Time-sequence of polar magnetic substorms

Details Time-sequence of polar magnetic substorms Time-sequence of polar magnetic substorms

Nov 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975p%26ss...23.1483s&link_type=abstract

Planetary and Space Science, Volume 23, Issue 11, p. 1483-1494.

Physics

1

Scientific paper

The time-sequence of polar magnetic substorms is discussed to clarify some controversies on the magnetospheric substorm model including the growth phase. The main purpose of the analyses is to examine magnetic variations in the polar cap and in low latitudes. The onset of the expansion phase is confirmed to be reasonably defined by a vector change of polar-cap magnetic disturbance, a sharp intensification of the auroral electrojet disturbance and the beginning of positive ΔH disturbance in midlatitudes near midnight. It is shown that the growth phase signatures so far proposed are consistent when the onset of the expansion phase is identified from the above mentioned features. Now at Applied Physics Laboratory, The Johns Hopkins University, Maryland, U.S.A.

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