Farkas-Takács, A.; Kiss, C.; Vilenius, E.; Marton, G.; Müller, T. G.; Mommert, M.; Stansberry, J.; Lellouch, E.; Lacerda, P.; Pál, A.: “TNOs are Cool”: A survey of the trans-Neptunian region XV. Physical characteristics of 23 resonant trans-Neptunian and scattered disk objects. Astrophysics & Astronomy 638, A23 (2020)
Sorsa, L.-I.; Takala, M.; Bambach, P.; Deller, J.; Vilenius, E.; Pursiainen, S.: Bistatic Full-wave Radar Tomography Detects Deep Interior Voids, Cracks, and Boulders in a Rubble-pile Asteroid Model. The Astrophysical Journal 872 (1), A44 (2019)
Takala, M.; Bambach, P.; Deller, J.; Vilenius, E.; Wittig, M.; Lentz, H.; Braun, H. M.; Kaasalainen, M.; Pursiainen, S.: Far-Field Inversion for the Deep Interior Scanning CubeSat. IEEE Transactions on Aerospace and Electronic Systems 55 (4), pp. 1683 - 1697 (2019)
Bambach, P.; Deller, J.; Vilenius, E.; Pursiainen, S.; Takala, M.; Braun, H. M.; Lentz, H.; Wittig, M.: DISCUS – The Deep Interior Scanning CubeSat mission to a rubble pile near-Earth asteroid. Advances in Space Research 62 (12), pp. 3357 - 3368 (2018)
Vilenius, E.; Stansberry, J.; Müller, T.; Mueller, M.; Kiss, C.; Santos-Sanz, P.; Mommert, M.; Pál, A.; Lellouch, E.; Ortiz, J. L.et al.; Peixinho, N.; Thirouin, A.; Lykawka, P. S.; Horner, J.; Duffard, R.; Fornasier, S.; Delsanti, A.: “TNOs are Cool”: A survey of the trans-Neptunian region XIV. Size/albedo characterization of the Haumea family observed with Herschel and Spitzer. Astronomy and Astrophysics 618, A136 (2018)
Kovalenko, I. D.; Doressoundiram, A.; Lellouch, E.; Vilenius, E.; Müller, T.; Stansberry, J.: “TNOs are Cool”: A survey of the trans-Neptunian region XIII. Statistical analysis of multiple trans-Neptunian objects observed with Herschel Space Observatory. Astronomy and Astrophysics 608, A19 (2017)
Santos-Sanz, P.; French, R. G.; Pinilla-Alonso, N.; Stansberry, J.; Lin, Z.-Y.; Zhang, Z.-W.; Vilenius, E.; Müller, T.; Ortiz, J. L.; Braga-Ribas, F.et al.; Bosh, A.; Duffard, R.; Lellouch, E.; Tancredi, G.; Young, L.; Milam, S. N.; Group, t. J. O. F.: James Webb Space Telescope Observations of Stellar Occultations by Solar System Bodies and Rings. Publications of the Astronomical Society of the Pacific 128, 018011 (2015)
Takala, M.; Bambach, P.; Deller, J.; Vilenius, E.; Wittig, M.; Lentz, H.; Braun, H. M.; Pursiainen, S.: CubeSat Based Radio Tomography for a Rubble Pile Asteroid: DISCUS Mission Concept. In: 2018 2nd URSI Atlantic Radio Science Meeting (AT-RASC). 2nd URSI AT-RASC, Gran Canaria, Spain, May 28, 2018 - June 01, 2018. (2018)
Farkas Anikó, T.; Kiss, C.; Mueller, T. G.; Mommert, M.; Vilenius, E.: Properties of resonant trans-Neptunian objects based on Herschel Space Observatory data. AAS/Division for Planetary Sciences Meeting Abstracts 48, 113.06, (2016)
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.