The relation of hydrogen auroras and magnetic storms to ring-current dynamics

Details The relation of hydrogen auroras and magnetic storms to ring-current dynamics The relation of hydrogen auroras and magnetic storms to ring-current dynamics

Feb 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ge%26ae..31...96t&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 31, Jan.-Feb. 1991, p. 96-105. In Russian.

Computer Science

Auroras, H Lines, Magnetic Storms, Ring Currents, Solar Flares, Solar Protons, Auroral Irradiation, Earth Magnetosphere, Magnetically Trapped Particles, Proton Precipitation, Solar Activity Effects

Scientific paper

The space-time distribution of hydrogen auroras during various types of global magnetic storms was investigated in relation to solar proton flares and the state of the ring current. It is shown that the compression of the magnetosphere after a sudden storm commencement is accompanied by intense hydrogen auroras at latitudes ranging from 61 to 73 deg. The proton precipitation in the auroral zone is not connected with solar proton flares and the type of storm. Rather, it depends on the storm intensity; the most intense proton auroras are observed during a storm with /Dst/ not greater than about 100 nTl.

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