Brkovic, A.; Peter, H.; Solanki, S. K.: Relative brightness variability vs. averaged Doppler shift in the quiet Sun. In: Proc. SOHO 11 Symposium, ``From Solar Min to Max: Half a Solar Cycle with SOHO'', pp. 281 - 282 (Ed. Wilson, A.). ESA Publ. Div., Noordwijk (2002)
Curdt, W.; Wang, T. J.; Innes, D. E.; Solanki, S. K.; Dammasch, I. E.; Kliem, B.; Ofman, L.: Doppler oscillations in hot coronal loops. In: Proc. 10th European Solar Physics Meeting ``Solar Variability: From Core to Outer Frontiers'', pp. 581 - 584 (Ed. Wilson, A.). ESA Publ. Div., Noordwijk (2002)
Khomenko, E. V.; Collados, M.; Lagg, A.; Solanki, S. K.; Trujillo-Bueno, G.: Statistical properties of magnetic fields in intranetwork. In: SOLMAG 2002, Proceedings of the Magnetic Coupling of the Solar Atmosphere, Euroconference and IAU Colloquium 188,, pp. 445 - 448 (Ed. Sawaya-Lacoste, H.). ESA Publications Division, Noordwijk, The Netherlands (2002)
Krivova, N. A.; Solanki, S. K.; Fligge, M.: How large is the Sun's total magnetic flux. In: SOLMAG 2002, Proceedings of the Magnetic Coupling of the Solar Atmosphere, Euroconference and IAU Colloquium 188,, pp. 461 - 464 (Ed. Sawaya-Lacoste, H.). ESA Publications Division, Noordwijk (2002)
Mathew, S. K.; Lagg, A.; Solanki, S. K.; Collados, M.; Berdyugina, S.; Krupp, N.; Woch, J.; Frutiger, C.: Inversion of 1.5 μm spectral data of a sunspot. In: Proc. ``Probing the Sun with High Resolution'' (Eds. Venkatkrishnan, S.; Tripathy, S. C.; Venkatkrishnan, P. V.). Alpha Science, Pangbourne (2002)
Mathew, S. K.; Solanki, S. K.; the VIM Team: A Fabry-Perot Etalon Filter System for a Visible Light Imager and Magnetograph on-board Solar Orbiter. In: Proc. ``Probing the Sun with High Resolution'' (Eds. Tripathy, S. V. S. C.; Venkatkrishnan, P. V.). Alpha Science, Pangbourne (2002)
Mathew, S. K.; Solanki, S. K.; Lagg, A.; Collados, M.; Berdyugina, S.; Frutiger, C.; Krupp, N.; Woch, J.: Thermal-magnetic relation of a sunspot from the inversion of IR spectral data. In: 1st Potsdam Thinkshop on Sunspots and Starspots Poster Proceedings, pp. 117 - 118 (Eds. Strassmeier, K. G.; Washuettl, A.). Brandenburgische Universitätsdruckerei, Golm (2002)
Mathew, S. K.; Solanki, S. K.; Lagg, A.; Collados, M.; Berdyugina, S.; Frutiger, C.; Krupp, N.; Woch, J.: Thermal-magnetic relation of a sunspot as inferred from inversion of 1.5 μm spectral data. In: SOLMAG 2002, Proceedings of the Magnetic Coupling of the Solar Atmosphere, Euroconference and IAU Colloquium 188,, pp. 501 - 504 (Ed. Sawaya-Lacoste, H.). ESA Publ. Div., Noordwijk (2002)
Ortiz, A.; Domingo, V.; Sanahuja, B.; Solanki, S. K.: Variation of the facular and network contrast during the rising phase of cycle 23. In: Proc. SOHO-11 Symposium `From Solar Min to Max: Half a Solar Cycle with SOHO', pp. 185 - 188 (Ed. Wilson, A.). ESA Publ. Div., Noordwijk (2002)
Pauluhn, A.; Lang, J.; Schühle, U.; Solanki, S. K.; Wilhelm, K.; Pike, C. D.; Thompson, W. T.; Rüedi, I.; Hollandt, J.; Huber, M. C. E.: Intercalibration of CDS and SUMER. In: Proc. SOHO 11 Symposium, ``From Solar Min to Max: Half a Solar Cycle with SOHO'', pp. 223 - 226 (Ed. Wilson, A.). ESA Publ. Div., Noordwijk (2002)
Pauluhn, A.; Solanki, S. K.: Dependence of UV radiance of the quiet Sun on the solar cycle. In: Proc. SOHO 11 Symposium, ``From Solar Min to Max: Half a Solar Cycle with SOHO'', pp. 227 - 230 (Ed. Wilson, A.). ESA Publ. Div., Noordwijk (2002)
Pauluhn, A.; Solanki, S. K.: Surface magnetic fields and UV radiance of the quiet Sun. In: SOLMAG 2002, Proceedings of the Magnetic Coupling of the Solar Atmosphere, Euroconference and IAU Colloquium 188,, pp. 521 - 524 (Ed. Sawaya-Lacoste, H.). ESA Publ. Div., Noordwijk (2002)
Solanki, S. K.: How does the magnetic cycle change radiance and irradiance of the Sun? In: Proceedings SOHO-11 Symposium ``From Solar Min to Max: Half a Solar Cycle with SOHO'', pp. 173 - 180 (Ed. Wilson, A.). ESA Publ. Div., Noordwijk (2002)
Solanki, S. K.: Solar variability. In: The Radiometric Calibration of SOHO, pp. 1 - 19 (Eds. Pauluhn, A.; Huber, M. C. E.; von Steiger, R.). ESA Publ. Div., Noordwijk (2002)
Solanki, S. K.: Flows and oscillations in small-scale magnetic structures. In: Reports on Astronomy, pp. 159 - 161 (Ed. Appenzeller, I.). Kluwer, Dordrecht (2002)
Solanki, S. K.; Schüssler, M.; Curdt, W.; Lites, B. W.; Martinez-Pillet, V.; Schmidt, W.; Title, A. M.; the Sunrise Team: SUNRISE: A 1-m balloon borne solar telescope. In: SOLMAG 2002, Proceedings of the Magnetic Coupling of the Solar Atmosphere, Euroconference and IAU Colloquium 188,, pp. 27 - 32 (Ed. Sawaya-Lacoste, H.). ESA Publ. Div., Noordwijk (2002)
Wang, T. J.; Solanki, S. K.; Curdt, W.; Innes, D. E.; Dammasch, I. E.: Oscillating hot loops observed by SUMER. In: Proc. SOHO 11 Symposium, ``From Solar Min to Max: Half a Solar Cycle with SOHO'', pp. 465 - 468 (Ed. Wilson, A.). ESA Publ. Div., Noordwijk (2002)
Wang, T.; Solanki, S. K.; Curdt, W.; Innes, D. E.; Dammasch, I. E.: Hot loop oscillations seen by SUMER: Examples and statistics. In: SOLMAG 2002, Proceedings of the Magnetic Coupling of the Solar Atmosphere, Euroconference and IAU Colloquium 188,, pp. 199 - 202 (Ed. Sawaya-Lacoste, H.). ESA Publ. Div., Noordwijk (2002)
Wang, T. J.; Solanki, S. K.; Innes, D. E.; Curdt, W.: Initial features of an X-class flare observed with SUMER and TRACE. In: SOLMAG 2002, Proceedings of the Magnetic Coupling of the Solar Atmosphere, Euroconference and IAU Colloquium 188,, pp. 607 - 610 (Ed. Sawaya-Lacoste, H.). ESA Publ. Div., Noordwijk (2002)
Wenzler, T.; Solanki, S. K.; Fluri, D. M.; Frutiger, C.; Fligge, M.; Ortiz, A.: Modelling solar irradiance variations: separate models for the network and active region faculae. In: Proc. SOHO-11 Symposium `From Solar Min to Max: Half a Solar Cycle with SOHO', pp. 231 - 234 (Ed. Wilson, A.). ESA Publ. Div., Noordwijk (2002)
How does our star heat its outer atmosphere, the solar corona, to unimaginable temperatures of up to 10 million degrees Celsius? With unprecedented observational data from ESA's Solar Orbiter spacecraft and powerful computer simulations, ERC starting grant awardee Pradeep Chitta intends to bring new momentum to the search for the coronal heating mechanism.
The research group “Solar Lower Atmosphere and Magnetism” (SLAM) studies the conditions and dynamic processes in the atmospheric layer between the solar surface (photosphere) and the overlying chromosphere, an approximately 2000 km thick gas layer.
The main research fields of the department "Sun and Heliosphere" are covered by the research groups "Solar and Stellar Coronae", "Solar Lower Atmosphere and Magnetism", "Solar and Stellar Magnetohydrodynamics" and "Solar Variability and Climate".