L. Zasova

发表

South-polar features on Venus similar to those near the north pole

T. Encrenaz, S. Erard, P. Drossart, 2007, Nature.

A dynamic upper atmosphere of Venus as revealed by VIRTIS on Venus Express

S. Erard, L. Marinangeli, B. Saggin, 2007, Nature.

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

N. Ignatiev, I. Khatuntsev, L. Zasova, 2022, Journal of Geophysical Research: Planets.

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

G. Piccioni, I. Khatuntsev, L. Zasova, 2018 .

Radiation in the Atmosphere of Venus

D. Crisp, D. Titov, N. Renno, 2013 .

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

M. A. Ivanov, O. Korablev, N. Ignatiev, 2017, Solar System Research.

Studies of the planetary atmospheres in Russia (2007–2010)

Anna Fedorova, Oleg Korablev, Alexander V. Rodin, 2012, Izvestiya, Atmospheric and Oceanic Physics.

First detection of hydroxyl in the atmosphere of Venus

Giuseppe Piccioni, Franklin P. Mills, Alessandra Migliorini, 2008 .

Structure of the Venus atmosphere

V. M. Linkin, N. Ignatiev, L. Zasova, 2007 .

New in the physics of planetary atmosphere

A. Fedorova, O. Korablev, N. Ignatiev, 2009 .

Mount Etna as a terrestrial laboratory to investigate recent volcanic activity on Venus by future missions: A comparison with Idunn Mons, Venus

L. Zasova, S. Bhiravarasu, M. E. Yazidi, 2024, Icarus.

O2 (а1Δg) Airglow at 1.27 μM and upper Mesosphere Dynamics on the Night Side of Venus

N. Ignatiev, I. Khatuntsev, L. Zasova, 2023, Solar System Research.