Coordinated measurements made by the Sondrestrom radar and the Polar Bear ultraviolet imager

Journal Article · Sun Mar 01 00:00:00 EST 1992 · Journal of Geophysical Research; (United States)

DOI:https://doi.org/10.1029/91JA02803· OSTI ID:5398340

Robinson, R; Vondrak, R ^[1]; Dabbs, T; Vickrey, J ^[2]; Eastes, R; Del Greco, F; Huffman, R ^[3]; Meng, C ^[4]; Daniell, R; Strickland, D; Vondrak, R ^[5]

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1. Lockheed Palo Alto Research Lab., CA (United States)
2. SRI International, Menlo Park, CA (United States)
3. Phillips Lab., Hanscom AFB, MA (United States)
4. John Hopkins Univ., Laurel, MD (United States)
5. Computational Physics Inc., Newton, MA (United States)

In 1986 and 1987 the Sondrestrom incoherent scatter radar in Greenland was operated routinely in coordination with selected overpasses of the Polar Bear satellite. For these experiments the auroral ionospheric remote sensor on Polar Bear obtained images of auroral emissions in two far ultraviolet wavelength bands centered at approximately 136 and 160 nm and one visible band centered at 391.4 nm. Measurements at these three wavelengths were extracted from the images for comparison with the coincident radar measurements. Model calculations have shown that for Maxwellian incident electron distributions the ratio between the 136-nm luminosity and 391.4-nm luminosity can be used to estimate the mean energy of precipitating electrons. Once the mean energy is known, then either of the two emissions can be used to determine the total energy flux. This procedure is used to determine the properties of the incident electron distribution during three midnight sector auroral events over Sondre Stromfjord. The incident electron flux is then used to calculate the expected height profile of electron density which is compared with the simultaneous and coincident radar measurements. The results show that the derived profiles agree well with the measured profiles both in the peak electron density and the altitude of the peak. The accuracy with which the peak of the profile is predicted by this technique is such that many important ionospheric parameters can be reliably inferred from remote measurements, including, for example, the height-integrated electrical conductivities.

• OSTI ID: 5398340
• Journal Information: Journal of Geophysical Research; (United States), Vol. 97:A3; ISSN 0148-0227
• Country of Publication: United States
• Language: English

Related Subjects

71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
AURORAE
REMOTE SENSING
IONOSPHERE
ELECTRON DENSITY
COMPARATIVE EVALUATIONS
ELECTRIC CONDUCTIVITY
ELECTRON PRECIPITATION
EMISSION SPECTRA
LUMINOSITY
RADAR
SATELLITES
ULTRAVIOLET SPECTRA
CHARGED-PARTICLE PRECIPITATION
EARTH ATMOSPHERE
ELECTRICAL PROPERTIES
EVALUATION
MEASURING INSTRUMENTS
OPTICAL PROPERTIES
PHYSICAL PROPERTIES
PLANETARY IONOSPHERES
RANGE FINDERS
SPECTRA
661320* - Auroral
Ionospheric
& Magnetospheric Phenomena- (1992-)