Solanki, S. K.: Wie stark beeinflusst die Sonne das Klima und den derzeitigen Klimawandel? In: Klimawandel im 20. und 21. Jahrhundert, pp. 111 - 121. Verlag Dr. Friedrich Pfeil, München (2005)
Solanki, S. K.; Schüssler, M.: Small-scale solar magnetic elements: simulations and observations. In: The Solar-B Mission and the Forefront of Solar Physics, pp. 105 - 114 (Eds. Sakurai, T.; Sekii, T.). Astronomical Society of the Pacific, San Francisco (2005)
Teriaca, L.; Schühl{}e, U.; Solanki, S. K.; Curdt, W.; Marsch, E.: The structure of the lower transition region as inferred from the hydrogen Lyman-α line radiance. In: Proceedings of the International Scientific Conference on Chromospheric and Coronal Magnetic Fields (Eds. Innes, D. E.; Lagg, A.; Solanki, S. K.; Danesy, D.). ESA Publ. Div., Noordwijk (2005)
Teriaca, L.; Schühle, U.; Solanki, S. K.; Curdt, W.; Marsch, E.: The dynamics of the lower transition region as inferred from the hydrogen Lyman-α line radiance. In: Proceedings of the 11th European Solar Physics Meeting - The Dynamic Sun: Challenges for Theory and Observations, 11-16 September 2005 (Eds. Danesy, D.; Poedts, S.; De Groof, A.; Andries, J.). ESA Publ. Div., Noordwijk (2005)
Tripathi, D.; Bothmer, V.; Solanki, S. K.; Schwenn, R.; Mierla, M.; Stenborg, G.: SOHO/EIT observation of a coronal inflow. In: Coronal and Stellar Mass Ejections, Proc. IAU Symp. 226, pp. 133 - 134 (Eds. Dere, K. P.; Wang, J.; Yan, Y.). Cambridge University Press, Cambridge (2005)
Usoskin, I. G.; Schüssler, M.; Solanki, S. K.; Mursula, K.: Solar activity over the last 1150 years: does it correlate with climate? In: Proc. The 13th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun, pp. 19 - 22 (Eds. Favata, F.; Hussain, G. A. J.; Battrick, B.). ESA Publ. Div., Noordwijk (2005)
Wiegelmann, T.; Lagg, A.; Solanki, S. K.; Inhester, B.; Woch, J.: Magnetic loops: A comparison of extrapolations from the photosphere with chromospheric measurements. In: Proceedings of the International Scientific Conference on Chromospheric and Coronal Magnetic Fields (Eds. Innes, D. E.; Lagg, A.; Solanki, S. K.; Danesy, D.). ESA Publ. Div., Noordwijk (2005)
Aznar Cuadrado, R.; Solanki, S. K.; Lagg, A.; Thomas, R. M.: Signature of current sheets as seen by TIP at VTT in the HeI multiplet at 1083.0 nm. In: Proc. SOHO 15 `Coronal Heating', pp. 593 - 596 (Eds. Walsh, R. W.; Ireland, J.; Danesy, D.; Fleck, B.). ESA Publ. Div., Noordwijk (2004)
Gandorfer, A. M.; Solanki, S. K.; Schüssler, M.; Curdt, W.; Lites, B. W.; Martínez Pillet, V.; Schmidt, W.; Title, A. M.; the Sunrise Team: SUNRISE: High resolution UV/VIS observations of the Sun from the stratosphere. In: Astronomical Telescopes and Instrumentation - The Industrial Revolution in Astronomy, pp. 732 - 741 (Ed. Oschmann, J. M.). SPIE, Bellingham (2004)
Khomenko, E. V.; Shelyag, S.; Solanki, S. K.; Vögler, A.; Schüssler, M.: Stokes diagnostics of magneto-convection. Profile shapes and asymmetries. In: Multi-Wavelength Investigations of Solar Activity, Proc. IAU Symp. 223, pp. 635 - 636 (Eds. Stepanov, A. V.; Benevolenskaya, E. E.; Kosovichev, A. G.). University Press, Cambridge (2004)
Lagg, A.; Woch, J.; Krupp, N.; Gandorfer, A.; Solanki, S. K.: Temporal evolution of chromospheric downflows. In: Multi-Wavelength Investigations of Solar Activity, Proc. IAU Symp. 223, pp. 279 - 280 (Eds. Stepanov, A. V.; Benevolenskaya, E. E.; Kosovichev, A. G.). University Press, Cambridge (2004)
Loukitcheva, M. A.; Solanki, S. K.; White, S.: The solar chromosphere as seen in high-resolution millimeter observations. In: Multi-Wavelength Investigations of Solar Activity, Proc. IAU Symp. 223, pp. 643 - 644 (Eds. Stepanov, A. V.; Benevolenskaya, E. E.; Kosovichev, A. G.). University Press, Cambridge (2004)
Ning, Z.; Innes, D. E.; Solanki, S. K.: Dynamic behaviors of the quiet Sun seen by SUMER. In: Proc. SOHO 13 `Waves, Oscillations and Small-Scale Transient Events in the Solar Atmosphere: A Joint View from SOHO and TRACE', pp. 297 - 302 (Ed. Lacoste, H.). ESA Publ. Div., Noordwijk (2004)
Pauluhn, A.; Solanki, S. K.: Radiance emission by flaring activity. In: Proc. SOHO 13 `Waves, Oscillations and Small-Scale Transient Events in the Solar Atmosphere: A Joint View from SOHO and TRACE', pp. 323 - 328 (Ed. Lacoste, H.). ESA Publ. Div., Noordwijk (2004)
Pauluhn, A.; Solanki, S. K.: Small-Scale flares as the cause of quiet Sun EUV emission. In: Proc. SOHO 15 `Coronal Heating', pp. 501 - 506 (Eds. Walsh, R. W.; Ireland, J.; Danesy, D.; Fleck, B.). ESA Publ. Div., Noordwijk (2004)
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)
Raouafi, N.-E.; Solanki, S. K.: Effect of the electron density stratification on the off-limb O VI line profiles. In: Multi-Wavelength Investigations of Solar Activity, Proc. IAU Symp. 223, pp. 481 - 482 (Eds. Stepanov, A. V.; Benevolenskaya, E. E.; Kosovichev, A. G.). University Press, Cambridge (2004)
Seleznyov, A. D.; Krivova, N. A.; Solanki, S. K.: Understanding solar variability as groundwork for planet transit detection. In: Stars as Suns: Activity, Evolution, and Planets, p. CD-815-CD-819 (Eds. Dupree, A. K.; Benz, A. O.). Cambridge Univ. Press (2004)
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".
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.