Zanetti, L. J.; Kessel, R. L.; Mauk, B. H.; Ukhorskiy, A. Y.; Fox, N. J.; Barnes, R. J.; Weiss, M.; Sotirelis, T. S.; Raouafi, N. E.: The Van Allen Probes' Contribution to the Space Weather System. Johns Hopkins APL Tech. Dig. 33 (3), pp. 194 - 201 (2016)
Sahal-Brechot, S.; Raouafi, N. E.: Doppler redistribution of anisotropic radiation and resonance polarization in moving scattering media - Predicted results for the coronal O VI 1032 angstrom line. Astronomy and Astrophysics 445 (2), pp. 681 - 692 (2006)
Raouafi, N.-E.; Mancuso, S.; Solanki, S. K.; Inhester, B.; Mierla, M.; Stenborg, G.; Delaboudiniere, J. P.; Benna, C.: Shock wave driven by an expanding system of loops. Astronomy and Astrophysics 424 (3), pp. 1039 - 1048 (2004)
Raouafi, N.-E.; Solanki, S. K.: Effect of the electron density stratification on off-limb OVI line profiles: How large is the velocity distribution anisotropy in the solar corona? Astronomy and Astrophysics 427 (2), pp. 725 - 733 (2004)
Raouafi, N.-E.; Solanki, S. K.: Effect of anisotropic velocity distribution on the linear polarization of coronal lines. Does the ion cyclotron exist in the inner corona? Astronomy and Astrophysics 412, pp. 271 - 280 (2003)
Raymond, J. C.; Ciaravella, A.; Dobrzycka, D.; Strachan, L.; Ko, Y. K.; Uzzo, M.; Raouafi, N.-E.: Far-ultraviolet spectra of fast coronal mass ejections associated with X-class flares. Astrophysical Journal 597 (2), pp. 1106 - 1117 (2003)
Raouafi, N.-E.: Stokes parameters of resonance lines scattered by a moving, magnetic medium - Theory of the two-level atom. Astronomy and Astrophysics 386 (2), pp. 721 - 731 (2002)
Raouafi, N.-E.; Sahal-Bréchot, S.; Lemaire, P.: Linear polarization of the O VI λ l031.92 coronal line. II. Constraints on the magnetic field and the solar wind velocity field vectors in the coronal polar holes. Astronomy and Astrophysics 396, pp. 1019 - 1028 (2002)
Raouafi, N.-E.; Sahal-Bréchot, S.; Lemaire, P.; Bommier, V.: Linear polarization of the O VI λ1031.92 coronal line. I. Constraints on the solar wind velocity field vector in the polar holes. Astronomy and Astrophysics 390, pp. 691 - 706 (2002)
Raouafi, N.-E.; Solanki, S. K.; Wiegelmann, T.: Hanle Effect Diagnostics of the Coronal Magnetic Field: A Test Using Realistic Magnetic Field Configurations. In: Solar Polarization 5: In Honor of Jan Stenflo, pp. 429 - 434 (Eds. Berdyugina, S. V.; Nagendra, K. N.; Ramelli, R.). (2009)
Raouafi, N.-E.; Manusco, S.; Solanki, S. K.; Inhester, B.; Mierla, M.; Stenborg, G.; Delaboudinière, J. P.; Benna, C.: Shock wave driven by an expanding system of loops. In: Coronal and Stellar Mass Ejections, Proc. IAU Symp. 226, pp. 127 - 128 (Eds. Dere, K. P.; Wang, J.; Yan, Y.). Cambridge University Press (2005)
Raouafi, N.-E.; Manusco, S.; Solanki, S. K.; Inhester, B.; Benna, C.; Delaboudinière, J. P.; Stenborg, G.; Mierla, M.: Interpretation of the coronal EUV signature of the CME event on June 27 1999. In: Proc. SOHO 13 `Waves, Oscillations and Small-Scale Transient Events in the Solar Atmosphere: A Joint View from SOHO and TRACE', pp. 317 - 322 (Ed. Lacoste, H.). ESA Publ. Div., Noordwijk (2004)
Raouafi, N.-E.; Solanki, S. K.: Effect of the line-of-sight integration on the profiles of coronal lines. In: Proc. SOHO 13 `Waves, Oscillations and Small-Scale Transient Events in the Solar Atmosphere: A Joint View from SOHO and TRACE', pp. 401 - 406 (Ed. Lacoste, H.). ESA Publ. Div., Noordwijk (2004)
Raouafi, N.-E.; Solanki, S. K.: Sensitivity of solar off-limb line profiles to electron density stratification and the velocity distribution anisotropy. In: Proc. SOHO 15 `Coronal Heating', pp. 170 - 175 (Eds. Walsh, R. W.; Ireland, J.; Danesy, D.; Fleck, B.). ESA Publ. Div., Noordwijk (2004)
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Arnaud, J.; Faurobert, M.; Raouafi, N.-E.; Solanki, S. K.: Molecular lines observations with THEMIS. In: SF2A 2003 ``Semaine de l'Astrophysique Française'', pp. 39 - 40 (Eds. F. Combes, D. B.; Contini, T.). EDP Sciences (2003)
Raouafi, N.-E.; Lemaire, P.; Sahal-Bréchot, S.: Effect of the coronal magnetic field and the solar wind velocity field vectors on the polarization of the O VI λ1032 line. In: Proc. SOHO 11 Symposium, ``From Solar Min to Max: Half a Solar Cycle with SOHO'', pp. 403 - 406 (Ed. Wilson, A.). ESA Publ. Div., Noordwijk (2002)
Raouafi, N.-E.; Sahal-Bréchot, S.; Lemaire, P.: Effect of the solar wind velocity field vector on the polarization of the O VI λ1032 coronal line. In: Proc. SOHO 11 Symposium, ``From Solar Min to Max: Half a Solar Cycle with SOHO'', pp. 471 - 474 (Ed. Wilson, A.). ESA Publ. Div., Noordwijk (2002)
Die ESA-Mission JUICE soll ab 2030 das Jupitersystem erkunden. Nach Vorbeiflügen an Europa und Callisto wird die Raumsonde erstmals in der Geschichte der Raumfahrt in eine Umlaufbahn um den Mond Ganymed einschwenken.
Das Submillimetre Wave Instrument (SWI) wird die Galileischen Monde, die Chemie, die Meteorologie und die Struktur der mittleren Jupiter-Atmosphäre, sowie atmosphärische und magnetosphärische Kopplungsprozesse untersuchen.
Mars Express ist eine ESA Mission zum Mars. Sie hat eine Nutzlast an Bord, die in der Lage ist, die bisher gründlichste Suche nach flüssigem Wasser, das unerlässlich ist für Leben wie wir es kennen, auf dem roten Planeten durchzuführen.
Ein Überblick über alle Arbeits- und Forschungsgruppen der Abteilung für Planetenwissenschaften: Atmosphären der Planeten, Inneres der Planeten, Kleine Körper und Kometen, Oberflächen der Planeten, Plasmaumgebung der Planeten.