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)
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)
Application deadline 1 October 2024. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...
In analyzing solar observations from the 19th century, scientists are turning to amateur researchers for help. The project will allow to better understand the history of our star.
Astronomical teamwork: By combining data from Solar Orbiter and SDO, a group of researchers has unambiguously determined the magnetic field at the solar surface.
Application deadline 1 October 2023. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...
Philipp Löschl has co-authored an excellent publication on Solar Orbiter data which has been awarded best Solar Physics paper of 2022 (Gherardo Valori et al. 2022)