DOCSLIB.ORG

Comment Response

Total Page：16

File Type：pdf, Size：1020Kb

Download full-text PDF Read full-text
Comment Response Expert and Government Review Comments on the IPCC WGI AR5 Second Order Draft – Chapter 2 Comment Chapter From From To To No Page Line Page Line Comment Response 2-1 2 0 0 0 0 First of all I want to convey my sincere admiration to the authors for attempting such a difficult enterprise as is Thanks reviewing all the scientific literature on atmospheric and surface observations. This task is made even more daunting (both from a scientific and writing viewpoint) by the mandate to build on the earlier AR4 report and the need to interpret differences therefrom. Not only does the text become inevitably repetitive, but the authors have had to constantly assess whether the most recent studies support earlier conclusions and what constitutes sufficient evidence to revise or question earlier statements. While I am fully aware of these major difficulties, I still think that the current draft feels rough and of uneven quality, with a lack of consistency (in background scientific information provided, length, level of regional detail, treatment of statistical significance, presence of error bars in graphics, summary statements) from section to section. The precipitation, surface humidity and cloud sections, in particular, seem incomplete. Some lack of uniformity is due to the fact that research has not progressed at the same rate in all observational fields; a a result, while some sections report significant improvements in our understanding, others simply list a myriad of varied regional results that cannot be interpreted in any particular way (is it necessary then to list them?). There are also several places where insufficient effort to assessing (as opposed to listing) results has been paid. From an editing perspective, I must also recommend that the authors undertake a thorough revision of the entire document looking to improve its readability and usefulness to a graduate student, post-doc or scientist not expert in the particular field itself. Currently the document is rather difficult to parse even for an interested reviewer. My take may be flawed but I am thinking of this document as something one could refer a graduate student to in order for him/her to gain an overview on a particular topic. There is a surprising absence of connecting words within paragraphs whose presence would allow the reader to follow the flow of ideas and gain a clearer notion of what the ovrall results mean (by the time the summary sentence arrives, the reader is sometimes at loss). In fact I wonder if there was a deliberate effort to postpone the “narrative touches” until the final draft. In places, the document also seems to be lacking an organized story (with some undesirable jumps, backtracking and repetitions within the text). [Ileana Bladé, Spain] 2-2 2 0 0 0 0 Chapter 2 reports new work on the global abundance and trends of all the important greenhouse gases Rejected - outside scope of Chapter 2. (GHGs), however there are no citations to papers describing and using the isotopic composition and trends of GHGs, a likely more important source of information about GHG sources and sinks than the abundance and trend data. This research could be reviewed in Chapter 6. Please ensure that these papers are reviewed in either Chapter 2 or Chapter 6. The GHG isotope variation papers that should be discussed are: Allison, C. & R. Francey, Verifying global trends in atmospheric carbon dioxide stable isotopes, J. Geophys. Res., 112, D21304, doi:10.1029/2006JD007345, 2007. Rayner, P., R. Law, C. Allison, R. Francey, C. Trudinger & C. Pickett-Heaps, The inter-annual variability of the global carbon cycle (1992-2005) inferred by inversion of atmospheric CO2 and δ13CO2, Global Biogeochem. Cycles, 22, GB3008, doi:10.1029/2007GB003068, 2008 Levin, I., T. Naegler, B. Kromer, M. Diehl, R. Francey, A. Gomez-Pelaez, P. Steele, D. Wagenbach, R. Weller & D. Worthy, Observations and modelling of the global distribution and long-term trend of atmospheric 14CO2, Tellus B, 62(1), 26-46, 2010 Welp, L., .....R. Francey, C. Allison et al., El Nino effects on the isotopic composition of oxygen in atmospheric CO2, Nature, 477, 579-582, 2011 Ferretti, D., J. Miller, J. White, K. Lassey, D. Lowe & D. Etheridge, Stable isotopes provide revised global limits of aerobic methane emissions from plants, Atmospheric Chemistry and Physics, 7, 237-241, 2007. Petrenko, V., D. Etheridge, R. Weiss, E. Brook, H. Schaefer, J. Severinghaus, A. Smith, D. Lowe, Q. Hua & K. Riedel, Methane from the East Siberian Arctic Shelf, Science, 329, 1146-1147, 2010 Park, S., D. Etheridge, P. Fraser, P. Krummel, R. Langenfelds, P. Steele, C. Trudinger et al., Trends and seasonal cycles in the isotopic composition of nitrous oxide since 1940, Nature Geosciences,5, 261-265, 2012 [Government of Australia] 2-3 2 0 0 0 0 Papers on greenhouse gas trends, sources and sinks that should be reviewed in Chapter 2 or Chapter 6: Rejected - outside scope of Chapter 2. Francey, R., C. Trudinger, M. van der Schoot, P. Krummel, P. Steele & R. Langenfelds, Differences between trends in atmospheric CO2 and the reported trends in anthropogenic CO2 emissions, Tellus B, 62: 316–328, doi: 10.1111/j.1600-0889.2010.00472.x, 2010 - this is an important paper because it describes an apparent inconsistency between 'bottom-up' and 'top-down' estimates of fossil fuel CO2 emissions. Do not Cite, Quote or Distribute Page 1 of 235 Expert and Government Review Comments on the IPCC WGI AR5 Second Order Draft – Chapter 2 Comment Chapter From From To To No Page Line Page Line Comment Response Pan, Y., .....J. Canadell, et al., A large and persistent carbon sink in the world’s forests, 1990-2007, Science, 333, 988-993, 2011 Peters, G., .....J. Canadell. M. Raupach et al., Rapid growth in CO2 emissions after the 2008-2009 global financial crisis, Nature Climate Change, 2, 2-4, 2012 Raupach, M., J. Canadell & C. Le Quere, Anthropogenic and biophysical contributors to increasing atmospheric CO2 growth rate and airborne fraction, Biogeosciences, 5, 1601-1613, 2008 Raupach, M., Pinning down the land carbon sink. Nature Climate Change, 1(3), 148-149, 2011 Le Quéré, C., C. Rodenbeck, E. Buitenhuis, T. Conway, R. Langenfelds, A. Gomez, C. Labuschagne, M. Ramonet, T. Nakazawa, N. Metzl, N. Gillett & M. Heimann, Saturation of the Southern Ocean CO2 sink due to recent climate change, Science, 316, 1735-1738, 2007 Le Quere, C., C. Rodenbeck, E. Buitenhuis, T. Conway, R. Langenfelds, A. Gomez, C. Labus change, M. Ramonet, T. Nakazawa, N. Metzl, N. Gillett & M. Heimann, Response to Comments on ‘Saturation of the Southern Ocean CO2 Sink Due to Recent Climate Change’, Science, 319, doi:10.1126/science.1147315, 2008. Law, R., R. Matear & R. Francey, Comment on ‘Saturation of the Southern Ocean CO2 Sink Due to Recent Climate Change, Science, 319, doi: 10.1126/science.1149077, 2008. Patra, P., M. Takigawa, K. Ishijima, B.-C. Choi, D. Cunnold, E. Dlugokencky, P. Fraser, A. Gomez-Pelaez, T.- Y. Goo, J.-S. Kim, P. Krummel, R. Langenfelds, F. Meinhardt, H. Mukai, S. O’Doherty, R. Prinn, P. Simmonds, P. Steele, Y. Tohjima, K. Tsuboi, K. Uhse, R. Weiss, D. Worthy & T. Nakazawa, Growth rate, seasonal, synoptic & diurnal variations and budget of methane in lower atmosphere, J. Meteorological Society of Japan, 87:4, 635-663, 2009 Patra, P., .....R. Law, Z. Loh, et al., , TransCom model simulations of CH4 and related species: linking transport, surface flux and chemical loss with CH4 variability in the troposphere and lower stratosphere, Atmos. Chem. Phys., 11, 12813-12837, 2011. Le Quéré, C., M. Raupach, J. Canadell, G. Marland, L. Bopp, P. Ciais, T. Conway, S. Doney, R. Feely, P. Friedlingstein, K. Gurney, R. Houghton, J. House, C. Huntingford, P. Levy, M. Lomas, J. Majkut, N. Metzl, J. Ometto, G. Peters, C. Prentice, J. Randerson, S. Running, J. Sarmiento, U. Schuster, S. Sitch, T. Takahashi, N. Viovy, G. van der Werf & I. Woodward, , Trends in the sources and sinks of carbon dioxide, Nature Geosciences, 2, doi:10.1038/ngeo689, 2009 Chevallier, F., P. Ciais , T. Conway, T. Aalto, B. Anderson, P. Bousquet, E. Brunke, L. Ciattaglia, Y. Esaki, M. Fröhlich, A. Gomez-Pelaez, L. Haszpra, P. Krummel, R. Langenfelds, M. Leuenberger, T. Machida, F. Maignan, H. Matsueda, J-A. Morguí, H. Mukai, T. Nakazawa, P. Peylin, M. Ramonet, L. Rivier, Y. Sawa, M. Schmidt, P. Steele, S. Vay, A. Vermeulen, S. Wofsy & D. Worthy: CO2 surface fluxes at grid point scale estimated from a global 21-year reanalysis of atmospheric measurements, J. Geophys. Res., 115, D21307,doi:10.1029/2010JD013887, 2010 [Government of Australia] 2-4 2 0 0 0 0 Papers on long-term ice core CO2 record that should be reviewed in Chapter 2 or Chapter 5 include: Rejected - outside scope of Chapter 2. Ahn, J., .....D. Etheridge, M. Rubino et al., Atmospheric CO2 over the last 1000 years: a high resolution record from the West Antarctic Ice Sheet (WAIS) Divide ice core, Global Biogeochemical Cycles, 26, GB2027, doi:10.1029/2011GB004247, 2012 Other ice core/firn papers that need to be reviewed in Chapter 2 or Chapter 5: Worton et al., CF4, C2F6, Environ. Sci. Tech., 41, 2184-2189, 2007 (may have been reviewed in the 4th Assessment) Witrant et al., trace gases in firn, Atmos. Chem. Phys. Disc., 11, 23029-23080, 2011 Buizert et al., trace gases in Greenland ice core, Atmos. Chem. Phys. Disc.,11, 15975-16021, 2011 [Government of Australia] 2-5 2 0 0 0 0 Important paper on CFC lifetimes that should be included in Chapter 2: Rejected - outside scope of Chapter 2. Do not Cite, Quote or Distribute Page 2 of 235 Expert and Government Review Comments on the IPCC WGI AR5 Second Order Draft – Chapter 2 Comment Chapter From From To To No Page Line Page Line Comment Response Rigby, M., .....P.
Load more

Recommended publications
  • The NEO Problem: Current Activities in Russia
    51-th Session of STSC UN COPUOS Vienna, Austria, February 10, 2014 TheThe NEONEO problem:problem: currentcurrent activitiesactivities inin RussiaRussia B. Shustov r. GeneralGeneral activitiesactivities (Feb(Feb 20132013 –– FebFeb 2014)2014) 2013 March,12 – Round table of the Committees for science and defense of the Federation Council (Upper chamber of the Russia Parliament); 2013 November, a series of meetings in Roscosmos on cooperative approach to the NEO problem; Telecon EMERCOM-FEMA January 28, 2014; A number of expeditions were organized to the region of the fall of Chelyabinsk meteorite; All Russia science conferences in Chelyabinsk (April 2013) and in Krasnodar (October 2013) were held. 2 BBasicasic aspectsaspects ofof thethe NEONEO problemproblem Major constituents of the NEO (Asteroid/Comet Impact Hazard - ACH) problem are: Detection and characterization Risk assessment Protection and mitigation We work in all areas both at national and international levels. 3 ToTo thethe NEONEO massivemassive detectiondetection AZT-33IR AZT-33VM The telescope АZТ-33VM ( ∅ 1.6 m) for massive detection of NEOs at large distances is under construction near Baikal Lake. We plan to complete it in 2017. This is supported by Academy of Sciences and Roscosmos. 4 ISONISON telescopestelescopes forfor NEONEO surveyssurveys andand followfollow -- upup observationsobservations ISON (International Scientific Optical Network) – one of largest Russian networks capable to observe NEOs at near space. It is partially supported by Roscosmos. 5 ISONISON :: resultsresults
    [Show full text]
  • Russian Networks Capable to Observe Neos at Near Space
    52-th Session of STSC UN COPUOS Vienna, Austria, February 3, 2015 The NEO problem: current activities in Russia V.Emel’yanenko Basic aspects of the NEO problem Major constituents of the NEO (Asteroid/Comet Impact Hazard - ACH) problem are: Detection and characterization Risk assessment Protection and mitigation We work in all areas at both national and international levels. 2 General activities (Feb 2014 – Feb 2015) Studies of the Chelyabinsk meteorite; Completion of the 1.6 m telescope for NEO detection; Work on the development of a moderate aperture telescope national network aimed to detection and monitoring of NEOs; Various projects of space based means to detect and to counteract dangerous bodies; Construction of a data-bank on impact consequences . 3 Some lessons of the Chelyabinsk event (15 Feb, 2013): Asteroids of decameter size could be very dangerous; We need to know about coming threat reasonably in advance; Day time asteroids are unobservable by any ground based facilities. 4 En route to the NEO detection AZT-33IR AZT-33VM The telescope АZТ-33VM ( ∅ 1.6 m) for the mass detection of NEOs at large distances is nearing completion. First light is expected in the fall of 2015. 5 ISON telescopes for NEO surveys and follow- up observations ISON (International Scientific Optical Network) – one of the largest Russian networks capable to observe NEOs at near space. 6 ISON : results on asteroids Hundreds of light curves were constructed for tens of NEAs (3122) Florence, (20187) Janapittichova, (25916) 2001 CP44, (162004) 1991 VE, (7888)
    [Show full text]
  • Astronomical Observations of Volatiles on Asteroids
    Astronomical Observations of Volatiles on Asteroids Andrew S. Rivkin The Johns Hopkins University Applied Physics Laboratory Humberto Campins University of Central Florida Joshua P. Emery University of Tennessee Ellen S. Howell Arecibo Observatory/USRA Javier Licandro Instituto Astrofisica de Canarias Driss Takir Ithaca College and Planetary Science Institute Faith Vilas Planetary Science Institute We have long known that water and hydroxyl are important components in meteorites and asteroids. However, in the time since the publication of Asteroids III, evolution of astronomical instrumentation, laboratory capabilities, and theoretical models have led to great advances in our understanding of H2O/OH on small bodies, and spacecraft observations of the Moon and Vesta have important implications for our interpretations of the asteroidal population. We begin this chapter with the importance of water/OH in asteroids, after which we will discuss their spectral features throughout the visible and near-infrared. We continue with an overview of the findings in meteorites and asteroids, closing with a discussion of future opportunities, the results from which we can anticipate finding in Asteroids V. Because this topic is of broad importance to asteroids, we also point to relevant in-depth discussions elsewhere in this volume. 1 Water ice sublimation and processes that create, incorporate, or deliver volatiles to the asteroid belt 1.1 Accretion/Solar system formation The concept of the “snow line” (also known as “water-frost line”) is often used in discussing the water inventory of small bodies in our solar system. The snow line is the heliocentric distance at which water ice is stable enough to be accreted into planetesimals.
    [Show full text]
  • On the Russian Contribution to the IAWN
    IAWN Steering Group Meeting Minor Planet Center & Harvard-Smithsonian Center for Astrophysics 13 – 14 January 2014 On the Russian contribution to the IAWN Boris Shustov Institute of Astronomy, RAS Plan of the talk ! " The need for a national NEO program ! " Astronomical requirements for NEO detection/ monitoring ! " Existing premises and recent activities ! " What we plan to do ! " How to contribute to the IAWN 2 Arguments pro national program in Russia (NEO aspects) 1." The NEO problem is a multi-problem. Various organizations (ministries) are to be involved (coordinated); 2." The expensive technologies of massive detection of NEO, preventing collisions and mitigation can be proposed but cannot be realized under the responsibility of individual research institution; 3." Cooperation of countries on the NEO problem implies the involvement of Russia Government (or authorized body); 4." Regular funding is vitally important for real progress. 3 Suggestion to the definitions of hazardous celestial bodies (HCB) PHO - MOID < 0.05 A.U. Threatening object (TO) D < LD, D - 3σD < RE Collisional object (CO) D < RE, 3σD < RE NB: In the definition of PHO limiting size (or H) is not included! -3 6 -4 For TO collision probability >~10 , (if LD = 10 km then >~10 ) For CO collision probability >~0.5 4 Two tasks and modes of detection Large Distant Detection (LDD). Major goal is to detect “all” PHO larger than ~ 50 m well beforehand (to ensure possibility of active counteraction). Near Earth Detection (NED). Major goal – to detect “all” PHO larger than ~ 5 m in the near space (D < LD). This makes possible warning. “all” means > 90% 5 LDD mode: NEO detection (general requirements and other inputs for design of detection instrument ) ! " Time interval between detection+characterisation and rendez-vous must be not less than warning time (tw).
    [Show full text]
  • ASPIN - ISON Asteroid Program: History, Current State and Future Prospects
    ASPIN - ISON asteroid program: history, current state and future prospects L. Elenin1,2, I. Molotov1,2, V. Savanevych3, A. Bruhovetskiy4, Yu. Krugly5, V. Nevski2, Yu. Ivaschenko6, A. Yudin1,2 1. Keldysh Instute of Applied Mathemacs RAS 2. CJSC “ANC” 3. Kharkiv Naonal University of Radioelectronics 4. JSC “Hartron” Evoluon of Comet ISON. D. Peach (2013) 5. Instute of Astronomy of Kharkiv Naonal University 6. Andrushivka Astronomical Observatory ABSTRACT OBSERVATORIES OF THE ASPIN PROGRAM ASPIN (Asteroid Search and Photometry Iniave) - ISON asteroid program started in September 2003 at Andrushivka astronomical observatory (A50, Andrushivka, Ukraine). For these purposes was used Zeiss-600 telescope with small CCD camera. In 2009, telescope was upgraded by new full-format CCD camera and lens corrector, which increased FOV to 72’x72’. During first 7 years, observatory discovered more than 350 asteroids, include 2 NEAs. Unfortunately, at present me, when rivalry of surveys was growing up, Andrushivka forced to stop observaon in 2013, due to bad astroclimate and, as result, low magnitude limit. In 2014, we planning to install new, wide-field ORI-50M (0.5-m f/2.3) telescope at new site with good astroclimate condions. Aer that, survey program will resume. Next ISON observatory, which started own survey, was ISON-NM (H15, Mayhill, NM, USA). Survey work started in July 2010 and connues to this day. First telescope of this Andrushivka observatory was Centurion-18, 0.45-m f/2.8 with full-frame CCD camera. In September 2013 with telescope replaced by our new telescope Santel-400AN (0.4-m f/3) with Chuguev Khuraltogot Kislovodsk 105’x105’ FOV.
    [Show full text]
  • Number Worked As Current Name Vol-Num Pg # Authors 1 Ceres 42-2 94 Melillo, F
    The "Worked As" column gives the name/designation used in the original article. If the object was subsequently named, the "Current Name" column gives the name currently in the MPCORB file. The page number gives the first page of the article in which the object appears. Only those references that include lightcurves, other photometric data, and/or shape/spin axis models are included. Number Worked As Current Name Vol-Num Pg # Authors 1 Ceres 42-2 94 Melillo, F. J. 2 Pallas 35-2 63 Higley, S. et al. (Shape/Spin Models) 5 Astraea 35-2 63 Higley, S. et al. (Shape/Spin Models) 8 Flora 36-4 133 Pilcher, F. 9 Metis 36-3 98 Timerson, B. et al. 10 Hygiea 47-2 133 Picher, F. 10 Hygiea 48-2 166 Ferrais, M. et al. 11 Parthenope 37-3 119 Pilcher, F. 11 Parthenope 38-4 183 Pilcher, F. 12 Victoria 40-3 161 Pilcher, F. 12 Victoria 42-2 94 Melillo, F. J. 13 Egeria 36-4 133 Pilcher, F. 14 Irene 36-4 133 Pilcher, F. 14 Irene 39-3 179 Aymani, J.M. 16 Psyche 38-4 200 Timerson, B. et al. 16 Psyche 43-2 137 Warner, B. D. 17 Thetis 34-4 113 Warner, B.D. (H-G, Color Index) 18 Melpomene 40-1 33 Pilcher, F. 18 Melpomene 41-3 155 Pilcher, F. 19 Fortuna 36-3 98 Timerson, B. et al. 22 Kalliope 30-2 27 Trigo-Rodriguez, J.M. 22 Kalliope 34-3 53 Gungor, C. 22 Kalliope 34-3 56 Alton, K.B.
    [Show full text]
  • Cumulative Index to Volumes 1-45
    The Minor Planet Bulletin Cumulative Index 1 Table of Contents Tedesco, E. F. “Determination of the Index to Volume 1 (1974) Absolute Magnitude and Phase Index to Volume 1 (1974) ..................... 1 Coefficient of Minor Planet 887 Alinda” Index to Volume 2 (1975) ..................... 1 Chapman, C. R. “The Impossibility of 25-27. Index to Volume 3 (1976) ..................... 1 Observing Asteroid Surfaces” 17. Index to Volume 4 (1977) ..................... 2 Tedesco, E. F. “On the Brightnesses of Index to Volume 5 (1978) ..................... 2 Dunham, D. W. (Letter regarding 1 Ceres Asteroids” 3-9. Index to Volume 6 (1979) ..................... 3 occultation) 35. Index to Volume 7 (1980) ..................... 3 Wallentine, D. and Porter, A. Index to Volume 8 (1981) ..................... 3 Hodgson, R. G. “Useful Work on Minor “Opportunities for Visual Photometry of Index to Volume 9 (1982) ..................... 4 Planets” 1-4. Selected Minor Planets, April - June Index to Volume 10 (1983) ................... 4 1975” 31-33. Index to Volume 11 (1984) ................... 4 Hodgson, R. G. “Implications of Recent Index to Volume 12 (1985) ................... 4 Diameter and Mass Determinations of Welch, D., Binzel, R., and Patterson, J. Comprehensive Index to Volumes 1-12 5 Ceres” 24-28. “The Rotation Period of 18 Melpomene” Index to Volume 13 (1986) ................... 5 20-21. Hodgson, R. G. “Minor Planet Work for Index to Volume 14 (1987) ................... 5 Smaller Observatories” 30-35. Index to Volume 15 (1988) ................... 6 Index to Volume 3 (1976) Index to Volume 16 (1989) ................... 6 Hodgson, R. G. “Observations of 887 Index to Volume 17 (1990) ................... 6 Alinda” 36-37. Chapman, C. R. “Close Approach Index to Volume 18 (1991) ..................
    [Show full text]
  • U.S. Spacesuit Knowledge Capture (KC) Series Synopsis
    JSC/EC5 U.S. Spacesuit Knowledge Capture (KC) Series Synopsis All KC events will be approved for public using NASA Form 1676. This synopsis provides information about the Knowledge Capture event below. Topic: Human Exploration of Near-Earth Asteroids Date: July 25, 2013 Time: 10:30-12:00 pm Location: JSC/B5S/R3102 DAA 1676 Form #: 29231 This is a link to all lecture material and video: \\js-ea-fs-01\pd01\EC\Knowledge-Capture\FY13 Knowledge Capture\20130725 Abell_Human Exploration of Near-Earth Asteroids\For 1676 Review and Public Release *A copy of the video will be provided to NASA Center for AeroSpace Information (CASI) via the Agency’s Large File Transfer (LFT), or by DVD using the USPS when the DAA 1676 review is complete. Assessment of Export Control Applicability: This Knowledge Capture event has been reviewed by the EC5 Spacesuit Knowledge Capture Manager in collaboration with the author and is assessed to not contain any technical content that is export controlled. It is requested to be publicly released to the JSC Engineering Academy, as well as to CASI for distribution through NTRS or NA&SD (public or non-public) and with video through DVD request or YouTube viewing with download of any presentation material. Presenter: Paul Abell Synopsis: A major goal for NASA's human spaceflight program is to send astronauts to near-Earth asteroids (NEA) in the coming decades. Missions to NEAs would undoubtedly provide a great deal of technical and engineering data on spacecraft operations for future human space exploration while conducting in-depth scientific examinations of these primitive objects.
    [Show full text]
  • The Minor Planet Bulletin
    THE MINOR PLANET BULLETIN OF THE MINOR PLANETS SECTION OF THE BULLETIN ASSOCIATION OF LUNAR AND PLANETARY OBSERVERS VOLUME 39, NUMBER 4, A.D. 2012 OCTOBER-DECEMBER 203. 8077 HOYLE: A SHORT PERIOD ASTEROID 2.7454 ± 0.0002 h with an amplitude of 0.20 ± 0.02 mag. While there is a fair amount of scatter in the individual data points, when Daniel A. Klinglesmith III, Ethan Risley, combined they produce a well-determined period, which was Janek Turk, Angelica Vargas found by using an 8th order fit in the FALC analysis algorithm Etscorn Campus Observatory, New Mexico Tech (Harris et al., 1989). 101 East Road Socorro, NM USA 87801 Acknowledgements [email protected] The Etscorn Campus Observatory operations are supported by the Xianming L. Han, Orry R. Heffner, Adam W. Kidd, Research and Economic Development Office of New Mexico Bradley J. Magnetta, Frederick W. Rastede Institute of Mining and Technology (NMIMT). Student support at Department of Physics and Astronomy, Butler University NMIMT is given by NASA EPScOR grant NNX11AQ35A. We Indianapolis, IN USA would like to thank F. Levinson for a generous gift enabling Butler University's membership in the SARA consortium. (Received: 30 May) References The main-belt asteroid 8077 Hoyle was observed on 13 Etscorn Campus Observatory (ECO) (2012). nights over a span of 47 days in 2012 April-May. A http://www.mro.nmt.edu/education-outreach/etscorn-campus- bimodal synodic period of 2.7454 ± 0.0002 h and an observatory/ amplitude of 0.20 ± 0.02 mag. were obtained. Southeastern Association for Research in Astronomy Observatory (SARA) (2012).
    [Show full text]
  • L'asteroide Nea 2012
    ASTRONOMIA NOVA L. Franco, P. Bacci, 2012 EG5 Pagina 54 n. 13, maggio 2012 L’ASTEROIDE NEA 2012 EG5 Lorenzo Franco e Paolo Bacci L‘Osservatorio astronomico di San Marcello Pistoiese L'asteroide NEA (Near Earth Asteroid, http:// Simone Vergari, nei giorni 21, 27 e 30 marzo. In parti- it.wikipedia.org/wiki/Oggetto_near-Earth ) 2012 EG5 è colare in quest'ultima data sono state effettuate alcune stato scoperto il 13 marzo 2012 dal telescopio Pan- sessioni osservative finalizzate alla fotometria per cerca- STARRS 1, Haleakala nelle Hawaii. Si tratta di un aste- re di determinare il periodo di rotazione dell'oggetto. roide di tipo Apollo (http://it.wikipedia.org/wiki/ Nel corso della sessione osservativa del 30 Marzo sono Asteroide_Apollo), con un diametro inferiore ai 100 state acquisite un totale di 479 immagini non filtrate da metri, che al momento della scoperta si trovava a circa 15 secondi di esposizione su un intervallo temporale di 36 volte la distanza Terra-Luna. L'asteroide è stato su- 2.5 ore. Tutte le immagini sono state riprese con il tele- bito classificato come un potenziale impattore virtuale scopio principale da 0.6 m ed una camera CCD Apogee dal JPL Sentry e dal NEODyS di Pisa. Le osservazioni Alta 1024 x 1024 con un campo di vista di 35x35 minuti astrometriche pervenute al Minor Planet Center nei d'arco ed un campionamento di 2 secondi d'arco per giorni successivi hanno permesso di determinare con pixel. Nonostante l'ampio campo inquadrato è stato ne- maggiore precisione l'orbita, scongiurando così ogni cessario spostare più volte l'inquadratura per seguire immediata possibilità di impatto.
    [Show full text]
  • The Astronomer Magazine Index
    The Astronomer Magazine Index The numbers in brackets indicate approx lengths in pages (quarto to 1982 Aug, A4 afterwards) 1964 May p1-2 (1.5) Editorial (Function of CA) p2 (0.3) Retrospective meeting after 2 issues : planned date p3 (1.0) Solar Observations . James Muirden , John Larard p4 (0.9) Domes on the Mare Tranquillitatis . Colin Pither p5 (1.1) Graze Occultation of ZC620 on 1964 Feb 20 . Ken Stocker p6-8 (2.1) Artificial Satellite magnitude estimates : Jan-Apr . Russell Eberst p8-9 (1.0) Notes on Double Stars, Nebulae & Clusters . John Larard & James Muirden p9 (0.1) Venus at half phase . P B Withers p9 (0.1) Observations of Echo I, Echo II and Mercury . John Larard p10 (1.0) Note on the first issue 1964 Jun p1-2 (2.0) Editorial (Poor initial response, Magazine name comments) p3-4 (1.2) Jupiter Observations . Alan Heath p4-5 (1.0) Venus Observations . Alan Heath , Colin Pither p5 (0.7) Remarks on some observations of Venus . Colin Pither p5-6 (0.6) Atlas Coeli corrections (5 stars) . George Alcock p6 (0.6) Telescopic Meteors . George Alcock p7 (0.6) Solar Observations . John Larard p7 (0.3) R Pegasi Observations . John Larard p8 (1.0) Notes on Clusters & Double Stars . John Larard p9 (0.1) LQ Herculis bright . George Alcock p10 (0.1) Observations of 2 fireballs . John Larard 1964 Jly p2 (0.6) List of Members, Associates & Affiliations p3-4 (1.1) Editorial (Need for more members) p4 (0.2) Summary of June 19 meeting p4 (0.5) Exploding Fireball of 1963 Sep 12/13 .
    [Show full text]
  • THESEUS-Full Report.Pdf
    Towards Human Exploration of Space: a EUropean Strategy - Roadmap ROADMAP March2012 1 THESEUS Consortium Project Coordination and Communication European Science Foundation, France Jean-Claude Worms - Coordinator Nicolas Walter – Project Officer Olivier White - Project Officer (Jan-Sept 2010) Johanne Martinez-Schmitt – Project Administrator Karina Marshall-Bowman - Editorial Support Work Package 1: Integrated systems physiology Centre National de la Recherche Scientifique - Institut Pluridisciplinaire Hubert Curien (CNRS-IPHC), France Stéphane Blanc – Work Package Leader Iman Monken – Work Package Support Work Package 2: Psychology and human-machine systems University of Sheffield, UK Bob Hockey – Work Package Leader Work Package 3: Radiation Deutschen Zentrums für Luft- und Raumfahrt (DLR), Germany Günther Reitz - Work Package Leader Work Package 4: Habitat management Belgian Nuclear Research Centre (SCK•CEN) Natalie Leys – Work Package Leader Felice Mastroleo – Work Package Support Work Package 5: Health care Institut de Médecine et de Physiologie Spatiales (MEDES), France Bernard Comet - Work Package Leader Work Package 6: Integration Deutschen Zentrums für Luft- und Raumfahrt (DLR), Germany Rupert Gerzer – Work Package Leader Gerda Horneck – Expert Support The THESEUS Coordination and Support Action has received funding from the European Community’s 7th Framework Programme (FP7/2007-2013) under grant agreement n°242482. This document only reflects the views of the THESEUS Consortium. The European Commission is not liable for any use that may be made of the information contained therein. THESEUS: Towards Human Exploration of Space – a European Strategy Past space missions in low Earth orbit have demonstrated that human beings can survive and work in space for long durations. However, there are pending technological, medical and psychological issues that must be solved before adventuring into longer-duration space missions (e.g.
    [Show full text]