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Taverna 2

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Anja Le Blanc

find events in xray and radio (7)

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instruments: hessiEC, phoenix2 attention: hessi name has changed!

Created: 2010-03-16 | Last updated: 2010-03-16

Credits: Anja Le Blanc

Taverna 2

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Donal Fellows

Associate hessi flares with active regions (3)

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This workflow is querying the HFC ActiveRegions list and HEC hessi_flare list. It requires a time periode and a search radius arround the centre of an Active Region as inputs It produces two outputs: AnnotatedFeatureTable is a modified VOTable where a field is added with the number of associated hessi flares. CombinedTable is a 2 dimensional list with an VOTable for each Active region and one with an VOTable for all associated flares for that Active Region.

Created: 2011-06-22 | Last updated: 2012-07-10

Credits: Donal Fellows

Taverna 2

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Anja Le Blanc

MDES simple execution (2)

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workflow to query MDES, obtaining the DES results and from it extracting the VOTable and the PNG plot for the time range queried.

Created: 2011-03-02 | Last updated: 2014-03-12

Credits: Anja Le Blanc

Taverna 2

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Anja Le Blanc

Extract content of columns from VOTables (3)

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Extracts all values from all columns which are passed from the input ColumnNames

Created: 2011-02-24 | Last updated: 2012-08-20

Credits: Anja Le Blanc

Taverna 2

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David PS

XPath From VOTable (1)

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A XPath From text version for VOTables. This is useful to extract certain information from the header of the VOTables but it could work for any XPath.

Created: 2014-03-12

Credits: David PS Anja Le Blanc

Attributions: Extracting data from VOTable format by using XPath query

Taverna 2

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Gab

When do the Fastest type II CME should be ... (1)

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The fastest CME is found from an interval of time, and propagated to Earth, in two steps, first to obtain the Solar wind speed at Earth and then propagated again with a more reasonable CME speed. The output produces Min-Max ETAs for each object in the heliosphere and the plots of the final propagation model. This Workflow was produced as one of the challenges in the HELIO CDAW-IV hosted at TCD

Created: 2013-03-21

Credits: Gab Anja Le Blanc David PS

Attributions: When did the fastest type II CME happened?

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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David PS

Finding the origins of Solar Wind events a... (6)

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This gives a comprenhensive overview of high speed solar wind events (CME or CIR) seen at Eart, by obtaining the maximum in-situ measure velocity from the data evaluation service (DES), propagating the even backwards to Earth using the HELIO processing service (HPS) and SHEBA propagation model, and search whether halo CMEs or CHs were observed on that time, and retrieves, besides all the previous information, a context solar wind plot (+/- 1 day) and a URL linking to a context movie for CMEs...