Tu, C.-Y.; Marsch, E.: Evidence for a ``background'' spectrum of solar wind turbulence in the inner heliosphere. Journal Geophysical Research 95, pp. 4337 - 4341 (1990)
Tu, C.-Y.; Marsch, E.; Rosenbauer, H.: The dependence of MHD turbulence spectra on the inner solar wind stream structure near solar minimum. Geophysical Research Letters 17, pp. 283 - 286 (1990)
Marsch, E.; Pilipp, W. G.; Thieme, K. M.; Rosenbauer, H.: Cooling of solar wind electrons inside 0.3 AU. Journal Geophysical Research 94, pp. 6893 - 6898 (1989)
Marsch, E.; Tu, C.-Y.: Dynamics of correlation functions with Elsässer variables for inhomogeneous MHD turbulence. Journal of Plasma Physics 41, pp. 479 - 491 (1989)
Thieme, K. M.; Marsch, E.; Rosenbauer, H.: Estimates of alpha particle heating in the solar wind inside 0.3 AU. Journal Geophysical Research 94, pp. 2673 - 2676 (1989)
Thieme, K. M.; Schwenn, R.; Marsch, E.: Are structures in high-speed streams signatures of coronal fine structures? Advances in Space Research 9, pp. 127 - 130 (1989)
Tu, C.-Y.; Marsch, E.; Thieme, K. M.: Basic properties of solar wind MHD turbulence near 0.3 AU analysed by means of Elsässer variables. Journal Geophysical Research 94, pp. 11739 - 11759 (1989)
Richter, A. K.; Marsch, E.: Helios observational constraints on the development of interplanetary slow shocks. Annales Geophysicae 6, pp. 319 - 324 (1988)
Hernandez, R.; Livi, S.; Marsch, E.: On the He2+ to H+ temperature ratio in slow solar wind. Journal Geophysical Research 92 (A7), pp. 7723 - 7727 (1987)
Livi, S.; Marsch, E.: Generation of solar wind proton tails and double beams by Coulomb collisions. Journal Geophysical Research 92 (A7), pp. 7255 - 7261 (1987)
Marsch, E.; Livi, S.: Observational evidence for marginal stability of solar wind ion beams. Journal Geophysical Research 92 (A7), pp. 7263 - 7268 (1987)
Marsch, E.; Richter, A. K.: On the equation of state and collision time for a multicomponent, anisotropic solar wind. Annales Geophysicae 5A, pp. 71 - 82 (1987)
Hernández, R.; Marsch, E.: Collisional transfer of energy and momentum between drifting tri-Maxwellians. Journal of Plasma Physics 35, pp. 473 - 482 (1986)
Livi, S.; Marsch, E.: Comparison of the Bhatnagar-Gross-Krook approximation with the exact Coulomb collision operator. Physical Review A 34 (1), pp. 533 - 540 (1986)
A star’s chemical composition strongly influences the ultraviolet radiation it emits into space and thus the conditions for the emergence of life in its neighbourhood.
A single star has provided information about the collision of the Milky Way with the dwarf galaxy Gaia-Enceladus. The event likely took place approximately 11.5 billion years ago.