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Röttger, J.: Investigations of lower and middle atmosphere dynamics with spaced antenna drifts radars. Journal of Atmospheric and Terrestrial Physics 43, pp. 277 - 292 (1981)
Röttger, J.: Equatorial spread-F by electric fields and atmospheric gravity waves generated by thunderstorms. Journal of Atmospheric and Terrestrial Physics 43, pp. 453 - 462 (1981)
Röttger, J.; Czechowsky, P.; Schmidt, G.: First low power VHF radar observations of tropospheric, stratospheric and mesospheric winds and turbulence at the Arecibo Observatory. Journal of Atmospheric and Terrestrial Physics 43, pp. 789 - 800 (1981)
Röttger, J.: Structure and dynamics of the stratosphere and mesosphere revealed by VHF radar investigations. J. Pure Appl. Geophys. 118, pp. 494 - 527 (1980)
Vincent, R. A.; Röttger, J.: Spaced antenna VHF radar observations of tropospheric velocities and irregularities. Radio Science 15, pp. 319 - 335 (1980)
Röttger, J.; Rastogi, P. K.; Woodman, R. F.: High-resolution VHF radar observations of turbulence structures in the mesosphere. Geophysical Research Letters 6, pp. 617 - 620 (1979)
Röttger, J.: Drifting patches of equatorial spread-F irregularities -experimental support for the spatial resonance mechanism in the ionosphere. Journal of Atmospheric and Terrestrial Physics 40, pp. 1103 - 1112 (1978)
Images from ESA’s Solar Orbiter offer the best look yet at a source region of the solar wind - and challenge our view of the continuous particle stream from the Sun.
Deciphering the magnetic origins of the Sun's hot corona: developing a framework for coronal heating by probing the elusive photosphere-corona connection
Using unique observational data and computer simulations, the MPS scientist is striving to understand the incredibly hot temperatures in the solar corona.
For the first time, images of the Sun have been taken from a distance of only 77 million kilometres enabling a completely new view of our star possible.
In his doctoral thesis, Sudip Mandal investigated how special pressure waves help maintain temperatures of several million degrees in the outermost solar atmosphere.