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Watermann, J.; Stauning, P.; Luehr, H.; Newell, P. T.; Christiansen, F.; Schlegel, K.: Are small-scale field-aligned currents and magneto sheath-like particle precipitation signatures of the same low-altitude cusp? Advances in Space Research 43 (1), pp. 41 - 46 (2009)
Cai, H. T.; Ma, S. Y.; Fan, Y.; Liu, Y. C.; Schlegel, K.: Climatological features of electron density in the polar ionosphere from long-term observations of EISCAT/ESR radar. Annales Geophysicae 25, pp. 2561 - 2569 (2007)
Dyrud, L.; Krane, B.; Oppenheim, M.; Pecseli, H. L.; Schlegel, K.; Trulsen, J.; Wernik, A. W.: Low-frequency electrostatic waves in the ionospheric E-region: a comparison of rocket observations and numerical simulations. Annales Geophysicae 24 (11), pp. 2959 - 2979 (2006)
Cai, H. T.; Ma, S. Y.; Schlegel, K.: Climatologic characteristics of high-latitude ionosphere - EISCAT observations and comparison with the IRI model. Chinese J. Geophys. 48 (3), pp. 471 - 479 (2005)
Haldoupis, C.; Ogawa, T.; Schlegel, K.; Koehler, J. A.; Ono, T.: Is there a plasma density gradient role on the generation of short scale Farley-Buneman waves? Annales Geophysicae 23, pp. 3323 - 3337 (2005)
Bosinger, T.; Hussey, G. C.; Haldoupis, C.; Schlegel, K.: Auroral E-region electron density height profile modification by electric field driven vertical plasma transport: some evidence in EISCAT CP-1 data statistics. Annales Geophysicae 22 (3), pp. 901 - 910 (2004)
Stolle, C.; Jakowski, N.; Schlegel, K.; Rietveld, M.: Comparison of high latitude electron density profiles obtained with the GPS radio occultation technique and EISCAT measurementss. Annales Geophysicae 22 (6), pp. 2015 - 2022 (2004)
Haldoupis, C.; Schlegel, K.; Hussey, G. C.; Koehler, J. A.: Radar observation of kinetic effects at meter scales for Farley-Buneman plasma waves. Journal Geophysical Research 107 (A10), 1272 (2002)
Jackel, B. J.; Moorcroft, D. R.; Foster, J. C.; Schlegel, K.: Spectral characteristics of UHF radar aurora. Journal Geophysical Research 107 (A7), 1122 (2002)
Ma, S. Y.; Cai, H. T.; Liu, H. X.; Schlegel, K.; Lu, G.: Positive storm effects in the dayside polar ionospheric F- region observed by EISCAT and ESR during the magnetic storm of 15 May 1997. Annales Geophysicae 20 (9), pp. 1377 - 1384 (2002)
Ma, S.-Y.; Liu, H.-X.; Schlegel, K.: A comparative study of magnetic storm effects on the ionosphere in the polar cap and auroral oval - F-region negative storm. Chinese J. Geophys. 45 (2), pp. 154 - 163 (2002)
First Light! The spectro-polarimeter of the world's largest solar telescope in Hawaii looks at the Sun for the first time. The instrument was developed in Germany.
Dr. Theodosios Chatzistergos receives award by the European Space Weather and Space Climate Association for his research findings on the historical activity of the Sun.
The Zdenĕk Švetska Senior Prize of the Solar Physics Division of the European Physical Society (EPS) recognizes Solanki’s pioneering contributions to solar research.
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.
Application deadline 1 October 2024. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...