Talk (390)

3601.
Talk
Warnecke, J.; Käpylä, P. J.; Käpylä, M. J.; Brandenburg, A.: Magnetic field generation in the Sun driven by rotating Rayleigh-Bénard convection in spherical wedges. International Conference on Rayleigh-Benard Turbulence, Göttingen, Germany (2015)
3602.
Talk
Warnecke, J.; Käpylä, P. J.; Käpylä, M. J.; Brandenburg, A.: Understanding the equatorward migration of the Sun's magnetic field. NASA LWS Workshop on Solar Dynamo Frontiers, Boulder, Colorado, USA (2015)
3603.
Talk
Warnecke, J.; Käpylä, P. J.; Käpylä, M. J.; Rheinhard, M.; Brandenburg, A.: Understanding the solar dynamo form global dynamo simulations. 2nd International Sino-German Symposium of Solar Physics: Multi Waveband Observations and Modeling of Solar Activity, Bad Honnef, Germany (2015)
3604.
Talk
Warnecke, J.; Käpylä, P. J.; Käpylä, M. J.; Rheinhard, M.; Brandenburg, A.: Understanding Solar and Stellar Dynamos with numerical simulations. Annual Meeting of the Astronomische Gesellschaft, Kiel, Germany (2015)
3605.
Talk
Warnecke, J.; Käpylä, P. J.; Käpylä, M. J.; Rheinhard, M.; Brandenburg, A.: Understanding Solar and Stellar Activity with Numerical Simulations. CS Forum, School of Science, Aalto University, Finland (2015)
3606.
Talk
Warnecke, J.; Losada, I. R.; Brandenburg, A.; Kleeorin, N.; Rogachevskii, I.: Bipolar region formation in stratified two-layer turbulence. Sunspot formation: theory, simulations and observations, Stockholm, Sweden (2015)
3607.
Talk
Warnecke, J.; Losada, I. R.; Brandenburg, A.; Kleeorin, N.; Rogachevskii, I.: Bipolar region formation in stratified turbulence. Flux Emergence Workshop, Boulder, Colorado, USA (2015)
3608.
Talk
Wiegelmann, T.: Coronal magnetic field extrapolation. Solar Magnetic Fields: from Measurements towards Understanding, Bern, Switzerland (2015)
3609.
Talk
Wiegelmann, T.: Coronal modelling for Solar Orbiter. 16th Solar Orbiter SWT Meeting Numerical modeling support for Solar Orbiter (special MADAWG session), Göttingen, Germany (2015)
3610.
Talk
Wiegelmann, T.: Advanced modelling of the coronal magnetic field. IUGG, Prague, Czech Republic (2015)
3611.
Talk
Wiegelmann, T.: Solar magnetic activity and space weather. Workshop and Research visit on: The synergy of magnetic reconnection and waves in evolution of the solar corona, Weihai, China (2015)
3612.
Talk
Wiegelmann, T.: Solar coronal magnetic fields: Source region for space weather activity. 4. Nationaler Weltraumwetterworkshop, Neustrelitz, Germany (2015)
3613.
Talk
Yeo, K. L.; Krivova, N. A.; Solanki, S. K.: Measurements and models of solar irradiance variability in the satellite-era. Conference on Sun-Climate Connections, Kiel, Germany (2015)
3614.
Talk
Yeo, K. L.; Krivova, N. A.; Solanki, S. K.: Measurements and models of solar irradiance variability in the satellite-era. Conference on Sun-Climate Connections, Kiel, Germany (2015)
3615.
Talk
Yeo, K. L.; Krivova, N. A.; Solanki, S. K.: Solar irradiance variability since 1978 Reconciling measurements and models. AOGS 12th Annual Meeting, Singapore (2015)
3616.
Talk
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)
3617.
Talk
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)
3618.
Talk
Yeo, K. L.; Solanki, S. K.; Krivova, N. A.: Solar magnetic activity and solar irradiance variability since 1978. 2nd SOLARNET Meeting, Palermo, Italy (2015)
3619.
Talk
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)
3620.
Talk
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)
Go to Editor View