Physics
Scientist
Space Research Institute RAS
INAF-IFSI, Via del Fosso del Cavaliere, 00144 Rome, Italy; IKI-RAS, Profsojuznaja 84 / 32, 117997 Moscow, Russia
INAF-IFSI, Via del Fosso del Cavaliere, 00144 Rome, Italy; IKI-RSSI, Profsojuznaja 84 / 32, 117997 Moscow, Russia
IKI RAS
Space Research Institute, Russian Academy of Sciences, Profsoyusnaya 84 / 32, 117810 Moscow, Russia
Space Research Institute of the Russian Academy of Science, Profsoyusnaya 84 / 32, 117810 Moscow, Russia
Joint Publications Research Service, Arlington, VA.
Space Research Institute, Russian Academy of Sciences, Moscow, Russia
IKI - RAS, Moscow, Russia, IFSI - INAF, Rome, Italy
IKI-RSSI, Moscow, Russia and IFSI-INAF, Rome, Italy
Space Research Institute of Russian Academy of Sciences, Profsoyuznaya 84 / 32, 117810 Moscow, Russia, RU
Space Research Institute, Russian Academy of Sciences;, Instituto di Fisica dello Spazio Interplanetario INAF-IFSI
Akademiia Nauk SSSR, Institut Kosmicheskikh Issledovanii, Moscow, USSR
National Aeronautics and Space Administration, Washington, DC.
Space Research Institute, Moscow
Russian Academy of Sciences, Moscow, Russia
Space Research Institute, IKI RAS, Planetary Physics and Small Bodies in the Solar System, Moscow, Russian Federation
IKI RAS, Moscow, Russia
Space Research Institute, IKI RAS, Moscow, Russian Federation
Russian Academy of Sciences, Space Research Institute, Moscow, Russia
Space Research Institute, Russian Academy of Sciences, Profsoyuznaya 84 / 32, 117997 Moscow, Russia; IFSI CNR, via Fosso del Cavaliere 100, 00133 Rome, Italy
IKI RAS, Moscow, Russia; IFSI INAF, Rome, Italy
A New Analysis of the Spectra Obtained by the Venera Missions in the Venusian Atmosphere. I. The Analysis of the Data Received from the Venera-11 Probe at Altitudes Below 37 km in the 0.44 0.66 µm Wavelength Range
A new interpretation of the Venera 11 spectra of Venus. I - The 0.94 micron water band
AOST: Fourier spectrometer for studying mars and phobos
Application of the method of discrete ordinates to the solution of the transfer equation in the case of an inhomogeneous planetary atmosphere
Application of the method of discrete ordinates to the solution of the transport equation in the case of an inhomogeneous planetary atmosphere
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