Workflow Entry: Connect flare events with proton events on Earth via propagation model

Created at: 15/11/11 @ 13:57:35      Last updated: 15/05/12 @ 13:09:09
Information Version 4 (latest) (of 4)
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Version created on: 15/05/12 @ 13:09:06 by: Anja Le Blanc   |   Revision comments Expand

Title: Connect flare events with proton events on Earth via propagation model

Type: Taverna 2


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Information 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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Information Workflow Components

Information Authors (1)
Information Titles (1)
Information Descriptions (1)
Inputs (5)
Processors (16)
Beanshells (6)
Outputs (1)
Datalinks (33)
Coordinations (0)

Information Workflow Type

Taverna 2

Information Original Uploader

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Version History

Earliest Version:
[1] - SEP event

Created on: Tuesday 15 November 2011 @ 13:57:35 (GMT)

Created by: Anja Le Blanc

Revision comments:

None

Previous Versions:
[2] - Connect flare events with proton events on Earth via propagation model

Created on: Monday 05 December 2011 @ 15:40:48 (GMT)

Created by: Anja Le Blanc

Revision comments:

first implementation

[3] - Connect flare events with proton events on Earth via propagation model

Created on: Tuesday 13 December 2011 @ 13:55:42 (GMT)

Created by: Anja Le Blanc

Revision comments:

adopted to changes in propagation model

Latest Version:
[4] - Connect flare events with proton events on Earth via propagation model

Created on: Tuesday 15 May 2012 @ 13:09:06 (GMT)

Created by: Anja Le Blanc

Revision comments:

adjusted to new propagation model inputs; bug fix in createOutput



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Workflow Other workflows that use similar services (15)

Only the first 2 workflows that use similar services are shown. View all workflows that use these services.


Original Uploader

Workflow Associate SEP events at Earth with flare, cme and radio events on the Sun (v1)

Created: 13/03/12 @ 14:38:31 | Last updated: 13/03/12 @ 14:53:22

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

License: Creative Commons Attribution-Share Alike 3.0 Unported License

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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.

Rating: 0.0 / 5 (0 ratings) | Versions: 1 | Reviews: 0 | Comments: 0 | Citations: 0

Viewed: 1 time | Downloaded: 2 times

Tags (12):

Show View Download Download (v1)

Original Uploader

Workflow Filter CME events to events which could have been observed at Earth and Mars (v1)

Created: 29/02/12 @ 14:59:28 | Last updated: 29/02/12 @ 14:59:30

Credits: User Anja Le Blanc

License: BSD License

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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):

Show View Download Download (v1)

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Non-Information Resource URI: http://www.myexperiment.org/workflows/2566


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