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Wsdl: http://cagnode58.cs.tcd.ie:8080/helio-hps-server/hpsService?wsdl
Original Uploader

Workflow Propagation of CME from the Sun (1)

Created: 27/02/12 @ 08:59:22 | Last updated: 27/02/12 @ 08:59:23

Credits: User Anja Le Blanc

License: BSD License

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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.

Rating: 0.0 / 5 (0 ratings) | Versions: 1 | Reviews: 0 | Comments: 0 | Citations: 0

Viewed: 3 times | Downloaded: 6 times

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Original Uploader

Workflow Associate a Shock at Earth with Flare and ... (2)

Created: 15/11/11 @ 14:02:29 | Last updated: 20/07/12 @ 13:17:35

Credits: User Anja Le Blanc User David PS

License: Creative Commons Attribution-Share Alike 3.0 Unported License

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Using start date and end date all shock events at Earth are backpropagated to the Sun. Arround the time all flares (above certain levels) and cmes are assoicated. The possition of the flare and speed of the CME are used to forward propagate the event to Mars.

Rating: 0.0 / 5 (0 ratings) | Versions: 2 | Reviews: 0 | Comments: 0 | Citations: 0

Viewed: 9 times | Downloaded: 6 times

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Original Uploader

Workflow Connect flare events with proton events on... (2)

Created: 09/12/11 @ 11:27:45 | Last updated: 13/12/11 @ 15:27:02

Credits: User Anja Le Blanc

Attributions: Workflow Connect flare events with proton events on Earth via propagation model

License: Creative Commons Attribution-Share Alike 3.0 Unported License

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This workflow uses flares listed in any HELIO HEC flare catalogue (using the semantic mapping service), checks whether these flares are connected to Earth via the Parker spiral, and looks for proton events at earth listed in the goes_proton_event list. The flare listing and the proton listing are combinded into a list of VOTable outputs (one VOTable per flare catalogue with results).

Rating: 0.0 / 5 (0 ratings) | Versions: 2 | Reviews: 0 | Comments: 0 | Citations: 0

Viewed: 17 times | Downloaded: 6 times

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Original Uploader

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

Created: 13/03/12 @ 15:19:39 | Last updated: 13/03/12 @ 15:19:41

Credits: User Anja Le Blanc

License: BSD License

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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

Rating: 0.0 / 5 (0 ratings) | Versions: 1 | Reviews: 0 | Comments: 0 | Citations: 0

Viewed: 12 times | Downloaded: 5 times

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Original Uploader

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

Created: 22/02/12 @ 13:51:13 | Last updated: 22/02/12 @ 13:51:14

Credits: User Anja Le Blanc

License: Creative Commons Attribution-Share Alike 3.0 Unported License

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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

Rating: 0.0 / 5 (0 ratings) | Versions: 1 | Reviews: 0 | Comments: 0 | Citations: 0

Viewed: 13 times | Downloaded: 6 times

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Original Uploader

Workflow Find source at Sun of SW events on Earth (5)

Created: 15/11/11 @ 13:51:37 | Last updated: 24/05/12 @ 08:56:15

Credits: User Anja Le Blanc User David PS

License: Creative Commons Attribution-Share Alike 3.0 Unported License

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Try to detect the solar wind source on the Sun. Use backpropagation, ILS, HEC and HFC.

Rating: 0.0 / 5 (0 ratings) | Versions: 5 | Reviews: 0 | Comments: 0 | Citations: 0

Viewed: 18 times | Downloaded: 5 times

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Original Uploader

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

Created: 29/02/12 @ 14:59:28 | Last updated: 29/02/12 @ 14:59:30

Credits: User Anja Le Blanc

License: BSD License

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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

Rating: 0.0 / 5 (0 ratings) | Versions: 1 | Reviews: 0 | Comments: 0 | Citations: 0

Viewed: 8 times | Downloaded: 5 times

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Original Uploader

Workflow Back CIR-CME propagation model (1)

Created: 24/10/12 @ 16:09:33

Credits: User David PS User Anja Le Blanc

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

License: Creative Commons Attribution-Share Alike 3.0 Unported License

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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.

Rating: 0.0 / 5 (0 ratings) | Versions: 1 | Reviews: 0 | Comments: 0 | Citations: 0

Viewed: 2 times | Downloaded: 0 times

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Original Uploader

Workflow Propagation of the Solar Energetic Particl... (2)

Created: 13/12/11 @ 13:21:33 | Last updated: 03/02/12 @ 15:14:15

Credits: User Anja Le Blanc Network-member HELIO

License: Creative Commons Attribution-Share Alike 3.0 Unported License

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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

Rating: 0.0 / 5 (0 ratings) | Versions: 2 | Reviews: 0 | Comments: 0 | Citations: 0

Viewed: 19 times | Downloaded: 6 times

Tags (5):

Original Uploader

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

Created: 14/03/12 @ 11:56:05 | Last updated: 14/03/12 @ 11:56:06

Credits: User Anja Le Blanc

License: BSD License

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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

Rating: 0.0 / 5 (0 ratings) | Versions: 1 | Reviews: 0 | Comments: 0 | Citations: 0

Viewed: 9 times | Downloaded: 4 times

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