Program
| Sunday, August 17 | ||||
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| @ | 13:16, 14:16, 15:16, 16:16, 17:17, 18:17, 19:14 | Shuttle busses from Marloie Railway station to Conference center | ||
| 19:00 | Welcome reception | |||
| Monday, August 18 | ||||
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| 8:30 | 9:00 | Registration | ||
| 9:00 | 9:15 | Welcome | ||
| Tutorial | ||||
| 9:15 | 9:55 | A whistle-stop tutorial on observational turbulence studies: Background and motivation for a statistical treatment – K. Kiyani | ||
| Session 2 : Optimal combination of in-situ and imaging data. | ||||
| 9:55 | 10:30 | Invited: Combining HI and in situ observations to constrain CME evolution - C. Möstl | ||
| 10:30 | 11:00 | Coffee Break | ||
| 11:00 | 12:30 | Invited: Processing and Analyzing Images of Coronal Mass Ejections - T. Howard | ||
| Visual Verification of Coronal Mass Ejections in ENLIL Ensemble Simulations through Optical Flow Analysis - A. Bock | ||||
| The new CORIMP CME catalog & 3D reconstructions - J. Byrne | ||||
| 12:30 | 14:00 | Lunch at Le Floreal | ||
| 14:00 | 14:40 | Kinematic of CMEs using SECCHI/HI observations - N. Srivastava | ||
| 3D morphological reconstruction of CMEs and CME-driven shocks from SECCHI COR and HI1 observations and their link to in-situ measurements - L. Feng | ||||
| Splinter Session | ||||
| 14:40 | 15:00 | Presentation of the Working Groups | ||
| 15:00 | 16:00 | Working group session (more information) | ||
| 16:00 | 16:30 | Coffee break | ||
| 16:30 | 18:00 | Poster presentation for Sessions 1, 2, 3 | ||
| 18:00 | 20:00 | Demo-session (more information) | ||
| 19:00 | 20:00 | A taste of regional beers & Snack | ||
| End of the day | ||||
| Tuesday, August 19 | ||||
|---|---|---|---|---|
| Tutorial | ||||
| 9:00 | 9:40 | Introduction to supervised learning – R. D’Ambrosio | ||
| Session 4: Tracking of small scale magnetic features and its applications | ||||
| 9:40 | 10:30 | Invited: Small-scale magnetic structure at the solar surface - M. Schüssler | ||
| 10:30 | 11:00 | Coffee Break | ||
| 11:00 | 12:30 | Invited: Surface magnetic flux and its evolution - C. Parnell. | ||
| Magnetic Feature Tracking and the Small-Scale Solar Dynamo - D. Lamb | ||||
| Analysis of long-term magnetic flux transport on the solar surface by auto-tracking technique of patches. - Y. Iida | ||||
| Discussion | ||||
| 12:30 | 14:00 | Lunch at Le Floréal | ||
| 14:00 | 15:00 | Calculating solar differential rotation by automatic tracking of CBPs with hybrid PSO-Snake algorithm - E. Shahamatnia | ||
| Can flux cancellation build-up magnetic flux ropes? - S. Yardley | ||||
| Continuous Solar Magnetic Carpet - A. Gorobets | ||||
| 15:00 | 15:30 | Coffee break | ||
| 15:30 | 16:30 | Poster presentation for Sessions 4, 5, and extra-session posters | ||
| Micro-workshop session | ||||
| 16:30 | 19:00 | Micro-workshop (more information) | ||
| End of the day | ||||
| Wednesday, August 20 | ||||
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| Session 3: How well can we predict solar eruptions and disturbances? | ||||
| 9:00 | 10:30 | Invited: The Physics Behind Flare Prediction and Present Methods for Flare Forecasting - G. Barnes | ||
| Invited: : Machine Learning for Solar Flare Prediction - R. D'Ambrosio | ||||
| 10:30 | 11:00 | Coffee Break | ||
| 11:00 | 12:30 | Automated Detection of δ-spots. - S. Padinhatteeri | ||
| Image patch analysis and clustering of sunspots: A dimensionality reduction approach - K. Moon | ||||
| Systematic measurements of global variations in the coronal magnetic field using ``EIT waves'' - D. Long | ||||
| Solar Demon - Detecting Flares, Dimmings and EUV waves on SDO/AIA images - E. Kraaikamp | ||||
| Discussion | ||||
| 12:30 | 14:00 | Lunch at Le Floréal | ||
| Session 5: Origin of variability and prediction of solar wind. | ||||
| 14:00 | 15:00 | Invited: A multi-scale approach to the analysis of anisotropic plasma turbulence (or studying turbulence wearing wavelet spectacles) - K. Kiyani | ||
| A multifractal analysis of air temperature signals based on the wavelet leaders method - A. Deliège | ||||
| 15:00 | 15:30 | Coffee break | ||
| Working group session | 15:30 | 17:30 | Working group session (more information) | |
| 18:00 | Sharp! | Departure for Bastogne (stop at Panoramic view in Nadrin and at Mardasson in Bastogne) |
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| 19:30 | Conference dinner | |||
| Return to La Roche around 23:30 | ||||
| Thursday, August 21 | ||||
|---|---|---|---|---|
| Session 1: Power laws in solar physics: observations and proper estimation. | ||||
| 9:00 | 10:30 | Invited: On Power-law Distributions of Observed Solar Features - C. Parnell | ||
| Invited: Bayesian Analysis of Power Law Models in High-Energy Astrophysics and in Solar Physics - D. van Dyk | ||||
| 10:30 | 11:00 | Coffee Break | ||
| Session 5: Origin of variability and prediction of solar wind. | ||||
| 11:00 | 11:45 | Invited: Turbulence, nonlinear dynamics, and sources of intermittency and variability in the solar wind. - W. Matthaeus | ||
| Future SIP Challenges | ||||
| 11:45 | 12:30 | Invited: Imaging Techniques for High-Resolution and Instantaneous Observations of the Solar Corona - F. Kamalabadi | ||
| 12:30 | 14:00 | Lunch at Le Floréal | ||
| 14:00 | 15:00 | Report from the Working groups | ||
| Panel discussion | 15:00 | 15:15 | Big Data, Big Challenges, and Big Ideas in 21st Century Astrostatistics - David Van Dyk | |
| 15:15 | 17:00 | Panel discussion on SIP challenges (more information) | ||
| 17:00 | 19:00 | Social activities | ||
| 19:30 | BBQ (organized by Le Floréal) See barbecue page for more info. | |||
| Friday, August 22 | ||||
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| @ | 7:45, 8:45, 9:45, 10:45, 11:45 | Shuttle busses from Conference center to Marloie Railway station (~40 minutes journey) | ||
