SH51D-01
Precursors to Interstellar Shocks of Solar Origin
Friday, 18 December 2015: 08:00
2011 (Moscone West)
Donald A Gurnett1, William S Kurth2, Edward C Stone3, Alan C Cummings3, Stamatios M Krimigis4, Robert B Decker5, Norman F Ness6 and Leonard F Burlaga7, (1)University of Iowa, Physics and Astronomy, Iowa City, IA, United States, (2)University of Iowa, Iowa City, IA, United States, (3)California Institute of Technology, Pasadena, CA, United States, (4)Applied Physics Laboratory Johns Hopkins, Laurel, MD, United States, (5)Applied Physics Laboratory Johns Hopkins, Space, Laurel, MD, United States, (6)IACS-CUA/NASA-GSFC, Landenberg, PA, United States, (7)NASA Goddard Space Flight Center, Greenbelt, MD, United States
Abstract:
On or about 2012 August 25, the Voyager 1 spacecraft crossed the heliopause into the nearby interstellar plasma. In the nearly three years that the spacecraft has been in interstellar space, three notable particle and field disturbances have been observed, each apparently associated with a shock wave propagating outward from the Sun. Here, we present a detailed analysis of the third and most impressive of these disturbances, with brief comparisons to the two previous events, both of which have been previously reported. The shock responsible for the third event was first detected on 2014 February 17 by the onset of narrowband radio emissions from the approaching shock, followed on 2014 May 13 by the abrupt appearance of intense electron plasma oscillations generated by electrons streaming outward ahead of the shock. Finally, the shock arrived on 2014 August 25, as indicated by a jump in the magnetic field strength and the plasma density. Various disturbances in the intensity and anisotropy of galactic cosmic rays were also observed ahead of the shock, some of which are believed to be caused by the reflection and acceleration of cosmic rays by the magnetic field jump at the shock, and/or by interactions with upstream plasma waves. Comparisons to the two previous weaker events show somewhat similar precursor effects, although differing in certain details. Many of these effects are very similar to those observed in the region called the "foreshock" that occurs upstream of planetary bow shocks, only on a vastly larger spatial scale.
