Interhemispheric Studies Through AON and PAntOS

1. IPY Cluster Project #63 Heliosphere Impact on Geospace Kick-off Workshop, Finnish Meteorological Institute Helsinki, Finland, 5-9 February 2007 Interhemispheric Studies Through AON and PAntOS Vladimir Papitashvili Department of Atmospheric, Oceanic and Space Sciences University of Michigan

2. GEOSPACE:Solar Wind and Earth’s Magnetosphere Courtesy of NASA

3. Solar Wind and Interplanetary Magnetic Field, Earth’s Magnetosphere, Plasmasphere, and IonosphereComplex, Coupled System with the Mass & Energy Transfer • Magnetic conjugacy studies are of general interest because of their implications concerning the processes that electrically couple the magnetosphere and ionosphere. … Four major categorizations seem to occur : • clearly conjugate features implying similar topologies and precipitation patterns; • conjugate features implying similar topologies, but with distinct differences in precipitation characteristics; • features that occur in both hemispheres but at different MLT; and • features that appear in only one hemisphere. • J. S. Murphree and J. D. Craven “Evaluation of the High Latitude Magnetic Conjugacy of Auroral Features Based on DE-1 and Viking Data”, AGU Fall Meeting 2001, Abstract #SM32A-0808.

4. What spacecraft can see from geospace? Could Earth’s Polar Regions be Windows to Geospace and to Heliosphere? Jupiter’s Polar Regions

5. Substorm’s Onset and Theta Aurora inOpposite Hemispheres: September 18, 2000 • Northern Hemisphere • 10-12 MLT • 74-80 degrees • No Theta Aurora • Southern Hemisphere • 11-15 MLT • 80-87 degrees • Theta Aurora Østgaard et al., GRL, 2003

6. IMAGE Spacecraft Far Ultra Violet Camera & Wide Imaging Camera Substorm Onset in Conjugate Hemispheres What controls asymmetry of substorm onset locations? POLAR Spacecraft Visible Imaging System Earth camera Courtesy of Nikolai Østgaard

7. Exceptionally synchronous discrete aurorasover Tjornes (Iceland) and Syowa (Antarctica) What controls the size, shape, and location of conjugate auroral forms? All-sky TV data (23:19:30- 23:23:50 UT, 10 sec interval) September 26, 2003 Sato et al., GRL, 2005

8. Polar Caps and Auroral Ovals in Corrected Geomagnetic Coordinates (dashed lines) http://modelweb.gsfc.nasa.gov/models/cgm/ North South with magnetospheric sources added (solid lines)

9. IMF-Dependent Maps of Ground Magnetic Field Perturbations Summer IMF BT = 5 nT Winter

10. DMSP-based IMF-Dependent Maps of Ionospheric Plasma Convection http://mist.engin.umich.edu/ Northern Summer IMF BT = 5 nT Southern Winter Papitashvili, V. O., and F. J. Rich, High-latitude ionospheric convection models derived from Defense Meteorological Satellite Program ion drift observations and parameterized by the interplanetary magnetic field strength and direction, J. Geophys. Res., 107, No. A8, 10.1029/2001JA000264, SIA 17(1-13), 2002.

11. IMF-Dependent Maps of Field-Aligned Currents http://mist.engin.umich.edu Northern Winter IMF = 5 nT Southern Summer Papitashvili, V. O., F. Christiansen, and T. Neubert, A new model of field-aligned currents derived from high-precision satellite magnetic field data, Geophys. Res. Lett., 29, No. 14, 10.1029/2001GL014207, 2002.

12. Magnetosphere-Ionosphere Voltage-Current Relation Experiment and Theory Siscoe et al., JGR, 2002: pc (kV) = 101  21.8 JR1 (MA) If JR1winter = 1.0 MA & JR1summer = 1.5 MA, then sum/win = (10133)/(10122)= 68 / 81 = 0.84 Ørsted-based S. Summer S. Equinox Field-Aligned --------------- --------------- Currents Ratio N. Winter N. Equinox Dayside 1.8 1.0 Dawn R1/R2 1.5 1.0 Dusk R1/R2 1.5 1.0 Nightside 1.0 1.0 R1/R2 field-aligned currents are 1.5 times stronger when they flow in sunlit polar cap DMSP-based Cross-Polar Cap Potential Ratio IMF ~ 0 IMF South N. Summer / S. Winter 0.94 0.64 S. Summer / N. Winter 0.83 0.88 N. Equinox / S. Equinox 0.89 0.90 Cross-polar cap potential drop in the sunlit polar cap is ~15% lower than in the dark cap

13. MHD-modelled Ionospheric Electrodynamics for the Northern Polar Cap Spring Summer Fall Winter Ionospheric potentials Pedersen conductance Field-aligned currents Ridley, A. J., The effects of seasonal changes in the ionospheric conductances on magnetospheric field-aligned currents, submitted to Geophys. Res. Letters, October 2006.

14. MHD-modelled Ionospheric Electrodynamics for the Northern Polar Cap Winter Spring Summer Fall Winter Winter = 83 kV Cross-polar cap potential ~15% Equinox-Summer = 72 kV Summer = 0.47 A/m2 Maximum of derived field-aligned currents ~1.6 times stronger Equinox-Winter = 0.30 A/m2 Ridley, A. J., The effects of seasonal changes in the ionospheric conductances on magnetospheric field-aligned currents, submitted to Geophys. Res. Letters, October 2006.

15. Mapping Magnetopause Reconnection to Conjugate Polar Caps Northern Winter Solstice for 05 UT • Note summer merging lines are shorter in length than winter ones • Difference in the merging lines length could be a geometrical effect due to the Earth’s dipole tilt • However, this could be the effect predicted from our sketch for the Hill’s voltage-current relationship Northern Summer Solstice for 17 UT Coleman, I. J., M. Pinnock, and A. S. Rodger, The ionospheric footprint of antiparallel merging regions on the dayside magnetopause, Annales Geophysicae, 18, 511-516, 2000.

16. Geomagnetic Conjugacy Greenland West Coast and Eastern Antarctic 85 75     A81  P3    P2   SPA  P4 VOS P1 P5 P6 65 80 60 BAS LPMs  70 Greenland West Coast Magnetometer Chain ~40CGM meridian (12 stations) Eastern Antarctic Magnetometer Sites ~40CGM meridian (6 stations)

17. SuperDARN Radars and Magnetometers in the Arctic and Antarctic NIPR LPM between Syowa & Dome F Syowa U. Michigan LPM test run at South Pole Existing Planned

18. THEMIS = Time History of Events and Macroscale Interactions in Substorms NASA Launch – February 15, 2007 Mission Science Objectives • Primary What macroscale instability causes substorm onset? • Secondary How are radiation belt (killer) electrons energized? • Tertiary Dayside solar wind -magnetosphere coupling processes

19. THEMIS – From Geospace to Ground 20 All-Sky Cameras Deployed Across Alaska and Canada

20. THEMIS and Interhemispheric Conjugacy Studies • Onset location and timing relative to boundaries etc. • Magnetosphere - Ionosphere coupling in substorms • Auroral signatures of magnetospheric dynamics • And on and on…

21. THEMIS and Interhemispheric Conjugacy Studies

22. COMMITTEE ON DESIGNING AN ARCTIC OBSERVING NETWORK W. Berry Lyons (Chair), The Ohio State University, Columbus Keith Alverson, Global Ocean Observing System Project Office, IOC/UNESCO, Paris David Barber, Univ. of Manitoba, Winnipeg James G. Bellingham, Monterey Bay Aquarium Research Institute, California Terry V. Callaghan, University of Sheffield, UK & Abisko Sci. Res. Station, Sweden Lee W. Cooper, University of Tennessee Margo Edwards, University of Hawaii Shari Gearheard, Univ. of Western Ontario Molly McCammon, Alaska Ocean Observing System, Anchorage Jamie Morison, Polar Science Center, Seattle Scott E. Palo, University of Colorado, Boulder Andrey Proshutinsky, Woods Hole Oceano- graphic Institution, Massachusetts Lars-Otto Reiersen, Arctic Monitoring and Assessment Programme, Oslo, Norway Vladimir E. Romanovsky, Univ. of Alaska Peter Schlosser, Lamont-Doherty Earth Observatory, Palisades, New York Julienne C. Stroeve, National Snow and Ice Data Center, Boulder, Colorado Craig Tweedie, University of Texas, El Paso John Walsh, University of Alaska, Fairbanks Out of 18 members, only Scott E. Palo, University of Colorado represented STP & Aeronomy

23. Summary • Observable changes, many of which have regional and global implications, are underway across the Arctic. • Although the Arctic is not the only region on Earth affected by environmental change, it … is a region with a limited record of observations … and yet, despite these constraints, rapid and systemic changes have clearly been identified. • The interconnectedness of physical, biological, chemical, and human components, together with the high amplitude of projected changes, make a compelling argument for an improved observation infrastructure that delivers a coherent set of pan-arctic, long-term, multidisciplinary observations. • Without such observations, it is very difficult to describe current conditions in the Arctic, let alone understand the changes that are underway or their connections to the rest of the Earth system. • Without such observations, society’s responses to these ongoing changes and its capability to anticipate, predict, and respond to future changes that affect physical processes, ecosystems, and arctic and global residents are limited. • This report outlines the potential scope, composition, and implementation strategy for an Arctic Observing Network (AON). Such a network would build on and enhance existing national and international efforts and deliver easily accessible, complete, reliable, timely, long-term, pan-arctic observations. • The goal is a system that can detect conditions and fundamental variations in the arctic system, provide data that are easily compared and analyzed, and help improve understanding of how the arctic system functions and changes. The network would serve both scientific and operational needs.

24. Evolution of the Arctic Observing Network

25. Pan-Antarctic Observations System (PAntOS)