Content from the HELIO group

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

Run a Workflow on Taverna Server (local t2... (1)

Uses a local t2flow file to submit and run this workflow on the taverna server. You need a user name and password to execute this workflow. Input to the workflow which runs remotely will be requested interactively.

Created: 2012-02-20

Credits: Anja Le Blanc

Attributions: Run a Workflow on Taverna Server

Run a Workflow on Taverna Server (1)

Uses the URL to a t2flow file to submit and run this workflow on the taverna server. You need a user name and password to execute this workflow. Input to the workflow which runs remotely will be requested interactively.

Created: 2012-02-17 | Last updated: 2012-02-17

Credits: Anja Le Blanc

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

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HELIO Service Provider Set

Created: 2012-02-01 08:23:53 | Last updated: 2012-02-01 15:24:42

Credits: Anja Le Blanc

License: Creative Commons Attribution-Share Alike 3.0 Unported License

File type: XML

Comments: 0 | Viewed: 44 times | Downloaded: 30 times

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

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HELIO: Discovery and Analysis of Data in Heliophysics

Created: 2011-12-12 14:19:40 | Last updated: 2011-12-12 14:21:29

Credits: Donal Fellows

License: Creative Commons Attribution-Noncommercial-Share Alike 3.0 Unported License

File type: Adobe PDF

Comments: 0 | Viewed: 39 times | Downloaded: 216 times