North-south component of the interplanetary magnetic field and large scale auroral dynamics

Details North-south component of the interplanetary magnetic field and large scale auroral dynamics North-south component of the interplanetary magnetic field and large scale auroral dynamics

Jul 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975natur.256..191a&link_type=abstract

Nature, vol. 256, July 17, 1975, p. 191, 192. NSF-USAF-supported research.

Astronomy and Astrophysics

Astronomy

Auroras, Interplanetary Magnetic Fields, Magnetic Field Configurations, Magnetic Storms, Magnetospheric Instability, Atmospheric Physics, Lines Of Force, Magnetic Effects, Polar Substorms, Satellite Observation, Spaceborne Astronomy

Scientific paper

Attention is given to the role of the north-south component of the interplanetary magnetic field in magnetospheric substorm processes. The investigation takes into account both large-scale auroral photographs obtained with the DMSP satellite and interplanetary magnetic field data received from the Heos satellite. It is found that the occurrence of substorms does not depend on the size of the auroral oval, except for periods when the oval contracts to its minimum size.

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