Publications of Oksana Shalygina

Korokhin, V.; Surkov, Y.; Mall, U.; Kaydash, V.; Velichko, S.; Velikodsky, Y.; Shalygina, O.: Applying machine learning to a nonlinear spectral mixing model for mapping lunar soils composition using CHANDRAYAAN-1 M³ data. Planetary and Space Science 244, p. 105870 (2024)

Shalygina, O.; Shalygin, E. V.; Ignatiev, N. I.; Petrova, E. V.: Comment on "Long-term Variations of Venus's 365 nm Albedo Observed by Venus Express, Akatsuki, MESSENGER, and the Hubble SpaceTelescope" by Lee et al. (2019, AJ, 158, 126). Research notes of the AAS 3 (11), 168 (2020)

Basilevsky, A. T.; Shalygin, E. V.; Bondarenko, N.V.; Shalygina, O.; Markiewicz, W. J.: Venus crater-related radar-dark parabolas and neighboring terrains: A comparison of 1-μm emissivity and microwave properties. Icarus 330, pp. 103 - 122 (2019)

Markiewicz, W. J.; Petrova, E.; Shalygina, O.: Aerosol properties in the upper clouds of Venus from glory observations by the Venus Monitoring Camera (Venus Express mission). Icarus 299, pp. 272 - 293 (2018)

Petrova, E. V.; Shalygina, O. S.; Markiewicz, W. J.: UV contrasts and microphysical properties of the upper clouds of Venus from the UV and NIR VMC/VEx images. Icarus 260, pp. 190 - 204 (2015)

Petrova, E. V.; Shalygina, O. S.; Markiewicz, W. J.: The VMC/VEx photometry at small phase angles: Glory and the physical properties of particles in the upper cloud layer of Venus. Planetary and Space Science 113, pp. 120 - 134 (2015)

Shalygina, O. S.; Petrova, E. V.; Markiewicz, W. J.; Ignatiev, N. I.; Shalygin, E. V.: Optical properties of the Venus upper clouds from the data obtained by Venus Monitoring Camera on-board the Venus Express. Planetary and Space Science 113, pp. 135 - 158 (2015)

Markiewicz, W. J.; Petrova, E.; Shalygina, O.; Almeida, M.; Titov, D. V.; Limaye, S. S.; Ignatiev, N.; Roatsch, T.; Matz, K.-D.: Glory on Venus cloud tops and the unknown UV absorber. Icarus 234, pp. 200 - 203 (2014)

Petrova, E. V.; Markiewicz, W. J.; Shalygina, O. S.: The latitude gradient of droplet sizes of the upper Venus clouds at 35-60S from the VMC/VEx observations. 40th COSPAR Scientific Assembly, Moscow, Russia (2014)