The structure and microphysical properties of the Venus clouds: Venera 9, 10, and 11 data

Marov, M. Ya.; Lystsev, V. E.; Lebedev, V. N.; Lukashevich, N. L.; Shari, V. P.

doi:10.1016/0019-1035(80)90131-1

Cited by 39 publications

(26 citation statements)

References 8 publications

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“…Photometric profiles obtained on Vll and V12 ( Figure 21) show a maximal optical density at heights corresponding to the B-region (Moroz et al, 1979). Photometry (Ekonomov et al, 1978) and nephelometry (Marov et al, 1978) on V9 and 10 demonstrate the structure of clouds closer to that obtained on the P-D.…”

Section: ~-mentioning

confidence: 53%

“…It is more by an order of two than given by in situ measurements (Table XVI). Some remarks about cloud structure (without quantitative evaluations) are in some other papers devoted to radio occultation data, for example, Yakovlev et al The unicle experiment on P-L (Knollenberg and Hunten , 1979a, b, 1980) V9, V10 -both versions (Marov et al, 1976(Marov et al, , 1978. Version (a) on all four Pioneer probes (Ragent andBlamont, 1979, 1980; and Vll (Marov et al, 1979) 66-0 km 62-20 km (d) In Table XIII The unicle experiment on V12 (Surkov et aL, 1979) (c) For nephelometer of V9, 10 (version (b)).…”

Section: (Iv)mentioning

confidence: 99%

“…(a) From nephelometric data of V9, 10 (Marov et al, 1978) and Pioneer (Ragent and Blamont, 1980). (~ Ragent and Blamont (1980).…”

Section: (Iv)mentioning

confidence: 99%

“…Nephelometric observations on V9, 10, and 11 (Marov et al, 1978(Marov et al, , 1979 have shown the presence of aerosol structures with an optical depth up to 1 and even more in the region F2. Nephelometric experiments on Pioneer (all of the four probes) haven't discovered aerosols here.…”

Section: ~-mentioning

confidence: 99%

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The atmosphere of Venus

Мороз

1981

Space Sci Rev

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The investigations of Venus take a special position in planetary researches. It was just the atmosphere of Venus where first measurements m situ were carried out by means of the equipment delivered by a space probe (Venera 4, 1967). Venus appeared to be the first neighbor planet whose surface had been seen by us in the direct nearness made possible by means of the phototelevision device (Venera 9 and Venera 10, 1975).The reasons for the high interest in this planet are very simple. This planet is like the Earth by its mass, size and amount of energy obtained from the Sun and at the same time it differs sharply by the character of its atmosphere and climate.

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Section: ~-mentioning

confidence: 53%

Section: (Iv)mentioning

confidence: 99%

“…(a) From nephelometric data of V9, 10 (Marov et al, 1978) and Pioneer (Ragent and Blamont, 1980). (~ Ragent and Blamont (1980).…”

Section: (Iv)mentioning

confidence: 99%

Section: ~-mentioning

confidence: 99%

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The atmosphere of Venus

Мороз

1981

Space Sci Rev

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“…The OCPP instrument obtains spin-scan maps using a positionable telescope, which can provide look angles in on the vertical structure and particle sizes below the cloud top (65 km altitude) region (Marov et al 1977, Marov 1978, the range from 0Њ to 145Њ from the direction of the spacecraft spin axis, whose nominal orientation is toward the 1979, Marov et al 1980, Knollenberg and Hunten 1980, Ragent and Blamont 1980, Sagdeev and Moroz 1986. Ta-South ecliptic pole.…”

Section: Table I Properties Of Venus Cloudsmentioning

confidence: 99%