Chae, J.; van Noort, M.; Madjarska, M. S.; Lee, K.; Kang, J.; Cho, K.: Large-amplitude transverse MHD waves prevailing in the Hα chromosphere of a solar quiet region revealed by MiHI integrated field spectral observations. Astronomy and Astrophysics 687, p. A249 (2024)
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)
Rouppe van der Voort, L. H. M.; van Noort, M.; de la Cruz Rodríguez, J.: Ultra-high-resolution observations of plasmoid-mediated magnetic reconnection in the deep solar atmosphere. Astronomy and Astrophysics 673, p. A11 (2023)
van Noort, M.; Doerr, H. -.: Data reduction and restoration of spectropolarimetric microlensed hyperspectral imager data. Astronomy and Astrophysics 668, p. A151 (2022)
Saranathan, S.; van Noort, M.; Solanki, S. K.: Correction of atmospheric stray light in restored slit spectra. Astronomy and Astrophysics 653, A17 (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: II. 6301 Å and 6302 Å lines formed in 3D NLTE. Astronomy and Astrophysics 647, A46 (2021)
Löptien, B.; Lagg, A.; van Noort, M.; Solanki, S. K.: No universal connection between the vertical magnetic field and the umbra-penumbra boundary in sunspots. Astronomy and Astrophysics 639, A106 (2020)
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)
Images from ESA’s Solar Orbiter offer the best look yet at a source region of the solar wind - and challenge our view of the continuous particle stream from the Sun.
Deciphering the magnetic origins of the Sun's hot corona: developing a framework for coronal heating by probing the elusive photosphere-corona connection
Using unique observational data and computer simulations, the MPS scientist is striving to understand the incredibly hot temperatures in the solar corona.
For the first time, images of the Sun have been taken from a distance of only 77 million kilometres enabling a completely new view of our star possible.
In his doctoral thesis, Sudip Mandal investigated how special pressure waves help maintain temperatures of several million degrees in the outermost solar atmosphere.