Isham, B.; La Hoz, C.; Rietveld, M. T.; Hagfors, T.; Leyser, T. B.: Cavitating Langmuir turbulence observed during EISCAT high latitude ionospheric interaction experiments. Physical Review Letters 83, pp. 2576 - 2579 (1999)
Isham, B.; Rietveld, M. T.; Hagfors, T.; La Hoz, C.; Mishin, E.; Kofman, W.; Leyser, T. B.; van Eyken, A. P.: Aspect angle dependence of HF enhanced incoherent backscatter. Advances in Space Research 24, pp. 1003 - 1006 (1999)
Brandolini, A.; Balsley, B. B.; Mabres, A.; Woodman, R. F.; Capsoni, C.; D'Amico, M.; Ecklund, W. L.; Hagfors, T.; Harper, R.; Heron, M. L.et al.; Hocking, W. K.; Lehtinen, M. S.; Röttger, J.; Sarango, M. F.; Sato, T.; Strauch, R. J.; Vaughn, J. M.; Wyatt, L. R.; Zrnic, D. S.: Report from the I}nternational {W}orkshop on {R}emote {S}ensing in {G}eophysics {U}sing {D}oppler {Techniques. Bull. Amer. Meteor. Soc. 79 (4), pp. 643 - 656 (1998)
Breus, T. K.; Pimenov, K. Y.; Luhmann, J. G.; Krymskii, A. M.; Hagfors, T.; Axford, W. I.; Kliore, A. J.: Application of Viking radio occultation data to the future studies of the Martian ionosphere. Advances in Space Research 22, pp. 463 - 470 (1998)
Kosch, M. J.; Hagfors, T.; Nielsen, E.: A new digital all-sky imager experiment for optical auroral studies in conjunction with the Scandinavian twin auroral radar experiment. Review of Scientific Instruments 69, pp. 578 - 584 (1998)
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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".