Search results for "helio"

When do the Fastest type II CME should be ... (2)

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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

Created: 2012-10-21 | Last updated: 2013-03-20

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

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

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HELIO Ontology

Created: 2012-03-05 11:25:21

Credits: Anja Le Blanc

License: Creative Commons Attribution 3.0 Unported License

File type: ZIP archive

Comments: 0 | Viewed: 53 times | Downloaded: 35 times

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

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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

Created: 2013-03-21

Credits: Gab Anja Le Blanc David PS

Attributions: When did the fastest type II CME happened?

Retrieve Instruments for event dates (2)

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Queries the HELIO ICS web service and returns a list of instruments available for the time periodes in VOTable format

Created: 2010-05-26

Credits: Anja Le Blanc

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HELIO Taverna Tutotial

Created: 2012-04-19 08:36:41 | Last updated: 2012-04-19 08:36:42

Credits: Anja Le Blanc

License: Creative Commons Attribution-Share Alike 3.0 Unported License

File type: PowerPoint presentation

Comments: 0 | Viewed: 54 times | Downloaded: 45 times

Propagation of the Co-roationg interaction... (2)

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use of the processing service to calculate time delays to the planets Inputs: time when propagation should start longitude of starting point on the sun speed of the solar wind error speed of the solar wind

Created: 2011-12-13 | Last updated: 2012-02-03

Credits: Anja Le Blanc

Connect flare events with proton events on... (2)

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This workflow uses flares listed in any HELIO HEC flare catalogue (using the semantic mapping service), checks whether these flares are 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 are combinded into a list of VOTable outputs (one VOTable per flare catalogue with results).

Created: 2011-12-09 | Last updated: 2011-12-13

Credits: Anja Le Blanc

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

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HELIO Service Provider Set

Created: 2012-02-01 08:23:53 | Last updated: 2012-02-01 15:24:42

Credits: Anja Le Blanc

License: Creative Commons Attribution-Share Alike 3.0 Unported License

File type: XML

Comments: 0 | Viewed: 44 times | Downloaded: 30 times

HFC Synoptic map from date (1)

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query the HELIO Feature Catalogue, and retrieves the image with all the features catalgued for certain date.

Created: 2012-11-05

Credits: David PS

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HELIO Service List for Taverna 2.4

Created: 2012-08-30 09:45:06

Credits: Anja Le Blanc

License: BSD License

File type: XML

Comments: 0 | Viewed: 41 times | Downloaded: 30 times