HR: 1340h
AN: SA13A-1120 [Abstracts]
TI: Magnetic Oscillations at Mars During the October 2003 Solar Storm
AU: * Espley, J R
EM: espley@rice.edu
AF: Rice University, MS-108
Dept. of Physics and Astronomy, Houston, TX 77005
United States
AU: Cloutier, P A
EM: pac@spacibm.rice.edu
AF: Rice University, MS-108
Dept. of Physics and Astronomy, Houston, TX 77005
United States
AU: Crider, D H
EM: dana.crider@gsfc.nasa.gov
AF: Catholic University of America, c/o 106 Driftwood Dr., Gibsonville, NC 27249
United States
AU: Brain, D A
EM: brain@ssl.berkeley.edu
AF: University of California, Berkeley, Space Sciences Laboratory, Berkeley, CA 94720
United States
AU: Acuna, M H
EM: mario.acuna@gsfc.nasa.gov
AF: NASA Goddard Space Flight Center, Code 695.0, Greenbelt, MD 20701
United States
AB:
The powerful x-class superflare which occurred on the Sun on October 28, 2003 had important effects on the plasma
environments of both the Earth and Mars. We present here observations of the effects at Mars from the Mars Global Surveyor
(MGS) Magnetometer/Electron Reflectometer experiment. In particular we focus on the changes in the nature of the magnetic
oscillations observed during the passage of the solar storm. We find that the types of plasma oscillations observed at the
MGS mapping altitude of 400 km are similar to the oscillations observed in the magnetosheath (which is normally at altitudes
higher than 1000 km). This result is consistent with other observations that show that the magnetosheath altitude is lowered
during the solar storm. We also observe relatively strong oscillations in the nightside tail region where such oscillations
are rarely observed. Such observations have implications for atmospheric loss since they raise the possibility that large
portions of the atmosphere are exposed to the solar wind and are hence subject to pickup escape during such large storm
events.
DE: 5421 Interactions with particles and fields
DE: 6225 Mars
DE: 2149 MHD waves and turbulence
DE: 2152 Pickup ions
SC: SPA-Aeronomy [SA]
MN: 2004 AGU Fall Meeting