Multiple correlation between auroral and magnetic pulsations

Details Multiple correlation between auroral and magnetic pulsations Multiple correlation between auroral and magnetic pulsations

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984esasp.217..391o&link_type=abstract

In ESA Achievements of the Intern. Magnetospheric Study (IMS) p 391-394 (SEE N85-24544 14-46)

Physics

Auroras, Electron Precipitation, Geomagnetic Pulsations, Ionospheric Conductivity, All Sky Photography, Luminosity, Statistical Correlation

Scientific paper

Multiple correlation analysis between ground magnetic pulsations observed at a control point and auroral pulsating patches in various parts of the sky observed by an all sky TV camera shows that the magnetic variations (time derivatives) can be well represented by linear combinations of luminosity fluctuation in various parts of the sky and that the linear coefficients, which relate the luminosity fluctuations to the magnetic fluctuations, can be stable for over 30 min. It is concluded that magnetic pulsation below a pulsating aurora is mainly due to conductivity fluctuation in the ionosphere caused by the pulsating precipitation of auroral electrons.

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