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Transport Characteristics of a Hierarchical Near-Surface Layer of the Nucleus of Comet 67P/Churyumov-Gerasimenko
DOI: 10.1134/S0038094622020071 Bibcode: 2022SoSyR..56..100R

Blum, J.; Hartogh, P.; Rezac, L. +3 more

In this paper, we develop previous studies that considered a free molecular gas flow through a dust porous mantle of a cometary nucleus. Before, we considered various types of both homogeneous and heterogeneous layers built of nonintersecting spheres, including the layers containing microscopic cracks and inner cavities. At the same time, data fro…

2022 Solar System Research
Rosetta 9
Spectral Signs of Simultaneous Sublimation Activity and the Appearance of a Dust Exosphere on Eight Asteroids of the Main Belt Near Perihelion
DOI: 10.1134/S0038094622020022 Bibcode: 2022SoSyR..56...84B

Shcherbina, M. P.; Busarev, V. V.; Savelova, A. A. +1 more

In December 2020, at the 2-m telescope of the Terskol branch of the Institute of Astronomy, we carried out spectrophotometric observations in the range of ~0.36-0.95 µm of nine asteroids of the Main Belt (19 Fortuna, 52 Europa, 102 Miriam, 177 Irma, 203 Pompeja, 250 Bettina, 266 Aline, 379 Huenna, and 383 Janina), which were near perihelia o…

2022 Solar System Research
SOHO 5
Simulation of Water Vapor Photodissociation during Dust Storm Season on Mars
DOI: 10.1134/S0038094622010051 Bibcode: 2022SoSyR..56...23S

Medvedev, A. S.; Rodin, A. V.; Shaposhnikov, D. S.

Within the framework of this work, using a three-dimensional numerical model of the general circulation of the Martian atmosphere MAOAM (Martian Atmosphere: Observation and Modeling), also known as MPI-MGCM (Max Planck Institute Martian General Circulation Model), we simulated the planet's hydrological cycle during the 28 and 34 Martian years (MY2…

2022 Solar System Research
ExoMars-16 2