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.: 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)
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 Sun’s planets and small objects have undergone substantial evolution. Deciphering the history of our cosmic home is not a simple task even though we now have access to a multitude of data gathered by space missions, remote observations, and laboratory studies of diverse samples. A significant fraction of materials available for the study of planetary bodies come from meteorites.
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).
The Solar Lower Atmosphere and Magnetism (SLAM) group covers many exciting subjects in solar physics, focussing on the development and testing of highly novel solar instrumentation, reduction and analysis of highest quality solar observations, or improving and developing advanced techniques for the analysis of solar observations.
Inversion codes are used to aid the detailed interpretation of solar spectro-polarimetric data. This computer code attempts to find the atmospheric structure that produced an observed spectrum by minimizing the difference between the observed spectrum and a Stokes spectrum.
The MPS is one of the leading institutes worldwide in building instruments for solar research, both for ground based observatories as well as for balloon and space-borne missions. Scientists and engineers of MPS conceive new observing methods and develop novel instruments of highest technological complexity. These instruments are built in house, tested, calibrated, and used at the best solar observatories in the world, or delivered to NASA and ESA to be launched to space.