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Group: HELIO Wsdl: http://manunja.cesr.fr/Amda-Helio/WebServices/HelioLongQueryService.wsdl
Original Uploader

Workflow Finding the origins of Solar Wind events a... (2)

Created: 16/11/12 @ 12:51:59 | Last updated: 16/11/12 @ 12:56:37

Credits: User David PS

Attributions: Workflow CME backwards propagation Workflow Co-rotating Interaction Regions backwards propagation Workflow HFC Synoptic map from date Workflow CDAW CME movie from date Workflow Solar Wind properties and plot Workflow Back CIR-CME propagation model Workflow LASCO_CME_QUERY

License: Creative Commons Attribution-Share Alike 3.0 Unported License

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This gives a comprenhensive overview of high speed solar wind events (CME or CIR) seen at Eart, by obtaining the maximum in-situ measure velocity from the data evaluation service (DES), propagating the even backwards to Earth using the HELIO processing service (HPS) and SHEBA propagation model, and search whether halo CMEs or CHs were observed on that time, and retrieves, besides all the previous information, a context solar wind plot (+/- 1 day) and a URL linking to a context movie for CMEs...

Rating: 0.0 / 5 (0 ratings) | Versions: 2 | Reviews: 0 | Comments: 0 | Citations: 0

Viewed: 7 times | Downloaded: 0 times

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Original Uploader

Workflow When do the Fastest type II CME should be ... (1)

Created: 21/10/12 @ 19:00:36

Credits: User David PS User Eoincar User Gab User Baptiste Cecconi User Shanem User Jbyrne User Florian Mayer User Natasha User A lynnyk

Attributions: Workflow LASCO_CME_QUERY Workflow LASCO_CME_QUERY Workflow DES simple execution Workflow timeToTimeRange Workflow Forward CME propagation model (SHEBA) - defined outputs Workflow When did the fastest type II CME happened? Workflow Goes Flare Check WF Workflow 100CME_task1 Workflow Extract average Solar wind speed from ACE data

License: Creative Commons Attribution-Share Alike 3.0 Unported License

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The fastest CME is found from an interval of time, and propagated to Earth, in two steps, first to obtain the Solar wind speed at Earth and then propagated again with a more reasonable CME speed. The output produces Min-Max ETAs for each object in the heliosphere and the plots of the final propagation model. This Workflow was produced as one of the challenges in the HELIO CDAW-IV hosted at TCD

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

Viewed: 23 times | Downloaded: 4 times

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Original Uploader

Workflow Solar Wind properties and plot (1)

Created: 25/10/12 @ 07:48:20

Credits: User David PS

Attributions: Workflow DES simple execution

License: Creative Commons Attribution-Share Alike 3.0 Unported License

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Using HELIO-MDES this workflow provides some properties of the solar wind from an input date and a mission and the plot +/-1 day for context.

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

Viewed: 4 times | Downloaded: 0 times

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Original Uploader

Workflow DES simple execution (1)

Created: 02/03/11 @ 15:19:52 | Last updated: 20/10/11 @ 15:34:11

Credits: User Anja Le Blanc

License: Creative Commons Attribution-Share Alike 3.0 Unported License

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workflow to test DES

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

Viewed: 23 times | Downloaded: 11 times

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