SH21B:
Physical Phenomena in the Outer Heliosphere and Beyond

Submit an Abstract to this Session



Session ID#: 31409

Session Description:
The Voyager 1/2 mission is performing in situ investigation of the physical phenomena that accompany the solar wind interaction with the local interstellar medium. In partially ionized plasmas, charge exchange, ionization, kinetic and fluid instabilities, and magnetic fields play important roles in determining the heliospheric structure. This session addresses the most challenging issues related to Voyager observations: (1) the effects of charge exchange, interstellar magnetic field draping, and time dependent phenomena on Voyager observations; (2) physics of non-thermal ions; (3) ion acceleration at the termination shock and in the heliosheath; (4) galactic cosmic ray transport throughout the heliosphere and LISM; (5) roles of plasma waves, turbulence, instabilities, and magnetic reconnection; (6) relation of Voyager measurements to remote observations from IBEX, Cassini, SOHO, HST, and air shower observatories. We solicit papers addressing these and other phenomena occurring in the outer heliosphere and LISM.
Primary Convener:  Nikolai V Pogorelov, University of Alabama in Huntsville, Department of Space Science, Huntsville, AL, United States
Convener:  John D Richardson, MIT, Cambridge, MA, United States
Chairs:  John D Richardson, MIT, Cambridge, MA, United States and Nikolai V Pogorelov, University of Alabama in Huntsville, Department of Space Science, Huntsville, AL, United States
OSPA Liaison:  Nikolai V Pogorelov, University of Alabama in Huntsville, Department of Space Science, Huntsville, AL, United States
Index Terms:

2104 Cosmic rays [INTERPLANETARY PHYSICS]
2124 Heliopause and solar wind termination [INTERPLANETARY PHYSICS]
2126 Heliosphere/interstellar medium interactions [INTERPLANETARY PHYSICS]
2152 Pickup ions [INTERPLANETARY PHYSICS]

Abstracts Submitted to this Session:

Edward C Stone, California Institute of Technology, Pasadena, CA, United States
Donald A Gurnett, University of Iowa, Physics and Astronomy, Iowa City, IA, United States
Robert B Decker1, Stamatios Mike Krimigis2, Matthew E Hill3 and Edmond C Roelof1, (1)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (2)Academy of Athens, Space, Athens, Greece, (3)Applied Physics Laboratory Johns Hopkins, Space, Laurel, MD, United States
Stephen A Fuselier, Southwest Research Institute, San Antonio, TX, United States, Maher A Dayeh, Southwest Research Institute, San Antonio, United States and Eberhard Möbius, Univ New Hampshire, Durham, NH, United States
Ming Zhang, Florida Institute of Technology, Melbourne, FL, United States and Nikolai Pogorelov, The University of Alabama in Huntsville, Space Science, Huntsville, United States
Matthew E Hill1, Peter Kollmann2, Ralph L McNutt Jr3, Alan Stern4, Harold A Weaver Jr5, Leslie A Young4, Catherine Olkin6, John R Spencer4 and The New Horizons Plasma and Particles Theme Team, (1)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (2)The Applied Physics Laboratory, John Hopkins University, Laurel, United States, (3)Applied Physics Laboratory Johns Hopkins, Laurel, MD, United States, (4)Southwest Research Institute, Boulder, United States, (5)Applied Physics Laboratory Johns Hopkins, Laurel, United States, (6)Southwest Research Institute, Boulder, CO, United States