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Showing 32 results. Use the filters on the left and the search box below to refine the results.
Type: Taverna 2 Tag: helio
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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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Workflow When did the fastest type II CME happened? (1)

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Simple query to the HELIO Event Catalogue to extract the start and end time of the fastest CME from the Wind Type II catalogue. Also it extracts the Xray Class from the flare associated to the CME

Created: 2012-10-21

Credits: User David PS User Eoincar

Attributions: Workflow Extract content of columns from VOTables

Workflow Get SecchiRH composites images (1)

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 This workflow extracts the composite image from the http://secchirh.obspm.fr survey page.

Created: 2012-09-06 | Last updated: 2012-09-06

Credits: User Baptiste Cecconi

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3463?size=60x60 Gab

Workflow LASCO_CME_QUERY (1)

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This workflows queries the LASCO CME list and returns a VOTable with the following fields pa, pa_width, v_final and v_diff which is abs(v_init-v_final)/2

Created: 2012-09-05

Credits: User Gab User Eoincar User Anja Le Blanc

Workflow Check the content of the Registry for mism... (1)

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This workflow check for tables which are registered in the HELIO registry but not available in the HFC and for tables which are in the UOC but which are not registred.

Created: 2012-07-26

Credits: User Anja Le Blanc

Workflow Check the content of the Registry for mism... (1)

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This workflow check for tables which are registered in the HELIO registry but not available in the UOC and for tables which are in the UOC but which are not registred.

Created: 2012-07-25

Credits: User Anja Le Blanc

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

Workflow Get data and images for a date +/- 12 hour... (1)

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From the date as input date +/- 12 hours of data from the MLSO web page is collated. Images for up to three images (closest to date; -1; +1) are created via autoplot

Created: 2012-05-24 | Last updated: 2012-05-24

Credits: User Anja Le Blanc

Workflow Available instruments through DPAS which a... (1)

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This workflow uses a DPAS servlet to obtain all available intrument keys in the DPAS (Data Provider Access Service) and formats the return as VOTable.

Created: 2012-03-16 | Last updated: 2012-03-16

Credits: User Anja Le Blanc

Attributions: Workflow Available instruments through DPAS Workflow Split VOTable into its values

Workflow Propagation of the Solar Energetic Particl... (1)

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use of the processing service to calculate time delays to the planets Inputs: time when propagation should start from the hit object hit_object where was the SEP event observed speed of the solar wind error value of solar wind speed beta traveling speed of energetic particals as percentage of the speed of light

Created: 2012-03-13 | Last updated: 2012-03-13

Credits: User Anja Le Blanc

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