Results 151 to 160 of about 4,644 (217)
Structural Analysis of Tilvestamab in Complex with AXL. [PDF]
ACS OmegaChristakou E +5 more
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Photochemical Haze Formation on Titan and Uranus: A Comparative Review. [PDF]
Int J Mol SciDubois D.
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Magnetic star-planet interaction in the young exoplanet system DS Tucanae Ab
Santos Ld +13 more
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Space Science Reviews, 1965
A review is given of the present state of the problem of upper atmospheric emission, in relation to the processes which take place in that region.
V. I. Krasovskij, N. N. Šefov
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A review is given of the present state of the problem of upper atmospheric emission, in relation to the processes which take place in that region.
V. I. Krasovskij, N. N. Šefov
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Proceedings of the Indian Academy of Sciences - Section A, 1964
The altitude variation of the intensity ofλ 6300 line of OI atom and that ofλ 3914 (0–0 band of the first negative system of N2+) in the day airglow have been calculated. It has been found that photodissociation of O2 by the Schumann-Range continuum is mainly responsible for the emission ofλ 6300 line (intensity 65 KR).
S. N. Ghosh, K. D. Sharma
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The altitude variation of the intensity ofλ 6300 line of OI atom and that ofλ 3914 (0–0 band of the first negative system of N2+) in the day airglow have been calculated. It has been found that photodissociation of O2 by the Schumann-Range continuum is mainly responsible for the emission ofλ 6300 line (intensity 65 KR).
S. N. Ghosh, K. D. Sharma
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Journal of Atmospheric and Terrestrial Physics, 1961
Abstract An increase of the OH emission intensity with increasing rotational temperature, and seasonal variations of the intensity and rotational temperature of OH have been established by spectral observations at Yakutsk. No such behaviour has been observed at Zvenigorod. At both locations variations of the relative populations of the OH vibrational
V.I. Krassovsky, N.N. Shefov, V.I. Yarin
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Abstract An increase of the OH emission intensity with increasing rotational temperature, and seasonal variations of the intensity and rotational temperature of OH have been established by spectral observations at Yakutsk. No such behaviour has been observed at Zvenigorod. At both locations variations of the relative populations of the OH vibrational
V.I. Krassovsky, N.N. Shefov, V.I. Yarin
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