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The atmospheres of mars and venus
Die Naturwissenschaften, 1970[1] Kundt, W.: Z. Physik 163, 77 (I961).---Robinson, I., Trautman, A.: Proc. Roy. Soc. A z6s, 463 (1962). Kundt, W., Trtimper, M. : Akad. Wiss. Mainz, Abh. math.-nat. K1. Nr. 12, 980 (1962).-Pirani, F. A. E., in : Trautman, A., Pirani, F. A. E., Boudi, H. : Brandeis Summer Inst. inTheor. Phys. 1964. Vol. 1. New Jersey: prentice Hall I965. [2] Kundt, W.,
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Oblateness of the atmosphere of Mars
Nature, 1976ON April 8, 1976 Mars occulted the bright star ɛ Geminorum (magnitude 3.2). Predictions1 were issued well in advance since such occurrences are very rare: indeed, it is estimated that Mars occults a star as bright as this about once in 500 yr. Accurate observations of the duration of the occultation were made from four sites on the Earth and these are ...
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Ionization in the Atmosphere of Mars
Proceedings of the IRE, 1929Assuming that the atmosphere at the surface of Mars consists of ⅕ oxygen and ⅘ other gases, as nitrogen, etc., the composition of the atmosphere to great heights is calculated, just as was done for the earth, from the actions of gas diffusion and gravity. The electron density in the atmosphere of Mars due to the ultraviolet light of the sun is found to
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The Mars Atmosphere and Volatile Evolution (MAVEN) Mission
Space Science Reviews, 2015B M Jakosky
exaly
No widespread dust in the middle atmosphere of Mars from Mars Climate Sounder observations
Icarus, 2015Armin Kleinböhl, David M Kass
exaly