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Tag: helio
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Blob HELIO: Discovery and Analysis of Data in Heliophysics

Created: 2011-12-12 14:19:40 | Last updated: 2011-12-12 14:21:29

Credits: User Donal Fellows

License: Creative Commons Attribution-Noncommercial-Share Alike 3.0 Unported License

 This is the camera-ready copy of the HELIO eScience paper for IEEE eScience 2011.

File type: Adobe PDF

Comments: 0 | Viewed: 39 times | Downloaded: 216 times

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Blob HELIO Presentation at IEEE eScience 2011

Created: 2011-12-12 14:16:54

Credits: User Donal Fellows

License: Creative Commons Attribution-Noncommercial-Share Alike 3.0 Unported License

 This is the presentation that I gave at the 7th IEEE International eScience Conference, Stockholm, December 2011. It is on the HELIO project, and particularly on the scientific challenges of heliophysics that are of interest to people working in the eScience domain.

File type: PowerPoint 2007 presentation

Comments: 0 | Viewed: 44 times | Downloaded: 29 times

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Workflow Produce vo table from helio catalogue (Cat... (1)

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A simple query of the Helio Event Catalogue (http://msslkz.mssl.ucl.ac.uk/helio_hec/HelioTavernaService?wsdl). User can enter catalogue name, time start, time end and desired paramter(s).

Created: 2014-01-13

Credits: User Eoincar

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Workflow Produce vo table from helio catalogue (Cat... (1)

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A simple query of the Helio Event Catalogue (http://msslkz.mssl.ucl.ac.uk/helio_hec/HelioTavernaService?wsdl). User can enter catalogue name, time start, time end, and an SQL condition on the query.

Created: 2014-01-13

Credits: User Eoincar

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Workflow Produce vo table from helio catalogue (Cat... (1)

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A simple query of the Helio Event Catalogue (http://msslkz.mssl.ucl.ac.uk/helio_hec/HelioTavernaService?wsdl). User can enter catalogue name, time start, time end, the desired parameter, parameter to order by, and limit on the search result.

Created: 2014-01-13

Credits: User Eoincar

Workflow Check registry for wrongly registed and un... (2)

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HELIO registry contains a list of tables available in the HEC. The HEC contains a table with available talbes itself. This workflow shows the differences between these two lists.

Created: 2012-07-24 | Last updated: 2012-07-24

Credits: User Anja Le Blanc

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Blob Introduction to Taverna and HELIO presentation

Created: 2012-04-19 09:00:18

Credits: User Anja Le Blanc

License: Creative Commons Attribution-Share Alike 3.0 Unported License

Introductorily presentation to Taverna for HELIO users. It was given as part of the Taverna workshop for HELIO.

File type: PowerPoint presentation

Comments: 0 | Viewed: 58 times | Downloaded: 55 times

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Workflow 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: 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 MDES 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

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Blob HELIO Ontology

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

Credits: User Anja Le Blanc

License: Creative Commons Attribution 3.0 Unported License

This zip file contains the current version of the HELIO Ontology, a heliophysics ontology containing the concepts of all sub-communities to enable cross-mapping.

File type: ZIP archive

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

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3463?size=60x60 Gab

Workflow 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: User Gab User Anja Le Blanc User David PS

Attributions: Workflow When did the fastest type II CME happened?

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