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Gurevich, A. V.; Rinnert, K.; Schlegel, K.: Long wave part of the plasma turbulence spectrum in the lower E-region. Izvestija VUZov Radiophys. 40, S. 37 - 56 (1997)
Schlegel, K.; Gurevich, A. V.: Radar backscatter from plasma irregularities of the lower E region induced by neutral turbulence. Annales Geophysicae 15 (7), S. 870 - 877 (1997)
Gurevich, A. V.; Lukyanov, A. V.; Zybin, K. P.: Anomalous absorption of powerful radio waves on the striations developed during ionospheric modification. Physics Letters A 211, S. 363 - 372 (1996)
Gurevich, A. V.; Borisov, N. D.; Lukina, N. A.; Sergeichev, K. F.; Sychov, I. A.; Kozlov, S. I.; Smirnova, N. V.: Intense growth of ozone concentration in subcritical fields in oxygen plasma. Physics Letters A 201, S. 234 - 238 (1995)
Gurevich, A. V.; Zybin, K. P.; Lukyanov, A. V.: Stationary striations developed in the ionospheric modification. Physical Review Letters 75, S. 2622 - 2632 (1995)
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Gurevich, A. V.; Zybin, K. P.: Influence of atmospheric turbulence on Farley-Bunemann instability. In: Plasma Instabilities in the Ionospheric E-Region. Proc. of Workshop in Katlenburg-Lindau 1995, S. 135 - 137 (Hg. Schlegel, K.). Cuvillier, Göttingen (1996)
Schlegel, K.; Gurevich, A. V.: Radar backscatter from E-region plasma irregularities induced by neutral turbulence. In: Plasma Instabilities in the Ionospheric E-Region. Proc. of Workshop in Katlenburg-Lindau 1995, S. 9 - 12 (Hg. Schlegel, K.). Cuvillier, Göttingen (1996)
Gurevich, A. V.; Borison, N. D.; Montecinos-Geisse, S. E.; Hartogh, P.: Artificial ozone layer. Max-Planck-Institut für Aeronomie, Katlenburg-Lindau, Germany (1995)
Erst eisige Kälte, dann Mitternachtssonne: Am Polarkreis bereitet das Team den Flug des ballongetragenen Sonnenobservatoriums vor – und hofft auf ein solares Feuerwerk.
Bewerbungsfrist 1 Oktober 2023. Promotionsprojekte in Planetenwissenschaften, Sonnenphysik, Astrophysik, Magnetfelder der Sonne, Helioseismologie, Asteroseismologie ...
In der mittleren Korona der Sonne entdeckt ein Forscherteam netzartige, dynamische Plasmastrukturen – und einen wichtigen Hinweis auf den Antrieb des Sonnenwindes.