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  • 1
    Series available for loan
    Series available for loan
    Canberra : Australian Gov. Publ. Service
    Associated volumes
    Call number: SR 93.0765(221)
    In: Bulletin
    Type of Medium: Series available for loan
    Pages: IX, 74 S. + 2 Kt.-Beil.
    ISBN: 0644088621
    Series Statement: Bulletin / Department of Primary Industries and Energy, Bureau of Mineral Resources, Geology and Geophysics 221
    Language: English
    Location: Lower compact magazine
    Branch Library: GFZ Library
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  • 2
    Publication Date: 1999-07-27
    Description: The Near Earth Asteroid Rendezvous (NEAR) spacecraft flew within 3830 kilometers of asteroid 433 Eros on 23 December 1998. The gravitational perturbation on NEAR was evident in the spacecraft tracking data. Ground-based Doppler and range tracking of the spacecraft as well as spacecraft images of the asteroid's center of figure and surface features were used to determine the mass and rotation pole of Eros. The mass of Eros is (7.2 +/- 1.8) x 10(18) grams and, coupled with a volume estimate provided by the NEAR imaging team, this mass suggests a bulk density of 2.5 +/- 0.8 grams per cubic centimeter. The rotation pole position is 15.6 (+/-3.7) degrees in right ascension and 16.4 (+/-1.8) degrees in declination, which is consistent with ground-based and NEAR imaging team observations.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Yeomans -- Antreasian -- Cheng -- Dunham -- Farquhar -- Gaskell -- Giorgini -- Helfrich -- Konopliv -- McAdams -- Miller -- Owen Jr -- Thomas -- Veverka -- Williams -- New York, N.Y. -- Science. 1999 Jul 23;285(5427):560-1.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Navigation and Flight Mechanics Section at the Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA. Applied Physics Laboratory, Johns Hopkins University, Laurel, MD 20723, USA. Cornell University, Ithaca, NY.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/10417380" target="_blank"〉PubMed〈/a〉
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  • 3
    Publication Date: 2001-04-21
    Description: On 25 October 2000, the Near Earth Asteroid Rendevous (NEAR)-Shoemaker spacecraft executed a low-altitude flyover of asteroid 433 Eros, making it possible to image the surface at a resolution of about 1 meter per pixel. The images reveal an evolved surface distinguished by an abundance of ejecta blocks, a dearth of small craters, and smooth material infilling some topographic lows. The subdued appearance of craters of different diameters and the variety of blocks and different degrees of their burial suggest that ejecta from several impact events blanketed the region imaged at closest approach and led to the building up of a substantial and complex regolith consisting of fine materials and abundant meter-sized blocks.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Veverka, J -- Thomas, P C -- Robinson, M -- Murchie, S -- Chapman, C -- Bell, M -- Harch, A -- Merline, W J -- Bell , J F 3rd -- Bussey, B -- Carcich, B -- Cheng, A -- Clark, B -- Domingue, D -- Dunham, D -- Farquhar, R -- Gaffey, M J -- Hawkins, E -- Izenberg, N -- Joseph, J -- Kirk, R -- Li, H -- Lucey, P -- Malin, M -- McFadden, L -- Miller, J K -- Owen , W M Jr -- Peterson, C -- Prockter, L -- Warren, J -- Wellnitz, D -- Williams, B G -- Yeomans, D K -- New York, N.Y. -- Science. 2001 Apr 20;292(5516):484-8.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Space Sciences Building, Cornell University, Ithaca, NY 14853, USA.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/11313490" target="_blank"〉PubMed〈/a〉
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  • 4
    Publication Date: 2000-09-23
    Description: We determined the mass of asteroid 433 Eros, its lower order gravitational harmonics, and rotation state, using ground-based Doppler and range tracking of the Near Earth Asteroid Rendezvous (NEAR)-Shoemaker spacecraft and images of the asteroid's surface landmarks. The mass of Eros is (6.687 +/- 0.003) x 10(18) grams, which, coupled with our volume estimate, implies a bulk density of 2. 67 +/- 0.03 grams per cubic centimeter. The asteroid appears to have a uniform density distribution. The right ascension and declination of the rotation pole are 11.37 +/- 0.05 and 17.22 +/- 0.05 degrees, respectively, and at least over the short term, the rotation state of Eros is stable with no measurable free precession of the spin pole. Escape velocities on the surface vary from 3.1 to 17.2 meters per second. The dynamical environment of Eros suggests that it is covered with regolith and that one might expect material transport toward the deepest potential wells in the saddle and 5.5-kilometer crater regions.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Yeomans -- Antreasian -- Barriot -- Chesley -- Dunham -- Farquhar -- Giorgini -- Helfrich -- Konopliv -- McAdams -- Miller -- Owen Jr -- Scheeres -- Thomas -- Veverka -- Williams -- New York, N.Y. -- Science. 2000 Sep 22;289(5487):2085-8.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Navigation and Mission Design Section, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA. Department of Terrestrial and Planetary Geodesy, Centre National d'Etudes Spatiales, Toulouse, France. Applied.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/11000104" target="_blank"〉PubMed〈/a〉
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  • 5
    Publication Date: 1999-07-27
    Description: During the 23 December 1998 flyby of asteroid 433 Eros, the Near-Earth Asteroid Rendezvous (NEAR) spacecraft obtained 222 images of Eros, as well as supporting spectral observations. The images cover slightly more than two-thirds of Eros (best resolution is approximately 400 meters per pixel) and reveal an elongated, cratered body with a linear feature extending for at least 20 kilometers. Our observations show that Eros has dimensions of 33 x 13 x 13 kilometers. The volume, combined with the mass determined by the NEAR radio science experiment, leads to a density of 2.5 +/- 0.8 grams per cubic centimeter. This relatively high density, and the presence of an extensive linear feature, suggest that Eros may be a structurally coherent body.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Veverka -- Thomas -- Bell 3rd -- Bell -- Carcich -- Clark -- Harch -- Joseph -- Martin -- Robinson -- Murchie -- Izenberg -- Hawkins -- Warren -- Farquhar -- Cheng -- Dunham -- Chapman -- Merline -- McFadden -- Wellnitz -- Malin -- Owen Jr -- Miller -- Williams -- et -- New York, N.Y. -- Science. 1999 Jul 23;285(5427):562-4.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Space Sciences Building, Cornell University, Ithaca, NY 14853, USA. Department of Geological Sciences, Northwestern University, 309 Locy Hall, Evanston, IL 60208, USA. Applied Physics Laboratory, 11100 Johns Hopkins Road, Laurel, MD 20723, USA. Sou.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/10417381" target="_blank"〉PubMed〈/a〉
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  • 6
    Publication Date: 2002-03-16
    Description: Multidrug-resistant tuberculosis (MDR) is perceived as a growing hazard to human health worldwide. Judgments about the true scale of the problem, and strategies for containing it, need to come from a balanced appraisal of the epidemiological evidence. We conclude in this review that MDR is, and will probably remain, a locally severe problem; that epidemics can be prevented by fully exploiting the potential of standard short-course chemotherapy (SCC) based on cheap and safe first-line drugs; and that best-practice SCC may even reduce the incidence of MDR where it has already become endemic. On the basis of the available, imperfect data, we recommend a three-part response to the threat of MDR: widespread implementation of SCC as the cornerstone of good tuberculosis control, improved resistance testing and surveillance, and the careful introduction of second-line drugs after a sound evaluation of cost, effectiveness, and feasibility.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Dye, Christopher -- Williams, Brian G -- Espinal, Marcos A -- Raviglione, Mario C -- New York, N.Y. -- Science. 2002 Mar 15;295(5562):2042-6.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Communicable Diseases, World Health Organization, CH-1211 Geneva 27, Switzerland. dyec@who.int〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/11896268" target="_blank"〉PubMed〈/a〉
    Keywords: Acquired Immunodeficiency Syndrome/complications ; Antitubercular Agents/pharmacology/*therapeutic use ; *Drug Resistance, Multiple, Bacterial ; Drug Therapy, Combination ; *Global Health ; HIV Infections/complications ; Humans ; Incidence ; Mycobacterium tuberculosis/*drug effects/physiology ; *Tuberculosis, Multidrug-Resistant/drug ; therapy/epidemiology/microbiology/prevention & control
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  • 7
    Publication Date: 1998-01-04
    Description: The terminal navigation of the Near Earth Asteroid Rendezvous (NEAR) spacecraft during its close flyby of asteroid 253 Mathilde involved coordinated efforts to determine the heliocentric orbits of the spacecraft and Mathilde and then to determine the relative trajectory of the spacecraft with respect to Mathilde. The gravitational perturbation of Mathilde on the passing spacecraft was apparent in the spacecraft tracking data. As a result of the accurate targeting achieved, these data could be used to determine Mathilde's mass as 1.033 (+/- 0.044) x 10(20) grams. Coupled with a volume estimate provided by the NEAR imaging team, this mass suggests a low bulk density for Mathilde of 1.3 grams per cubic centimeter.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Yeomans -- Barriot -- Dunham -- Farquhar -- Giorgini -- Helfrich -- Konopliv -- McAdams -- Miller -- Owen Jr -- Scheeres -- Synnott -- Williams -- New York, N.Y. -- Science. 1997 Dec 19;278(5346):2106-9.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉D. K. Yeomans, J. D. Giorgini, C. E. Helfrich, A. S. Konopliv, J. K. Miller, W. M. Owen Jr., D. J. Scheeres, S. P. Synnott, B. G. Williams, Navigation and Flight Mechanics Section, Jet Propulsion Laboratory (JPL), California Institute of Tech.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/9405343" target="_blank"〉PubMed〈/a〉
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  • 8
    Publication Date: 2003-08-16
    Description: Human immunodeficiency virus/acquired immunodeficiency syndrome (HIV/AIDS) has dramatically increased the incidence of tuberculosis (TB) in subSaharan Africa, where up to 60% of TB patients are coinfected with HIV and each year 200,000 TB deaths are attributable to HIV coinfection. Now HIV threatens control of TB in Asia, Eastern Europe, and Latin America. Antiretroviral (ARV) drugs can prevent TB by preserving immunity, but cohort analysis shows that early therapy, plus high levels of coverage and compliance, will be needed to avert a significant fraction of TB cases. However, ARV drugs could enhance the treatment of TB, and TB programs provide an important entry point for the treatment of HIV/AIDS.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Williams, Brian G -- Dye, Christopher -- New York, N.Y. -- Science. 2003 Sep 12;301(5639):1535-7. Epub 2003 Aug 14.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Communicable Diseases, World Health Organization, 1211 Geneva 27, Switzerland. williamsbg@who.int〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/12920302" target="_blank"〉PubMed〈/a〉
    Keywords: Acquired Immunodeficiency Syndrome/*complications/drug ; therapy/immunology/mortality ; Africa South of the Sahara/epidemiology ; Anti-HIV Agents/*therapeutic use ; Antitubercular Agents/therapeutic use ; CD4 Lymphocyte Count ; Cohort Studies ; Developing Countries ; Drug Therapy, Combination ; Female ; HIV Infections/*complications/drug therapy/immunology/mortality ; Hiv-1 ; Hiv-2 ; Humans ; Incidence ; Male ; Survival Rate ; Tuberculosis/complications/drug therapy/epidemiology/*prevention & control
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  • 9
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    American Association for the Advancement of Science (AAAS)
    Publication Date: 2010-05-15
    Description: More than 36 million patients have been successfully treated via the World Health Organization's strategy for tuberculosis (TB) control since 1995. Despite predictions of a decline in global incidence, the number of new cases continues to grow, approaching 10 million in 2010. Here we review the changing relationship between the causative agent, Mycobacterium tuberculosis, and its human host and examine a range of factors that could explain the persistence of TB. Although there are ways to reduce susceptibility to infection and disease, and a high-efficacy vaccine would boost TB prevention, early diagnosis and drug treatment to interrupt transmission remain the top priorities for control. Whatever the technology used, success depends critically on the social, institutional, and epidemiological context in which it is applied.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Dye, Christopher -- Williams, Brian G -- New York, N.Y. -- Science. 2010 May 14;328(5980):856-61. doi: 10.1126/science.1185449.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉World Health Organization, CH1211 Geneva 27, Switzerland. dyec@who.int〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/20466923" target="_blank"〉PubMed〈/a〉
    Keywords: AIDS-Related Opportunistic Infections/epidemiology/prevention & control ; Aging ; Antitubercular Agents/therapeutic use ; Disease Outbreaks ; Disease Susceptibility ; Endemic Diseases ; Genetic Predisposition to Disease ; HIV Infections/epidemiology/prevention & control ; Health Services ; Humans ; Incidence ; *Mycobacterium tuberculosis/drug effects/genetics/pathogenicity ; Polymorphism, Genetic ; Population Dynamics ; Prevalence ; Socioeconomic Factors ; Sputum/microbiology ; Tuberculosis/complications/*epidemiology/microbiology/*prevention & control ; Urban Health
    Print ISSN: 0036-8075
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  • 10
    Publication Date: 2015-10-17
    Description: The Pluto system was recently explored by NASA's New Horizons spacecraft, making closest approach on 14 July 2015. Pluto's surface displays diverse landforms, terrain ages, albedos, colors, and composition gradients. Evidence is found for a water-ice crust, geologically young surface units, surface ice convection, wind streaks, volatile transport, and glacial flow. Pluto's atmosphere is highly extended, with trace hydrocarbons, a global haze layer, and a surface pressure near 10 microbars. Pluto's diverse surface geology and long-term activity raise fundamental questions about how small planets remain active many billions of years after formation. Pluto's large moon Charon displays tectonics and evidence for a heterogeneous crustal composition; its north pole displays puzzling dark terrain. Small satellites Hydra and Nix have higher albedos than expected.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Stern, S A -- Bagenal, F -- Ennico, K -- Gladstone, G R -- Grundy, W M -- McKinnon, W B -- Moore, J M -- Olkin, C B -- Spencer, J R -- Weaver, H A -- Young, L A -- Andert, T -- Andrews, J -- Banks, M -- Bauer, B -- Bauman, J -- Barnouin, O S -- Bedini, P -- Beisser, K -- Beyer, R A -- Bhaskaran, S -- Binzel, R P -- Birath, E -- Bird, M -- Bogan, D J -- Bowman, A -- Bray, V J -- Brozovic, M -- Bryan, C -- Buckley, M R -- Buie, M W -- Buratti, B J -- Bushman, S S -- Calloway, A -- Carcich, B -- Cheng, A F -- Conard, S -- Conrad, C A -- Cook, J C -- Cruikshank, D P -- Custodio, O S -- Dalle Ore, C M -- Deboy, C -- Dischner, Z J B -- Dumont, P -- Earle, A M -- Elliott, H A -- Ercol, J -- Ernst, C M -- Finley, T -- Flanigan, S H -- Fountain, G -- Freeze, M J -- Greathouse, T -- Green, J L -- Guo, Y -- Hahn, M -- Hamilton, D P -- Hamilton, S A -- Hanley, J -- Harch, A -- Hart, H M -- Hersman, C B -- Hill, A -- Hill, M E -- Hinson, D P -- Holdridge, M E -- Horanyi, M -- Howard, A D -- Howett, C J A -- Jackman, C -- Jacobson, R A -- Jennings, D E -- Kammer, J A -- Kang, H K -- Kaufmann, D E -- Kollmann, P -- Krimigis, S M -- Kusnierkiewicz, D -- Lauer, T R -- Lee, J E -- Lindstrom, K L -- Linscott, I R -- Lisse, C M -- Lunsford, A W -- Mallder, V A -- Martin, N -- McComas, D J -- McNutt, R L Jr -- Mehoke, D -- Mehoke, T -- Melin, E D -- Mutchler, M -- Nelson, D -- Nimmo, F -- Nunez, J I -- Ocampo, A -- Owen, W M -- Paetzold, M -- Page, B -- Parker, A H -- Parker, J W -- Pelletier, F -- Peterson, J -- Pinkine, N -- Piquette, M -- Porter, S B -- Protopapa, S -- Redfern, J -- Reitsema, H J -- Reuter, D C -- Roberts, J H -- Robbins, S J -- Rogers, G -- Rose, D -- Runyon, K -- Retherford, K D -- Ryschkewitsch, M G -- Schenk, P -- Schindhelm, E -- Sepan, B -- Showalter, M R -- Singer, K N -- Soluri, M -- Stanbridge, D -- Steffl, A J -- Strobel, D F -- Stryk, T -- Summers, M E -- Szalay, J R -- Tapley, M -- Taylor, A -- Taylor, H -- Throop, H B -- Tsang, C C C -- Tyler, G L -- Umurhan, O M -- Verbiscer, A J -- Versteeg, M H -- Vincent, M -- Webbert, R -- Weidner, S -- Weigle, G E 2nd -- White, O L -- Whittenburg, K -- Williams, B G -- Williams, K -- Williams, S -- Woods, W W -- Zangari, A M -- Zirnstein, E -- New York, N.Y. -- Science. 2015 Oct 16;350(6258):aad1815. doi: 10.1126/science.aad1815.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Southwest Research Institute, Boulder, CO 80302, USA. astern@boulder.swri.edu. ; Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, CO 80303, USA. ; National Aeronautics and Space Administration (NASA) Ames Research Center, Space Science Division, Moffett Field, CA 94035, USA. ; Southwest Research Institute, San Antonio, TX 28510, USA. ; Lowell Observatory, Flagstaff, AZ 86001, USA. ; Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA. ; Southwest Research Institute, Boulder, CO 80302, USA. ; Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723, USA. ; Universitat der Bundeswehr Munchen, Neubiberg 85577, Germany. ; Planetary Science Institute, Tucson, AZ 85719, USA. ; KinetX Aerospace, Tempe, AZ 85284, USA. ; NASA Jet Propulsion Laboratory, La Canada Flintridge, CA 91011, USA. ; Massachusetts Institute of Technology, Cambridge, MA 02139, USA. ; University of Bonn, Bonn D-53113, Germany. ; NASA Headquarters (retired), Washington, DC 20546, USA. ; University of Arizona, Tucson, AZ 85721, USA. ; Cornell University, Ithaca, NY 14853, USA. ; NASA Headquarters, Washington, DC 20546, USA. ; Rheinisches Institut fur Umweltforschung an der Universitat zu Koln, Cologne 50931, Germany. ; Department of Astronomy, University of Maryland, College Park, MD 20742, USA. ; Search for Extraterrestrial Intelligence Institute, Mountain View, CA 94043, USA. ; Department of Environmental Sciences, University of Virginia, Charlottesville, VA 22904, USA. ; NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA. ; National Optical Astronomy Observatory, Tucson, AZ 26732, USA. ; NASA Marshall Space Flight Center, Huntsville, AL 35812, USA. ; Stanford University, Stanford, CA 94305, USA. ; Space Telescope Science Institute, Baltimore, MD 21218, USA. ; University of California, Santa Cruz, CA 95064, USA. ; Lunar and Planetary Institute, Houston, TX 77058, USA. ; Michael Soluri Photography, New York, NY 10014, USA. ; Johns Hopkins University, Baltimore, MD 21218, USA. ; Roane State Community College, Jamestown, TN 38556, USA. ; George Mason University, Fairfax, VA 22030, USA. ; Department of Astronomy, University of Virginia, Charlottesville, VA 22904, USA.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/26472913" target="_blank"〉PubMed〈/a〉
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