Find source at Sun of SW events on Earth

Created: 2011-11-15 13:51:37      Last updated: 2012-05-24 08:56:15

Try to detect the solar wind source on the Sun. Use backpropagation, ILS, HEC and HFC.

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1. D. Pérez-Suárez, S. A. Maloney, P. A. Higgins, D. S. Bloomfield, P. T. Gallagher, G. Pierantoni, X. Bonnin, B. Cecconi, V. Alberti, K. Bocchialini, M. Dierckxsens, A. Opitz, A. Le Blanc, J. Aboudarham, R. B. Bentley, J. Brooke, B. Coghlan, A. Csillaghy, C. Jacquey, B. Lavraud and M. Messerotti, Studying Sun–Planet Connections Using the Heliophysics Integrated Observatory (HELIO), Paper, 27 September 2012, http://link.springer.com/article/10.1007%2Fs11207-012-0110-x/fulltext.html, Accessed at: 01 July 2013


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Workflow Associate a Shock at Earth with Flare and ... (2)

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Using start date and end date all shock events at Earth are backpropagated to the Sun. Arround the time all flares (above certain levels) and cmes are assoicated. The possition of the flare and speed of the CME are used to forward propagate the event to Mars.

Created: 2011-11-15 | Last updated: 2012-07-20

Credits: User Anja Le Blanc User David PS

Workflow Associate SEP events at Earth with flare, ... (1)

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This is the implementation of a use case worked on during CDAW3 of the HELIO project. SEP events propagated backward from Earth to the Sun. We allow for +- 30 min around the predicted time to search for flare events. The timing of the flare event informs the search time for Type III radio event (time_start to time_peak) and for the CME event (time_start to time_start+1h). Results are presented in a mulitlayered VOTable.

Created: 2012-03-13 | Last updated: 2012-03-13

Credits: User Anja Le Blanc User Rositsa

Attributions: Workflow Propagation of the Solar Energetic Particles to the Sun Workflow Extract content of columns from VOTables