Zobrazeno 1 - 10
of 18
pro vyhledávání: '"Yu.V. Nikolsky"'
Autor:
R. Orfei, G. Bianchini, V. Gnedykh, Piotr Orleanski, A. P. Ekonomov, Giuseppe Piccioni, Vittorio Formisano, M. T. Capria, D. Patsaev, G. Chionchio, Yu.V. Nikolsky, N. Cafaro, Luigi Colangeli, H. Driesher, B. E. Moshkin, D. V. Titov, Francesco Angrilli, A. Russakov, Gabriele Arnold, A. Kiselev, A. M. Di Lellis, Sergio Fonti, Ernesto Palomba, Priscilla Cerroni, M. Michalska, L. V. Zasova, M. I. Blecka, Igor Khatuntsev, V. I. Moroz, W. Novosielski, J. J. López-Moreno, Fabrizio Capaccioni, Rafael Rodrigo, Angioletta Coradini, A. Grigorlev, G. Michel, Bortolino Saggin, Julio Rodriguez-Gomez, I. A. Matsygorin, V. Nechaev, H. Hirsch, E. Bussoletti, A. Jurewicz
Publikováno v:
Advances in Space Research. 19:1277-1280
The Planetary Fourier Spectrometer PFS has been designed for the study of the atmosphere and soil of Mars. PFS has two infrared channels: a long wavelength (LW) channel with range 250 - 2000 cm-’ and a short wavelength (SW) channel with range 2000
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::bd59d670c403307d3a0d717daab7a45e
https://doi.org/10.1016/s0273-1177(97)00282-2
https://doi.org/10.1016/s0273-1177(97)00282-2
Autor:
H. Hirsch, Julio Rodriguez-Gomez, L. V. Zasova, G. Michel, I. A. Matsygorin, Alberto Adriani, H. Driesher, Anatoly I. Grigoriev, M. I. Blecka, Priscilla Cerroni, Vittorio Formisano, Igor Khatuntsev, V. I. Moroz, Yu.V. Nikolsky, D. Mancini, Bortolino Saggin, Rafael Rodrigo, A. Kiselev, Gabriele Arnold, G. Chionchio, D. V. Titov, Sergio Fonti, E. Bussoletti, V. Gnedykh, Luigi Colangeli, Piotr Orleanski, G. Bianchini, Giuseppe Piccioni, Giancarlo Bellucci, E. Amata, B. E. Moshkin, M. Vitterbini, Angioletta Coradini, M. T. Capria, D. Patsaev, J. J. López-Moreno, Fabrizio Capaccioni, A. Carusi, Francesco Angrilli
Publikováno v:
Advances in Space Research. 17:61-64
PFS (the Planetary Fourier Spectrometer) covers the range 1.25 – 45 μm with spectral resolution about 2 cm−1 and angular resolution 0.035 – 0.070 rad (10 – 20 km on the Martian surface working at the periapsis). The instrument has two spectr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a6fb31646528c627527d6e3c38db608e
https://doi.org/10.1016/0273-1177(95)00759-8
https://doi.org/10.1016/0273-1177(95)00759-8
Autor:
A. V. Zharkov, Yu.V. Nikolsky, Marco Giuranna, Giancarlo Bellucci, Franck Montmessin, Igor Khatuntsev, A. B. Gvozdev, Alexey Shakun, Alexander Rodin, D. Patsaev, V. S. Makarov, Oleg Korablev, Ruslan O. Kuzmin, Nikolay Ignatiev, Anna Fedorova, A. V. Grigor’ev, G. Arnold, B. S. Mayorov, L. V. Zasova, B. E. Moshkin, S. V. Maksimenko, Alexander I. Terentiev, Viktor Shashkin
Publikováno v:
Astronomicheskii Vestnik / Solar System Research
Astronomicheskii Vestnik / Solar System Research, MAIK Nauka/Interperiodica, 2012, 46 (1), pp.31-40. ⟨10.1134/S0038094611060050⟩
Astronomicheskii Vestnik / Solar System Research, 2012, 46 (1), pp.31-40. ⟨10.1134/S0038094611060050⟩
Astronomicheskii Vestnik / Solar System Research, MAIK Nauka/Interperiodica, 2012, 46 (1), pp.31-40. ⟨10.1134/S0038094611060050⟩
Astronomicheskii Vestnik / Solar System Research, 2012, 46 (1), pp.31-40. ⟨10.1134/S0038094611060050⟩
International audience; An AOST Fourier spectrometer of the Phobos-Soil project is intended for studying Mars and Phobos by means of measurements of IR radiation spectra of the Martian surface and atmosphere, the Phobos surface, and the spectrum of s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3ea3f66b6208cd4f4810c34c0903daff
https://hal.archives-ouvertes.fr/hal-00672955
https://hal.archives-ouvertes.fr/hal-00672955
Autor:
Igor Khatuntsev, G. Fanti, G. Chionchio, Priscilla Cerroni, Francesco Angrilli, Anatoly I. Grigoriev, Rafael Rodrigo, N. Sanko, M. Combes, D. Mancini, P. Orleansky, Alberto Adriani, A. Matteuzzi, Giuseppe Piccioni, L. Colangeli, E. Amata, Fabrizio Capaccioni, A. Carusi, Vittorio Formisano, D. V. Titov, Giancarlo Bellucci, Sergio Fonti, M. Viterbini, Angioletta Coradini, Yu.V. Nikolsky, B. E. Moshkin, G. Bianchini, R. Orfei, V. Gnedykh, I. Olivares, A. Kiselev, E. Bussoletti, P. Baglioni, J. Rodríguez Gómez, S. Goncharov, G. Michel, H. Hirsh, L. V. Zasova, P. Baldetti, J. J. Lopez Moreno, Gabriele Arnold, V. I. Moroz
Publikováno v:
Il Nuovo Cimento C. 16:575-588
PFS is a two-channel Fourier spectrometer operating in the infra-red wavelengths between 1.25 and 45 μm. The instrument will be used mainly in the study of the Martian atmosphere. The principal goals are the measurements of the atmospheric temperatu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9aa30ed1865b60912085898c33e5a3f8
https://doi.org/10.1007/bf02512038
https://doi.org/10.1007/bf02512038
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:
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:
Alessandro Maturilli, Yu.V. Nikolsky, D. Patsaev, Alexey Grigoriev, B. E. Moshkin, H. Hirsh, Giuseppe Piccioni, Giancarlo Bellucci, Bortolino Saggin, Marco Giuranna, L. V. Zasova, Francesca Altieri, M. I. Blecka, A. P. Ekonomov, Sergio Fonti, Jean-Pierre Bibring, A. Mattana, Vittorio Formisano, Nikolay Ignatiev, Davide Grassi, M. Ratai, Emmanuel Lellouch, Igor Khatuntsev, V. I. Moroz, V. Gnedykh
Publikováno v:
Cosmic Research / Kosmicheskie Issledovaniya
Cosmic Research / Kosmicheskie Issledovaniya, 2006, 44, pp.305-316. ⟨10.1134/S0010952506040046⟩
Politecnico di Milano-IRIS
Cosmic Research / Kosmicheskie Issledovaniya, 2006, 44, pp.305-316. ⟨10.1134/S0010952506040046⟩
Politecnico di Milano-IRIS
We discuss the results of measurements made with the Planetary Fourier Spectrometer (PFS) onboard the Mars Express spacecraft. The data were obtained in the beginning of the mission and correspond to the end of summer in the southern hemisphere of Ma
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ba3b2aa64d2c391c49a3d9101d455c7e
http://hdl.handle.net/11311/244507
http://hdl.handle.net/11311/244507
Autor:
M. Combes, C. Emerich, J. M. Lamarre, N. F. Sanko, Yu.V. Nikolsky, J. Crovisier, F. Rocard, T. Encrenaz, N. Coron, R. Gispert, J. P. Bibring, V. I. Moroz
Publikováno v:
Advances in Space Research
Advances in Space Research, Elsevier, 1985, 5, pp.123-126
Advances in Space Research, Elsevier, 1985, 5, pp.123-126
The Infrared thermal emission of the nucleus has been observed by the imaging channel of the infrared spectrometer IKS during the fly-by of Comet Halley by the VEGA 1 probe. An emissive region with a temperature in excess of 300 K has been detected.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f3cd2cc777b4fffb77733ab6e056066b
http://hal.in2p3.fr/in2p3-00002076
http://hal.in2p3.fr/in2p3-00002076
Autor:
Yu.V. Nikolsky, A.V. Dyachkov, Ph. Masson, L.V. Ksanfomality, C. Cara, Olivier Forni, N.G. Havinson, A. Kiselev, Pierre Drossart, Yves Langevin, Emmanuel Lellouch, M. Combes, A. Soufflot, B. Gondet, Christophe Sotin, J. P. Bibring, I. V. Khatuntsev, V. I. Moroz, J. Rosenqvist, A.V. Grygoriev, Stéphane Erard, T. Encrenaz
Publikováno v:
Scopus-Elsevier
The measurement of the CO 2 column density on Mars, from the 2 μm band, in the Phobos /ISM spectra allows the determination of the altitude of the surface of Mars, with a horizontal spatial resolution of 20 km. The uncertainties involved in this met
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::11c4a21dbe37e6b54c1bd57f3bdee263
http://www.scopus.com/inward/record.url?eid=2-s2.0-0000296167&partnerID=MN8TOARS
http://www.scopus.com/inward/record.url?eid=2-s2.0-0000296167&partnerID=MN8TOARS
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