Štverák, Š.; Trávníček, P.; Maksimovic, M.; Marsch, E.; Fazakerley, A. N.; Scime, E. E.: Electron temperature anisotropy constraints in the solar wind. Journal Geophysical Research 113, A03103 (2008)
Tian, H.; Marsch, E.; Tu, C.-Y.; Xia, L.-D.; He, J.-S.: Sizes of transition-region structures in coronal holes and in the quiet Sun. Astronomy and Astrophysics 482, pp. 267 - 272 (2008)
Tu, C.-Y.; Schwenn, R.; Donovan, E.; Marsch, E.; Wang, J.-S.; Xia, L.-D.; Zhang, Y.-W.; the working team, K.: Space weather explorer - The KuaFu mission. Advances in Space Research 41, pp. 190 - 209 (2008)
Marsch, E.: The radial wavefunction of a relativistic binary of two fermions bound by the Coulomb force. Annalen der Physik 16 (7-8), pp. 553 - 562 (2007)
Matteini, L.; Landi, S.; Hellinger, P.; Pantellini, F.; Maksimovic, M.; Velli, M.; Goldstein, B. E.; Marsch, E.: Evolution of the solar wind proton temperature anisotropy from 0.3 to 2.5 AU. Geophysical Research Letters 34, L20105 (2007)
Tian, H.; Tu, C.-Y.; He, J.-S.; Marsch, E.: Emission heights of coronal bright points on Fe XII radiance map. Advances in Space Research 39, pp. 1853 - 1859 (2007)
Wilhelm, K.; Marsch, E.; Dwivedi, B. N.; Feldman, U.: Observations of the Sun at Vacuum-Ultraviolet Wavelengths from Space. Part II: Results and Interpretations. Space Science Reviews 133, pp. 103 - 179 (2007)
Zhou, G.-Q.; He, J.-S.; Tu, C.-Y.; Marsch, E.: Correlation Height of the Source Region of Si II Emission Lines in Coronal Hole Regions. Chinese Astronomy and Astrophysics 31, pp. 137 - 145 (2007)
Boswell, R. W.; Marsch, E.; Charles, C.: The current-free electric double layer in a coronal magnetic funnel. Astrophysical Journal 640, pp. L199 - L202 (2006)
Marsch, E.: Addendum and erratum, The relativistic energy spectrum of hydrogen [Ann.Phys.(Leipzig) 14, 324(2005)]. Annalen der Physik 15 (6), pp. 434 - 437 (2006)
Marsch, E.; Zhou, G.-Q.; He, J.-S.; Tu, C.-Y.: Magnetic structure of the solar transition region as observed in various ultraviolet lines emitted at different temperatures. Astronomy and Astrophysics 457, pp. 699 - 706 (2006)
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.
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".