Krimigis, S. M.; Armstrong, T. P.; Axford, W. I.; Bostrom, C. O.; Gloeckler, G.; Keath, E. P.; Lanzerotti, L. J.; Carbary, J. F.; Hamilton, D. C.; Roelof, E. C.: Low energy charged particles (LECP). In: AGU Fall Meeting. (1981)
Webb, G. M.; Axford, W. I.; Forman, M. A.: Cosmic ray acceleration by stellar winds: I. Total density, pressure and energy flux. In: Proc. 17th International Cosmic Ray Conference, Paris, 13-25 July 1981, pp. 309 - 312. (1981)
Axford, W. I.: Comets and cometary missions - an introductory review. In: Proc. Workshop on Cometary Missions, Bamberg, Germany, 20-22 February 1979, pp. 1 - 12. Remeis-Sternwarte Bamberg und Astronomisches Institut der Universität Erlangen-Nürnberg (1979)
Hamilton, D. C.; Gloeckler, G.; Armstrong, T. P.; Axford, W. I.; Bostrom, C. O.; Fan, C. Y.; Krimigis, S. M.; Lanzerotti, L. J.: Recurrent energetic particle events associated with forward/reverse shock pairs near 4 AU in 1978. In: Conference papers, 16th International Cosmic Ray Conference, Kyoto, Japan, 06-18 August 1979, pp. 363 - 367. (1979)
Axford, W. I.; Leer, E.; Skadron, G.: The acceleration of cosmic rays by shock waves. In: Proc. 10th Leningrad Seminar on Space Physics, 6-8 October 1978, pp. 125 - 133 (Eds. Dergachov; Kocharov). (1978)
Axford, W. I.; Leer, E.; Skadron, G.: The acceleration of cosmic rays by shock waves. In: Conference papers, 15th International Cosmic Ray Conference, Plovdiv, Bulgaria, 13-26 August 1977, pp. 132 - 137. (1977)
Axford, W. I.: Flow of mass and energy in the solar system. In: Proc. International Symposium on Solar-Terrestrial Physics, Boulder, Colorado, 07-18 June 1976. (1976)
Axford, W. I.; Feldman, W.; Forman, M. A.; Habbal, S. R.; Ling, J. C.; Moses, S.; Title, A.; Woo, R.; Young, D. T.: Close encounter with the Sun. Report of the Minimum Solar Mission Science Definition Team. Jet Propulsion Laboratory, Pasadena (1995)
Nielsen, E.; Axford, W. I.; Hagfors, T.; Kopka, H.; Armand, N. A.; Andrianov, V. A.; Shtern, D. J.; Breus, T.: The ``Long wavelength radar'' on the Mars-94 orbiter. Max-Planck-Institut für Aeronomie, Katlenburg-Lindau, Germany (1994)
Hartmann, G.; Schanda, E.; Kunzi, E.; Axford, W. I.: Microwave atmosphere sounder for earth limb observations from space. Project and program description. Dornier-IAP, Univ. of Bern - MPAE Lindau (1981)
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".