Physics
Scientific paper
Dec 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011agufmsm33a2147d&link_type=abstract
American Geophysical Union, Fall Meeting 2011, abstract #SM33A-2147
Physics
[2730] Magnetospheric Physics / Magnetosphere: Inner, [2740] Magnetospheric Physics / Magnetospheric Configuration And Dynamics, [2752] Magnetospheric Physics / Mhd Waves And Instabilities, [2753] Magnetospheric Physics / Numerical Modeling
Scientific paper
We have previously shown that the median value of electron density at geosynchronous orbit peaks at solar minimum while the median value of mass density peaks at solar maximum. Correspondingly, the composition of bulk plasma at geosynchronous orbit changes drastically over the solar cycle, with typical concentration of O+ varying from near zero at solar minimum to about 20% at solar maximum. Here we extend our study to other dependencies. Combining measurements of the fundamental and harmonic frequencies of Alfven waves by GOES spacecraft (from which we get the mass density and its field line dependence), measurements of weighted (by the inverse particle mass) ion density by the Los Alamos National Lab (LANL) Magnetospheric Plasma Analyzer (MPA), and electron density measurements from plasma wave data measured by several spacecraft passing through geosynchronous orbit, we derive the density, composition, and mass density field line dependence of bulk plasma at geosynchronous orbit. We explore the variation of these quantities with respect to phase of the solar cycle (based on the EUV solar radiation index F10.7), season, and magnetic local time MLT.
Amoh J.
Anderson Rachel
Denton Richard E.
Huo Jia
Litscher L.
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