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Explore the latest research in space and atmospheric sciences conducted by the Australian Antarctic Division, focusing on cosmic rays, neutron monitoring, and space weather prediction.
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Australian AntarcticDivision Space Science Research Marc Duldig
Space and Atmospheric Sciences • Emphasis has shifted away from Space • Concentration is Atmosphere and Climate • Still operate Digisonde at Davis • Ray Morris will discuss this in Hobart • Still operate Cosmic Ray facilities • Mawson, Kingston and Liapootah • Cosmic Ray International Networks • Surface Muon telescope networks • Underground Muon telescope networks • Space Ship Earth neutron monitor network • Still provide infrastructure & support for Universities
Incident Primary Particle N n o p p P + - - p p P + p - p g g N + - + - a g n n g - - p + - + - n n + g N p + + g m - m g - - - + + + p N g n - - m + - n + + + + m - - + g + p - - n - + - - + - - n + - <5x1010 eV >1012 eV 109 - 1012 eV Atmospheric Cascade Process
Surface Muon Telescopes • Global network viewing CMEs • Currently in operation • Mawson, Kingston, Nagoya, San Martino (to be enhanced) • Funded • Griefswald, Kuwait • Searching for loss cone anisotropies • Presently uneven cover but some useful results • With newly funded instruments global coverage
Griefswald Surface Muon Telescopes (2)
Underground muon telescopes • Mawson, Liapootah, Matsushiro • Main areas of interest are: • Solar cycle modulation • Anisotropies • Density gradients in the inner heliosphere • Sidereal anisotropies – local galactic interactions • Forbush decreases associated with • CME Shock passage • Fast solar wind stream shocks
Space Ship Earth Network • Participating agencies • Lead - Bartol Research Institute, Uni of Delaware • IZMIRAN, Russia • AAD, Australia • Global neutron monitor network • Equally spaced equatorial viewing directions • N and S polar views • Real time near earth radiation environment measurement (1 or 5 minute resolution)
The IQSY Neutron Monitor (NM64) Polyethylene Lead Anode B10 + n1à Li7 + He4 5032 Directionality lost but Geomagnetic field orders arrival
Research Aims of SSE • Study space weather storm arrival • Link storm effects to cosmic ray anisotropy • During events • Precursor signatures • Study relativistic solar proton events • Analysis of Ground Level Enhancements • If possible develop warning protocols and issue warnings
Annual Latitude Survey • In conjunction with Bartol • Operate a Uni of Tas/AAD built mobile neutron monitor housed in a standard shipping container • Use USCG Ice Breakers Polar Sea and Polar Star • Return Seattle - McMurdo each Austral summer • Determine the cosmic ray spectrum variation throughout the solar cycle • Determine the changed atmospheric response with changing spectrum • Determine the Geomagnetic cutoff effects
GLE Modelling • In conjunction with • Peg Shea and Don Smart (formerly AFRL) • Uni of Bern • Continue development of leading GLE arrival model • Spectrum, pitch angle distribution, arrival direction • Deduce IMF transport effects • Input to source acceleration mechanism knowledge (flare, shock, stochastic etc)
Flight Radiation Exposure • Radiation dosage rates in aircraft • In situ measurements • Comparison with CARI, EPCARD • Develop capacity to account for transients • Forbush decreases • Geomagnetic cutoff variations • GLEs
Forbush decrease and GLEs Data from Space Ship Earth
LAX - JFK QF107 29th Oct 2003 Route 2 Initial cruising altitude 37,000ft giving a mean 3 Micro Sieverts/hr. 19
LAX - JFK QF107 11th Jan 2004 Route 2 Same profile as closely as allowed by air traffic control on quiet day. Initial cruise at 37,000ft shows a higher background CR level commencing at 3.5 Micro Sv/hr increasing to 3.9 Micro Sv/hr with latitude increase. 21
Flight Radiation Exposure (2) • Cutoff calculations • Attempt grid computing solution • Produce DVD of cutoff values • Include Kp, Dst, date & time (≤ hour resolution) • 1 x 1 degree resolution plus all monitor sites • Influence legislators and industry • Duty of care responsibility • Pre-emptive management planning • AAD jet flight to Casey, Antarctica @ 51k ft