chernov, E V Chulkov and P M Echenique Plasmon tsunamis on metallic nanoclustersA A Lucas and M Sunjic Ab initio characterization of graphene nanoribbons and their polymer precursorsRengin Pekz, Xinliang Feng and Davide Donadio First-principles phonon calculations of Fe4+ impurity in SrTiO3E Blokhin, E A Kotomin and J Maier Phonon dispersion of quasi-freestanding graphene on Pt(111)Antonio Politano, Antonio Raimondo Marino and Gennaro Chiarello Vibrations of Au13 and FeAu12 nanoparticles and the limits of the Debye temperature conceptGhazal Shafai, Marisol Alcntara Ortigoza and Talat S Rahman Triple quantum dots as charge rectifiers M Busl and G Platero

  11. Eventos de Desconexão no Cometa P/Halley sob a Ótica do Modelo de Reconexão Magnética

    NASA Astrophysics Data System (ADS)

    Voelzke, M. R.; Matsuura, O. T.

    1998-08-01

    531 imagens contidas no The International Halley Watch Atlas of Large-Scale Phenomena (Brandt et al., 1992) cobrindo o período de setembro de 1985 a julho de 1986 foram analisadas visando identificar, caracterizar as propriedades e correlacionar estruturas morfológicas da cauda de plasma do cometa P/Halley. A análise revelou 47 eventos de desconexão (DEs) (Niedner & Brandt, 1979; Jockers, 1985; Celnik et al., 1988; Delva et al., 1991). A análise completa de todas as imagens encontra-se publicada em Voelzke & Matsuura, 1998. A distribuição dos DEs na distância heliocêntrica apresenta um caráter bimodal possivelmente associado com a distribuição espacial das fronteiras de setor magnético do meio interplanetário. Os 47 DEs fotografados em 47 imagens distintas permitiram determinar 19 origens de DEs, ou seja, o instante em que supostamente o cometa cruzou a fronteira entre setores magnéticos do vento solar. Tais dados cometários foram comparados com dados do vento solar provenientes de medidas realizadas in situ pelas sondas IMP-8, ICE e PVO, que mediram a variação da velocidade do vento solar, da densidade e da pressão dinâmica durante o intervalo analisado. Os dados destas sondas espaciais em conjunto com os da sonda Vega 1 foram usados para determinar o tempo das passagens do lençol de corrente. Com base nos dados das sondas foram calculadas as coordenadas heliográficas retroativas do lençol de corrente na "superfície fonte" dos mapas sinóticos do campo magnético de Hoeksema, 1989. O cálculo retroativo é feito através de um modelo simples de expressão do vento solar com velocidade uniforme, sendo considerada a co-rotação da magnetosfera com o Sol. Este trabalho apresenta os resultados desta comparação e a análise cinemática da origem dos DEs, determinada sob a hipótese que o plasma desconectado de um dado DE afasta-se com velocidade constante do núcleo cometário (Voelzke & Matsuura, 1998) e compara esta análise com outras que determinam o tempo de desconexão a partir de um movimento linear constantemente acelerado (Yi et al., 1994). A velocidade de um DE para outro varia enormemente. - Brandt, J.C., Niedner, M.B.Jr. and Rahe, J., (1992) The International Halley Watch Atlas of Large-Scale Phenomena (printed by: Johnson Printing Co., Boulder, CO), University of Colorado-Boulder. - Celnik, W.E., Koczet, P., Schlosser, W., Schulz, R., Svejda, P. and Weissbauer, K., (1988) Astron. Astrophys. Suppl. Ser. 72, 89. - Delva, M., Schwingenschuh, K., Niedner, M.B.Jr. and Gringauz, K.I., (1991) Planet. Space Sci. 39, Number 5, 697. - Hoeksema, J.T., (1989) Adv. Space Res. 9, 141. - Jockers, K., (1985) Astron. Astrophys. Suppl. Ser. 62, 791. - Niedner, M.B.Jr. and Brandt, J.C., (1979) Astrophys. J. 234, 723. - Voelzke, M.R. and Matsuura, O.T., (1988) Planet. Space Sci. 46, 835. - Yi, Y., Caputo, M.F. and Brandt, J.C., (1994) Planet. Space Sci. 42, Number 9, 705.

  12. The Shadow of a Gnomon Along a Year: Routine Observations and Teaching of Apparent Motion of the Sun and the Four Seasons. (Spanish Title: La Sombra de un Gnomon lo Largo de un Ao: Observaciones de Rutina y la Enseanza del Movimiento Aparente del Sol y Las Cuatro Estaciones.) A Sombra de um Gnmon ao Longo de um Ano: Observaes Rotineiras e o Ensino do Movimento Aparente do Sol E das Quatro Estaes

    NASA Astrophysics Data System (ADS)

    Trogello, Anderson Giovani; Danhoni Neves, Marcos Cesar; de Carvalho Rutz da Silva, Sani

    2013-12-01

    Many misconceptions are recognized among the various groups of students, especially in the elementary school. Among them, the apparent motion of the Sun, in spite of its daily occurrence, is subject to varied interpretations. Thus, the observation and recording of the motion of the stars in the celestial vault is a necessary task for astronomy education. The work presented here proposes the presentation of the results of observations of the apparent movement of the sun by marking the shadow of a vertical gnomon by the students in a class of sixth graders of elementary rural school of Paran. The project itself was conducted in four stages, on dates near the March equinox, the June solstice, the September equinox and the December solstice. In addition, lectures were developed in the classroom. Such methods sought to build concepts around the apparent movement of the Sun and the alternation of the seasons. Given the results of the activities, an evaluation was applied and the data demonstrated a desired student learning such as: the recognition of the cardinal points, the description of the apparent solar motion and the occurrence of the seasons and their alternation from astronomical observations at naked eye. Muchos conceptos aternativos son conocidos entre los distintos grupos de alumnos, sobre todo en la educacin bsica. Entre ellos, el movimiento aparente del Sol, por ms cotidiano que sea, se presta a interpretaciones variadas. Por lo tanto, observar y registrar el movimiento de las estrellas en la bveda celeste se torna una tarea necesaria para la educacin en astronoma. El trabajo que aqu se presenta propone la presentacin de los resultados de la observacin del movimiento aparente del sol a travs de la marcacin de la sombra del gnomon vertical a cargo de los estudiantes en una divisin de sexto grado de de la escuela primaria rural de Paran. El proyecto en s se llev a cabo en cuatro etapas, en fechas cercanas al equinoccio de marzo, al solsticio de junio, al equinoccio de septiembre y al solsticio de diciembre. Adems, se dictaron clases tericas en la sala de aula. Estos mtodos buscaron construir conceptos en torno al movimiento aparente del Sol y la sucesin de las estaciones. Teniendo en cuenta los resultados de las actividades se aplic una evaluacin cuyos datos demuestran la existencia de un aprendizaje deseado por los estudiantes en cuanto a: el reconocimiento de los puntos cardinales, la descripcin del movimiento solar aparente y la aparicin de las estaciones y su alternancia a partir de observaciones astronmicas visuales sin instrumentos. Muitas concepes alternativas so reconhecidas entre os diversos grupos de estudantes, em especial nos da educao bsica. Dentre elas, o movimento aparente do Sol, por mais quotidiano que seja, proporciona variadas interpretaes. Deste modo, observar e registrar o movimento dos astros na abboda celeste uma tarefa necessria ao ensino de Astronomia. O trabalho que ora se apresenta prope a apresentao dos resultados da observao do movimento aparente do Sol por intermdio da marcao da sombra de um gnmon vertical por alunos de uma turma do sexto ano do ensino fundamental de uma escola do campo do Paran. O projeto em si ocorreu em quatro etapas, em datas prximas do equincio de maro, do solstcio de junho, do equincio de setembro e do solstcio de dezembro. Alm disso, foram desenvolvidas aulas tericas em sala de aula. Tais mtodos buscaram construir conceitos em torno da movimentao aparente do Sol e da alternncia das estaes do ano. Diante dos resultados provenientes das atividades desenvolvidas foi aplicada uma avaliao e os dados demonstraram um aprendizado desejado dos alunos quanto: ao reconhecimento dos pontos cardeais; descrio do movimento solar aparente e a ocorrncia das estaes do ano e sua alternncia a partir de observaes astronmicas a olho nu.

  13. Chemical response to groundwater extraction southeast of Mexico City

    NASA Astrophysics Data System (ADS)

    Huizar-Alvarez, R.; Carrillo-Rivera, J. J.; Ángeles-Serrano, G.; Hergt, T.; Cardona, A.

    An alternative procedure of pumping test data interpretation is used through a joint analysis of the standard time-drawdown curve and simultaneous field measurements of total dissolved solids (TDS); additional support is also provided by the temperature of extracted groundwater and the chemical composition of extracted water. The overall information was applied to characterise the groundwater flow system and its sources, the hydraulic conditions of the aquifer and hydraulic response of extraction boreholes. The analysis of this information suggests the presence of: (i) a local flow system that circulates at shallow depth through basalt units interstratified with fine grained sediments and pyroclastics; these materials contain water with TDS of 127-600 mg/L and Na of 24-178 mg/L, and temperature of 18-19.5 °C (ii) intermediate flow in granular material under reducing conditions by the oxidation of organic matter in aquitard sediments; this water has TDS and Na values of 203-940 and 30-370 mg/L, respectively, and temperatures of about 20-22 °C (iii) regional flow through volcanic rocks and limestone, with TDS content of 300-700 mg/L, Na of 80-230 mg/L and temperature of 23.0-24.8 °C. The hydraulic response and the chemical composition of the water produced by some boreholes are affected by the seepage inflow from sewage effluents, the input from an overlying aquitard unit and the inducement of regional flow. The conception of the flow regime thus obtained allowed the recognition of hydraulic conditions which were more consistent with the hydrogeological setting, than if only a time vs. drawdown test analysis would have been carried out. L'interprétation simultanée de pompages d'essais, des données de température et résidu sec (RS) de L'eau souterraine pompée, mesurées simultanément sur le terrain et la composition chimique de L'eau pompée comme un aide additionnelle, est utilisée comme une différent procédure pour interpréter les pompages d'essais. La procédure a été appliquée pour caractériser le système d'écoulement souterraine et sa source, les conditions hydrauliques de l'aquifère et la réponse hydraulique des puits considéré. L'analyse de cette information suggérer la présence des systèmes d'écoulement suivantes. (i) local avec18 et 19.5 °C de température, RS de 127-600 mg/L, et Na de 24-178 mg/L, (ii) intermédiaire avec une température de 20 á 22 °C, le RS de 203-940 mg/L et Na 30-370 mg/L, (iii) régional avec 300 à 700 mg/L de RS et 80 à 230 mg/L de Na, une température de 23 à 24.8 °C. Dans le premier cas, l'eau traverse des roches basaltiques, dans le deuxième, des sédiments clastiques avec matière organique de l'aquitard, dans le troisième, des roches volcaniques et calcaires. La chimie de l'eau des quelques puits et sa réponse hydraulique met en évidence l'influence de l'eau de L'aquitard, des effluents de surface et écoulement régional. La conception du régime d'écoulement obtenu, a permis reconnaître les conditions hydrauliques des puits plus correspondantes au contexte hydrogéologique, que si uniquement les données rabattement vs temps auraient été analysé La interpretación conjunta de la gráfica de prueba de bombeo, valores de temperatura y sólidos totales disueltos (STD) del agua subterránea extraída, medidos simultáneamente en campo y la composición química del agua extraída como apoyo adicional; se utilizó como un procedimiento alternativo para interpretar los datos de pruebas de bombeo. Toda esa información fue aplicada para caracterizar el sistema de flujo subterráneo y el origen de éste, las condiciones hidráulicas del acuífero y la respuesta hidráulica de los pozos de extracción. El análisis de la información indica la presencia de: (i) flujo local con temperatura de 18-19.5 °C, STD de 127-600, y Na de 24-178 mg/L (ii) flujo intermedio con temperatura de 20-22 °C, los STD y Na son de (203-940 y 30-370 mg/L), respectivamente; (iii) regional con STD de 300-700 y Na de 80-230 mg/L, y temperatura de 23-24.8 °C. En el primer caso el agua circula a través de rocas basálticas, en el segundo viaja por material granular y materia orgánica en sedimentos del acuitado. El flujo regional circula por material volcánico y rocas calizas. La respuesta hidráulica y la composición química del agua extraída por algunos pozos, es afectada por infiltración de efluentes de agua residual, entrada de agua del acuitardo sobreyacente y la inducción de flujo regional. La concepción del régimen de flujo obtenida, permitió reconocer a las condiciones hidráulicas de los pozos, más correspondientes con el contexto hidrogeológico, que sí únicamente se hubieran analizado los datos de abatimiento vs tiempo.

  14. Geologically based model of heterogeneous hydraulic conductivity in an alluvial setting

    NASA Astrophysics Data System (ADS)

    Fogg, Graham E.; Noyes, Charles D.; Carle, Steven F.

    Information on sediment texture and spatial continuity are inherent to sedimentary depositional facies descriptions, which are therefore potentially good predictors of spatially varying hydraulic conductivity (K). Analysis of complex alluvial heterogeneity in Livermore Valley, California, USA, using relatively abundant core descriptions and field pumping-test data, demonstrates a depositional-facies approach to characterization of subsurface heterogeneity. Conventional textural classifications of the core show a poor correlation with K; however, further refinement of the textural classifications into channel, levee, debris-flow, and flood-plain depositional facies reveals a systematic framework for spatial modeling of K. This geologic framework shows that most of the system is composed of very low-K flood-plain materials, and that the K measurements predominantly represent the other, higher-K facies. Joint interpretation of both the K and geologic data shows that spatial distribution of K in this system could not be adequately modeled without geologic data and analysis. Furthermore, it appears that K should not be assumed to be log-normally distributed, except perhaps within each facies. Markov chain modeling of transition probability, representing spatial correlation within and among the facies, captures the relevant geologic features while highlighting a new approach for statistical characterization of hydrofacies spatial variability. The presence of fining-upward facies sequences, cross correlation between facies, as well as other geologic attributes captured by the Markov chains provoke questions about the suitability of conventional geostatistical approaches based on variograms or covariances for modeling geologic heterogeneity. Résumé Les informations sur la texture des sédiments et leur continuité spatiale font partie des descriptions de faciès sédimentaires de dépôt. Par conséquent, ces descriptions sont d'excellents prédicteurs potentiels des variations spatiales de la conductivité hydraulique (K). L'analyse de l'hétérogénéité des alluvions complexes de la vallée de Livermore (Californie, États-Unis), sur la base de descriptions de carottes relativement nombreuses et de données d'essais de pompage, montre que l'hétérogénéité souterraine peut être caractérisée par une approche des faciès de dépôt. Des classifications conventionnelles de la texture de la carotte montrent une corrélation médiocre avec K; toutefois, une amélioration ultérieure des classifications de texture en faciès de dépôt de chenal, de levée d'inondation, de coulée boueuse et de plaine d'inondation a fourni un cadre systématique pour une modélisation spatiale de K. Ce cadre géologique montre que le système est composé pour l'essentiel par des matériaux d'inondation à très faible perméabilité ceci laisse envisager qu'on ne peut pas supposer que K suit une distribution log-normal, sauf peut-être à l'intérieur de chaque faciès. Une modélisation par chaîne de Markov de la probabilité de passage, représentant la corrélation spatiale dans les faciès et entre eux, prend en compte les faits géologiques intéressants tout en fournissant une approche nouvelle pour une caractérisation statistique de la variabilité spatiale des faciès. La présence de séquences à faciès tronqués vers le haut, d'une corrélation croisée entre faciès, ainsi que d'autres caractères géologiques pris en compte par les chaînes de Markov conduisent à se poser des questions sur l'adéquation des approches géostatistiques conventionnelles utilisant les variogrammes ou les covariances pour modéliser l'hétérogénéité géologique. Resumen La información respecto a la textura de los sedimentos y la continuidad espacial es inherente a las descripciones de las facies deposicionales sedimentarias. De este modo, estas descripciones se convierten en excelentes predictores potenciales de las variaciones espaciales de la conductividad hidráulica (K). El análisis de la heterogeneidad en un aluvial en el Valle de Livermore (California, EEUU), a partir de las relativamente abundantes descripciones de testigos y de datos de ensayos de bombeo es una muestra del método de la facies deposicional para caracterizar la heterogeneidad subsuperficial. Las clasificaciones texturales convencionales de los testigos muestran una correlación pobre con K; sin embargo, el posterior refinamiento de la clasificación en canales, diques, flujo de derrubios y llanura de inundación revela un marco sistemático para la modelización espacial de K. Este marco geológico muestra que la mayor parte del sistema está compuesto por materiales de la llanura de inundación, de muy baja permeabilidad, y sugiere que no debe asumirse que K tiene una distribución log-normal, excepto quizás para cada facies por separado. Un modelo de cadena de Markov, tanto para representar la correlación espacial en cada facies como la relación entre las distintas facies, capta las características geológicas más importantes, a la vez que presenta un nuevo método para la caracterización estadística de la variabilidad espacial de las hidrofacies. La presencia de secuencias de facies más finas hacia la superficie, la correlación cruzada entre facies y otros atributos captados por las cadenas de Markov cuestionan lo adecuado de los métodos geoestadísticos convencionales basados en variogramas y covarianzas para modelar la heterogeneidad.

  15. Land subsidence caused by groundwater exploitation in Suzhou City, China

    NASA Astrophysics Data System (ADS)

    Chen, Chongxi; Pei, Shunping; Jiao, Jiu Jimmy

    2002-09-01

    Suzhou City, located at the lower reaches of the Yangtze River in southeastern Jiangsu Province, is one of the few cities in China which suffer from severe ground settlement. A research project was carried out to investigate this problem. Geological and hydrogeological studies show that there is a multi-layered aquifer system with three distinct, soft mud layers of marine and lagoonal origins. An examination of historical records of groundwater extraction, water levels, and ground settlement shows that the ground subsidence is associated with the continuously increasing groundwater extraction in the deep, confined aquifer. It is believed that the consolidation of the soft mud layers, especially the third layer which is thick and close to the main pumped aquifer, contributes to the ground settlement. A three-dimensional finite difference numerical model representing the multi-layered aquifer system was developed to study the ground settlement in response to groundwater extraction. By calibrating the model with both the measured groundwater level and ground settlement, the aquifer parameters were estimated. The model outputs fit reasonably well with the observed results, which indicates that the numerical model can reproduce the dynamic processes of both groundwater flow and soil consolidation. The hydraulic conductivity of the third mud layer near the center of the ground settlement has been reduced by over 30% in the last 14 years. The gradual deterioration in the hydraulic conductivity of the mud may have significant adverse effect on the sustainable groundwater resource of the deep confined aquifer, since the recharge from the shallow aquifers through the mud layer is the only source of water to the deep aquifer. An analysis of the spatial distributions of groundwater drawdown and ground settlement shows that the area with maximum drawdown is not necessarily the area with maximum ground settlement due to the occurrence of the soft mud layer. A simple reallocation in pumping rates on the basis of the spatial distribution of the thick mud layer could significantly reduce the ground settlement. Résumé. La ville de Suzhou, située dans la basse vallée du fleuve Yangtsé dans le sud-est de la province de Jiangsu, est l'une des rares villes de Chine qui souffrent cruellement de tassements du sol. Un projet de recherche a été mené pour étudier ce problème. Des études géologiques et hydrogéologiques montrent qu'il existe un système aquifère multicouche constitué de trois niveaux distincts de limons non consolidés d'origine marine et lagunaire. Un examen des historiques des prélèvements d'eau souterraine, des niveaux de nappe et des tassements de sol montrent que la subsidence du sol est associée à des prélèvements continuellement croissants d'eau souterraine dans l'aquifère captif profond. On pense que le compactage des couches limoneuses non consolidées, en particulier de la troisième couche qui est épaisse et proche du principal aquifère pompé, contribue aux tassements du sol. Un modèle numérique aux différences finies en trois dimensions, représentant l'aquifère multicouche, a été réalisé pour étudier les tassements du sol en réponse aux prélèvements d'eau souterraine. Les paramètres de l'aquifère ont été estimés par calibration du modèle au moyen à la fois des niveaux piézométriques et des tassements du sol. Les résultats de la simulation s'ajustent convenablement aux résultats observés, ce qui indique que le modèle numérique peut reproduire les processus dynamiques aussi bien des écoulements souterrains que de compactage du sol. La conductivité hydraulique de la troisième couche de limon non consolidé au voisinage du centre du tassement de sol a été réduit de plus de 30% au cours des 14 dernières années. La dégradation progressive de la conductivité hydraulique du limon peut avoir un effet significatif néfaste sur la pérennité de la ressource en eau souterraine dans l'aquifère captif profond, puisque la recharge à partir des aquifères superficiels au travers de la couche de limon est la seule alimentation de l'aquifère profond. Une analyse des distributions spatiales de l'abaissement du niveau piézométrique et des tassements du sol montre que la région soumise à l'abaissement maximal de piézométrie n'est pas nécessairement celle des tassements maximaux du sol liés à la présence de la couche de limon non consolidé. Une simple révision des débits de pompage basée sur la distribution spatiale de la couche de limon épaisse peut réduire significativement les tassements du sol. Resumen. La ciudad de Suzhou, situada en el tramo inferior del Río Yangtze, al sudeste de la provincia de Jiangsu, es una de las pocas ciudades chinas que padece problemas serios de subsidencia. Esto ha motivado la realización de un proyecto de investigación en la zona. Estudios geológicos e hidrogeológicos apuntan a un modelo de acuífero multicapa, con tres niveles distintos de lodos blandos de orígenes marino y lacustre. Examinando los registros históricos de extracciones de agua subterránea, así como de nivel piezométrico y de subsidencia, se observa que ésta se halla asociada al bombeo cada vez mayor del acuífero confinado profundo. La hipótesis es que las capas de lodos blandos se van consolidando, si bien la que más contribuye a ello es la tercera, potente y próxima al acuífero más explotado. Se ha realizado un modelo numérico tridimensional en diferencias finitas que representa el sistema acuífero multicapa, con lo que se puede estudiar el efecto de la extracción de agua subterránea en la subsidencia. Calibrando el modelo con niveles piezométricos medidos y con datos de subsidencia, se ha podido estimar los parámetros del acuífero. Los resultados del modelo ajustan de forma razonable con los datos medidos, por lo que el modelo numérico es capaz de reproducir los procesos dinámicos de flujo de aguas subterráneas y consolidación del terreno. La conductividad hidráulica de la tercera capa de lodo cerca del centro de asentamiento se ha reducido en más del 30% durante los últimos 14 años. El deterioro gradual de la conductividad hidráulica del lodo puede tener efectos adversos notables en la sustentabilidad de los recursos de agua subterránea del acuífero confinado profundo, ya que se recarga exclusivamente de acuíferos más someros a través de la capa de lodo. El análisis de la distribución espacial de descenso del nivel piezométrico y de subsidencia muestra que el área de extracción máxima no coincide necesariamente con la de máxima subsidencia, debido a la existencia de la capa de lodos blandos. Una mera redistribución de los caudales de bombeo en función de las propiedades espaciales de la gruesa capa de lodos podría reducir drásticamente los problemas de subsidencia.

  16. Some current methods to represent the heterogeneity of natural media in hydrogeology

    NASA Astrophysics Data System (ADS)

    de Marsily, G.; Delay, F.; Teles, V.; Schafmeister, M. T.

    We have known for a long time that the material properties of the subsurface are highly variable in space. We have learned that this variability is due to the extreme complexity and variation with time of processes responsible for the formation of the earth's crust, from plate tectonics to erosion, sediment transport, and deposition, as well as to mechanical, climatic, and diagenetic effects. As geologists, we learned how to "read" this complex history in the rocks and how to try to extrapolate in space what we have understood. As physicists, we then learned that to study flow processes in such media we must apply the laws of continuum mechanics. As mathematicians using analytical methods, we learned that we must simplify by dividing this complex continuum into a small number of units, such as aquifers and aquitards, and describe their properties by (constant) equivalent values. In recent years, as numerical modelers, we learned that we now have the freedom to "discretize" this complex reality and describe it as an ensemble of small homogeneous boxes of continuous media, each of which can have different properties. How do we use this freedom? Is there a need for it? If the answer is "yes," how can we assign different rock-property values to thousands or even millions of such little boxes in our models, to best represent reality, and include confidence levels for each selected rock property? As a tribute to Professor Eugene S. Simpson, with whom the first author of this paper often discussed these questions, we present an overview of three techniques that focus on one property, the rock permeability. We explain the motivation for describing spatial variability and illustrate how to do so by the geostatistical method, the Boolean method, and the genetic method. We discuss their advantages and disadvantages and indicate their present state of development. This is an active field of research and space is limited, so the review is certain to be incomplete, but we hope that it will encourage the development of new ideas and approaches. Résumé On sait depuis longtemps que les propriétés des roches en profondeur sont éminemment variables dans l'espace. On sait que cette variabilité est due à la complexité extrême et à la variation au cours du temps des processus responsables de la formation de la croûte terrestre, de la tectonique des plaques à l'érosion, au transport sédimentaire et au dépôt, sans oublier les effets mécaniques, climatiques et de diagenèse. En tant que géologues, nous avons appris a "lire" cette histoire complexe au sein des roches, et à tenter d'extrapoler dans l'espace notre compréhension. En tant que physiciens, nous avons ensuite appris que pour étudier les écoulements dans de tels milieux, nous devions appliquer les concepts de la mécanique des milieux continus. En tant que mathématiciens utilisant des méthodes analytiques pour résoudre les problèmes d'écoulement, nous avons de plus appris que nous devions simplifier cette réalité complexe en un très petit nombre d'unités, tels que les aquifères et les aquitards, dont chacune est décrite par des propriétés équivalentes constantes. Enfin, dans les années récentes, en tant que numériciens, nous avons appris que nous avions désormais la liberté de "discrétiser" cette réalité complexe, et de la décrire comme un ensemble de petites "boîtes" homogènes de milieu continu, chacune d'entre elles pouvant avoir des propriétés différentes. Comment utilisons nous cette liberté nouvellement acquise? En avons-nous réellement besoin? Si la réponse est "oui", comment pouvons nous attribuer des propriétés différentes aux roches des milliers ou même millions de petites "boîtes" dans nos modèles, pour représenter au mieux la réalité, et comment déterminer les intervalles de confiance des propriétés choisies pour chaque roche? En hommage au Professeur Eugène S. Simpson, avec lequel le premier auteur de cet article a eu souvent l'occasion de discuter de ces questions, nous présentons ici un survol général de quelques techniques de génération de telles propriétés se focalisant sur une seule d'entre elles, la perméabilité des roches. Nous expliquons d'abord quels sont les raisons qui engagent à tenter de décrire la variabilité spatiale, puis nous illustrons trois méthodes pour le faire, la méthode géostatistique, la méthode Booléenne et la méthode génétique. Nous présentons leurs avantages et inconvénients respectifs, et donnons l'état actuel de leur développement. Ces méthodes constituant un domaine de recherche actif, et la place étant ici limitée, ce survol est nécessairement incomplet, mais nous espérons qu'il encouragera l'essor de nouvelles idées et de nouvelles approches. Resumen Sabemos desde hace tiempo que las propiedades del subsuelo son altamente variables espacialmente. Hemos aprendido que esta variabilidad es debida a la extrema complejidad y variabilidad temporal de los procesos responsables de la formación de la corteza terrestre, desde la tectónica de placas a la erosión, transporte de sedimentos y deposición, así como a efectos mecánicos, climáticos y diagenéticos. Como geólogos, hemos aprendido a "leer" esta compleja historia en las rocas y a cómo tratar de extrapolar en el espacio lo que ya sabemos. Como físicos, aprendimos después que para estudiar los procesos en este tipo de medios debemos aplicar las leyes de la mecánica de los medios continuos. Como matemáticos que usan métodos analíticos, hemos aprendido que debemos simplificar el medio dividiéndolo en un número menor de unidades, como serían los acuíferos y acuitardos, y describiendo sus propiedades mediante valores equivalentes (constantes). En los últimos años, como modelistas, también hemos aprendido que tenemos la libertad de "discretizar" esta realidad compleja y describirla como un conjunto de pequeñas cajas homogéneas de medio continuo, cada una con propiedades diferentes. ¿Cómo usamos esta libertad?¿Tenemos necesidad de ella? Si la respuesta es "sí", ¿cómo podemos asignar valores de las distintas propiedades de las rocas a miles e incluso millones de estas pequeñas cajas en nuestros modelos, con la pretensión de representar la realidad, y a la vez dar intervalos de confianza para cada propiedad seleccionada? Como un tributo al Profesor Eugene S. Simpson, con quien el autor de este artículo a menudo discutió sobre estas cuestiones, se presenta una recopilación de tres técnicas que se centran en una propiedad, la permeabilidad de la roca. Se explica la motivación para describir la variabilidad espacial y se ilustra cómo hacerlo mediante el método geoestadístico Booleano y mediante el método genético. Para cada método se discuten sus ventajas e inconvenientes y se indica su estado actual de desarrollo. Se trata éste de un campo activo de investigación y el espacio es limitado, por lo que la revisión es incompleta, pero esperamos que pueda servir para animar el desarrollo de nuevas ideas.

  17. Caracterización espectroscópica de hielos de interés atmosférico y astrofísico

    NASA Astrophysics Data System (ADS)

    Escribano, R.

    En años recientes se ha incrementado el estudio de procesos físicos y químicos que tienen lugar en la superficie o el interior de hielos, tanto en medios astrofísicos como en la atmósfera terrestre y en otros cuerpos del sistema solar. Se ha comprobado que las partículas heladas actúan como catalizadores de reacciones químicas, que no ocurrirían en su ausencia. En la atmósfera terrestre, es bien conocida la importancia de partículas de hidratos de ácido nítrico, formando las llamadas nubes estratosféricas polares, en los procesos de destrucción de ozono estratosférico. En hielos astrofísicos, átomos como H, C, N y O pueden adherirse o introducirse en la estructura cristalina o amorfa del hielo, y dar lugar a reacciones de formación de moléculas evitando su barrera de activación. Existen partículas heladas en el medio interestelar formando parte de las llamadas nubes moleculares densas y frías, con valores del orden de 106 átomos de H por cm3 y temperaturas entre 3 y 90 K. Alrededor de protoestrellas, pueden formarse hielos de distinta composición, polares o apolares, en las zonas de alejamiento y temperatura decreciente a partir del núcleo caliente. Por su parte, los cometas están formados por un núcleo de hielo y rocas, sobre el que se encuentran adheridas moléculas gaseosas, y una cola, formada por los gases liberados por efecto del calentamiento debido a la radiación solar incidente. En nuestro sistema solar, los polos de La Tierra y de Marte están cubiertos de hielo, así como la mayoría de los cuerpos externos. Los satélites de Júpiter han sido estudiados detalladamente, y se han encontrado en ellos, y en Tritón (satélite de Neptuno), hielos de moléculas como SON2, CO2, N2, CH4 y otros. Para la caracterización espectroscópica de estos hielos se precisan medidas en el laboratorio, aún conociendo la imposibilidad intrínseca de reproducir exactamente las condiciones en que se formaron y se encuentran en los medios astrofísicos. El montaje experimental requiere un sistema que permita alcanzar bajas presiones y temperaturas, formado usualmente por una cámara en cuyo interior se forman películas de hielo de la composición deseada, depositadas sobre un sustrato inerte. Las películas pueden ser a continuación tratadas por diversas técnicas, tales como irradiación UV, bombardeo con electrones o iones, calentamiento y enfriamiento, etc. Habitualmente todos los procesos se controlan por espectroscopía de infrarrojo. La radiación proveniente de un espectrómetro se hace incidir sobre la muestra y se extrae de la cámara mediante ventanas, y se enfoca posteriormente sobre el detector. En el laboratorio de Física Molecular del Instituto de Estructura de la Materia disponemos de un montaje experimental diseñado para el estudio de partículas de hielo similares a las formadas en las nubes estratosféricas polares de nuestra atmósfera. El montaje es similar al descrito anteriormente, excepto en lo que se refiere a las condiciones de presión y temperatura, que son menos estrictas en nuestros experimentos. La extensión de estas condiciones de trabajo a las requeridas en medios astrofísicos es una posibilidad a discutir. Por otra parte, disponemos de un método de cálculo de estructuras periódicas, basado en el programa SIESTA (acrónimo de Spanish Initiative for Electronic Simulations of Thousands of Atoms), que ha proporcionado excelentes resultados en lo relativo a la determinación de estructuras cristalinas y predicción de su espectro infrarrojo, en los sistemas estudiados hasta la fecha, es decir, los hidratos de ácido nítrico de interés atmosféricos. Su aplicación para el estudio de hielos de relevancia astrofísica podría ser del máximo interés.

  18. Sexual competitiveness and compatibility between mass-reared sterile flies and wild populations of Anastrepha Ludens (Diptera: Tephritidae) from different regions in Mexico

    SciTech Connect

    Orozco-Davila, D.; Hernandez, R.; Meza, S.; Dominguez, J.

    2007-03-15

    The mass-reared colony of Anastrepha ludens (Loew) currently used in Mexico for suppression of the Mexican fruit fly has been in use for over 10 years. Sterile flies are released into a wide range of environmental conditions as part of an integrated area-wide approach to suppress diverse populations of this pest in the Mexican Republic. This paper assesses the performance of the sterile flies interacting with wild populations from the different environments. We investigated the sexual compatibility and competitiveness of the sterile flies when competing with wild populations from 6 representatives Mexican states: Nuevo Leon, Tamaulipas, Sinaloa, Nayarit, Michoacan, and Chiapas. Results show that the males of the wild populations differed in the time to the onset and peak of sexual activity. Nevertheless, the index of sexual isolation (ISI) reflected sexual compatibility between the populations and the mass-reared strain, indicating that the sterile individuals mate satisfactorily with the wild populations from the 6 states. The male relative performance index (MRPI) showed that the sterile male is as effective in copulating as the wild males. The female relative performance index (FRPI) reflected a general tendency for wild females to copulate in greater proportion than the sterile females, except for the strains from Tamaulipas and Chiapas. In general, the lower participation of the sterile females in copulation increases the possibilities of sterile males to mate with wild females. The relative sterility index (RSI) showed that the acceptance by wild females of the sterile males (25-55%) was similar to that of wild males. Females of the Chiapas strain showed the lowest acceptance of sterile males. Finally, the results obtained in the Fried test (which measures induced sterility in eggs) showed a competitiveness coefficient ranging from 0.2 to 0.5. This suggests that sterile males successfully compete and are compatible with flies from different geographic origins. (author) [Spanish] La colonia actualmente usada para controlar la mosca mexicana de la fruta, Anastrepha ludens (Loew), en Mexico tiene mas de 10 anos en cria masiva. Los insectos esteriles son liberados en una gran variedad de condiciones ambientales como parte de un control integrado para suprimir diversas poblaciones de esta plaga dentro de la Republica Mexicana. El objetivo de este documento esta dirigido a revisar el desempeno de las moscas esteriles frente a poblaciones silvestres procedentes de diferentes ambientes y para esto se realizaron comparaciones de compatibilidad y competitividad sexual de las moscas esteriles contra poblaciones silvestres de seis estados representativos de la Republica Mexicana: Nuevo Leon, Tamaulipas, Sinaloa, Nayarit, Michoacan y Chiapas. Los resultados obtenidos manifiestan diferencias en el horario de inicio de llamado y mayor actividad sexual del macho entre las moscas provenientes de cada estado. Sin embargo el indice de aislamiento (ISI) reflejo compatibilidad sexual entre la cepa de laboratorio y todas las poblaciones analizadas, indicando que los individuos esteriles pueden aparearse satisfactoriamente con las poblaciones silvestres de los seis estados. El indice de efectividad de apareamiento del macho (MRPI) reflejo de manera global que los machos esteriles son tan efectivos para copular como los silvestres. El indice de efectividad de apareamiento de la hembra (FRPI) reflejo que en la mayoria de los estados las hembras silvestres copularon en mayor proporcion que las hembras esteriles, excepto para las poblaciones de Tamaulipas y Chiapas. En general, la baja participacion de las hembras esteriles en el campo permitio al macho esteril ampliar su probabilidad de apareamiento con las hembras silvestres. En cuanto al indice de esterilidad relativa (RSI), observamos que la aceptacion de las hembras silvestres al macho esteril (25-55%) fue similar a la de los machos silvestres. Las hembras de la poblacion de Chiapas registro la menor aceptacion. Finalmente, los resultados obtenidos en la prueba de Fried, la cual determina la esterilidad inducida presentaron un coeficiente de competitividad entre 0.2 y 0.5. Esto sugiere que los machos esteriles compliten exitosamente y son compatibles con moscas de diferentes origenes geograficos. (author)

  19. Revisiting an era in Germany from the perspective of adolescents in mother-headed single-parent families.

    PubMed

    Sharma, Deepali; Silbereisen, Rainer K

    2007-02-01

    Much of the documented work on families headed by single mothers is based on empirical evidence from North America and a few Anglo-Saxon countries. Many researchers consider single-mother families to be at a disadvantage because of nonsupportive family policies. This paper uses data from a social context that differed hugely in this respect-the German Democratic Republic (GDR). The GDR provided extensive state support to single-mother families and, thus, was vastly different from other countries. Based on a literature review and using Hill's family stress theory, this paper is based on the hypothesis that adolescents living in mother-headed single-parent families and those living with their biological parents would have near-similar social outcomes (display of psychosomatic symptoms, perception of stress, display of delinquent behaviour, life satisfaction, academic self-efficacy, and academic grades) and family-related outcomes (relationship with parents and perception of family environment). Further, it was hypothesized that adolescents from stepfather families would display more negative social and family-related outcomes when compared with respondents from the other two family types. The sample comprised 1302 adolescents (M = 13.82 years, SD = 1.88) who were recruited from the city of Leipzig in the year immediately following German unification, 1991. Respondents reported on measures of psychosomatic symptoms, stress, delinquency, life satisfaction, academic achievement, and family-related variables. ANCOVAs, with a control for income adjusted for household size, indicated adolescents from single-mother families to have very similar experiences to respondents living with their biological parents on all measures except for their assessment of family environment. Adolescents living in stepfather families reported the least favourable experiences. Results are indicative of a social context in Germany that, despite unification and the early hardships for single-mother families, still provided these families with more opportunities than constraints. This paper was completed during a postdoctoral research fellowship from the Alexander von Humboldt Foundation awarded to the first author at the Department of Developmental Psychology and Centre for Applied Developmental Science, University of Jena, Germany. La plupart de la recherche publie sur les familles diriges par des mres monoparentales est base sur l'videnceempirique de l'Amrique du Nord et de quelques pays anglo-saxons. Plusieurs chercheurs considrent les familles de mres monoparentales comme tant dsavantages cause des politiques familiales non supportantes. Cet article utilise des donnes provenant d'un contexte social qui diffre largement dans ce sens, soit la Rpublique dmocratique allemande (RDA). La RDA a offert un large soutien de l'tat aux familles de mres clibataires et tait ainsi largement diffrente des autres pays. En se fondant sur une recension des crits et en utilisant la thorie du stress familial de Hill, cet article est bas sur l'hypothse que les adolescents vivant dans des familles monoparentales diriges par des mres et ceux vivant avec leurs parents biologiques auraient des rsultats sociaux (manifestation de symptmes psychosomatiques, perception du stress, expression du comportement dlinquant satisfaction de la vie, auto-efficacit scolaire et notes scolaires) et des rsultats familiaux (relation avec les parents et perception de l'environnement familial) quasi similaires. De plus, nous avons mis l'hypothse que les adolescents de familles recomposes avec beau-predmontreraient plus de rsultats familiaux et sociaux ngatifs, en comparaison aux rpondants des deux autres types de familles. L'chantillon comprend 1302 adolescents (M=13.82 ans, cart-type=1.88) et tait recrut de la ville de Leipzig pendant l'anne qui a immdiatement suivi l'unification allemande, soit 1991. Les rpondants ont rapport sur des mesures de symptmes psychosomatiques, de stress, de dlinquance, de satisfaction de la vie, de l'accomplissement scolaire et des variables relies a la famille. Des ANCOVAs, en contrlant pour le revenu ajust pour la taille du mnage, ont indiqu que les adolescents provenant de familles de mres monoparentales ont des expriences trs similaires aux rpondants vivant avec leurs parents biologiques sur toutes les mesures l'exception de leur valuation de l'environnement familial. Les adolescents vivant dans des familles recomposes avec beau-pre ont rapport les expriences les moins favorables. Les rsultats de cette tude dvoilent un contexte social en Allemagne qui, malgr l'unification du pays et ses difficults initiales pour les familles de mres monoparentales, leur a quand mme offert plus d'opportunits que de contraintes. Gran parte de trabajo documentado con familias encabezadas por una madre soltera se basa en datos de pases del norte de Amrica y anglo sajones. Muchos investigadores consideran a las familias de madre soltera en desventaja, debido a polticas que no apoyan a las familias. Este trabajo emplea datos de un contexto social diferente, la Repblica Democrtica Alemana (RDA). La RDA proporcion gran apoyo estatal a las familias de madres solteras y, por lo tanto, difera ampliamente de otros pases. Este trabajo, basado en la revisin de la literatura y empleando la teora del estrs familiar de Hill, propone como hiptesis que habra similitud entre los adolescentes que viven en familias de madre soltera y aqullos que viven con ambos padres biolgicos respecto a desenlaces sociales (manifestacin de sntomas psicosomticos, percepcin de estrs, manifestacin de conducta delincuente, satisfaccin con la vida, autoeficacia acadmica, y calificaciones escolares) y desenlaces relativos a la familia ( relacin con los padres y percepcin del ambiente familiar). Es ms, se propuso la hiptesis de que los adolescentes de familias con padrastro manifestaran ms efectos sociales y familiares negativos al compararse con adolescentes provenientes de los otros dos tipos de familias. La muestra, compuesta por 1302 adolescentes (M=13.82 aos, SD=1.88), se reclut en la ciudad de Leipzig al ao siguiente de la unificacin de Alemania, 1991. Los participantes respondieron a medidas de sntomas psicosomticos, estrs, delincuencia, satisfaccin por la vida, desempeo acadmico y variables relativas a la familia. Los anlisis de covarianza aplicados, controlando el ingreso ajustado al tamao de la familia, sugirieron que los adolescentes de familias de madre soltera tenan experiencias muy similares a las de aqullos que vivan con sus padres biolgicos en todas las medidas, excepto en la de evaluacin del ambiente familiar. Los adolescentes que vivan en familias con padrastro informaron experiencias menos favorables. Los resultados son indicativos de que el contexto social en Alemania proporcion an ms oportunidades que restricciones a las familias de madre soltera, a pesar de la unificacin y el comienzo de las dificultades que sta les impuso. PMID:24274779

  20. Seizures, cysticercosis and rural-to-urban migration: the PERU MIGRANT study

    PubMed Central

    Gonzales, Isidro; Miranda, J Jaime; Rodriguez, Silvia; Vargas, Victor; Cjuno, Alfredo; Smeeth, Liam; Gonzalez, Armando E; Tsang, Victor C W; Gilman, Robert H; Garcia, Hector H

    2015-01-01

    Objectives To examine the prevalence of seizures, epilepsy and seropositivity to cysticercosis in rural villagers (cysticercosis-endemic setting), rural-to-urban migrants into a non-endemic urban shanty town and urban inhabitants of the same non-endemic shanty town. Methods Three Peruvian populations (n = 985) originally recruited into a study about chronic diseases and migration were studied. These groups included rural inhabitants from an endemic region (n = 200), long-term rural-to-urban migrants (n = 589) and individuals living in the same urban setting (n = 196). Seizure disorders were detected by a survey, and a neurologist examined positive respondents. Serum samples from 981/985 individuals were processed for cysticercosis antibodies on immunoblot. Results Epilepsy prevalence (per 1000 people) was 15.3 in the urban group, 35.6 in migrants and 25 in rural inhabitants. A gradient in cysticercosis antibody seroprevalence was observed: urban 2%, migrant 13.5% and rural group 18% (P < 0.05). A similarly increasing pattern of higher seroprevalence was observed among migrants by age at migration. In rural villagers, there was strong evidence of an association between positive serology and having seizures (P = 0.011) but such an association was not observed in long-term migrants or in urban residents. In the entire study population, compared with seronegative participants, those with strong antibody reactions (≥ 4 antibody bands) were more likely to have epilepsy (P < 0.001). Conclusions It is not only international migration that affects cysticercosis endemicity; internal migration can also affect patterns of endemicity within an endemic country. The neurological consequences of cysticercosis infection likely outlast the antibody response for years after rural-to-urban migration. Objectifs Examiner la prévalence des crises d’épilepsie, de l’épilepsie et de la séropositivité à la cysticercose chez les villageois des zones rurales (cadre endémique pour la cysticercose), chez les migrants des zones ruraux vers les zones urbaines dans un bidonville urbain non endémique et chez les habitants urbains du même bidonville non endémique. Méthodes Trois populations péruviennes (n = 985) recrutées initialement dans une étude sur les maladies chroniques et la migration, ont été étudiées. Ces groupes comprenaient des habitants de zones rurales d'une région d'endémie (n = 200), des migrants de long terme de zones ruraux vers les villes (n = 589) et les personnes vivant dans le même milieu urbain (n = 196). Les troubles épileptiques ont été détectés par un sondage et un neurologue a examiné les répondants positifs. Des échantillons de sérum de 981/985 individus ont été testés pour les anticorps de cysticercose par Immunoblot. Résultats La prévalence de l’épilepsie (pour 1000 personnes) était de 15,3 dans le groupe urbain; 35,6 chez les migrants et 25 dans la population rurale. Un gradient dans la séroprévalence des anticorps de la cysticercose a été observé: dans le groupe urbain 2%, le groupe de migrants 13,5% et le groupe rural 18% (p <0,05). Une tendance croissante similaire de séroprévalence plus élevée a été observée chez les migrants selon l’âge à la migration. Chez les villageois ruraux, il y avait des preuves solides d'une association entre une sérologie positive et le fait d'avoir des crises (p = 0,011), mais une telle association n'a pas été observée chez les migrants de long terme ou chez les résidents urbains. Dans l'ensemble de la population de l’étude, ceux avec de fortes réactions d'anticorps (≥ 4 bandes d'anticorps) étaient plus susceptibles d'avoir l’épilepsie (p <0,001) comparé aux participants séronégatifs. Conclusions La migration internationale n'est pas la seule qui affecte l'endémicité de la cysticercose; la migration interne peut aussi modifier les profils d'endémicité au sein d'un même pays d'endémie. Les conséquences neurologiques de l'infection par la cysticercose sont susceptibles de survivre à la réponse d'anticorps durant des années après la migration des zones rurales vers les zones urbaines. Objetivos Examinar la prevalencia de convulsiones, epilepsia, y seropositividad para cisticercosis entre población rural (de zonas endémicas para cisticercosis), inmigrantes provenientes de zonas rurales a tugurios urbanos no endémicos, y habitantes urbanos de los mismo tugurios urbanos no endémicos. Métodos Se estudiaron tres poblaciones peruanas (n=985) originalmente reclutadas en un estudio de enfermedades crónicas y migración. Estos grupos incluían habitantes rurales de una región endémica (n=200), inmigrantes de larga duración de zonas rurales a urbanas (n=589), e individuos que vivían en la misma zona urbana (n=196). Las convulsiones se detectaron mediante una encuesta y un neurólogo examinó a quienes habían respondido positivamente. Se procesaron muestras de suero de 981/985 individuos en busca de anticuerpos para cisticercosis mediante inmunoblot. Resultados La prevalencia de epilepsia (por 1,000 personas) era de 15.3 en el grupo urbano, 35.6 en inmigrantes y 25 en habitantes rurales. Se observó un gradiente en la seroprevalencia de los anticuerpos para cisticercosis: grupos urbano 2%, inmigrante 13.5% y rural 18% (p<0.05). Se observó un patrón de aumento similar de mayor seroprevalencia entre inmigrantes según la edad que tenían en el momento de emigrar. En pobladores rurales, había una evidencia importante de asociación entre tener una serología positiva y sufrir convulsiones (p=0.011), pero esta asociación no se observaba en inmigrantes de larga duración o residentes urbanos. En la población al completo, comparada con los participantes seronegativos, aquellos con una fuerte reactividad de anticuerpos (≥4 bandas de anticuerpos) tenían una mayor probabilidad de sufrir epilepsia (p<0.001). Conclusiones No solo la migración internacional afecta la endemicidad de cisticercosis; la migración interna también puede afectar los patrones de endemicidad dentro de un país endémico. Las consecuencias neurológicas de la infección por cisticercos podrían durar más que la respuesta a anticuerpos años después de la migración de zonas rurales a zonas urbanas. PMID:25581851

  1. Hydrodynamic characteristics of the western Doñana Region (area of El Abalario), Huelva, Spain

    NASA Astrophysics Data System (ADS)

    Trick, Thomas; Custodio, Emilio

    The Doñana region, in southwestern Spain, comprises a large and important nature reserve, the wetlands of which are affected by human activity. Planting of an extensive eucalyptus forest in the 1950s and, more recently, the use of aquifers for irrigation and water supply for some coastal tourist resorts, have altered the natural groundwater-flow system. The area of the study is the western sector of the region, called El Abalario, which is a gentle topographic elevation between the Atlantic coast and La Rocina Creek (Arroyo de la Rocina). Underneath a variable layer of eolian sands with high dunes near the coast, thick Plio-Quaternary detritic strata, mostly fine silica sands, overlie marls. Near the base there is a variable, deltaic-origin layer of coarse sands and gravels. The dome-shaped water table, inside the sands, is close to the surface everywhere except beneath the dune belt, and small, temporary, shallow lagoons are numerous. The coarse sand and gravel layer conditions groundwater flow and behaves as a semiconfined layer between sands. A cross section through the area was simulated with a model to check the validity of the conceptual groundwater-flow pattern and its sensitivity to the hydraulic parameters. The model was calibrated using parameter values obtained by pumping tests and multilevel piezometric data, and checked against the estimated groundwater discharge into La Rocina Creek. Groundwater flows peripherally to the sea coast, to La Rocina Creek, or directly east and southeastward into the Doñana marshlands, in the Guadalquivir River delta. The average net aquifer recharge rate was calculated to be between 100 and 200 mm year-1 for the area covered by brush, but is remarkably lower in the areas of eucalyptus trees. The transient-state model shows that recharge varies spatially and is not clearly proportional to annual precipitation. Phreatic evapotranspiration plays an important role in decreasing the net value of aquifer recharge to approximately 0.4-0.6 of that calculated with a soil-balance model. The cross section model was used to study the effect of groundwater ion on water-table depth by subtracting the contribution of vertical flow, calculated by a well-hydraulics formula, to the semiconfined deep aquifer. The result was a decrease in phreatic evapotranspiration, flow into La Rocina Creek, and lagoon-inundation frequency. Replacement of the eucalyptus forest with native vegetation may raise water-table levels and even reactivate old tributaries to La Rocina Creek. La région de Doñana, située dans le sud ouest de l'Espagne, comprend une importante réserve naturelle avec des zones humides, affectée par l'activité humaine. L'exploitation de vastes plantations d'eucalyptus pendant les années 50 et l'usage plus récent des nappes souterraines pour l'irrigation et l'alimentation en eau des centres touristiques côtiers ont modifié le système de flux d'eau souterraine dans cette zone. La présente étude a été réalisée dans le secteur occidental, appelé El Abalario. Ce secteur consiste en une légère élévation située entre l'Océan Atlantique et la ravine de La Rocina. Une couverture variable de sables éoliens, formant une haute crête dunaire côtière, recouvre des sédiments detritiques plio-quaternaires, déposés eux même sur des sables siliceux lesquels reposent à leur tour sur des marnes. Près de la base se trouvent des sables grossiers et des graviers d'origine deltaïque, dont l'épaisseur varie spatialement. Le flux d'eau souterraine est conditionné par l'aquifère semi confinés des graviers et des sables grossiers. Le niveau phréatique de l'aquifère libre des sables fluvio-marins est peu profond, excepté sous les dunes. On y trouve souvent des petites lagunes temporaires peu profondes. Le flux de l'eau souterraine a été simulé dans une section verticale pour vérifier le modèle hydrogéologique conceptuel et la sensibilité aux variations des paramètres. Le modèle a été calé en utilisant d'une part les valeurs des paramètres hydrauliques obtenus par des essais de pompage et d'après les données piezométriques mesurées à différentes profondeurs, et d'autre part l'apport estimé de la ravine de La Rocina. L'écoulement d'eau souterraine s'effectue par drainage latérale dans trois directions, d'une part vers la côte, d'autre part à travers la ravine de La Rocina et finalement directement vers les Marais de Doñana situés à l'est et sud-est dans le delta du fleuve Guadalquivir. Avec une pluviométrie moyenne comprise entre 550 et 600 mm, la recharge nette moyenne annuelle des nappes, pour des périodes de temps assez longues, est estimée entre 100 et 200 mm dans les aires de végétation autochtone, et elle est nettement inférieure dans les aires plantées deucalyptus. Le modèle transitoire montre que la recharge varie dans l'espace et qu'elle n'est pas clairement proportionnelle aux précipitations annuelles. L'évapotranspiration phréatique joue un rôle important et diminue la valeur nette de la recharge des nappes de 0,4 à 0,6 de la valeur calculée avec un modèle de bilan d'eau dans le sol. La section modélisée est utilisée pour étudier l'effet de l'extraction d'eau souterraine sur la profondeur du niveau phréatique en soustrayant le flux vertical, calculé grâce à une formule d'hydraulique des puits, de la nappe profonde semi-confinée. Le résultat de cette extraction est une diminution de l'évapotranspiration phréatique, du flux au niveau de la ravine de La Rocina et de la fréquence d'inondation des lagunes. La substitution de forêts d'eucalyptus par de la végétation autochtone peut permettre la remonté des niveaux phréatiques et même réactiver d'anciens ravins affluents à La Rocina. La región de Doñana, situada en el sudoeste de España, incluye una gran e importante reserva natural, cuyos humedales están siendo afectados por la actividad humana. La extensa plantación de eucaliptus en la década de 1950 y el uso más reciente de los acuíferos para riego y para abastecimiento de centros turísticos costeros han modificado el sistema de flujo del agua subterránea en esta zona. Este estudio se ha realizado en el sector occidental, llamado El Abalario. Se trata de una elevación suave situada entre el océano Atlántico y el arroyo de La Rocina. Debajo de un manto variable de arenas eólicas, que forma un alto cordón dunar costero, se encuentran sedimentos detríticos plio-cuaternarios formados por arenas silíceas finas, que hacia la base incluyen una capa de arenas gruesas y gravas de origen deltrico, los que a su vez yacen sobre margas. El flujo de agua subterránea está relacionado con niveles de gravas y gravillas semiconfinadas por las arenas fluvio-marinas que contienen el nivel freático. El nivel freático es somero excepto debajo del cordón dunar. Son frecuentes pequeñas lagunas temporales. Se ha simulado el flujo de agua subterránea en una sección para comprobar el modelo de flujo conceptual y la sensibilidad a variaciones de los parámetros. El modelo fue calibrado usando los valores de los parámetros hidráulicos obtenidos en ensayos de bombeo y datos piezométricos medidos a diferentes profundidades, y la descarga estimada al arroyo de La Rocina. La recarga de agua subterránea drena lateralmente, por un lado hacia la costa y por otro lado a través del arroyo de La Rocina, o directamente hacia las Marismas de Doñana situadas en el delta del río Guadalquivir. Con una lluvia media anual entre 550 y 600 mm, la recarga neta media estacionaria anual del acuífero, considerando periodos de tiempo largos, se estima entre 100 y 200 mm en las zonas de vegetación autóctona, y es notablemente menor en las zonas de plantación de eucaliptos. El modelo transitorio indica que la recarga varia espacialmente y no es claramente proporcional a la precipitación para periodos de un año. La evapotranspiración freática varia espacialmente y juega un papel importante; disminuye el valor neto de la recarga al acuífero para dejarlo en 0,4 a 0,6 de lo que se calcula mediante un balance de agua en el suelo. La sección modelada sirve para estudiar el efecto de la extracción de agua subterránea sobre la profundidad del nivel freático mediante la substracción del flujo vertical, que se calcula mediante una fórmula de hidráulica de pozos para el acuífero semiconfinado profundo. El resultado es una disminución de la evapotranspiración freática, del flujo al arroyo de la Rocina y de la frecuencia de inundación de las lagunas. La substitución del bosque de eucaliptus por vegetación nativa puede elevar los niveles freáticos e incluso reactivar antiguos "caños" tributarios al arroyo de La Rocina.

  2. Constraining performance assessment models with tracer test results: a comparison between two conceptual models

    NASA Astrophysics Data System (ADS)

    McKenna, Sean A.; Selroos, Jan-Olof

    Tracer tests are conducted to ascertain solute transport parameters of a single rock feature over a 5-m transport pathway. Two different conceptualizations of double-porosity solute transport provide estimates of the tracer breakthrough curves. One of the conceptualizations (single-rate) employs a single effective diffusion coefficient in a matrix with infinite penetration depth. However, the tracer retention between different flow paths can vary as the ratio of flow-wetted surface to flow rate differs between the path lines. The other conceptualization (multirate) employs a continuous distribution of multiple diffusion rate coefficients in a matrix with variable, yet finite, capacity. Application of these two models with the parameters estimated on the tracer test breakthrough curves produces transport results that differ by orders of magnitude in peak concentration and time to peak concentration at the performance assessment (PA) time and length scales (100,000 years and 1,000 m). These differences are examined by calculating the time limits for the diffusive capacity to act as an infinite medium. These limits are compared across both conceptual models and also against characteristic times for diffusion at both the tracer test and PA scales. Additionally, the differences between the models are examined by re-estimating parameters for the multirate model from the traditional double-porosity model results at the PA scale. Results indicate that for each model the amount of the diffusive capacity that acts as an infinite medium over the specified time scale explains the differences between the model results and that tracer tests alone cannot provide reliable estimates of transport parameters for the PA scale. Results of Monte Carlo runs of the transport models with varying travel times and path lengths show consistent results between models and suggest that the variation in flow-wetted surface to flow rate along path lines is insignificant relative to variability in the amount of diffusive capacity that can be accessed along the transport pathway. Contraindre le bilan des performances des modèles avec les résultats de traçages: une comparaison entre deux modèles conceptuels. Des tests de traçage sont mis en oeuvre pour étudier les paramètres de transport de soluté d'une roche sur une longueur de 5 m. Deux différents modèles de transport de soluté dans un milieu à double porosité fournissent des estimation des courbes de restitution. L'une des conceptualisations (unique taux de restitution) emploie un seul coefficient effectif de diffusion dans une matrice possédant une pénétration infinie en profondeur. Par ailleurs, la rétention du traceur entre les différentes lignes d'écoulement peut varier comme le rapport des débits aux surfaces mouillées et comme le rapport de la différence de débits entres les lignes d'écoulement. L'autre conceptualisation (taux multiple) emploie une distribution continue de coefficients de diffusion dans une matrice à capacité variable et finit. L'application de ces deux modèles avec les pa! ramètres estimés grâce aux courbes de restitution produit des résultats de transport qui différent de plusieurs ordres de grandeur dans la magnitude du pic, le temps du pic de concentration, au bilan des performances (PA) et aux échelles de distance (100,000 ans et 1,000 m). Ces différences sont éxaminées par l'intermédiaire des temps limites pour que la capacité diffusive équivaille à un milieu infini. Ces limites sont comparées à travers les modèles conceptuels ainsi que les temps caractéristiques de diffusion à l'échelle du test de traçage et à l'échelle du PA. Par ailleurs, les différences entre les modèles sont éxaminées en réestimant les paramètres pour le modèle à taux multiple à partir des résultats du modèle à double porosité à l'échelle du PA. Les résultats indiquent que pour chaque modèle la valeur de la capacité diffusive dans un milieu infini sur une période de temps spécifiée explique les différences entre les modèles et le ! fait que le test de traçage seul ne permet pas de déterminer les paramètres de transport à l'échelle du PA. Les résultats des simulations Monte Carlo du modèle de transport avec des temps et des distances de transport variables montrent des résultats concordances entre les différents modèles et suggère que la variation que la variation entre surface mouillée et le rapport de la différence de débits entre les lignes d'écoulement est insignifiante, en regard de la variabilité du montant de la capacité diffusive qui peut être accessible le long de la ligne de transport. Delimitando la eficacia de modelos de evaluación con resultados de pruebas de trazadores: una comparación entre dos modelos conceptuales. Se llevaron a cabo pruebas de trazadores para evaluar los parámetros de transporte de solutos en un rasgo rocoso a lo largo de una trayectoria de transporte de 5 m. Dos diferentes conceptualizaciones del transporte de solutos de porosidad doble aportan estimados de las curvas de avance de trazadores. Una de las conceptualizaciones (ritmo único) utiliza un coeficiente de difusión efectiva único en una matriz con profundidad de penetración infinita. Sin embargo, la retención del trazador entre diferentes trayectorias de flujo puede variar debido a que la relación entre la superficie mojada de flujo y el ritmo de flujo difiere entre las líneas de trayectoria. La otra conceptualización (multi-ritmo) utiliza una distribución continua de coeficientes de ritmos de difusión múltiple en una matriz con capacidad variable pero finita. La aplicación de los dos modelos con los parámetros estimados en base a las curvas de avance de trazadores producen resultados de transporte que difieren en varios órdenes de magnitud, tanto en concentración pico como en el tiempo en que se alcanza la concentración pico, en las escalas de evaluación de eficacia (PA) de tiempo y longitud (100,000 años y 1,000 m). Estas diferencias se examinan mediante el cálculo de límites de tiempo en que se considera que la capacidad difusiva actúa como un medio infinito. Estos límites se comparan en ambos modelos conceptuales y contra los tiempos característicos para difusión en escalas de PA y de prueba de trazador. Adicionalmente, se examinan las diferencias entre los modelos calculando de nuevo los parámetros para el modelo multi-ritmo a partir del modelo tradicional de doble porosidad a escala PA. Los resultados indican que para cada modelo la cantidad de la capacidad difusiva que actúa como un medio infinito sobre la escala de tiempo especificada explica las diferencias entre los resultados del modelo y que las pruebas de trazadores por sí solas no aportan cálculos confiables de los parámetros de transporte para la escala PA. Los resultados provenientes de corridas Monte Carlo de los modelos de transporte con distintos tiempos de viaje y diferentes longitudes de trayectorias muestran resultados consistentes entre modelos y sugieren que la variación en la relación de superficie de flujo mojada a ritmo de flujo a lo largo de las líneas de trayectoria es insignificante en relación con la variabilidad en la cantidad de capacidad difusiva que puede alcanzarse a lo largo de la trayectoria de transporte.

  3. Farmyard Manure and Fertilizer Effects on Seed Potato (Solanum tuberosum L.) Yield in Green House Production

    NASA Astrophysics Data System (ADS)

    László, M.

    2009-04-01

    Nowadays is widely well know that the potato is an important vegetable crop at Brazíl. It is grown on about 173.000 ha, with total yield of 2.6 million tons year-1. The average yield is 15 t ha-1. This level is very low because degeneration of crop is rapid under high temperature and high viruses pressure. Therefore seed potato propagation and production is principal on consumption potato production. This is why we found it necessary to develop it. The latossolo vermelho soil-farmyard manure- burnt rice straw-fertilizer 4N:14P:8K greenhouse pot trial was set up at the National Vegetable Crops Research Center, Brasília-DF, Brazíl in 1990. The methods of the experiments were soil x farmyard manure x burnt rice straw, soil x 4N:14P:8K fertilizer and soil x farmyard manure x burnt rice straw x 4N:14P:8K fertilizer on randomized block design in total 29 combination of treatments in 5, 5 and 3 repetitions with in a total parcel of 116. According to chemical analysis of the a., soil, b., farmyard manure and c., burnt rice straw the agrochemistry parameters were as follows (estimated datas): a., latossolo vermelho soil: CaCO3 0.3-0.7%, humo 0.9-1.0%, pH (H2O) 5.3, pH (KCl) 4.5, AL- P2O5 3.2-3.5 mg kg-1, AL- K2O 180 mg kg-1, Mg (KCl) 70 mg kg-1, EDTA-Zn 0.5-0.8 mg kg-1, EDTA-Cu 0.5-0.6 mg kg-1, b., farmyard manure: N 1.8 g kg-1, P2O5 2.0 g kg-1, K2O 4.0 g kg-1, c., burnt rice straw: N 0.8 g kg-1, P2O5 7.0 g kg-1, K2O 4.5 g kg-1. The experimental datas were estimated by analysis of variance, ANOVA and MANOVA. The main conclusions were as follows: 1. Mixture of 80% latossolo vermelho, 10% burnt rice straw and 10% farmyard manure were shown best performance on seed potato productivity. The piece of tubers with a 0-20 mm (consumption seeds) was increased by 77%. 2. Total seed potato number was reached maximum at 10.8 g pot-1 4N:14P:8K fertilizer regarding to average of treatments with a 33%. 3. Dry biomassa production plant-1 was decreased by high dose of 4N:14P:8K fertilizer (18.0 g pot-1) with a hard effect (57%). Our results are shown that it was possible developing of the seed potato production under tropical greenhouse conditions by optimalised soil-organic matter-fertilizer system. This datas should be as indicators to sustainable field potato advisory systems. Keywords: potato (Solanum tuberosum L.), greenhouse, latossolo vermelho soil, farmyard manure, burnt rice straw, 4N:14P:8K fertilizer, sustainability, yield Introducáo: Importância e situação actual em produção da batata no Brazíl A batata é atualmente uma das hortaliças de maior importância no Brasíl (Márton 2000a., 2000b.) com um cultivo annual médio de 173.000 ha e uma produção de 2600000 t. A produtividade médio nacional é de 15 t ha-1, muito baixa se considerar que é possivel a obtenção de rendimentos acima de 40 t ha-1. Observa- se também, que existe variação no produtividade entre regiões e estados. E importante como fonte de alimento pelo seu alto valor nutricional a quantidade produzida muito superior por unidade de área a tempo, se comparada com diversas outras culturas (László 2000b., 2000c.). Os estados que tradicionalmente produzem batata em maior ou menor escala são indicados em seguente: Pernambuco, Ceará, Sergipe, Goiás, Mato Grosso, Mato Grosso do Sul, Rondonia e Acre. Os plantios predominantes são o das águas e das secas, sendo o de inverno bem menos expressivo, pois poucas áreas permitem o seu cultivo, na maioria dos casos necessitando- se de irrigação. Considerando as três épocas de plantio e diferentes condições climaticas brasileiras, podemos definir de um modo geral o plantio de batata no Brasíl da seguinte maneira: Nordeste e Centro- Oeste- plantio de inverno, Sudeste- plantio das águas, secas e inverno, Sul- plantio das aguas, secas e inverno. Sendo este último em áreas muito limitadas. Dentre as hortaliças a batata é uma das culturas mais estudadas actualmente. Os principais problemas que afetam a cultura da batata podem ser de ordem agronómica, economica e comercial. Como exemplos destes podem ser citados: o uso racional de matérias orgânicos, esterco de curral e inorgânico fertilizantes. Efeito de materias orgnicânicos e N, P, K elementos minerais para produção da batata As necessidades em N, P, e K elementos minerais da batata são superidas pela aplicação apropriada de matérias orgânicos, esterco de currals, fertilizantes ao solo, combinada com a ambiente (Márton 2001a., 2001b.), época adequada e posição ideal de aplicá- lo. Efeito da materias orgânicos O suprimento de N á batateira provém principalmente da matéria orgânica do solo e do fertilizante aplicado (László 2000a., Márton et all. 2000.). Embora não seja muito praticado no Brasíl, a incorporação de esterco ao solo é fator de aumento da produção de tuberculos. Este resultado favorável poderia ser atribuído ao melhoramento da estrutura do solo, á maior retenção de água pelo e mesmo favorecendo o melhor desenvolvimento do sistema radicular da planta. A batata pode ser cultivada em todo tipo de solo desde que tenha boa drenagem e seja bem estruturado. Isto é tem que ser bem aerado e permitir o bom desenvolvimento dos órgãos subterráneos da batateira. Sem de matéria orgânicos e esterco de curral a tendencia de determinados solos formar crosta, oferecendo uma alta resisténcia mecánica á emergéncia das plantas, pode ser um determinante de stands desuniformes. A cause primaria da formação de crostas é a destruição dos agregados do solo pela excessiva manipulação mecánica resultando em aeração reduzida e aumento da densidade e coesão das particulas do solo. O encrostamento do solo pode ser reduzido através com matérias orgânicos. De maneira geral, a produção de tuberculos em solo de baixa potencialidade (aqueles em que a penetração das raizes é dificultada pela compactação, textura argilosa ou com camadas no solo) será menor do que nagueles com alta potencialidade (boa textura e adequada retenção de agua). Efeito do nitrogênio No Brazíl em todas regiões onde se cultiva batata é raro encontrar solos com elevado teor de nitrogênio e que não precisam de quantidades desta elemento. É o elemento que governa o padrão de desenvolvimento da planta, estimulando principalmente o crescimento da parte aérea (Kádár et all. 2000., László 2000.). Para se obter rendimento de tubérculos é necessário um rápido e curto periodo de desenvolvimento da parte aérea e uma fase de acúmulo maior possível. Para tanto, devem ser evitadas doses muito altas de nitrogênio e, principalmente, se aplicadas tardiamente, pois haverá demasiado desenvolvimento de folhas que demorarão mais a finalizar seu crescimento e maturação. Isto implicará na redução do periodo de intenso desenvolvimento dos tubérculos e armazenagem do amido, resultando em menor produção. Há risco para a saúde na ingestão de alimentos com altos teores de nitrato e nitrito, havendo preocupação com o efeito de doses mais altas de nitrogênio sobre os teores dos mesmos nos tuberculos. Embora haja diferenças entre cultivares, localidades e períodos de armazenamento, há estudos mostrando que a fertilização com até 150 kg ha-1 de nitrogênio não foi suficiente para propiciar niveis preocupantes de nitrato nos tuberculos colhidos. Efeito do fósforo A grande maioria dos solos brasileiros cultivados com batata apresentam limitações ao bom desenvolvimento e produção da cultura em função dos baixos níveis de fósforo. Isto significa que aumentos de produção quase sempre ocorrem quando o solo recebe adubação fosfatada (László 2001a.). Estes aumentos são mais marcantes em solos nunca antes adubados ou com baixo teor de fósforo. Nestes, dificilmente alcanca- se a produção máxima com níveis reduzidos de fósforo. Não seria exagerado supor níveis de 600 a 800 kg ha-1 de P2O5, como sendo aqueles que iriam proporcionar produção máximas, principalmente em solos mais ácidos e pobres em matéria orgânico. A adubação fosfatada é muito importante no crescimento inicial da planta e, além de aumentar a produção de tuberculos em peso e números, aumenta também a quantidade e qualidade do amido neles contidos e reduz perdas durante o armazenamento dos mesmos. A quantidade de fósforo a aplicar dependerá da análise do solo considerando- se principalmente o nível de P existente e a textura do solo. Solos de textura média e arenosa necessitam maior conteúdo de fósforo do que os de textura argilosa para serem considerandos solos de baixo, médio ou alto teor de fósfato. Efeito da potássica Embora seja o elemento mais absorbido pela batateira, nem sempre há resposta positiva da aduba potássica sobre o rendimento da cultura. Provavelmente isto esteja relacionado com níveis elevados deste elemento no solo (Kurnik et all. 2001.). Entretanto, em solos com médios e baixos teores de potássio, aumentos significativos são conseguidos. Por isto, as recomendações de adubação com potássio, nas diversas regiões do mundo, variam de 50-300 kg ha-1 de K2O. Resultados de trabalhos em brasiléiros têm demonstrado que a aduba potássica pode ser substituída pela aplicação de 150 m3 ha-1 de vinhaça de cana de açúcar. Ao elevar- se a dose de fertilização potássica deverá haver precaução para que a adubação magnesiana seja suficiente. O K além de aumentar a produção, em solos deficientes, aumenta também o tamanho dos tubérculos produzidos, e a proporção de tubérculos grandes. Deficiência no suprimento de potássio á planta pode acarretar produção de tubérculos com elevada susceptibilidade aos danos mecánicos pós-colheita. Os tubérculos injuriados enegrecem facilmente e este enegrecimento é inversamente proporcional á quantidade de potássio nos tuberculos. Ademais, quando fritos dão origem a um produto escuro, de baixa valor comercial. Manejo de adubação Diversos fatores como potencial de produção do solo, modo de aplicação do fertilizante dentre outro fatores afetam a resposta da batateira á aplicação de fertilizantes (Refschneider 1987.). Depreende- se pois que no estabelecimento de um nivel ideal de fertilização as variáveis planta, solo e condições climaticas devem ser visualizadas como um sistema pouco provável de ser homogeneo mesmo em nivel de fazenda. Como tal, generalizações a respeito de doses ou niveis de fertlização são difíceis de serem feitas, recomendações exigem julgamento hábil por parte do fazendeiro ou do tecnico responsavel pela cultura (Márton 2001a., 2001b.). Este julgamento será mais preciso conhecendo- se pontos que serão rápidamente discutidos a seguir. A taxa de absorção de nutrientes é governada pela concentração externa ou suprimento de nutrientes pelo solo e a demanda do nutriente criada pelo desenvolvimento e funcinamento normal dos diversos órgãos das plantas. O nivel de nutrientes na solução do solo deve ser suficiamente alto para que suas taxas de absorção não sejam limitantes ao crescimento. Por outro lado, não deve ser demasiado para causar excessiva absorção de outros nutrientes. Forte associação existe entre a absorção de nutrientes e o desenvolvimento da planta. De maneira geral, a fase de rapido desenvolvimento da cultura é acompanhada por um grande aumento na absorção de nutrientes com a taxa de absorção declinado quando a taxa de crescimento diminuiu. Normalmente todos os fertilizantes potássicos e fosfatados são adicionados ao solo na época do plantio. O nitrogênio normalmente é parcelado. Cerca de 2 por 3 do nível recomendado é colocado no sulco de plantio e o restante adicionado por ocasião da amontoa. É uma prática tradicinal e com pouco suporte experimental no condiõces brasileiras. Espera -se que a aplicação parcelada do nitrogênio e mesmo do potássio possem ser benéficas quando houver chuva excessiva ou irrigações mal executadas principalmente em solos mais arenosos onde poderá ocorrer a lixiviacão dos mesmos (Márton 2001a., 2001b.). O parcelamento poderá também ser benéfico quando elevados níveis de fertilizantes porém recomendandos e a aplicação por feita nos sulcos de plantio, pois evitar-se ia assim, elevada concentração salina em torno dos tubérculos plantados, embora a aplicação á lanco, em toda área, possa ser opção vantajosa. Quantidades corretas de fertilizantes, posição ideal e época certa de aplicação, combinadas adequadamente, definem o programa de adubação da batata. Esse programa é variável de acordo com o solo, a batata e condisões ambientais (Márton 2001a.). A dose de um elemento a ser aplicada em batata, é função da quantidade desse elemento suprida pelo solo e da percentagem de recuperação do elemento adicionado ao solo como fertilizante. Resultados experimentais comparando a aplicação de fertilizante á lanco ou localizado mostram respostas variadas sobre a produção. E possivel encontrar resultados iguais em ambos os métodos, de supremacia da aplicação á lanco ou da aplicação localizada (Kurnik et all. 2001.). Parece que baixas quantidades de fertilizantes são mais eficiemente utilizadas quando aplicação nos sulcos de plantios. Entretanto o potancial de produção pode ser aumentando com alta ou mesmo moderada quantidade de fertilizantes aplicados á lanço. A recomendação geral de colocar o adubo no sulco de plantio da batata merece ser questionada. É uma recomendação válida ao entender- se que a batata responde bastante á aplicação de fósforo, que os solos brasileiros tem alta capacidade de absorção de fósforo e que haverá maior proliferação de raízes na área fertilizada. Uma indagação aparece: um solo com baxa disponibilidade de fósforo fora da zona fertilizada permitiria o desenvolvimento ótimo da planta. Algumas evidéncias mostram, para outras espécies, que grande parte do sistema radicular, deve estar exposta ao fósforo para suprir as necessidades das plantas. Ademais, há um determinado valor de concentração de fósforo, na solução do solo, acima da qual a taxa de absorção não é aumentada. Essas considerações suscitam a possibilidade de questionar se a aplicação de fósforo em sulcos seria a forma mais eficiente de usá-lo quando se pretende alcancar elevadas produções. Deve-se lembrar entretanto, que solos tropicais, ainda com baixos teores fósforo e alta capacidade de adsorção, seria necessária dose muito elevada de P, quando aplicada á lanço, em todo o terreno. Se a aplicação localizada do fósforo pode, em parte, ser explicada, a do nitrogênio e potássio não são facilmente justificadas sob o aspecto de eficiéncia de utilização. Pelo contrário, ela pode ser questionada, principalmente pelas suas caracteristicas de difusão, pelo efeito que altas concentração de amónio e cloreto podem ter sobre a pressão osmotica da solução do solo junto aos tubérculos plantados, pelo efeito negativo do cloreto sobre a absorção de fósforo e também sobre a capacidade produtiva das plantas. Portanto, existe a possibilidade de ocorrer toxidez de amónio e de cloreto ao se aplicar doses altas dos fertilizantes nos sulcos de plantios. Isto pode determinar uma menor eficiéncia no uso dos fertilizantes. Materiais e Metodos: Nos desenvolverémos os três experimentos (i.e.: 1., 2., 3.) para aumentár-se do produção e produtividade da batata (Solanum tuberosum L.) semente pré- básica no casa de vegetação com diferentes doságens do latossolo vermelho novo, do esterco de curral e do adubo fórmula 4N:14P:8K no Empresa Brasileira de Pesquisa Agropecuaria- Centro Nacional de Pesquisas de Hortaliças, da Brazília-DF no 1990. Caracteristicas agroquímicas do solo em faixa arado (dados estimados), e conteudos N, P2O5, K2O do esterco de curral e palha de arroz queimado (dados estimados): a., caracteristicas agroquímicas do solo latossolo vermelho (solo novo: nunca foi usado para produção da batata semente): CaCO3 0.3-0.7%, humo 0.9-1.0%, pH (H2O) 5.3, pH (KCl) 4.5, AL- P2O5 3.2-3.5 mg kg-1, AL- K2O 180 mg kg-1, Mg (KCl) 70 mg kg-1, EDTA-Zn 0.5-0.8 mg kg-1, EDTA-Cu 0.5-0.6 mg kg-1 com abastecer fraco destes elementos, b., conteudos N, P2O5, K2O do esterco de curral (qualidade médio): N 1.8 g kg-1, P2O5 2.0 g kg-1, K2O 4.0 g kg-1, c., conteudos N, P2O5, K2O do palha de arroz queimado (palha de arroz foi queimado em um especial forno): N 0.8 g kg-1, P2O5 7.0 g kg-1, K2O 4.5 g kg-1. Nestas provas usarémos para controle a *mistura padrão. O este tratamento é a composição usual neste programa i.e.: 150 l de solo novo, 50 l de palha de arroz queimado, 50 l de esterco de curral, 350 gramas de cal e 300 gramas de adubo da fórmula 4N:14P:8K. Experimento 1. Efeito de diferentes misturas para produção da batata semente pré- básica em casa de vegetação O experimento foi instalado considerando-se sete misturas de substrato (latossolo vermelho novo, esterco de curral, palha de arroz queimado) em 3000 cm3 volume de capacidade de vasos preto com cinco repetições, no delineamento experimental de blocos ao acaso, na mésas experimentais em caso de vegetação. A cultivar foi a Achat, com plãntulas provenientes de cultura de tecidos. A data de plantio foi 18.04.1990. Plantarémos em cada vaso 3-3 "in vitro" plantulas com raiz embaixo de 4cm de superficie da mistura no vasos. Irrigarémos com 12 mm quantidade da augua 2 vezes por semana. Para produção aplicarémos sistema de proteção de plantas como usados no Brasíl. Ambiente foi controlado com ventilação automatizado. Temperatura médio foi 22 0C e humidade médio foi 68% durante de experimento. A data de colheta foi 04.07.1990. As pesagens foram feitos como peso fresco. Os resultados foram submetidos a analise de variáncia, ANOVA. As misturas do substrato utilizadas foram como a seguir no Tabela 1. Experimento 2. Efeito de adubo 4N:14P:8K para produção da batata semente pré- básica em casa de vegetação O experimento foi instalado considerando-se 9 dosagens de adubo da fórmula 4N:14P:8K com latossolo vermelho novo em 3000 cm3 volume de capacidade de vasos preto com cinco repetições, no delineamento experimental de blocos ao acaso na mésas experimentais em casa de vegetação. O adubo foi posicionando no solo de 4 cm abaixo de superficie do solo. A cultivar foi a Achat, com plãntulas provenientes de cultura de tecidos. A data de plantio foi 18.04.1990. Plantarémos em cada vaso 3-3 "in vitro" plantulas com raiz embaixo de 4cm de superficie da mistura no vasos. Irrigarémos com 12 mm quantidade da augua 2 vezes por semana. Para produção aplicarémos sistema de proteção de plantas como usados no Brasíl. Ambiente foi controlado com ventilação automatizado. Temperatura médio foi 22 0C e humidade médio foi 68% durante de experimento. A data de colheta foi 04.07.1990. As pesagens foram feitos como peso fresco. Os resultados foram submetidos a analise de variáncia, ANOVA. As doságens de adubo foram como a seguir no Tabela 2. Experimento 3. Efeito de latossolo vermelho novo, palha de arroz queimado e adubo 4N:14P:8K para produção da batata semente pré- básica em casa de vegetação Para pesquisar estes efeitos o experimento tipo de (2 x 6) foi instalado considerando-se as combinações entre duas misturas (i.e.: 1., 2.) e seis doságens de adubo complexo 4N:14P:8K, com três repetições, no delineamento experimental de bloco ao acaso, sendo 1 vaso (3000 cm3 volume de capacidade de vasos preto) por parcela na mésas experimentais em casa de vegetação. O adubo foi posicionando no solo de 4 cm abaixo de superficie do solo. A cultivar utilizada foi Baraka e o tamanho de tuberculos foi com 0-20 mm. A data de plantio foi 25.09.1990. Plantarémos em cada vaso 3-3 tuberculos com embaixo de 4cm de superficie da mistura no vasos. Irrigarémos com 12 mm quantidade da augua 2 vezes por semana. Para produção aplicarémos sistema de proteção de plantas como usados no Brasíl. Ambiente foi controlado ventilação automatizado. Temperatura médio foi 21 0C é humidade médio foi 66% durante de experimento. A data de colheta foi 14.12.1990. As pesagens foram feitos como peso fresco e matéria seca. Os resultados foram submetidos a analise de variáncia, MANOVA. Os manejos foram como a seguir no Tabela 3. Resultados e Discuscáo Experimento 1. Efeito de diferentes misturas para produção da batata semente pré- básica em casa de vegetação O tratamento 3. i.e.: mistura de 80% latossolo vermelho novo, 10% palha de arroz queimado e 10% esterco de curral, apresentou os maiores valores para numero de tuberculos com 0-20 mm (tamanho de comercial), peso de tuberculos com 0-20 mm e peso total de tuberculos por vaso. Porém, não houve diferencas significativas para o numero tuberculos comerciais, i.e.: com 0-20 mm, para os tratamentos 2., 3., 4., e 5. Portanto, a mistura poderá ter uma composição entre 60 a 90% de latossolo vermelho novo, 6 a 24% de palha de arroz queimado e de 4 a 16% de esterco de curral. Não houve diferenca significativa entre a mistura padrão utilizada e as misturas incluidas nos extremos indicados anteriormente. Porém, a mistura padrão recebeu adubação quimica de 4N:14P:8K (3.6 grama vaso-1) e calcário na dosagem de 4.2 grama vaso-1, o que não aconteceu com as parcelas das misturas em analise. Experimento 2. Efeito de adubo 4N:14P:8K para produção da batata semente pré- básica em casa de vegetação Há um efeito crescente das dóses de 4N:14P:8K nos caracteres observados. Porém, a maior dóse não chegou a ultrapassar a mistura padrão. Experimento 3. Efeito de latossolo vermelho novo, palha de arroz queimado e adubo 4N:14P:8K para produção da batata semente pré- básica em casa de vegetação Efeitos de misturas As duas misturas (i.e.: 1 e 2) deram resultados significativos mais alto que a mistura padrão, em média 54 %. Entre as misturas 1 e 2, foi melhor a 2. (80% latossolo vermelho novo, 10% palha de arroz queimado, 10% esterco de curral). Examinando-se 15 fatores, entre 11 casos afirmou-se a mistura como para melhor que a mistura 1. (70% latossolo vermelho novo, 20% palha de arroz queimado, 10% esterco de curral). Em caso de número de tuberculos 0-20 mm com a mistura 2. foi possivel aumentar geralmente os números de tuberculos em 77% que a mistura padrão. Efeitos de adubação 1. Área da folhas por planta entre manejo foi melhor de modo significativo a doságem de 3.6 grama vaso-1 adubo complexo (3103 cm2 plantas-1). 2. Peso fresco da folhas e de hastes por plantas as tendencias foram parecidos com o da área de folhas. 3. Peso fresco de raizis por planta até 7.2 grama vaso-1 diminuiu depois aumentou. 4. Peso fresco total de tuberculos por planta as crescentes doságens de um modo forte diminuiram a produção de tuberculos de 0 e 18.0 grama vaso-1 em 160% em os dois caso da mistura. 5. Peso de fitomassa fresco por planta foi melhor a 3.6 g vaso-1 (239 grama planta-1 em médio da dois mistura), depois os dados diminuirám. 6. Produção de biomassa fresco por planta a maxima produção (188 grama planta-1) foi obtida com 3.6 grama vaso-1. Deste ponto de modo forte caiu a produção. 7. Peso da matéria seca de folhas, hastes e raizis por planta somente em caso de mistura padrão o resultado foi significativo em relação aos outros tratamentos. 8. Péso da matéria seca de tuberculos total por planta modo significativo diminuiu a produção (0 e 18.0 grama vaso-1 = 360%) em médio da duas misturas. 9. Biomassa produção de materia seca por planta modo significativo diminuiu para efeito de alta dosagens de adubo complexo (0 e 18.0 grama vaso-1 = 158%) em médio da duas misturas. 10. Peso fresco de tuberculos com 0-20 mm as crescentes dosagens de 0 e 18.0 grama vaso-1 diminuiram a produção em 213% em médio da duas misturas. 11. Peso fresco de tuberculos com 20 mm-1 as crescentes dosagens de 0 e 18.0 grama vaso-1 diminuiram a produção assima de 250% em médio da duas misturas. 12. Numero de tuberculos 0-20 mm e 20 mm- por planta com os manejos de 0 e 18.0 grama vaso-1 foi possível aumentar em media 200% sobre a mistura padrão. Os manejo de 18.0 grama de adubo vaso-1 já causaram importante diminuição em relação caso a absoluto controle. 13. Numero total de tuberculos por planta entre manejos foi melhor a dosagem de 7.2 grama vaso-1 adubo complexo 4N:14P:8K comparando da mistura padrão. Nos verificamos-se que a mistura padrão sempre deu menor rasultados do que as outras misturas (i.e.: 1 e 2). Entre as misturas 1 e 2 a melhor foi a número 2. (80% latossolo vermelho novo, 10% palha de arroz queimado, 10% esterco de curral). Com esta mistura e com relação a mistura padrão, foi possível aumentar o número de tuberculos 0-20 mm com 77%. No caso do adubação, verificamos que grande quantidades de adubo acima de 7.2 grama vaso-1, de modo rigoroso diminuiu a produção de batata-semente pré- básica. Este fato deve ser considerado para a eleição das dosagens de adubos. Deve-se indicar o caso de número de tuberculos acima 20 mm-, onde em relação mistura padrão foi possivel aumentar em média 73% os resultados. Reconhecimento: Esta pesquisa foi apoio da Empresa Brasileira de Pesquisa Agropecuaria- Centro Nacional de Pesquisas de Hortaliças, Brasília-DF e Centro Pesquisa de Solo e Agroquímica do Academia Húngara de Ciências, Budapest References Kádár I-Márton L.-Horváth S. 2000. Mineral fertilisation of potato (Solanum tuberosum L.) on calcareous chernozem soil. Plant Production. 49: 291-306. Kurnik E.-Németh T.-Márton L.-Radimszki L. 2001. Effects of a new environment friendly deep fertilization system on a limy chernozem soil parameters. Agrochemistry and Soil Science. Budapest. In press László M. 2000. Nutrition of potato (Solanum tuberosum L.) on Hungary on a chernozem soil. Acta Agronomica Óváriensis. 42: 81-93. László M. 2001a. Climate change and N, P, K, Mg fertilization effects on potato (Solanum tuberosum L.) yield and quality. EAPR. Hamburg. In press László M. 2001b. Year and fertilization effect analysis in long field term experiments. XLIII. Georgikon Days. University of Veszprém. Keszthely László M.-Imre K.-Jose E.M. 2000a. Effects of Crotalaria juncea L. and Crotalaria spectabilis ROTH. on soil fertility and soil conservation in Hungary. Acta Agronomica Óváriensis. 42: 99-106. László M.-Silva J.C.-Jose A.B. 2000b. Ecological friendly dragée technics on different crops and vegetables seeds. Acta Agronomica Óváriensis. 42: 107-111. László M.-Silva J.B.C.-Jose A.B. 2000c. Ecological friendly dragée technics to sustainable precision agriculture. Fertilization in the Third Millenium. CASISCF. Beijing Márton L. 2000a. Effects of NPK fertilizers on potato (Solanum tuberosum L.) yield. Doctoral Ph.D Dissertation. University of Veszprém, Keszthely Márton L. 2000b. Effects of NPK fertilizers on potato (Solanum tuberosum L.) yield. Doctoral Ph.D Thesis. University of Veszprém, Keszthely Márton L. 2001a. Climete change effets on rye (Secale cereale L.) yield. Agrochemistry and Soil Science. Budapest. In press Márton L. 2001b. Climate change and fertilization effect analysis at the Tisza- river basin on rye yield. SZINET. University of Szent István. Gödöllő Márton L.-Kádár I.-Estáquio M.J. 2000. Effects of Crotalaria juncea L. and Crotalaria spectabilis ROTH on soil fertility and soil conservation. ESSC. Man and Soil at the Third Millennium. Abstract Book. 195. Valencia Reifschneider F.J.B. 1987. Produção de batata. Linha Gráfica e Editora. Brasília. p. 239. Tabela 1. Tratamentos do experimento 1. (Brasília-DF, 1990) ------------------------------------------------------------------ Numero de Composição em % Tratamento Solo novo Palha de arroz queimado Esterco de curral ------------------------------------------------------------------ 1. 100 0 0 2. 90 6 4 3. 80 10 10 4. 70 18 12 5. 60 24 16 6. 50 30 20 7. 40 36 24 ----------------------------------------------------------------- Tabela 2. Tratamentos do experimento 2. (Brasília-DF, 1990) ------------------------------------------------------- Numero de Adubo 4:14:8 N P2O5 K2O Tratamento Grama vaso-1 ------------------------------------------------------- 1. 0.0 0.000 0.000 0.000 2. 1.8 0.072 0.252 0.144 3. 3.6 0.144 0.504 0.288 4. 5.4 0.216 0.756 0.432 5. 7.2 0.288 1.008 0.576 6. 9.0 0.360 1.260 0.720 7. 10.8 0.432 1.512 0.864 8. 12.6 0.504 1.764 1.008 9. 14.4 0.576 2.016 1.152 ------------------------------------------------------- Tabela 3. Tratamentos do experimento 3. (Brasília-DF, 1990) ------------------------------------------------------------------------ Num. de Mistura % Trat. Solo novo Palea de arr. Q Esterco de curral 4N:14P:8K g vaso-1 ------------------------------------------------------------------------ 1. 70 20 10 0.0 2 70 20 10 3.6 3. 70 20 10 7.2 4. 70 20 10 10.8 5. 70 20 10 14.4 6. 70 20 10 18.0 7. 80 10 10 0.0 8. 80 10 10 3.6 9. 80 10 10 7.2 10. 80 10 10 10.8 11. 80 10 10 14.4 12. 80 10 10 18.0 ------------------------------------------------------------------------