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)
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.