Rietveld, M. T.; Isham, B.; Grydeland, T.; La Hoz, C.; Leyser, T. B.; Honary, F.; Ueda, H.; Kosch, M.; Hagfors, T.: HF-pump-induced parametric instabilities in the auroral E-region. Advances in Space Research 29 (9), pp. 1363 - 1368 (2002)
Borisov, N. D.; Hagfors, T.: Excitation of heater-enhanced plasma and ion lines near the reflection level of a hight-frequency pump wave. Journal of Plasma Physics 66 (1 & 2), pp. 71 - 89 (2001)
Hagfors, T.: Time-varying propagation circuits, description and applications. Journal of Atmospheric and Solar-Terrestrial Physics 63, pp. 215 - 220 (2001)
Kosch, M. J.; Honary, F.; del Pozo, C. F.; Marple, S. R.; Hagfors, T.: High-resolution maps of the characteristic energy of precipitating auroral particles. Journal Geophysical Research 106 (A12), pp. 28925 - 28937 (2001)
Mishin, E. V.; Hagfors, T.; Isham, B.: A generation mechanism of the topside enhanced incoherent backscatter during high frequency modification experiments in Tromsø. Geophysical Research Letters 28 (3), pp. 479 - 482 (2001)
Cierpka, K.; Kosch, M. J.; Rietveld, M.; Schlegel, K.; Hagfors, T.: Ion-neutral coupling in the high-latitude F-layer from incoherent scatter and Fabry-Perot interferometer measurements. Annales Geophysicae 18 (9), pp. 1145 - 1153 (2000)
Kosch, M. J.; Ishii, M.; Kohsiek, A.; Rees, D.; Schlegel, K.; Hagfors, T.; Cierpka, K.: A comparison of vertical thermospheric winds from Fabry-Perot interferometer measurements over a 50 km baseline. Advances in Space Research 26, pp. 985 - 988 (2000)
Kosch, M. J.; Ishii, M.; Nozawa, S.; Rees, D.; Cierpka, K.; Kohsiek, A.; Schlegel, K.; Fujii, R.; Hagfors, T.; Fuller-Rowell, T. J.et al.; Lathuillere, C.: A comparison of thermospheric winds and temperatures from Fabry-Perot interferometer and EISCAT radar measurements with models. Advances in Space Research 26, pp. 979 - 984 (2000)
Kosch, M.; Rietveld, M. T.; Hagfors, T.; Leyser, T. B.: High-latitude HF-induced airglow displaced equatorwards of the pump beam. Geophysical Research Letters 27 (17), pp. 2817 - 2820 (2000)
Mishin, E. V.; Carlson, H. C.; Hagfors, T.: On the electron distribution function in the F region and airglow enhancements during HF modification experiments. Geophysical Research Letters 27 (18), pp. 2857 - 2860 (2000)
Rietveld, M. T.; Isham, B.; Kohl, H.; La Hoz, C.; Hagfors, T.: Measurements of HF-enhanced plasma and ion lines at EISCAT with high altitude resolution. Journal Geophysical Research 105 (A4), pp. 7429 - 7439 (2000)
Barbin, Y.; Kofman, W.; Nielsen, E.; Hagfors, T.; Seu, R.; Picardi, G.; Svedhem, H.: The CONSERT instrument for the ROSETTA mission. Advances in Space Research 24, pp. 1115 - 1126 (1999)
Gurevich, A.; Carlson, H.; Kelley, M.; Hagfors, T.; Karashtin, A.; Zybin, K.: Nonlinear structuring of the ionosphere modified by powerful radio waves at low latitudes. Physics Letters A 251, pp. 311 - 321 (1999)
Herique, A.; Kofman, W.; Hagfors, T.; Caudal, G.; Ayanides, J.-P.: A characterization of a comet nucleus interior: inversion of simulated radio frequency data. Planetary and Space Science 47, pp. 885 - 904 (1999)
Isham, B.; Hagfors, T.; Mishin, E.; Rietveld, M. T.; La Hoz, C.; Kofman, W.; Leyser, T.: A search for the location of the HF excitation of enhanced ion acoustic and Langmuir waves with EISCAT and the Tromsø heater. Radiophys. Quantum Electron. 42 (7), pp. 607 - 618 (1999)
Analyzing the high spatial resolution solar Ca II H and K emission data obtained by the SUNRISE mission and building a model of other stars more active than the Sun
For PhD students whose project is already funded and who are applying for admission to the IMPRS, or for applicants who want to bring their own funding and their own project idea to the IMPRS.
The magnetic field in the solar atmosphere exceeds the geomagnetic field strength by four orders of magnitude. It greatly influences the processes of energy transport within the solar atmosphere, and dominates the morphology of the solar chromosphere and corona. Kinetic energy from convective motions in the Sun can be efficiently stored in magnetic fields and subsequently released - to heat the solar corona to several million degrees or to blast off coronal mass ejections.
The Solar Lower Atmosphere and Magnetism (SLAM) group covers many exciting subjects in solar physics, focussing on the development and testing of highly novel solar instrumentation, reduction and analysis of highest quality solar observations, or improving and developing advanced techniques for the analysis of solar observations.