Yeo, K. L.; Krivova, N. A.; Solanki, S. K.: Discrepancy between the various UV SSI records and reconstructions, and the underlying causes. SOLARIS-HEPPA Working Group Meeting, Boulder, Colorado, USA (2015)
Yeo, K. L.; Krivova, N. A.; Solanki, S. K.: SATIRE-S reconstruction of TSI and SSI since 1974. 2015 Sun-Climate Symposium, Savannah, Georgia, USA (2015)
Yeo, K. L.; Solanki, S. K.; Krivova, N. A.: Solar magnetic activity and solar irradiance variability since 1978. 2nd SOLARNET Meeting, Palermo, Italy (2015)
Ball, W.; Haigh, J.; Krivova, N.; Unruh, Y.; Solanki, S.: The SATIRE-S model and why getting solar cycle spectral irradiance trends correct is so important. EGU General Assembly, Vienna, Austria (2014)
Ball, W. T.; Krivova, N. A.; Solanki, S. K.; Unruh, Y. C.; Haigh, J. D.; Mortlock, D.; Jaffe, A.; Egerton, J.; Harder, J.: Spectral solar irradiance and the limits in understanding the effect of irradiance on stratospheric ozone. seminar, Cambridge University, UK (2014)
Ball, W. T.; Krivova, N. A.; Solanki, S. K.; Unruh, Y. C.; Haigh, J. D.; Mortlock, D.; Jaffe, A.; Egerton, J.; Harder, J.: Solar irradiance and Stratospheric ozone. Seminar, University of Montreal, Canada (2014)
Ball, W. T.; Krivova, N. A.; Solanki, S. K.; Unruh, Y. C.; Haigh, J. D.; Mortlock, D.; Jaffe, A.; Egerton, J.; Harder, J.: Our current understanding of solar irradiance and its effect on stratospheric ozone. Seminar, Davos, Switzerland (2014)
Ball, W. T.; Yeo, K. L.; Krivova, N. A.; Solanki, S. K.; Unruh, Y. C.; Haigh, J. D.; Mortlock, D.; Egerton, J. S.: Spectral solar irradiance and limits on understanding the effect on stratospheric ozone. seminar, Kiel, Germany (2014)
Dasi-Espuig, M.; Unruh, Y.; Krivova, N. A.; Solanki, S. K.; Jiang, J.: Modeling of spectral irradiance based on modeled proxies. SOLID annual meeting, Bremen, Germany (2014)
Krivova, N.: Spectral And Total IRradiance REconstructions (SATIRE): Update. TOSCA/SOLID Workshop Long-term variations of solar activity and their impacts: From the Maunder Minimum to the 21st century, Corfu, Greece (2014)
Krivova, N.: The solar cycle 24 and predictions of future solar variability. 5th International HEPPA Workshop in conjunction with SPARC/SOLARIS-HEPPA, Baden-Baden, Germany (2014)
Yeo, K. L.; Solanki, S. K.; Krivova, N. A.: Solar irradiance variability and the Earth's climate. SCOSTEP's 13th Quadrennial Solar-Terrestrial Physics Symposium, Xi'an, China (2014)
Wu, C.-J.; Krivova, N.; Solanki, S.; Usoskin, I.: Solar Total and Spectral Irradiance reconstruction over last 9000 years. Space Climate 6, Levi, Finland (2016)
Wu, C.-J.; Krivova, N.; Solanki, S. K.; Usoskin, I.: Solar Total and Spectral Irradiance Reconstruction over Last 9000 Years. Space Climate 6 symposium, Levi, Finland (2016)
Wu, C.-J.; Krivova, N.; Solanki, S. K.; Usoskin, I.: Solar Total and Spectral Irradiance Reconstruction over Last 9000 Years. AGU Fall Meeting, San Francisco, USA (2016)
First Light for Sunrise III: the first tests with real sunlight were successful. The balloon-borne solar observatory should be ready for launch at the end of May.
First icy cold, then midnight sun: at the Arctic Circle, the team will prepare the next flight of the balloon-borne solar observatory - and hopes for solar fireworks.
Astronomical teamwork: By combining data from Solar Orbiter and SDO, a group of researchers has unambiguously determined the magnetic field at the solar surface.
The magnetic field in the solar atmosphere exceeds the geomagnetic field strength by four orders of magnitude. It greatly influences the processes of energy transport within the solar atmosphere, and dominates the morphology of the solar chromosphere and corona. Kinetic energy from convective motions in the Sun can be efficiently stored in magnetic fields and subsequently released - to heat the solar corona to several million degrees or to blast off coronal mass ejections.