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pro vyhledávání: '"L.V. Ksanfomality"'
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Autor:
L.V. Ksanfomality
Publikováno v:
Acta Astronautica. 105:521-533
Hypothetical habitability of some of extrasolar planets is a fundamental question of science. Some of exoplanets possess physical conditions close to those of Venus. Therefore, the planet Venus, with its dense and hot (735 K) oxygen-free atmosphere o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::30cade067bbb559cf2c54ecf5d4cb009
https://doi.org/10.1016/j.actaastro.2014.07.004
https://doi.org/10.1016/j.actaastro.2014.07.004
Autor:
L.V. Ksanfomality
Publikováno v:
Advances in Space Research. 38:594-598
In recent years, considerable progress has been achieved in producing resolved images of Mercury electronically with short exposures at Earth-based telescopes. For the purpose of obtaining images of the unknown portion of Mercury, the previously star
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::35514509482599f36c69f40d83206e97
https://doi.org/10.1016/j.asr.2005.05.071
https://doi.org/10.1016/j.asr.2005.05.071
Publikováno v:
Planetary and Space Science. 53:849-859
Plans to send orbiter missions to Mercury (e.g., NASA's Messenger and ESA's BepiColombo) have prompted renewed efforts to investigate the surface of Mercury using ground-based remote sensing. While the highest resolution instrumentation optical teles
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6958a96f7de97900f77778e74759d7e8
https://doi.org/10.1016/j.pss.2005.03.003
https://doi.org/10.1016/j.pss.2005.03.003
Autor:
L.V. Ksanfomality
Publikováno v:
Astrophysics and Space Science. 252:41-50
The emergence of life based on amino acids and RNA/DNA on an Earth-type planet requires quite narrow ranges for many of the planet's physical parameters, most notably its mass and temperature conditions. In addition, only stars of F to K spectral typ
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ca256cf333afda67d56a0d812ab8ac94
https://doi.org/10.1023/a:1000893511391
https://doi.org/10.1023/a:1000893511391
Publikováno v:
Planetary and Space Science. 41:569-585
A new analysis of the data of the KRFM experiment (Phobos mission) is presented. The five complete photometric profiles (eight wavelengths for each) obtained in this experiment have been processed, and the calibration and the method of modelling calc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5ae144ea14cff9b13198e6746f2226d3
https://doi.org/10.1016/0032-0633(93)90077-f
https://doi.org/10.1016/0032-0633(93)90077-f
Autor:
L.V. Ksanfomality, J. P. Bibring, Yu.V. Nikolsky, Igor Khatuntsev, V. I. Moroz, I. Langevin, A. V. Zharkov, A. V. Grigoryev, M. Combes
Publikováno v:
Advances in Space Research. 12:13-16
The spectrum of some portion of the Phobos surface was measured at the same points by two instruments (KRFM and ISM) on board the Phobos-2 mission in two ranges: 0.315–0.6 and 0.8–3.1 μm. An example of a spectrum based on data from both experime
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c1da98ef0f0decf22c9b84995d29399c
https://doi.org/10.1016/0273-1177(92)90313-m
https://doi.org/10.1016/0273-1177(92)90313-m
Autor:
A. V. Zharkov, V. I. Moroz, L.V. Ksanfomality, G. E. Nikitin, J. P. Bibring, O.F. Ganpantzerova, E. V. Petrova, M. Combes, Larry W. Esposito, A. Soufflot, N. V. Goroshkova
Publikováno v:
Advances in Space Research. 12:3-12
Photometric limb to limb profiles of Mars were obtained in 8 narrow bands between 315 and 550 nm from the Phobos-2 spacecraft. Tentative results of analysis are presented in terms of optical properties of the atmosphere and surface. Imaginary part of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a85df7c9a53f2b7202b650c54efd4ddf
https://doi.org/10.1016/0273-1177(92)90312-l
https://doi.org/10.1016/0273-1177(92)90312-l
Autor:
Emmanuel Lellouch, Olivier Forni, Yves Langevin, A. Soufflot, D. V. Titov, Yu.V. Nikolsky, V. I. Moroz, M. Combes, J. Rosenqvist, Stéphane Erard, J. P. Bibring, B. Gondet, Christophe Sotin, N. F. Sanko, T. Encrenaz, C. Cara, Pierre Drossart, Ph. Masson, L.V. Ksanfomality, A.V. Grygoriev
Publikováno v:
Scopus-Elsevier
Observations with the infrared spectrometer ISM on board the Phobos 2 spacecraft have provided spectra of Mars in the range 0.7–3.2 μm, with a spatial resolution of the order of 20 km. Spectra between 1.6 and 3.2 μm show evidence for scattering (
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cd01ec74765f43dcd011ed976b3f1272
https://doi.org/10.1016/0032-0633(91)90141-v
https://doi.org/10.1016/0032-0633(91)90141-v
Autor:
L.V. Ksanfomality, V. I. Moroz, G. E. Nikitin, N. V. Goroshkova, Daniel T. Britt, E. Kuhrt, Thomas C. Duxbury, A. Soufflot, Scott L. Murchie, A. V. Zharkov, Carle M. Pieters, James W. Head, P. C. Fisher, B. S. Zhukov, Bruce C. Murray, E. V. Petrova
Publikováno v:
Planetary and Space Science. 39:311-326
A 0.3–0.6 (μm UV-visible spectrophotometer and a 5–50 μm radiometer in the KRFM experiment on Phobos 2 measured two groundtracks in the equatorial region of Phobos. Preliminary results indicate that three surface units can be recognized on the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c5b53a508ec6738bf9b9cd2a55d46059
https://doi.org/10.1016/0032-0633(91)90152-z
https://doi.org/10.1016/0032-0633(91)90152-z