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Showing 6 results. Use the filters on the left and the search box below to refine the results.
Category: Workflow Type: Taverna 2 Tag: heliophysics User: Anja Le Blanc Licence: BSD Group: HELIO

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 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: User Anja Le Blanc

Workflow 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: User Anja Le Blanc

Workflow 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: User Anja Le Blanc

Workflow Filter CME events to events which could ha... (1)

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This workflow uses the initial time period to search for time periods where Earth and Mars are not further appart than 80 degrees. These time periods are used to find Halo CME events. The CME events are forward propagated to Earth and Sun. Only events were the propagation model predicts that both planets are on the propagation path will be included in the final VOTable

Created: 2012-02-29 | Last updated: 2012-02-29

Credits: User Anja Le Blanc

Workflow Propagation of CME from the Sun (1)

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Uses the processing service to calculate the objects (planets and observatories) which a CME might hit. Required longitude input is the longitude of the associated flare event.

Created: 2012-02-27 | Last updated: 2012-02-27

Credits: User Anja Le Blanc

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