Zobrazeno 1 - 10
of 21
pro vyhledávání: '"V. V. Kerzhanovich"'
Autor:
A. N. Lipatov, A. B. Manukin, A. P. Ekonomov, P. V. Struct, V. S. Makarov, V. M. Linkin, V. V. Kerzhanovich
Publikováno v:
SPACE, TIME AND FUNDAMENTAL INTERACTIONS. 2:68-74
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3d569ad6cdfc74b4c29949a1ff368ca1
https://doi.org/10.17238/issn2226-8812.2018.2.68-74
https://doi.org/10.17238/issn2226-8812.2018.2.68-74
Autor:
G.-P. Lepazg, J. Avrar, J. Ortis, V. M. Linkin, I.V. Trifonov, A.M. Zashchirinskii, K.M. Pichkhadze, L.B. Sazonov, R.S. Kremnev, N.G. Polukhina, V. V. Kerzhanovich, B.B. Kotov, K.A. Kotelnikov, V.A. Pavlov, D.N. Nazarov, O.V. Makartsev
Publikováno v:
Advances in Space Research. 17:77-80
For experimental testing of a Mars balloon probe in the upper layers of the Earth's atmosphere a specified parachute system was developed, fabricated and tested in 3 high-altitude balloon flights. The balloon volumes were 130000 and 180000 m 3 with t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c456cd042323b7094ab0b5b06682129d
https://doi.org/10.1016/0273-1177(95)00679-9
https://doi.org/10.1016/0273-1177(95)00679-9
Autor:
K.M. Pichkhadze, L. Boloh, C. E. Hildebrand, M. Roy, V. M. Linkin, D. Patsaev, V. V. Kerzhanovich, Michael V. Kurgansky, L. Matveenko, Robert A. Preston, J. E. Blamont, L. Kogan, T. Young
Publikováno v:
Advances in Space Research. 13:145-152
On June 11 and 15, 1985 two packages with balloons have been inserted in the atmosphere of Venus from the Soviet VEGA landing modules. This paper summarizes the pressure, temperature, wind illumination and backscattering data from the balloons.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3923d4c8bd5dcee8f9d473f65830a7a6
https://doi.org/10.1016/0273-1177(93)90289-n
https://doi.org/10.1016/0273-1177(93)90289-n
Autor:
V. V. Kerzhanovich, M. Ya. Marov
Publikováno v:
Icarus. 30:320-325
Some features of the wind-velocity determination based on the results of Doppler shift measurements from the Venera probes during their descent in the Venus atmosphere are discussed. The validity of assumptions used in the reduction and analysis of t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3c6c693ae0e7dfd6479d1d69467553c6
https://doi.org/10.1016/0019-1035(77)90167-1
https://doi.org/10.1016/0019-1035(77)90167-1
Autor:
M.R. Traxler, J. P. Berthias, James K. Campbell, E. L. Lau, Irwin I. Shapiro, R. W. Hellings, James G. Williams, J.A. Dunne, E. L. Akim, J. E. Blamont, John F. Chandler, V. M. Linkin, N.J. Borderies, Jordan Ellis, V. V. Kerzhanovich, Robert D. Reasenberg, John D. Anderson, Robert A. Preston, N. M. Ivanov, C. F. Yoder
Publikováno v:
Advances in Space Research. 9:71-74
A planned experiment to obtain range and Doppler data with the Phobos 2 Lander on the surface of the Martian satellite Phobos is described. With the successful insertion on January 29, 1989 of Phobos 2 into Mars orbit, it is anticipated that the Land
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::68541f61225cba67caaabec62509cd93
https://doi.org/10.1016/0273-1177(89)90009-4
https://doi.org/10.1016/0273-1177(89)90009-4
Autor:
M. Ya. Marov, John T. Schofield, Alvin Seiff, Henry E. Revercomb, Fredric W. Taylor, Sanjay S. Limaye, Lawrence A. Sromovsky, Arvydas J. Kliore, V. I. Moroz, V. V. Kerzhanovich
Publikováno v:
Advances in Space Research. 5:3-58
From a critical comparison and synthesis of data from the four Pioneer Venus Probes, the Pioneer Venus Orbiter, and the Venera 10, 12, and 13 landers, models of the lower and middle atmosphere of Venus are derived. The models are consistent with the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4ecb8e1b620a65cecdbfd37e0717c33b
https://doi.org/10.1016/0273-1177(85)90197-8
https://doi.org/10.1016/0273-1177(85)90197-8
Autor:
H. Jahn, D. Spänkuch, I.A. Matsgorin, D. Oertel, A. A. Shurupov, V. M. Linkin, A. N. Lipatov, V. I. Moroz, W. Döhler, Ludmila Zasova, W. Stadthaus, E. A. Ustinov, J. Nopirakowski, J. Güldner, H. Becker-Ross, R. Dubois, V. V. Kerzhanovich, Klaus Schäfer
Publikováno v:
Advances in Space Research. 5:25-36
Fourier spectrometers for the investigation of infrared spectra of Venus were installed on the recent Soviet orbiters “Venera-15” and “Venera-16”. Many spectra with reliable absolute calibration were obtained in the 280–1500 cm −1 region
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6368296a2acd586b2e9a4b22b6100aff
https://doi.org/10.1016/0273-1177(85)90267-4
https://doi.org/10.1016/0273-1177(85)90267-4
Autor:
V. V. Kerzhanovich
Publikováno v:
Icarus. 30:1-25
More exact Doppler data, obtained by digital processing of the radio signals received from the Mars 6 descent module, provide, by direct conversion, estimates of the parameters of the Martian atmosphere at 12–90 km: the mass density at altitude 12
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e855c82c0568dadcc02343541bb566f8
https://doi.org/10.1016/0019-1035(77)90117-8
https://doi.org/10.1016/0019-1035(77)90117-8
Autor:
Sanjay S. Limaye, V. V. Kerzhanovich
Publikováno v:
Advances in Space Research. 5:59-83
A reference model of the atmospheric circulation on Venus based on available observations is presented. The reference atmosphere has the following main features: (1) the entire atmosphere below 85 km moves predominantly from east to west in the plane
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::fde155b114643a1bdcd7b97664867c3c
https://doi.org/10.1016/0273-1177(85)90198-x
https://doi.org/10.1016/0273-1177(85)90198-x
Autor:
O. L. Ryabov, V. P. Lysov, M. Ya. Marov, N. F. Borodin, V. S. Avduevsky, B.Ye. Moshkin, A. P. Ekonomov, M. K. Rozhdestvensky, V. V. Kerzhanovich
Publikováno v:
Icarus. 20:407-421
The Venera 8 descent module measured pressure, temperature, winds and illumination as a function of altitude in its landing on July 22, 1972, just beyond the terminator in the illuminated hemisphere of Venus. The surface temperature and pressure is 7
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c34ece05c571268388013086cff3e5fe
https://doi.org/10.1016/0019-1035(73)90014-6
https://doi.org/10.1016/0019-1035(73)90014-6