Storm-time dynamics of the low-energy solar proton boundaries in the magnetosphere

Details Storm-time dynamics of the low-energy solar proton boundaries in the magnetosphere Storm-time dynamics of the low-energy solar proton boundaries in the magnetosphere

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.477..575t&link_type=abstract

In: Proceedings of the Second Solar Cycle and Space Weather Euroconference, 24 - 29 September 2001, Vico Equense, Italy. Editor:

Computer Science

1

Earth Magnetosphere, Solar Protons

Scientific paper

The ~1 MeV solar proton boundaries in the magnetosphere is studied using the data of Cosmos satellites (polar orbits at ~500-1000 km altitude). Unique data of simultaneous detection of >1 MeV solar proton boundaries were obtained onboard three Cosmos satellites during a strong magnetic storm of ~200 nT Dst amplitude. The lowest storm-time position of the boundaries is observed some hours before the storm maximum at early dusk hours, when the largest local time asymmetry of the boundaries occurs. The dynamics of the equatorial and polar boundaries of solar protons in the magnetosphere is compared with the substorm development during the magnetic storm.

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