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

Journal Article · · Journal of Geophysical Research; (United States)
; ; ;  [1];  [2]
  1. Naval Research Lab., Washington, DC (United States)
  2. Univ. of California, Berkeley (United States)
Simultaneous observations of the Lyman {alpha} and 1,026 {angstrom} airglow by a spectrometer on the STP 78-1 satellite have been analyzed. A spherical model of the multiple scattering of solar Lyman {alpha} and Lyman {beta} radiation was utilized which includes the effect of pure absorption by O{sub 2} and a nonisothermal temperature profile. Analysis of data near 0{degrees} latitude yields an exobase temperature T{sub c} = 1,300 {+-} 200 K, exobase density N{sub c} = 2.6 {+-} 0.2 {times} 10{sup 4} cm{sup {minus}3}, and escape flux F{sub c} = 2{+-} 0.5 {times} 10{sup 8} cm{sup {minus}2} s{sup {minus}1}. The solar Lyman {alpha} line center flux determined form analysis of the Lyman {alpha} airglow was 6.0 {+-} 1.2 {times} 10{sup 11} photons cm{sup {minus}2} s{sup {minus}1} {angstrom}{sup {minus}1}. Analysis of the 1,026 {angstrom} 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.
OSTI ID:
5615092
Journal Information:
Journal of Geophysical Research; (United States), Journal Name: Journal of Geophysical Research; (United States) Vol. 92:A8; ISSN 0148-0227; ISSN JGREA
Country of Publication:
United States
Language:
English