Chen, Y.; Mandal, S.; Peter, H.; Chitta, L. P.: Bidirectional propagating brightenings in arch filament systems observed by Solar Orbiter/EUI. Astronomy and Astrophysics 692, p. A119 (2024)
Chitta, L. P.; Zhukov, A. N.; Berghmans, D.; Peter, H.; Parenti, S.; Mandal, S.; Aznar Cuadrado, R.; Schühle, U.; Teriaca, L.; Auchère, F.et al.; Barczynski, K.; Buchlin, É.; Harra, L.; Kraaikamp, E.; Long, D. M.; Rodriguez, L.; Schwanitz, C.; Smith, P. J.; Verbeeck, C.; Seaton, D. B.: Picoflare jets power the solar wind emerging from a coronal hole on the Sun. Science 38, pp. 867 - 872 (2023)
Lim, D.; Van Doorsselaere, T.; Berghmans, D.; Morton, R. J.; Pant, V.; Mandal, S.: The Role of High-frequency Transverse Oscillations in Coronal Heating. The Astrophysical Journal 952, p. L15 (2023)
Yardley, S. L.; Owen, C. J.; Long, D. M.; Baker, D.; Brooks, D. H.; Polito, V.; Green, L. M.; Matthews, S.; Owens, M.; Lockwood, M.et al.; Stansby, D.; James, A. W.; Valori, G.; Giunta, A.; Janvier, M.; Ngampoopun, N.; Mihailescu, T.; To, A. S. H.; van Driel-Gesztelyi, L.; Démoulin, P.; D'Amicis, R.; French, R. J.; Suen, G. H. H.; Rouillard, A. P.; Pinto, R. F.; Réville, V.; Watson, C. J.; Walsh, A. P.; De Groof, A.; Williams, D. R.; Zouganelis, I.; Müller, D.; Berghmans, D.; Auchère, F.; Harra, L.; Schühle, U. H.; Barczynski, K.; Buchlin, É.; Aznar Cuadrado, R.; Kraaikamp, E.; Mandal, S.; Parenti, S.; Peter, H.; Rodriguez, L.; Schwanitz, C.; Smith, P.; Teriaca, L.; Verbeeck, C.; Zhukov, A. N.; De Pontieu, B.; Horbury, T.; Solanki, S. K.; del Toro Iniesta, J. C.; Woch, J.; Gandorfer, A. M.; Hirzberger, J.; Súarez, D. O.; Appourchaux, T.; Calchetti, D.; Sinjan, J.; Kahil, F.; Albert, K.; Volkmer, R.; Carlsson, M.; Fludra, A.; Hassler, D.; Caldwell, M.; Fredvik, T.; Grundy, T.; Guest, S.; Haberreiter, M.; Leeks, S.; Pelouze, G.; Plowman, J.; Schmutz, W.; Sidher, S.; Thompson, W. T.; Louarn, P.; Federov, A.: Slow Solar Wind Connection Science during Solar Orbiter's First Close Perihelion Passage. The Astrophysical Journal Supplement Series 267, p. 11 (2023)
Jha, B. K.; Hegde, M.; Priyadarshi, A.; Mandal, S.; Ravindra, B.; Banerjee, D.: Extending the sunspot area series from Kodaikanal Solar Observatory. Frontiers in Astronomy and Space Sciences 9, p. 1019751 (2022)
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
For PhD students whose project is already funded and who are applying for admission to the IMPRS, or for applicants who want to bring their own funding and their own project idea to the IMPRS.
The magnetic field in the solar atmosphere exceeds the geomagnetic field strength by four orders of magnitude. It greatly influences the processes of energy transport within the solar atmosphere, and dominates the morphology of the solar chromosphere and corona. Kinetic energy from convective motions in the Sun can be efficiently stored in magnetic fields and subsequently released - to heat the solar corona to several million degrees or to blast off coronal mass ejections.
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.