Workflows

find events in xray and radio (7)

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instruments: hessiEC, phoenix2 attention: hessi name has changed!

Created: 2010-03-16 | Last updated: 2010-03-16

Credits: Anja Le Blanc

MDES simple execution (2)

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workflow to query MDES, obtaining the DES results and from it extracting the VOTable and the PNG plot for the time range queried.

Created: 2011-03-02 | Last updated: 2014-03-12

Credits: Anja Le Blanc

Extract content of columns from VOTables (3)

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Extracts all values from all columns which are passed from the input ColumnNames

Created: 2011-02-24 | Last updated: 2012-08-20

Credits: Anja Le Blanc

Instrument Capability Service Invocation w... (1)

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This workflow is an invocation ofthe Instrument Capability Service using the HELIO plugin built by Kevin Benson

Created: 2014-02-27

Invocation of instrument capability service (1)

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Simple invocation of the instrument capability service (ICS). Also shows what tables and table fields are available for searching.

Created: 2014-02-27

Credits: Eoincar

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?

Associate SEP events at Earth with flare, ... (1)

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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.

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

Credits: Anja Le Blanc Rositsa

Attributions: Propagation of the Solar Energetic Particles to the Sun Extract content of columns from VOTables

Radio lists search over time period (2)

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This workflow searches the wind stereo II IV radioburst list, wind tyhpe II soho cme list, hfc radioburst type III list, tsrs solar radio event list and combines the return of these lists chronologically. Only time_start, time_end, and comment sections are preserved in the result list.

Created: 2012-02-13 | Last updated: 2012-02-14

Credits: Anja Le Blanc

Propagation of the Solar Energetic Particl... (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 value of solar wind speed traveling speed of energetic particals as percentage of the speed of light

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

Credits: Anja Le Blanc HELIO

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