Terrestrial kilometric radiation: 2-emission from the magnetospheric cusp and dayside magnetosheath
Measurements of the location of sources of terrestrial kilometric radiation obtained with the lunar orbiting Radio Astronomy Explorer-2 satellite have revealed a class of emission associated with the cusp and dayside magnetosheath. At frequencies near 250 kHz this emission is observed at radial distances between 2 and 20 R/sub E/ at magnetic latitudes of 75 deg to 80 deg and is most often detected during periods of auroral activity (AE approximately = 250) and southward orientation of the interplanetary magnetic field vertical component. During very disturbed times, the emission at the lowest frequencies (< or approximately= 200 kHz) appears to come from the dayside magnetosheath at distances approximately = 12 R/sub E/. Whenever the geomagnetic dipole is tilted significantly with respect to the ecliptic pole (> or approximately = 10 deg) the cusp emission is confined to the hemisphere containing the subsolar point. The measurements also suggest that the region of cusp emission is rather narrowly confined in longitude to within +- a few hours of the noon meridian. (auth)
- Research Organization:
- National Aeronautics and Space Administration, Greenbelt, MD (USA). Goddard Space Flight Center
- OSTI ID:
- 7112439
- Report Number(s):
- N-76-27752; NASA-TM-X-71152; X-695-76-139; TRN: 77-011020
- Resource Relation:
- Other Information: Subm-Submitted for Publication
- Country of Publication:
- United States
- Language:
- English
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Related Subjects
GENERAL PHYSICS
MAGNETOSHEATH
LONG WAVE RADIATION
AURORAE
EMISSION
MAGNETIC STORMS
MAGNETOSPHERE
POLAR REGIONS
SOLAR WIND
EARTH ATMOSPHERE
ELECTROMAGNETIC RADIATION
RADIATIONS
RADIOWAVE RADIATION
SOLAR ACTIVITY
640203* - Atmospheric Physics- Magnetospheric Phenomena- (-1987)