Observations of stellar scintillations caused by temperature variations in the atmosphere at heights of 40-50 KM

Details Observations of stellar scintillations caused by temperature variations in the atmosphere at heights of 40-50 KM Observations of stellar scintillations caused by temperature variations in the atmosphere at heights of 40-50 KM

Feb 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993fizao..29....5g&link_type=abstract

Rossiiskaia Akademiia Nauk, Izvestiia, Fizika Atmosfery i Okeana (ISSN 0002-3515), vol. 29, no. 1, p. 5-10.

Physics

1

Atmospheric Refraction, Atmospheric Temperature, Mir Space Station, Scintillation, Stellar Luminosity, Stratosphere, Temperature Distribution, Vertical Distribution

Scientific paper

Results of limb observations of stellar scintillations performed on the
Mir orbital station in 1989 are presented. It is shown that the
scintillation spectra and the retrieved vertical spectra of temperature
fluctuations at heights of 40-50 differ significantly in the
high-frequency region from the spectra obtained at lower heights.

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