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Wsdl: http://msslkz.mssl.ucl.ac.uk/helio-dpas/HelioTavernaService?wsdl

or http://msslkz.mssl.ucl.ac.uk/helio-hec/HelioTavernaService?wsdl

or http://msslkz.mssl.ucl.ac.uk/helio-ics/HelioTavernaService?wsdl

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Taverna 2

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David PS

Find data from a list of instruments and a... (1)

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For a certain time range, it looks for flares between a energy range (GOES x-ray flare class), and it provides the observations for such time range for the list of instruments asked. It also provides the table of flares with its properties. Note: This workflow does not look whether the instrument was not looking to the right field of view (eg., CDS)

Created: 2013-03-20

Credits: David PS Anja Le Blanc Nadia Cerezo Gab

Attributions: find events in xray and radio

Taverna 2

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Anja Le Blanc

Available instruments through DPAS which a... (1)

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This workflow uses a DPAS servlet to obtain all available intrument keys in the DPAS (Data Provider Access Service) and formats the return as VOTable.

Created: 2012-03-16 | Last updated: 2012-03-16

Credits: Anja Le Blanc

Attributions: Available instruments through DPAS Split VOTable into its values

Taverna 2

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Anja Le Blanc

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

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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.