I. E. Stepanova
Russian Academy of Sciences
11 Papers
3 Citations
I. E. Stepanova is an academic researcher from Russian Academy of Sciences. The author has contributed to research in topics: Mars Exploration Program & Inverse problem. The author has an hindex of 2, co-authored 10 publications.
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Papers
Crust stratigraphy and heterogeneities of the first kilometers at the dichotomy boundary in western Elysium Planitia and implications for InSight lander
Lu Pan,C. Quantin-Nataf,Benoit Tauzin,Benoit Tauzin,Chloé Michaut,Matthew P. Golombek,P. H. Lognonné,Peter Grindrod,Benoit Langlais,Tamara Gudkova,I. E. Stepanova,Sebastien Rodriguez,Antoine Lucas +12 more
TL;DR: In this paper, the authors investigate the subsurface structure and composition from the analysis of mineralogy and morphology of exposures in impact craters as well as on scarps and knobs in the general region of Elysium Planitia.
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Density Anomalies in Subsurface Layers of Mars: Model Estimates for the Site of the InSight Mission Seismometer
TL;DR: In this article, a model distribution of anomalous masses in the southwestern part of Elysium Planitia under the surface of the site of the InSight mission seismometer has been obtained.
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Analytical Modeling of the Magnetic Field of Mars from Satellite Data Using Modified S-Approximations
TL;DR: An analytical model of the magnetic field over the Martian surface in the southwestern part of the Elysium Planitia is constructed using satellite data and modified S-approximations within the framework of the structural-parametric approach as mentioned in this paper.
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Recovering the Magnetic Image of Mars from Satellite Observations.
TL;DR: One of the possible approaches to reconstructing the map of the distribution of magnetization parameters in the crust of Mars from the data of the Mars MAVEN orbiter mission is considered in this article.
10
Recovering the Near-Surface Magnetic Image of Mercury from Satellite Observations
TL;DR: In this article , a new technique for reconstructing the magnetic image of Mercury from satellite observation data is proposed, which is based on extracting from the general observational data only the part that is associated with magnetic field sources concentrated in Mercury's crust.