Chitta, L. P.; van Noort, M.; Smitha, H. N.; Priest, E.R.; van der Voort, L.H.M.R.: Photospheric Hot Spots at Solar Coronal Loop Footpoints Revealed by Hyperspectral Imaging Observations. ASTROPHYSICAL JOURNAL (1) (2024)
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)
Analyzing the high spatial resolution solar Ca II H and K emission data obtained by the SUNRISE mission and building a model of other stars more active than the Sun
First Light for Sunrise III: the first tests with real sunlight were successful. The balloon-borne solar observatory should be ready for launch at the end of May.
First icy cold, then midnight sun: at the Arctic Circle, the team will prepare the next flight of the balloon-borne solar observatory - and hopes for solar fireworks.
Astronomical teamwork: By combining data from Solar Orbiter and SDO, a group of researchers has unambiguously determined the magnetic field at the solar surface.