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Dive into the research topics where Igor Khatuntsev is active.

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Featured researches published by Igor Khatuntsev.


Journal of Geophysical Research | 2016

Influence of Venus topography on the zonal wind and UV albedo at cloud top level: The role of stationary gravity waves.

Igor Khatuntsev; Alain Hauchecorne; W. J. Markiewicz; Emmanuel Marcq; Sebastien Lebonnois; Marina Patsaeva; Alexander Turin; Anna Fedorova

Based on the analysis of UV images (at 365 nm) of Venus cloud top (altitude 67 ± 2 km) collected with VMC (Venus Monitoring Camera) on board Venus Express (VEX), it is found that the zonal wind speed south of the equator (from 5°S to 15°S) shows a conspicuous variation (from -101 to -83 m/s) with geographic longitude of Venus, correlated with the underlying relief of Aphrodite Terra. We interpret this pattern as the result of stationary gravity waves produced at ground level by the up lift of air when the horizontal wind encounters a mountain slope. These waves can propagate up to the cloud top level, break there and transfer their momentum to the zonal flow. Such upward propagation of gravity waves and influence on the wind speed vertical profile was shown to play an important role in the middle atmosphere of the Earth by Lindzen [1981], but is not reproduced in the current GCM of Venus atmosphere from LMD. In the equatorial regions, the UV albedo at 365 nm varies also with longitude. We argue that this variation may be simply explained by the divergence of the horizontal wind field. In the longitude region (from 60° to -10°) where the horizontal wind speed is increasing in magnitude (stretch), it triggers air upwelling which brings the UV absorber at cloud top level and decreases the albedo, and vice-versa when the wind is decreasing in magnitude (compression). This picture is fully consistent with the classical view of Venus meridional circulation, with upwelling at equator revealed by horizontal air motions away from equator: the longitude effect is only an additional but important modulation of this effect. This interpretation is comforted by a recent map of cloud top H2O [Fedorova et al., 2015], showing that near the equator the lower UV albedo longitude region is correlated with increased H2O. We argue that H2O enhancement is the sign of upwelling, suggesting that the UV absorber is also brought to cloud top by upwelling.


Journal of Geophysical Research | 2009

Venus cloud top winds from tracking UV features in Venus Monitoring Camera images

Richard Moissl; Igor Khatuntsev; Sanjay S. Limaye; D. V. Titov; Wojciech J. Markiewicz; Nikolay Ignatiev; Thomas Roatsch; Klaus-Dieter Matz; R. Jaumann; Miguel Almeida; Ganna Portyankina; Thomas Behnke; S. F. Hviid


Icarus | 2013

Cloud level winds from the Venus Express Monitoring Camera imaging

Igor Khatuntsev; M. V. Patsaeva; D. V. Titov; N. I. Ignatieva; A. V. Turina; Sanjay S. Limaye; Wojciech J. Markiewicz; Miguel Almeida; Thomas Roatsch; Richard Moissl


Space Science Reviews | 2018

The Atmospheric Chemistry Suite (ACS) of Three Spectrometers for the ExoMars 2016 Trace Gas Orbiter

Oleg Korablev; Franck Montmessin; Alexander Trokhimovskiy; Anna Fedorova; A. Shakun; A. V. Grigoriev; B. Moshkin; Nikolay Ignatiev; Francois Forget; Franck Lefèvre; K. Anufreychik; I. Dzuban; Yuriy S. Ivanov; Yurii K. Kalinnikov; Tatiana O. Kozlova; A. Kungurov; V. Makarov; F. Martynovich; I. Maslov; D. Merzlyakov; Pavel P. Moiseev; Y. Nikolskiy; Andrei Patrakeev; D. Patsaev; A. Santos-Skripko; O. Sazonov; N. Semena; A. Semenov; V. Shashkin; A. Sidorov


European Space Agency, (Special Publication) ESA SP | 2004

PFS: The planetary Fourier spectrometer for mars express

Vittorio Formisano; D. Grassi; R. Orfei; D. Blondi; E. Mencarelli; A. Mattana; F. Nespoli; A. Maturilli; M. Giuranna; M. Rossi; M. Maggi; P. Baldetti; G. Chionchio; Bortolino Saggin; F. Angrilli; G. Bianchini; Giuseppe Piccioni; A. M. Di Lellis; P. Cerroni; F. Capaccioni; M. T. Capria; A. Coradini; S. Fonti; V. Orofino; A. Blanco; L. Colangeli; E. Palomba; F. Esposito; D. Patsaev; V.I. Moroz


Journal of Geophysical Research | 2017

Winds in the Middle Cloud Deck From the Near‐IR Imaging by the Venus Monitoring Camera Onboard Venus Express

Igor Khatuntsev; Marina Patsaeva; Dmitrij V. Titov; Nikolay Ignatiev; Alexander Turin; Anna Fedorova; Wojciech J. Markiewicz


Journal of Geophysical Research | 2016

Influence of Venus topography on the zonal wind and UV albedo at cloud top level: The role of stationary gravity waves: GEOGRAPHIC MAPPING OF VENUS WIND/ALBEDO

Igor Khatuntsev; Alain Hauchecorne; W. J. Markiewicz; Emmanuel Marcq; Sebastien Lebonnois; Marina Patsaeva; Alexander Turin; Anna Fedorova


Mars Express: The Scientific Investigations | 2009

PFS: Planetary fourier spectrometer

V. Formisano; F. Angrilli; Gabriele Arnold; Sushil K. Atreya; G. Bianchini; D. Biondi; M. I. Blecka; Angioletta Coradini; L. Colangeli; V. Cottini; A. Ekonomov; Th. Encrenaz; F. Esposito; C. Fiorenza; S. Fonti; Marco Giuranna; D. Grassi; V. Gnedykh; Anatoly I. Grigoriev; Gary B. Hansen; H. Hirsh; Igor Khatuntsev; N. h Ignatiev; A. Jurewicz; E. Lellouch; J. J. Lopez Moreno; A. Mattana; Alessandro Maturilli; M. Michalska; B. Moshkin


Journal of Geophysical Research | 2017

Winds in the Middle Cloud Deck From the Near-IR Imaging by the Venus Monitoring Camera Onboard Venus Express: Winds in the Middle Cloud Deck of Venus

Igor Khatuntsev; Marina Patsaeva; Dmitrij V. Titov; Nikolay Ignatiev; Alexander Turin; Anna Fedorova; W. J. Markiewicz


Japan Geoscience Union | 2017

The Venera-D Mission Concept for Exploring Venus

L. V. Zasova; David Senske; Sanjay S. Limaye; Thomas Economou; Natan Eismont; M. Gerasimov; M Ivanov; Nikolay Ignatiev; Kandi Lea Jessup; Igor Khatuntsev; Oleg Korablev; Tibor Kremic; I Lomakin; M. Martynov; Adriana Ocampo

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Sanjay S. Limaye

University of Wisconsin-Madison

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Anna Fedorova

Moscow Institute of Physics and Technology

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L. V. Zasova

Russian Academy of Sciences

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