Watanabe, T.; Barnes, A.; Hewish, A.; Kakinuma, T.; Kojima, M.; Schwenn, R.; Tappin, S. J.: IPS and spacecraft observations relevant to STIP interval IX (15 February - 16 March 1980). preprint (1985)
Woo, R.; Armstrong, J. W.; Sheeley Jr., N. R.; Howard, R. A.; Koomen, M. J.; Michels, D. J.; Schwenn, R.: Doppler Scintillation Observations of Interplanetary Shocks Within 0.3 AU. Journal Geophysical Research 90, pp. 154 - 162 (1985)
Bougeret, J.-L.; King, J. H.; Schwenn, R.: Solar radio bursts and in situ determination of interplanetary electron density. Solar Physics 90, pp. 401 - 412 (1984)
Burlaga, L. F.; McDonald, F. B.; Ness, N. F.; Schwenn, R.; Lazarus, A. J.; Mariani, F.: Interplanetary Flow Systems Associated with Cosmic Ray Modulation in 1977-1980. Journal Geophysical Research 89, pp. 6579 - 6587 (1984)
Valdés-Galicia, J. F.; Moussas, X.; Quenby, J. J.; Neubauer, F. M.; Schwenn, R.: Mean Free Paths and Diffusion Coefficients for Energetic Protons at Small Heliodistances Calculated Using Helios 1 and 2 Data. Solar Physics 91, pp. 399 - 413 (1984)
Burlaga, L. F.; Schwenn, R.; Rosenbauer, H.: Dynamical evolution of interplanetary magnetic fields and flows between 0.3 AU and 8.5 AU: Entrainment. Geophysical Research Letters 10, pp. 413 - 416 (1983)
Marsch, E.; Mühlhäuser, K.-H.; Rosenbauer, H.; Schwenn, R.: On the Equation of State of Solar Wind Ions Derived From Helios Measurements. Journal Geophysical Research 88, pp. 2982 - 2992 (1983)
Pizzo, V.; Schwenn, R.; Marsch, E.; Rosenbauer, H.; Mühlhäuser, K.-H.; Neubauer, F. M.: Determination of the solar wind angular momentum flux from the Helios data - an observational test of the Weber and Davis theory. Astrophysical Journal 271, pp. 335 - 354 (1983)
Burlaga, L. F.; Klein, L.; Sheeley, N. R.; Michels, D. J.; Howard, R. A.; Koomen, M. J.; Schwenn, R.; Rosenbauer, H.: A magnetic cloud and a coronal mass ejection. Geophysical Research Letters 9, pp. 1317 - 1320 (1982)
Marsch, E.; Mühlhäuser, K.-H.; Rosenbauer, H.; Schwenn, R.; Neubauer, F. M.: Solar wind helium ions: Observations of the Helios solar probes between 0.3 and 1 AU. Journal Geophysical Research 87, pp. 35 - 51 (1982)
Volkmer, P. M.; Neubauer, F. M.; Schwenn, R.: Observation of flare-generated shock waves by Helios-2 near the sun. Space Science Reviews 32, pp. 131 - 144 (1982)
Burlaga, L.; Sittler, E.; Mariani, F.; Schwenn, R.: Magnetic loop behind an interplanetary shock: Voyager, Helios, and IMP 8 observations. Journal Geophysical Research 86, pp. 6673 - 6684 (1981)
Marsch, E.; Mühlhäuser, K.-H.; Rosenbauer, H.; Schwenn, R.; Denskat, K. U.: Pronounced proton core temperature anisotropy, ion differential speed, and simultaneous Alfvén wave activity in slow solar wind at 0.3 AU. Journal Geophysical Research 86, pp. 9199 - 9203 (1981)
Burlaga, L.; Lepping, R.; Weber, R.; Armstrong, T.; Goodrich, C.; Sullivan, J.; Gurnett, D.; Kellogg, P.; Keppler, E.; Mariani, F.et al.; Neubauer, F. M.; Rosenbauer, H.; Schwenn, R.: Interplanetary particles and fields, November 22 to December 6, 1977: Helios, Voyager, and IMP observations between 0.6 and 1.6 AU. Journal Geophysical Research 85, pp. 2227 - 2242 (1980)
Schwenn, R.; Rosenbauer, H.; Mühlhäuser, K.-H.: Singly-ionized helium in the driver gas of an interplanetary shock wave. Geophysical Research Letters 7, pp. 201 - 204 (1980)
Gurnett, D. A.; Marsch, E.; Pilipp, W.; Schwenn, R.; Rosenbauer, H.: Ion-Acoustic Waves and Related Plasma Observations in the Solar Wind. Journal Geophysical Research 84, pp. 2029 - 2038 (1979)
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.