Rodriguez, J. d. l. C.; van Noort, M.: Radiative Diagnostics in the Solar Photosphere and Chromosphere. Space Science Reviews 210 (1-4), pp. 109 - 143 (2017)
Siu-Tapia, A. L.; Lagg, A.; Solanki, S. K.; van Noort, M.; Jurčák, J.: Normal and counter Evershed flows in the photospheric penumbra of a sunspot: SPINOR 2D inversions of Hinode-SOT/SP observations. Astronomy and Astrophysics 607, A 36 (2017)
Danilovic, S.; Rempel, M.; van Noort, M.; Cameron, R.: Observed and simulated power spectra of kinetic and magnetic energy retrieved with 2D inversions. Astronomy and Astrophysics 594, A103 (2016)
Danilovic, S.; van Noort, M.; Rempel, M.: Internetwork magnetic field as revealed by two-dimensional inversions. Astronomy and Astrophysics 593, A93 (2016)
Tiwari, S. K.; van Noort, M.; Solanki, S. K.; Lagg, A.: Depth-dependent global properties of a sunspot observed by Hinode using the Solar Optical Telescope/Spectropolarimeter. Astronomy and Astrophysics 583, A119 (2015)
Rodriguez, J. d. l. C.; van der Voort, L. R.; Socas-Navarro, H.; van Noort, M.: Physical properties of a sunspot chromosphere with umbral flashes. Astronomy and Astrophysics 556, A115 (2013)
Schnerr, R. S.; Rodriguez, J. d. l. C.; van Noort, M.: Stokes imaging polarimetry using image restoration: a calibration strategy for Fabry-Perot based instruments. Astronomy and Astrophysics 534, A45 (2011)
Scharmer, G. B.; Narayan, G.; Hillberg, T.; Rodriguez, J. d. l. C.; Loefdahl, M. G.; Kiselman, D.; Suetterlin, P.; van Noort, M.; Lagg, A.: Crisp Spectropolarimetric Imaging of Penumbral Fine Structure. Astrophysical Journal 689 (1), pp. L69 - L72 (2008)
van Noort, M.; Rouppe van der Voort, L. H. M.: Stokes imaging polarimetry using image restoration at the Swedish 1-m solar telescope. Astronomy and Astrophysics 489, pp. 429 - 440 (2008)
Löptien, B.; Lagg, A.; van Noort, M.; Solanki, S. K.: Relating the magnetic field strength with the umbra-penumbra boundary in sunspots. SolarPolarization Workshop 9, Göttingen, Germany (2019)
The research group “Solar Lower Atmosphere and Magnetism” (SLAM) studies the conditions and dynamic processes in the atmospheric layer between the solar surface (photosphere) and the overlying chromosphere, an approximately 2000 km thick gas layer.
The main research fields of the department "Sun and Heliosphere" are covered by the research groups "Solar and Stellar Coronae", "Solar Lower Atmosphere and Magnetism", "Solar and Stellar Magnetohydrodynamics" and "Solar Variability and Climate".
How does our star heat its outer atmosphere, the solar corona, to unimaginable temperatures of up to 10 million degrees Celsius? With unprecedented observational data from ESA's Solar Orbiter spacecraft and powerful computer simulations, ERC starting grant awardee Pradeep Chitta intends to bring new momentum to the search for the coronal heating mechanism.