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Steep plasma depletion in dayside polar cap during a CME‐driven magnetic storm
Author(s) -
Sakai J.,
Taguchi S.,
Hosokawa K.,
Ogawa Y.
Publication year - 2013
Publication title -
journal of geophysical research: space physics
Language(s) - English
Resource type - Journals
eISSN - 2169-9402
pISSN - 2169-9380
DOI - 10.1029/2012ja018138
Subject(s) - ionosphere , solar wind , physics , magnetosphere , plasmasphere , atmospheric sciences , geophysics , polar , f region , van allen probes , daytime , local time , geology , plasma , van allen radiation belt , astronomy , statistics , mathematics , quantum mechanics
A series of steep plasma depletions was observed in the dayside polar cap during an interval of highly enhanced electron density on 14 October 2000 through EISCAT Svalbard Radar (ESR) field‐aligned measurements and northward‐directed low‐elevation measurements. Each depletion started with a steep dropoff to as low as 10 11 m − 3 from the enhanced level of ∼3 × 10 12 m −3 at F2 region altitudes, and it continued for 10–15 min before returning to the enhanced level. These depletions moved poleward at a speed consistent with the observed ion drift velocity. DMSP spacecraft observations over an extended period of time which includes the interval of these events indicate that a region of high ion densities extended into the polar cap from the equatorward side of the cusp, i.e., a tongue of ionization existed, and that the ion densities were very low on its prenoon side. Solar wind observations show that a sharp change from IMF B y > 0 to B y < 0 is associated with each appearance of the ESR electron density dropoff. From this unprecedented clear correlation we present a specific scenario: the series of plasma density depletions observed using the ESR is a result of the poleward drift of the undulating boundary of the tongue of ionization; this undulation is created in the cusp roughly 20 min before the ESR observation by the azimuthal intrusion, in response to the rapid prenoon shift of the footprint of the reconnection line, of the low‐density plasmas originating in the morning sector.