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)
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)
The Planetary Plasma Environments group (PPE) has a strong heritage in the exploration of planetary magnetospheres and space plasma interactions throughout the solar system. It has contributed instruments to several past missions that flew-by or orbited Jupiter (Galileo, Cassini, Ulysses). The PPE participates in the JUICE mission by contributing hardware and scientific expertise to the Particle Environment Package (PEP).
Application deadline 1 October 2024. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...
Call for applications: PhD positions in planetary science, solar physics, stellar physics, with a starting date in September 2024, at the IMPRS in Göttingen.