Nielsen, E.; Whitehead, J. D.; Hedberg, L. A.; Jones, T. B.: A test of the cosine relationship using three-radar velocity measurements. Radio Science 18, p. 230 (1983)
Opgenoorth, H. J.; Oksman, J.; Kaila, K. U.; Nielsen, E.; Baumjohann, W.: Characteristics of eastward drifting omega bands in the morining sector of the auroral oval. Journal Geophysical Research 88, p. 9171 (1983)
Opgenoorth, H. J.; Pellinen, R. J.; Baumjohann, W.; Nielsen, E.; Marklund, G.; Eliason, L.: Three-dimensional current flow and particle precipitation in a westward travelling surge (observed during the Barivin-GEOS rocket experiment). Journal Geophysical Research 88, p. 3138 (1983)
Rietveld, M. T.; Barr, R.; Dowden, R. L.; Kopka, H.; Nielsen, E.; Stubbe, P.: Ionospheric elctric field pulsation: A comparison between VLF results from an ionospheric heating experiment and STARE. Journal Geophysical Research 88, p. 2140 (1983)
Rietveld, M. T.; Kopka, H.; Nielsen, E.; Stubbe, P.; Dowden, R. L.: Ionospheric elctric field pulsation: A comparison between ULF results from an ionospheric heating experiment and STARE. Radio Science 88, p. 2140 (1983)
Uspensky, M. V.; Pellinen, R. J.; Baumjohann, W.; Starkov, G. V.; Nielsen, E.; Sofko, G. J.; Kaila, K. U.: Spatial variations of ionospheric conductivity and radar auroral amplitude in the eastward electrojet region during pre-substorm conditions. Journal Geophysical Research 52, p. 40 (1983)
Waldock, J. A.; Jones, T. B.; Nielsen, E.; Southwood, D. J.: First results of micropulsaiton activity observed by SABRE. Planetary and Space Science 31, p. 573 (1983)
Waldock, J. A.; Thomas, E. C.; Stewart, C. P.; Jones, T. B.; Nielsen, E.: SABRE observations of a sequence of Pc5 micropulsations. Radio Science 18, p. 1133 (1983)
Whitehead, J. D.; Ierkic, H. M.; Nielsen, E.: Splitting and divergence of ``STARE'' auroral radar velocities. Journal Geophysical Research 88, p. 2147 (1983)
Allan, W.; Poulter, E. M.; Nielsen, E.: STARE observations of a Pc5 pulsation with large azimuthal wave number. Journal Geophysical Research 87, p. 6163 (1982)
Haldoupis, C. I.; Nielsen, E.; Goertz, C.: Experimental evidence on the dependence of 140 MHz radar auroral backscatter characteristics on ionospheric conductivity. Journal Geophysical Research 87, p. 7666 (1982)
Haldoupis, C. I.; Nielsen, E.; Holtet, J. A.; Egeland, A.; Chivers, H. A. J.: Radar auroral observations during a burst of irregular magnetic pulsations. Journal Geophysical Research 87, p. 1541 (1982)
Nielsen, E.; Korth, A.; Kremser, G.; Mariani, F.: The electron pitch angle distribution at geosynchronous orbit associated spikes during the substorm expansion phase. Journal Geophysical Research 87, p. 887 (1982)
Poulter, E. M.; Nielsen, E.: The interpretation of gound-based observations of energetic electron fluxes modulated by Pc5 hydromagnetic oscillations. Journal Geophysical Research 87, p. 2549 (1982)
Poulter, E. M.; Nielsen, E.: The hydromagnetic oscillation of individual shells of the geomagnetic field. Journal Geophysical Research 87, p. 432 (1982)
Poulter, E. M.; Nielsen, E.; Potemra, T. A.: Field-aligned currents associated with Pc5 pulsaitons:STARE and TRIAD observations. Journal Geophysical Research 87, p. 2331 (1982)
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, ...