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Atomic hydrogen and solar Lyman-alpha flux deduced from STP 78-1 uv observations

Technical Report ·
OSTI ID:5312196
Simultaneous observations of the Lyman-alpha and 1026-A airglow by a spectrometer on the STP 78-1 satellite were analyzed. A spherical model of a multiple scattering of solar Lyman-alpha and Lyman-beta radiation was utilized that nonisothermal temperature profile. Analysis of the data near 0 latitude yields an exobase density N/sub c/ = 26000 + or - 2000/cu cm/sup -3/, and escape flux F/sub c/ = 2 + or - 0.5 x 10/sup 8//sq cm/s. The solar Lyman-alpha line center flux determined from analysis of the Lyman-alpha airglow was 6.0 + or - 1.2 x 10/sup 11/ photons/sq cm/sA. Analysis of the 1026-A airglow showed that this emission is dominated by multiple scattering of solar Lyman-beta photons by atomic oxygen and that the Lyman-beta airglow contributes less than 20% to the observed emission.
Research Organization:
California Univ., Berkeley (USA). Space Sciences Lab.
OSTI ID:
5312196
Report Number(s):
AD-A-188764/5/XAB
Country of Publication:
United States
Language:
English