1979
DOI: 10.1038/281463a0
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Near IR variability of the quiet Sun

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1981
1981
1981
1981

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“…As the model by Parker (1979a) implies a depth dependent umbral dot structure, a comparison of our intensity observations and a 2-component depth dependent model calculation may be of interst. Markov et al (1979), have observed short-period variations in the radiative flux from the quiet Sun, at wavelengths between 4.05 and 5.25 txm. They attributed this variation to a complete disappearance and reformation of CO molecules.…”
Section: M)mentioning
confidence: 99%
“…As the model by Parker (1979a) implies a depth dependent umbral dot structure, a comparison of our intensity observations and a 2-component depth dependent model calculation may be of interst. Markov et al (1979), have observed short-period variations in the radiative flux from the quiet Sun, at wavelengths between 4.05 and 5.25 txm. They attributed this variation to a complete disappearance and reformation of CO molecules.…”
Section: M)mentioning
confidence: 99%