Ionosonde observations of the northern magnetospheric cleft during December 1974 and January 1975

Computer Science – Sound

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Auroral Zones, Interplanetary Magnetic Fields, Ionosondes, Ionospheric Disturbances, Magnetic Disturbances, Magnetospheric Instability, Ground Stations, Ionograms, Ionospheric Sounding, Rocket Sounding, Satellite Observation, Solar Wind Velocity

Scientific paper

During December 1974 and January 1975, the northern magnetospheric cleft was monitored by ionosondes at Cape Parry and Sachs Harbor, Northwest Territories, Canada, in support of rocket shots into the cleft. Ionograms were taken nominally at 15-min intervals but as rapidly as two per minute during times of particular interest. Analysis of 5 days of data shows the ionosphere at cleft latitudes to be very complex and dynamic. The ionograms often show considerable structure and can change appearance significantly in a minute or two. The cleft at times appears to move equatorward in response either to a southward turning of the interplanetary magnetic field or to the occurrence of geomagnetic disturbances. This response is in agreement with the conclusions of previous satellite studies. Behavior contrary to this generalization is not uncommon, however, and therefore it may not always hold on time scales considerably shorter than the satellite orbital period of at least 1 hour. The rate of the cleft's motion may vary from about 0.05 to 0.5 deg/min.

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