SPACE AND COSMIC RAY PHYSICS SEMINAR

University of Maryland
Computer & Space Science Building, Room 2400
4:30 PM Monday, April 7, 2008
Coffee, Tea & Cookies 4:15-4:30 PM

Robert B. Decker

Johns Hopkins Applied Physics Laboratory


Voyager 2 at the Termination Shock: Energetic Particle Perspective

Broad regions on both sides of the solar wind termination shock are populated by high intensities of non-thermal ions and electrons. The pre-shock particles in the solar wind were measured at Voyager 1 from mid-2002 through Dec. 2004 and at Voyager 2 from early 2005 through mid- 2007. The post-shock particles in the inner heliosheath have also been measured at Voyager 1 since it crossed the termination shock in Dec. 2004. However, it had not been clear what effect these particles might have on the physics of the shock transition until Voyager 2 crossed the shock during days 242-245 of 2007. Unlike Voyager 1, Voyager 2 is making plasma measurements. Data from the plasma and magnetic field instruments on Voyager 2 indicate that non-thermal ion distributions likely play key roles in mediating dynamical processes at the termination shock and in the inner heliosheath. Intensities of low-energy ions measured at Voyager 2 produce non-thermal partial ion pressures in the heliosheath that are comparable to (or exceed) both the thermal plasma pressures and the scalar magnetic field pressures. These ions are evidently the >0.028 MeV portion of the non-thermal ion distribution that determines termination shock structure and whose acceleration extracts a large fraction of bulk flow kinetic energy from the incident solar wind. We discuss these results, compare energetic particle data from the two Voyagers, and summarize recent observations.


Sponsored by: Department of Physics and the Institute for Physical Science and Technology, University of Maryland. For information call Debbie Jenkins at (301) 405-4780 or go to the UMD Space Physics group seminar web site.

For free parking please park in lot DD or anywhere on levels 1-2 in lot B (the big parking garage) after 4:00 pm. Make sure that you park in a spot WITHOUT a parking meter. More parking information is at the seminar website.