Annual Report 2019-20

Total Page:16

File Type:pdf, Size:1020Kb

Annual Report 2019-20 Australia’s National Science Agency Australia Telescope National Facility Annual Report 2019–20 Contents Chair’s report 2 Director’s report 3 Management team 4 About us 5 Performance indicators 9 Science highlights 13 Observatory reports 19 Square Kilometre Array 29 Technology development 33 People and community 37 Appendices 45 A: Financial summary 46 B: Staff list 47 C: Demographic data 50 D: Committee membership 51 E: Postgraduate students 52 F: PhD theses 53 G: Observing programs 54 H: Publications 60 I: Abbreviations 72 CSIRO Australia Telescope National Facility Annual Report 2019–20 ISSN 1038-9554 This is the report of the CSIRO Australia Telescope National Facility for the period 1 July 2019 to 30 June 2020 and is approved by its Steering Committee. Editor: Nic Svenson Science highlights: Helen Sim Cover: The Parkes radio telescope with the Moon and the surface of the Moon. Images: Alex Cherney and NASA. Inside cover: Buzz Aldrin steps onto the lunar surface, as received by the Parkes radio telescope. Image: NASA. Chair’s report The Australia Telescope National The mid-term review and the ATSC Facility Steering Committee (ATSC) also both made recommendations met twice this year. By our May 2020 highlighting the importance of Prof David Skellern, Chair, ATNF Steering meeting, COVID-19 constraints were instrumentation development. We Committee. Photo: John Sarkissian. in full force and we met virtually, hold that the ATNF’s radio astronomy not in Perth as had been planned. engineering and computing group investment in ASKAP and potentially is of long-term value to CSIRO. Its provide the global astronomy While we didn’t get to see the work sustains and advances the community with cost effective remarkable Australian Square nation’s science in astronomy, and commercial solutions for radio Kilometre Array Pathfinder (ASKAP), it demonstrably adds value to other interference mitigation. we were impressed mightily by the telescopes around the world. But it also results coming from it. The images adds value to Australia’s growing space Another commercial activity endorsed from the Rapid ASKAP Continuum sector (where ATNF know-how is being this year is that of a small team Survey (RACS) are beautiful, while the applied) and it could be better utilised undertaking a feasibility study of latest news from the fast radio burst in support of advanced manufacturing, potential near horizon business (FRB) team is truly extraordinary (see computing, big data, and models that leverage the telescopes Science highlights) and the critically telecommunications, the latter notably and other infrastructure of the ATNF. important ASKAP pilot survey in software defined radio engineering. While opportunistic commercial use program has provided more than Ensuring an appropriately skilled has occurred in the past, the team is just hints of how impressive full-scale workforce is vital to Australia’s future taking a more structured approach to surveys will be. A fully functioning industries. While the ATNF is playing its the sale of telescope time, scoping in ASKAP and transition to the era of part in ensuring that Australia’s future areas such as future Lunar missions, the Square Kilometre Array (SKA) engineering, computing and data deep space missions, space situational are clearly, and rightly, the ATNF’s analytics professionals acquire high awareness (including asteroid top priorities. level occupational skills, we believe tracking), education and tourism. We were this year presented with there is untapped potential here. We continue our strong endorsement a science case for the Australia After a year of rigorous market of the ATNF’s plans to increase Telescope Compact Array (ATCA). analysis and thorough consultation gender diversity, particularly in The ATNF, and facilities around the with industry, the ATSC was this the engineering disciplines. The world, are being asked to keep aging year presented with a plan that appointment this year of the instruments operational longer would see technology developed first Macquarie University, CSIRO than expected. That is, until the SKA for ASKAP applied to the looming Astronomy and Space Science Women is online. We found the case for bottleneck in satellite communications. in Engineering Scholarship holder is ATCA operation until this time to be Development of the plan was led a welcome step. compelling, a position mirrored by by commercialisation specialist, On the operational front, the ATSC the Australian Academy of Science Dr Ilana Feain, whose position we National Committee for Astronomy’s appoints the ATNF Users’ Committee recommended be created, so it is (ATUC) and the Time Assignment mid-term review of its Decadal tremendously satisfying to see a solid Plan for Australian Astronomy. The Committee (TAC). We are grateful commercial opportunity that leverages for the connection to the community ATNF’s partners in the university ATNF technology laid out in detail. sector clearly feel the same way and provided by ATUC and of the diligence We wish Dr Feain every success in her of the TAC. were this year successful in securing efforts to get the plan funded. Apart Australian Research Council funding from solving a pressing problem for The ATSC is an advisory committee for an urgent and essential upgrade the satellite communication industry to the CSIRO Board. As such, of ATCA’s digital system that should and end users, the realisation of we commend this Annual see it through until at least 2025. this opportunity would provide a Report to the Board and to the clear demonstration of return on astronomy community. 2 Australia Telescope National Facility | Annual Report 2019–20 Director’s report This year our newest telescope, Our innovative low frequency ASKAP, achieved a major milestone by ultra-wideband receiver has been completing a program of pilot surveys operating on Parkes for a year and Dr Douglas Bock, Director, ATNF. with the full 36-antenna array. Each is now requested by almost all Photo: Wheeler Studios. of the survey teams received around users. Parkes continued to support 100 hours of observing time to test the Breakthrough Listen program These include using our high-speed and optimise their survey strategies. searching for ‘technosignatures’ digital processing expertise on The strong engagement of the wider (evidence of technology) beyond our small satellites, our antennas for ASKAP community throughout Solar System and to follow up pulsar space situational awareness and the pilot surveys was particularly discoveries made by China’s Five- our cutting-edge receivers for space important. hundred metre Aperture Spherical communications. Telescope (where our 19-beam The scientific highlight of the year receiver has been in operation for This year has been a challenging one. was again ASKAP fast radio burst some two years). The next major The summer was one of the hottest (FRB) detections. These flashes of receiver development for Parkes is a on record and catastrophic bushfires high intensity radio waves have now cryogenically cooled, next-generation, raged in the eastern states. While our been used to discover the missing phased array feed receiver, supported telescopes were largely unscathed, ‘ordinary’ matter of the Universe. by our university partners and the some staff lost property, and many Sadly, celebrations were cut short Australian Research Council (ARC). spent their holidays volunteering with with the death of one of the principal emergency services or community investigators: Jean-Pierre Macquart. Also with the support of the ARC and groups supporting them and the university partners, we commenced affected communities. Then came The Square Kilometre Array (SKA) a project to replace the Australia the COVID-19 pandemic. We took project made a major advance by Telescope Compact Array’s aging special precautions around our passing its Critical Design Reviews. digital signal processing ‘back end’ operations staff and telescope sites. We continued to prepare for with cutting-edge digital technology As a consequence, and because construction and commenced work as developed in our Technologies for the virus did not spread in regional the Site Entity, delivering Australia’s Radio Astronomy program. Along Australia, we were able to maintain obligations under the SKA Convention with increased bandwidth and greater operations. The stresses of these (treaty). South Africa became the first observing flexibility, this technology strange times have been felt by all of SKA host nation to ratify the treaty: will allow active mitigation of radio us and I particularly wish to thank the it was also examined by Australia’s frequency interference, which is staff of the ATNF for their tolerance, parliamentary Joint Standing an important area of research as perseverance and for the support that Committee on Treaties, which interference continues to increase. they have provided one another. supported ratification in Australia. The planned partnership between Alongside growth in Australia’s space My thanks to the ATSC, ATUC, TAC, and CSIRO and the SKA Observatory to industry, we started to explore new my management team, for their advice operate SKA in Australia is reflected applications for our technologies. and guidance over the year. in a memorandum of understanding negotiated during the year. 2019 marked the 50th anniversary of the Apollo 11 Moon landing and we include here a feature on the role our Parkes radio telescope, and Australia’s space tracking facilities, played in the legendary broadcast.
Recommended publications
  • Digital Back End Development and Interference Mitigation Methods for Radio Telescopes with Phased-Array Feeds
    Brigham Young University BYU ScholarsArchive Theses and Dissertations 2014-08-20 Digital Back End Development and Interference Mitigation Methods for Radio Telescopes with Phased-Array Feeds Richard Allen Black Brigham Young University - Provo Follow this and additional works at: https://scholarsarchive.byu.edu/etd Part of the Electrical and Computer Engineering Commons BYU ScholarsArchive Citation Black, Richard Allen, "Digital Back End Development and Interference Mitigation Methods for Radio Telescopes with Phased-Array Feeds" (2014). Theses and Dissertations. 4233. https://scholarsarchive.byu.edu/etd/4233 This Thesis is brought to you for free and open access by BYU ScholarsArchive. It has been accepted for inclusion in Theses and Dissertations by an authorized administrator of BYU ScholarsArchive. For more information, please contact [email protected], [email protected]. Digital Back End Development and Interference Mitigation Methods for Radio Telescopes with Phased-Array Feeds Richard Black A thesis submitted to the faculty of Brigham Young University in partial fulfillment of the requirements for the degree of Master of Science Brian D. Jeffs, Chair Karl F. Warnick Neal K. Bangerter Department of Electrical and Computer Engineering Brigham Young University August 2014 Copyright c 2014 Richard Black All Rights Reserved ABSTRACT Digital Back End Development and Interference Mitigation Methods for Radio Telescopes with Phased-Array Feeds Richard Black Department of Electrical and Computer Engineering, BYU Master of Science The Brigham Young University (BYU) Radio Astronomy group, in collaboration with Cornell University, the University of Massachusetts, and the National Radio Astron- omy Observatory (NRAO), have in recent years developed and deployed PAF systems that demonstrated the advantages of PAFs for astronomy.
    [Show full text]
  • Hunting Down Stars with Unusual Infrared Properties Using Supervised Machine Learning
    . Magnificent beasts of the Milky Way: Hunting down stars with unusual infrared properties using supervised machine learning Julia Ahlvind1 Supervisor: Erik Zackrisson1 Subject reader: Eric Stempels1 Examiner: Andreas Korn1 Degree project E in Physics { Astronomy, 30 ECTS 1Department of Physics and Astronomy { Uppsala University June 22, 2021 Contents 1 Background 2 1.1 Introduction................................................2 2 Theory: Machine Learning 2 2.1 Supervised machine learning.......................................3 2.2 Classification...............................................3 2.3 Various models..............................................3 2.3.1 k-nearest neighbour (kNN)...................................3 2.3.2 Decision tree...........................................4 2.3.3 Support Vector Machine (SVM)................................4 2.3.4 Discriminant analysis......................................5 2.3.5 Ensemble.............................................6 2.4 Hyperparameter tuning.........................................6 2.5 Evaluation.................................................6 2.5.1 Confusion matrix.........................................6 2.5.2 Precision and classification accuracy..............................7 3 Theory: Astronomy 7 3.1 Dyson spheres...............................................8 3.2 Dust-enshrouded stars..........................................8 3.3 Gray Dust.................................................9 3.4 M-dwarf.................................................. 10 3.5 post-AGB
    [Show full text]
  • Sixty Years of Australia in Space
    Journal & Proceedings of the Royal Society of New South Wales, vol. 153, part 1, 2020, pp. 46–57. ISSN 0035-9173/20/010046-12 Sixty years of Australia in space Kerrie Dougherty Space Humanities Department, International Space University, Strasbourg, France Email: [email protected] Abstract Australia’s involvement in space activities commenced in 1957, at the beginning of the Space Age, with space tracking and sounding rocket launches at Woomera. By 1960, Australia was considered one of the leading space-active nations and in 1967 became one of the earliest countries to launch its own satellite. Yet by 1980, Australia’s space prominence had dwindled, with the country lacking both a national space agency and a coherent national space policy. Despite attempts in the latter part of the 1980s to develop an Australian space industry, the lack of a coherent and consistent national space policy and an effective co-ordinating body, left Australia constantly “punching below its weight” in global space activities until the Twenty First Century. This paper will briefly examine the often-contradictory history of Australian space activities from 1957 to the announcement of the Australian Space Agency in 2017, providing background and context for the later papers in this issue. Introduction Launchpad: the Woomera or 60,000 years the Indigenous people of Rocket Range FAustralia have looked to the sky, using “If the Woomera Range did not already exist, the stars to determine their location, find the proposal that Australia should engage in their way across the land and mark the a program of civil space research would be passage of the seasons and the best times unrealistic”.
    [Show full text]
  • Extremely Extended Dust Shells Around Evolved Intermediate Mass Stars: Probing Mass Loss Histories,Thermal Pulses and Stellar Evolution
    EXTREMELY EXTENDED DUST SHELLS AROUND EVOLVED INTERMEDIATE MASS STARS: PROBING MASS LOSS HISTORIES,THERMAL PULSES AND STELLAR EVOLUTION A Thesis presented to the Faculty of the Graduate School at the University of Missouri In Partial Fulfillment of the Requirements for the Degree Doctor of Philosophy by BASIL MENZI MCHUNU Dr. Angela K. Speck December 2011 The undersigned, appointed by the Dean of the Graduate School, have examined the dissertation entitled: EXTREMELY EXTENDED DUST SHELLS AROUND EVOLVED INTERMEDIATE MASS STARS PROBING MASS LOSS HISTORIES, THERMAL PULSES AND STELLAR EVOLUTION USING FAR-INFRARED IMAGING PHOTOMETRY presented by Basil Menzi Mchunu, a candidate for the degree of Doctor of Philosophy and hereby certify that, in their opinion, it is worthy of acceptance. Dr. Angela K. Speck Dr. Sergei Kopeikin Dr. Adam Helfer Dr. Bahram Mashhoon Dr. Haskell Taub DEDICATION This thesis is dedicated to my family, who raised me to be the man I am today under challenging conditions: my grandfather Baba (Samuel Mpala Mchunu), my grandmother (Ma Magasa, Nonhlekiso Mchunu), my aunt Thembeni, and my mother, Nombso Betty Mchunu. I would especially like to thank my mother for all the courage she gave me, bringing me chocolate during my undergraduate days to show her love when she had little else to give, and giving her unending support when I was so far away from home in graduate school. She passed away, when I was so close to graduation. To her, I say, ′′Ulale kahle Macingwane.′′ I have done it with the help from your spirit and courage. I would also like to thank my wife, Heather Shawver, and our beautiful children, Rosemary and Brianna , for making me see life with a new meaning of hope and prosperity.
    [Show full text]
  • ATNF News Issue No
    Galaxy Pair NGC 1512 / NGC 1510 ATNF News Issue No. 67, October 2009 ISSN 1323-6326 Questacon "astronaut" street performer and visitors at the Parkes Open Days 2009. Credit: Shaun Amy, CSIRO. Cover page image Cover Figure: Multi-wavelength color-composite image of the galaxy pair NGC 1512/1510 obtained using the Digitised Sky Survey R-band image (red), the Australia Telescope Compact Array HI distribution (green) and the Galaxy Evolution Explorer NUV -band image (blue). The Spitzer 24µm image was overlaid just in the center of the two galaxies. We note that in the outer disk the UV emission traces the regions of highest HI column density. See article (page 28) for more information. 2 ATNF News, Issue 67, October 2009 Contents From the Director ...................................................................................................................................................................................................4 CSIRO Medal Winners .........................................................................................................................................................................................5 CSIRO Astronomy and Space Science Unit Formed ........................................................................................................................6 ATNF Distinguished Visitors Program ........................................................................................................................................................6 ATNF Graduate Student Program ................................................................................................................................................................7
    [Show full text]
  • CASKAR: a CASPER Concept for the SKA Phase 1 Signal Processing Sub-System
    CASKAR: A CASPER concept for the SKA phase 1 Signal Processing Sub-system Francois Kapp, SKA SA Outline • Background • Technical – Architecture – Power • Cost • Schedule • Challenges/Risks • Conclusions Background CASPER Technology MeerKAT Who is CASPER? • Berkeley Wireless Research Center • Nancay Observatory • UC Berkeley Radio Astronomy Lab • Oxford University Astrophysics • UC Berkeley Space Sciences Lab • Metsähovi Radio Observatory, Helsinki University of • Karoo Array Telescope / SKA - SA Technology • NRAO - Green Bank • New Jersey Institute of Technology • NRAO - Socorro • West Virginia University Department of Physics • Allen Telescope Array • University of Iowa Department of Astronomy and • MIT Haystack Observatory Physics • Harvard-Smithsonian Center for Astrophysics • Ohio State University Electroscience Lab • Caltech • Hong Kong University Department of Electrical and Electronic Engineering • Cornell University • Hartebeesthoek Radio Astronomy Observatory • NAIC - Arecibo Observatory • INAF - Istituto di Radioastronomia, Northern Cross • UC Berkeley - Leuschner Observatory Radiotelescope • Giant Metrewave Radio Telescope • University of Manchester, Jodrell Bank Centre for • Institute of Astronomy and Astrophysics, Academia Sinica Astrophysics • National Astronomical Observatories, Chinese Academy of • Submillimeter Array Sciences • NRAO - Tucson / University of Arizona Department of • CSIRO - Australia Telescope National Facility Astronomy • Parkes Observatory • Center for Astrophysics and Supercomputing, Swinburne University
    [Show full text]
  • Jpc-Final-Program.Pdf
    49th AIAA/ASME/SAE/ASEE Joint Propulsion Conference and Exhibit (JPC) Advancing Propulsion Capabilities in a New Fiscal Reality 14–17 July 2013 San Jose Convention Center 11th International Energy Conversion San Jose, California Engineering Conference (IECEC) FINAL PROGRAM www.aiaa.org/jpc2013 www.iecec.org #aiaaPropEnergy www.aiaa.org/jpc2013 • www.iecec.org 1 #aiaaPropEnergy GET YOUR CONFERENCE INFO ON THE GO! Download the FREE Conference Mobile App FEATURES • Browse Program – View the program at your fingertips • My Itinerary – Create your own conference schedule • Conference Info – Including special events • Take Notes – Take notes during sessions • Venue Map – San Jose Convention Center • City Map – See the surrounding area • Connect to Twitter – Tweet about what you’re doing and who you’re meeting with #aiaaPropEnergy HOW TO DOWNLOAD Any version can be run without an active Internet connection! You can also sync an Compatible with itinerary you created online with the app by entering your unique itinerary name. iPhone/iPad, MyItinerary Mobile App MyItinerary Web App Android, and • For optimal use, we recommend • For optimal use, we recommend: rd BlackBerry! iPhone 3GS, iPod Touch (3 s iPhone 3GS, iPod Touch (3rd generation), iPad iOS 4.0, or later generation), iPad iOS 4.0, • Download the MyItinerary app by or later searching for “ScholarOne” in the s Most mobile devices using Android App Store directly from your mobile 2.2 or later with the default browser device. Or, access the link below or scan the QR code to access the iTunes s BlackBerry Torch or later device Sponsored by: page for the app.
    [Show full text]
  • Global Exploration Roadmap
    The Global Exploration Roadmap January 2018 What is New in The Global Exploration Roadmap? This new edition of the Global Exploration robotic space exploration. Refinements in important role in sustainable human space Roadmap reaffirms the interest of 14 space this edition include: exploration. Initially, it supports human and agencies to expand human presence into the robotic lunar exploration in a manner which Solar System, with the surface of Mars as • A summary of the benefits stemming from creates opportunities for multiple sectors to a common driving goal. It reflects a coordi- space exploration. Numerous benefits will advance key goals. nated international effort to prepare for space come from this exciting endeavour. It is • The recognition of the growing private exploration missions beginning with the Inter- important that mission objectives reflect this sector interest in space exploration. national Space Station (ISS) and continuing priority when planning exploration missions. Interest from the private sector is already to the lunar vicinity, the lunar surface, then • The important role of science and knowl- transforming the future of low Earth orbit, on to Mars. The expanded group of agencies edge gain. Open interaction with the creating new opportunities as space agen- demonstrates the growing interest in space international science community helped cies look to expand human presence into exploration and the importance of coopera- identify specific scientific opportunities the Solar System. Growing capability and tion to realise individual and common goals created by the presence of humans and interest from the private sector indicate and objectives. their infrastructure as they explore the Solar a future for collaboration not only among System.
    [Show full text]
  • CSIRO Annual Report 2000-01
    CSIRO 2000 - 2001 Annual Report CSIRO Annual Report 2000-2001 www.csiro.au CSIRO – the Commonwealth Scientific and Industrial Research Organisation - is one of the largest and most diverse scientific institutions in the world. It has a staff of over 6 000 located at 60 sites throughout Australia. CSIRO is an independent statutory authority constituted and operating under the provisions of the Science and Industry Research Act 1949 and the Commonwealth Authorities and Companies Act 1997. Enquiries Tel 1300 363 400 Email [email protected] Web www.csiro.au csiro annual report 00-01 [i] csiro annual report 00-01 [ii] Letter of Transmittal >> Senator The Honourable Nick Minchin Minister for Industry, Science and Resources Parliament House CANBERRA ACT 2600 We have pleasure in submitting to you, for presentation to Parliament, the fifty-third Annual Report of the Commonwealth Scientific and Industrial Research Organisation. This report has been prepared in compliance with the requirements of the Science and Industry Research Act 1949 and the Commonwealth Authorities and Companies Act 1997. We commend the Organisation’s achievements to you. D Charles K Allen, AO Geoff G Garrett Chairman of the Board Chief Executive September 2001 letter of transmittal csiro annual report 00-01 [iii] Board resolution >> The 2000-01 CSIRO Annual Report has been approved for presentation to the Minister for Science, Industry and Resources. Signed this 3rd day of September 2001 in accordance with a resolution of the Board Members. D Charles K Allen, AO Geoff G Garrett
    [Show full text]
  • Program Plan
    PROGRAM PLAN 1999 NATIONAL RADIO ASTRONOMY OBSERVATORY Cover: A "movie" of the radio emission from the exploding star Supernova 1993J in the galaxy M81. This time-sequence of images was made at a wavelength of 3.6 cm (8.3 Ghz) with a global array of telescopes that included the VLBA and the VIA. The resolution, or clarity of image detail, is 4000 AU (about 20 light-days), hundreds of times finer than can be achieved by optical telescopes on such a distant object. Observers: M. Rupen, N. Bartel, M. Bietenholz, T. Beasley. NATIONAL RADIO ASTRONOMY OBSERVATORY CALENDAR YEAR 1999 PROGRAM PLAN RSI rrao NOVEMBER 1,1998 The National Radio Astronomy Observatory is a facility of the National Science Foundation operated by Associated Universities, Inc. TABLE OF CONTENTS I. INTRODUCTION 1 II. 1999 SCIENTIFIC PROGRAM 2 1. The Very Large Array . 2 .2. The Very Long Baseline Array 8 3. The 12 Meter Telescope 11 4. The 140 Foot Telescope 13 HI. USER FAdLITIES 15 1. The Very Large Array 15 2. The Very Long Baseline Array 18 3. The 12 Meter Telescope 21 4. The 140 Foot Telescope 26 IV. TECHNOLOGY DEVELOPMENT 29 1. Electronics Development Equipment 29 2. Computing 34 V. GREEN BANK TELESCOPE 42 VI. MAJOR INITIATIVES 51 1. The Millimeter Array 51 2. VLA Upgrade 57 3. AIPS++Project 65 VII. NON-NSF RESEARCH 67 1. United States Naval Observatory 67 2. Green Bank Interferometer 67 3. NASA - Green Bank Orbiting VLBI Earth Station 67 VIII. EDUCATION PROGRAM 68 IX. 1999 PRELIMINARY FINANCIAL PLAN 75 APPENDIX A - NRAO SCIENTIFIC STAFF ACTIVITIES 78 1.
    [Show full text]
  • Astrometrically Registered Maps of H2O and Sio Masers Toward VX Sagittarii
    ARTICLE DOI: 10.1038/s41467-018-04767-8 OPEN Astrometrically registered maps of H2O and SiO masers toward VX Sagittarii Dong-Hwan Yoon1,2, Se-Hyung Cho2,3, Youngjoo Yun2, Yoon Kyung Choi2, Richard Dodson4, María Rioja4,5, Jaeheon Kim6, Hiroshi Imai7, Dongjin Kim3, Haneul Yang1,2 & Do-Young Byun2 The supergiant VX Sagittarii is a strong emitter of both H2O and SiO masers. However, previous VLBI observations have been performed separately, which makes it difficult to 1234567890():,; spatially trace the outward transfer of the material consecutively. Here we present the astrometrically registered, simultaneous maps of 22.2 GHz H2O and 43.1/42.8/86.2/129.3 GHz SiO masers toward VX Sagittarii. The H2O masers detected above the dust-forming layers have an asymmetric distribution. The multi-transition SiO masers are nearly circular ring, suggesting spherically symmetric wind within a few stellar radii. These results provide the clear evidence that the asymmetry in the outflow is enhanced after the smaller molecular gas clump transform into the inhomogeneous dust layers. The 129.3 GHz maser arises from the outermost region compared to that of 43.1/42.8/86.2 GHz SiO masers. The ring size of the 129.3 GHz maser is maximized around the optical maximum, suggesting that radiative pumping is dominant. 1 Astronomy Program, Department of Physics and Astronomy, Seoul National University, 1 Gwanak-ro, Gwanak-gu, Seoul 08826, Korea. 2 Korea Astronomy and Space Science Institute, 776 Daedeokdae-ro, Yuseong-gu, Daejeon 34055, Korea. 3 Department of Astronomy, Yonsei University, 50 Yonsei-ro, Seodaemun-gu, Seoul 03722, Korea.
    [Show full text]
  • SPACE EXPLORATION SYMPOSIUM (A3) Space Exploration Overview (1)
    68th International Astronautical Congress 2017 Paper ID: 36776 oral SPACE EXPLORATION SYMPOSIUM (A3) Space Exploration Overview (1) Author: Dr. Ed Kruzins Commonwealth Scientific and Industrial Research Centre, Australia, [email protected] DEEP SPACE EXPLORATION AND AUSTRALIA'S ROLE THROUGH THE CANBERRA DEEP SPACE COMMUNICATION COMPLEX Abstract For over 5 decades, the Canberra Space Communications Complex (CDSCC) managed by the Com- monwealth Scientific and Industrial Research Organisation (CSIRO) has been the leading Australian ground station facility for the US Deep Space Network (DSN). In collaboration with NASA JPL and sister stations in Spain and the USA, CDSCC tracks more than 40 International spacecraft to every planet in the solar system through the robotic science exploration missions of NASA, ESA, JAXA and other international space agencies. From the first Pioneer and Voyager missions to visit the outer planets and fly through the then unchartered Asteroid Belt to the Dawn missions exploration of Vesta and Ceres, to the Spirit, Opportunity and 2012 Curiosity rover landing on the Martian planet, CDSCC has provided a critical node to planetary scientists as they explore deep space. Among the hundreds of successful missions supported, CDSCC was global prime for the Galileo mission as the European Space Agency's Huygens probe descended towards the surface of Saturn's largest moon, Titan. In 2010 CDSCC provided support to the JAXA Hyabusa mission as it re-entered over Australia and in 2015 was a key downlink station for the New Horizons Pluto Charon flyby providing the first ever detailed images of Pluto. This paper will discuss the key role that this NASA-JPL-CSIRO Australian ground station continues to play in robotic solar system exploration, the important science diplomacy achieved and the future place Australia has through CDSCC and the DSN, in manned space flight.
    [Show full text]