Version 4 (latest)
(of 4)
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Version created on:
15/05/12 @ 13:09:06
by:
Anja Le Blanc
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Revision comments
Title: Connect flare events with proton events on Earth via propagation model
Type: Taverna 2
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Description
This workflow uses flares listed in the goes_sxf_flare list, checks wether this flare is connected to Earth via the Parker spiral, and looks for proton events at earth listed in the goes_proton_event list.
The flare listing and the proton listing is combinded into a VOTable output.
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Earliest Version:
[1] - SEP event
Previous Versions:
[2] - Connect flare events with proton events on Earth via propagation model
Latest Version:
[4] - Connect flare events with proton events on Earth via propagation model
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Original Uploader |
Created: 13/03/12 @ 14:38:31 | Last updated: 13/03/12 @ 14:53:22
Credits:
Attributions:
License: Creative Commons Attribution-Share Alike 3.0 Unported License
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.
Rating: 0.0 / 5 (0 ratings) | Versions: 1 | Reviews: 0 | Comments: 0 | Citations: 0 Viewed: 1 time | Downloaded: 2 times Tags (12): |
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Original Uploader |
Created: 29/02/12 @ 14:59:28 | Last updated: 29/02/12 @ 14:59:30
Credits:
License: BSD License
This workflow uses the initial time period to search for time periods where Earth and Mars are not further appart than 80 degrees. These time periods are used to find Halo CME events. The CME events are forward propagated to Earth and Sun. Only events were the propagation model predicts that both planets are on the propagation path will be included in the final VOTable
Rating: 0.0 / 5 (0 ratings) | Versions: 1 | Reviews: 0 | Comments: 0 | Citations: 0 Viewed: 3 times | Downloaded: 3 times Tags (8): |
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Non-Information Resource URI: http://www.myexperiment.org/workflows/2566
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