Workflows

Back CIR-CME propagation model (1)

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With a observing time at an object and the type of PM that you want to run executes it and provides the plots and the time and longitude where it should be seen the origin of the event.

Created: 2012-10-24

Credits: David PS Anja Le Blanc

Attributions: CME backwards propagation Co-rotating Interaction Regions backwards propagation

Get all applications available on the HPS (1)

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This workflow requests all available applications on the HPS which do not require authentication to run. No inputs. Outputs contain all information to execute the application on the HPS such as the ID of the application and the names of all parameters.

Created: 2012-07-03

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

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: Anja Le Blanc

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

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: Anja Le Blanc

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: Anja Le Blanc

CME backwards propagation (1)

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Workflow propagates an CME event from its observing point (planet/spacecraft) back to the sun. The propagation also provides the timing of this event at other points in space (planet/spacecraft)

Created: 2012-02-23 | Last updated: 2012-02-23

Credits: Anja Le Blanc

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: 2012-02-22 | Last updated: 2012-02-22

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