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?

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: Anja Le Blanc

Check in UOC which instruments were observ... (2)

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Query of the UOC to find the instrument_observatory keys for instruments which were observing at a given time period and a given location.

Created: 2012-03-15 | Last updated: 2012-03-15

Credits: Anja Le Blanc

Split VOTable into its values (1)

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This workflow takes a single VOTable and splits it up in a vector for the names of fields, a vector for the UCDs of the fields, a vector for the UTypes of the fields, and a two dimensional vector for the values.

Created: 2012-03-14 | Last updated: 2012-03-14

Credits: Anja Le Blanc

Co-rotating Interaction Regions backwards ... (1)

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Run the cir backwards propagation code on the HELIO processing service. Required inputs: time start of backwards propagation, the object (planet/spacecraft) from where the propagation should start, assumed solar wind speed at the time, assumed error of solar wind speed Output: VOTable with times at different points in solar system

Created: 2012-03-14 | Last updated: 2012-03-14

Credits: Anja Le Blanc