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Circulation of Venusian Atmosphere at 90–110 km Based on Apparent Motions of the O2 1.27 μm Nightglow From VIRTIS‐M (Venus Express) Data

Geophysical research letters, 2018-03, Vol.45 (5), p.2554-2562

2018

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Resonant Orbits in the Problem of Expanding the Reachable Landing Areas on the Surface of Venus

Astronomy letters, 2021-05, Vol.47 (5), p.316-330

2021

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Winds From the Visible (513 nm) Images Obtained by the Venus Monitoring Camera Onboard Venus Express

Journal of geophysical research. Planets, 2022-04, Vol.127 (4), p.n/a

2022

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Thermal structure of Venusian nighttime mesosphere as observed by VIRTIS-Venus Express

Journal of Geophysical Research: Planets, 2010-09, Vol.115 (E9), p.n/a

2010

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Solar‐Related Variations of the Cloud Top Circulation Above Aphrodite Terra From VMC/Venus Express Wind Fields

Journal of geophysical research. Planets, 2019-07, Vol.124 (7), p.1864-1879

2019

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Phyllosilicates on Mars and implications for early martian climate

Nature, 2005-12, Vol.438 (7068), p.623-627

2005

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Near‐IR oxygen nightglow observed by VIRTIS in the Venus upper atmosphere

Journal of Geophysical Research - Planets, 2009-05, Vol.114 (E5), p.E00B38-n/a

2009

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Morphology and dynamics of Venus oxygen airglow from Venus Express/Visible and Infrared Thermal Imaging Spectrometer observations

Journal of Geophysical Research - Planets, 2008-05, Vol.113 (E5), p.E00B02-n/a

2008

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A warm layer in Venus' cryosphere and high-altitude measurements of HF, HCl, H2O and HDO

Nature (London), 2007-11, Vol.450 (7170), p.646-649

2007

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Structure of the Venus atmosphere

Planetary and space science, 2007-10, Vol.55 (12), p.1712-1728

2007

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Martian Atmospheric Thermal Structure and Dust Distribution During the MY 34 Global Dust Storm From ACS TIRVIM Nadir Observations

Journal of geophysical research. Planets, 2022-09, Vol.127 (9), p.n/a

2022

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First detection of hydroxyl in the atmosphere of Venus

Astronomy and astrophysics (Berlin), 2008-06, Vol.483 (3), p.L29-L33

2008

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Retrieval of air temperature profiles in the Venusian mesosphere from VIRTIS-M data: Description and validation of algorithms

Journal of Geophysical Research - Planets, 2008-09, Vol.113 (E9), p.E00B09-n/a

2008

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The nature of terrains of different types on the surface of Venus and selection of potential landing sites for a descent probe of the Venera-D Mission

Solar system research, 2017, Vol.51 (1), p.1-19

2017

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Estimates of abundance of the short-baseline (1-3 meters) slopes for different Venusian terrains using terrestrial analogues

Solar system research, 2017-03, Vol.51 (2), p.87-103

2017

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Planetary Fourier spectrometer data analysis: Fast radiative transfer models

Planetary and space science, 2005-08, Vol.53 (10), p.1035-1042

2005

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Methods for the analysis of data from the Planetary Fourier Spectrometer on the Mars Express Mission

Planetary and space science, 2005-08, Vol.53 (10), p.1017-1034

2005

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PFS/MEX observations of the condensing CO2 south polar cap of Mars

Icarus (New York, N.Y. 1962), 2008-10, Vol.197 (2), p.386-402

2008

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The Planetary Fourier Spectrometer (PFS) onboard the European Mars Express mission

Planetary and space science, 2005-08, Vol.53 (10), p.963-974

2005

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Modeling VIRTIS/VEX O2(a1∆g) nightglow profiles affected by the propagation of gravity waves in the Venus upper mesosphere

Journal of geophysical research. Planets, 2014-11, Vol.119 (11), p.2300-2316

2014

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The composition of the atmosphere of Venus below 100 km altitude: An overview

Planetary and space science, 2006-11, Vol.54 (13), p.1389-1397

2006

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Oxygen airglow emission on Venus and Mars as seen by VIRTIS/VEX and OMEGA/MEX imaging spectrometers

Planetary and space science, 2011-08, Vol.59 (10), p.981-987

2011

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Structure of the Venusian atmosphere from surface up to 100 km

Cosmic research, 2006-07, Vol.44 (4), p.364-383

2006

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Circulation of Venusian Atmosphere at 90–110 km Based on Apparent Motions of the O 2 1.27 μm Nightglow From VIRTIS‐M (Venus Express) Data

Geophysical research letters, 2018-03, Vol.45 (5), p.2554-2562

2018

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No detection of methane on Mars from early ExoMars Trace Gas Orbiter observations

Nature (London), 2019-04, Vol.568 (7753), p.517-520

2019

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Circulation of Venusian Atmosphere at 90–110 km Based on Apparent Motions of the O2 1.27 μm Nightglow From VIRTIS‐M (Venus Express) Data

Resonant Orbits in the Problem of Expanding the Reachable Landing Areas on the Surface of Venus

Winds From the Visible (513 nm) Images Obtained by the Venus Monitoring Camera Onboard Venus Express

Thermal structure of Venusian nighttime mesosphere as observed by VIRTIS-Venus Express

Solar‐Related Variations of the Cloud Top Circulation Above Aphrodite Terra From VMC/Venus Express Wind Fields

Phyllosilicates on Mars and implications for early martian climate

Near‐IR oxygen nightglow observed by VIRTIS in the Venus upper atmosphere

Morphology and dynamics of Venus oxygen airglow from Venus Express/Visible and Infrared Thermal Imaging Spectrometer observations

A warm layer in Venus' cryosphere and high-altitude measurements of HF, HCl, H2O and HDO

Structure of the Venus atmosphere

Martian Atmospheric Thermal Structure and Dust Distribution During the MY 34 Global Dust Storm From ACS TIRVIM Nadir Observations

First detection of hydroxyl in the atmosphere of Venus

Retrieval of air temperature profiles in the Venusian mesosphere from VIRTIS-M data: Description and validation of algorithms

The nature of terrains of different types on the surface of Venus and selection of potential landing sites for a descent probe of the Venera-D Mission

Estimates of abundance of the short-baseline (1-3 meters) slopes for different Venusian terrains using terrestrial analogues

Planetary Fourier spectrometer data analysis: Fast radiative transfer models

Methods for the analysis of data from the Planetary Fourier Spectrometer on the Mars Express Mission

PFS/MEX observations of the condensing CO2 south polar cap of Mars

The Planetary Fourier Spectrometer (PFS) onboard the European Mars Express mission

Modeling VIRTIS/VEX O2(a1∆g) nightglow profiles affected by the propagation of gravity waves in the Venus upper mesosphere

The composition of the atmosphere of Venus below 100 km altitude: An overview

Oxygen airglow emission on Venus and Mars as seen by VIRTIS/VEX and OMEGA/MEX imaging spectrometers

Structure of the Venusian atmosphere from surface up to 100 km

Circulation of Venusian Atmosphere at 90–110 km Based on Apparent Motions of the O 2 1.27 μm Nightglow From VIRTIS‐M (Venus Express) Data

No detection of methane on Mars from early ExoMars Trace Gas Orbiter observations

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