Smitha, H. N.; Holzreuter, R.; van Noort, M.; Solanki, S. K.: The influence of NLTE effects in Fe I lines on an inverted atmosphere: II. 6301 Å and 6302 Å lines formed in 3D NLTE. Astronomy and Astrophysics 647, A46 (2021)
Smitha, H. N.; Holzreuter, R.; van Noort, M.; Solanki, S. K.: The influence of NLTE effects in Fe I lines on an inverted atmosphere: I. 6301 Å and 6302 Å lines formed in 1D NLTE. Astronomy and Astrophysics 633, A157 (2020)
Smitha, H. N.; Solanki, S. K.: Probing the photospheric magnetic fields with new spectral line pairs. Annual Meeting of the Astronomische Gesellschaft 2017 , Göttingen, Germany (2017)
Smitha, H. N.; Anusha, L. S.; Solanki, S. K.; Riethmueller, T. L.: Flux emergence rate in the quiet Sun from SUNRISE data. SOLARNET IV, The Physics of the Sun from the Interior to the Outer Atmosphere, Lanzarote, Spain (2017)
The dwarf planet is a bizarre, cryovolcanic world. However, the organic deposits discovered on its surface so far are unlikely to originate from its interior.
The Uranian magnetic field is more expansive than previously thought, according to newly analyzed data from Voyager 2, making it easier to search for moons with oceans.
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).