Geomagnetic field fluctuations at synchronous orbit. I - Power spectra

Details Geomagnetic field fluctuations at synchronous orbit. I - Power spectra Geomagnetic field fluctuations at synchronous orbit. I - Power spectra

Aug 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978jgr....83.3859a&link_type=abstract

Journal of Geophysical Research, vol. 83, Aug. 1, 1978, p. 3859-3865.

Physics

3

Ats 6, Geomagnetism, Geosynchronous Orbits, Magnetic Variations, Power Spectra, Kp Index, Magnetic Measurement, Magnetic Storms, Magnetosheath, Satellite Observation, Synchronous Satellites

Scientific paper

ULF power spectra of geomagnetic variations at synchronous orbit are calculated for August 1974 on the basis of data from the UCLA triaxial fluxgate magnetometer on ATS 6. Emphasis is placed on the examination of the background spectrum, and therefore the diurnal differences and all relationships in magnetic activity as reflected in the Kp index. The average power spectrum at synchronous orbit is also compared with reported observations from the interplanetary medium, the magnetosheath, the region inside the magnetosphere near the magnetopause, and the ground.

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