Propagation of the Co-roationg interaction region from the Sun

Created: 2011-12-13 11:09:59      Last updated: 2012-02-03 15:39:23

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

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Review Title: Propagation model

Rating: 5 out of 5

Created: 2012-01-03 17:07:51 | Updated: 2012-01-03 17:07:51

I have been running this workflow as part of a learning curve in the use of Taverna in heliophysics. I used the cut and paste method from the URL given on the myExperiment page into the Taverna workbench. The workflow ran very nicely and is well documented on the myExperiment site so that it is clear what the inputs and ouputs refer to. It is a nice evocation of the Trinity College propagation model which is a good example of how to present an application as a web service.

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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

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