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Fifth Solar Orbiter Workshop
September 10 - 14, 2012 - Brugge, Belgium
PRESENTATIONS
Session 1 - Solar magnetism and the solar cycle
A. Brandenburg - The Solar Dynamo
M. Roth - Review on Helioseismology and Helioseismology with Solar Orbiter
S. Brun - Solar Magnetic Field Reversal and the Role of the Dynamo Families
A. Birch - Planning for Helioseismology with SO/PHI
J. Borrero - Recent Observations of Solar Magnetic Fields with Hinode, SDO and Sunrise
V. Domingo - Small Magnetic Elements, Bright Points and Solar Irradiance
C.J. Schrijver - Reaction fo the Outer Solar Atmosphere to the Solar Cycle
M.J. Owens - The Solar Cycle as seen in the Heliospheric Magnetic Field
G. Erdos - The heliospheric magnetic flux density through several solar cycles
Session 2 - Processes of slow/steady energy release in the solar atmosphere and heliosphere
H. Warren - Heating of the Solar Corona: An Observational Perspective
B. Gudiksen - Heating of the Solar Corona: Modeling Perspective
P. Zacharias - Ejection of Cool Plasma into the Corona - Comparison of 1D and 3D Loop Models
A. Gabriel - Outflow Velocity Structure in the Upper Transition Region and Corona
A.F. Rappazzo - Interchange Reconnection in a Turbulent Corona
M. Velli - Acceleration of Fast and Slow Solar Wind
L. Abbo - Slow Solar Wind Coronal Sources: Comparison between two Solar Minima of UVCS/SOHO Data and New perspectives with METIS/SOLO Data
J.D. Moses - The Helium corona as observed by the HERSCHEL Sounding Rocket
G. Del Zanna - Linking in-situ Measurements with SPICE
S.T. Lepri - Understanding the Nature of the Solar Wind in the Solar Orbiter Era
L. Matteini - Kinetic Processes in the Solar Wind
A. De Groof - SWAP/PROBA2 Observations of the Large-scale, Long-term Evolution of the EUV Corona
A. Vourlidas - The Slow Solar Wind Structure as Revealed by Periodic Analysis of White Light Images
Session 3 - Eruptive processes in the solar atmosphere and their manifestations in the heliosphere
E. Kontar - Physics of solar flares
M. Battaglia - Direct Imaging and Spectroscopy of Flare Accelerated Electron Beams with STIX
L. Harra - Pre-flare Signatures in Large Flares
A. Asai - CME Eruption and Accompanying Phenomena Observed in the Low Corona
A. Bemporad - Observations of Coronal Mass Ejections in the Outer Corona
S. Matthews - Changes in the Photospheric Magnetic Field during CMEs
I. Roussev - Recent Advances in Understanding the Nature of CMEs by Combining Solar Observations with Numerical Simulations
M. Zhang - CMEs: Taking Magnetic Helicity from Low Corona into Interplanetary Space
R. Susino - Observation of a Post-CME Current Sheet with SOHO/UVCS and RHESSI
B. Lavraud - Magnetic Cloud Erosion by Magnetic Reconnection during Propagation, and Impact on Geo-Effectiveness
D. Telloni - Evidence for Rayleigh-Taylor plasma instabilities at the front of solar Coronal Mass Ejections
C. Cohen - Energetic Particle Acceleration on the Sun and in the Heliosphere
K.L. Klein - Solar Energetic Particle Events and their Parent Activity - A Reassessment of Statistical Relationships
D. Lario - Radial Dependence of Solar Energetic Particle Intensities
A. Aran - Influence of the Interplanetary Shock on the Heliocentrical Radial Variations of Gradual SEP Events
R. Bruno - Observations of Solar Wind Coherent Structures During SEP Dropouts Events
Session 4 - Data assimilation, visualization and analysis
A. Rouillard - Connecting Solar and Heliospheric Observations
J. Linker - Modeling the Corona and Solar Wind using Synchronic Maps
D.R. Williams - Mass Estimates of Rapidly-moving Prominence Material from High-cadence EUV Images
A. Zaslavsky - Dust Detection with Radio Instruments: Possible Application for the Radio and Plasma Wave (RPW) Experiment onboard Solar Orbiter
M.K. Georgoulis - Solar Flare Forecasting from Solar Orbiter observations
D. Müller - Visualizing the Sun and Heliosphere in 3D
P. Gallagher - The Heliophysics Integrated Observatory (HELIO) - A new Tool to study the Heliosphere
C.E. Fischer - Pushing Solar Image Compression to its Limit
V. Delouille - Exploring Heterogeneous Solar Data
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