Session - Key solar observables for assessing long-term changes of the Geospace
Thierry Dudok de Wit, M. Haberreiter, A. Seppälä
Our understanding of long-term changes in the Heliosphere, and their potential impact on the Earth's climate, heavily relies on our ability to reconstruct past solar activity, on time scales of months to centuries. Most observables of past solar activity, such as the sunspot number, geomagnetic records, and cosmogenic isotope concentrations, are indirect, and thus rely on models to infer the state of the Sun. In recent years, major progress has been made in the collection of historic data, in their (re)analysis, thus shedding new light on how the Sun evolves on the long term.
We welcome contributions on the observables that describe the solar forcing of our Geospace, with a particular emphasis on long-term effects, and the impact on climate. Particular attention will be given to recent advances in the collection or understanding of these observables, but also important open issues, and roads for future improvement.
This session will have oral presentations (contributed and invited reviews), but we're also looking forward to going more in depth with an active and well-attended poster session. We welcome posters on important observables for climate research, including more technical and user-oriented issues such as data collection, data processing and the making of composites, how and where the data are available, how stable they are on the long run, etc.
Tuesday November 18, 11:00-13:00, auditorium Rogier
Tuesday November 18, 11:00-11:20, area in front of auditorium Rogier.
The posters will be introduced during the beginning of the oral part in auditorium Roger.
Talks: time schedule
|11:00||Introduction and Poster Summary followed by poster viewing|
||The New Sunspot Number: a Full Recalibration
||Clette, F et al.
||From Maunder Minimum to the recent Grand Solar Maximum
||Lockwood, M et al.
||On the Influence of Energetic Particle Precipitation on the Climate System: the Challenges and Problems in Measuring Energetic Electron Precipitation Into the Atmosphere.
||Clilverd, M et al.
||The Influence of Solar Variability Past, Present and Future, on North Atlantic Climate.
||Knight, J et al.
|13:00||End of session|
||A New "Brussels" Sunspot Number: Full Recomputation of the last 34 Years
||Clette, F; Lefèvre, L
||Making of Solar Spectral Irradiance Composites out of Multiple Datasets
||Scholl, M; Dudok de Wit, T; Haberreiter, M; Kopp, G; Kretzschmar, M
||Prediction of Amplitudes and Periods of Solar Cycles 24 and 25.
||Basurah, H; Baqatyan, S; Sharaf, A
||First Results of Statistical Analysis Applied on Different Solar Spectral Irradiance Datasets Acquired from Different Satellites
||Chehade, W; Weber, M; Burrows, J P
||Study of Solar cycle Evolution by a Recurrence Quantification Analysis of Solar cycle Indices
||Stangalini, M; Ermolli, I; Consolini, G; Giorgi, F
||Analysis of Ground-Based Full-Disk Synoptic Observations of the Solar Atmosphere for Solar Irradiance Reconstructions
||Ermolli, I; Giorgi, F; Cristaldi, A; Stangalini, M; Romano, P; Zuccarello, F|
||Error Analysis of a Multi-Instrument Composite Solar Mg II Index
||Weber, M; Chehade, W; Machol, J; Snow, M; Viereck, R
||Towards the Longterm Reconstruction of the Solar EUV Irradiance for Planetary Science Applications
||Haberreiter, M; Beer, J; Muscheler, R; Delouille, V; Mampaey, B4; Verbeeck, C; Schmutz, W
||Studying Solar Wind Properties using Pattern Recognition Methods
||Mursula, K; Holappa, L; Asikainen, T
||Solar EUV Modeling Efforts within the FP7 SOLID project
||Haberreiter, M; Dellouille, V; Del Zanna, G; Dammasch, I; Erhardt, C; Dominique, M; Erhardt, C; Jones, A; Kretzschmar, M; Mampaey, B; P, M; Schmitdke, G; Verbeeck, C; Wieman, S; Woods, T; Dudok de Wit, T; Schmutz, W
||Trend Detection and in Solar Irradiance Data: New Insight into the Recent Anomalous UV Observations
||Dudok de Wit, T; Kretzschmar, M; Schöll, M
||60 Years of Solar Multi-Wavelength Radio Observations as Proxies for Solar Radiative Forcing
||Dudok de Wit, T; Bruinsma, S; Shibasaki, K
: the note e
means this is an e-poster.