Group: HELIO
This group is for workflows in the domain of heliophysics and solar physics
Created at: Thursday 14 August 2008 13:06:20 (UTC)
Unique name: helio
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David PS shared XPath From VOTableA 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.Wednesday 12 March 2014 06:43:32 (UTC)
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Anja Le Blanc shared Connect flare events with proton events on Earth via propagation modelThis workflow uses flares listed in the goes_sxf_flare list, checks wether this flare is 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 is combinded into a VOTable output.Wednesday 08 May 2013 14:52:17 (UTC)
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Anja Le Blanc shared Available instruments through DPASThis workflow uses a DPAS servlet to obtain all available intrument keys in the DPAS (Data Provider Access Service) and formats the return as VOTable.Wednesday 08 May 2013 14:52:01 (UTC)
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Anja Le Blanc shared DPAS simpel query workflowcall of the simpleQuery web service; all inputs are requested from the user; xml list as output file formatWednesday 08 May 2013 14:52:01 (UTC)
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Anja Le Blanc shared HEC standard querycalls the HEC web service; inputs are start and stop time, which table should be queried and an optional where clause, as in an SQL statement output is of VOTable formatWednesday 08 May 2013 14:52:01 (UTC)
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Gab shared When do the Fastest type II CME should be detected throughout all the heliosphere? (Returns single values, not a list)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 propagatio …Thursday 21 March 2013 16:44:44 (UTC)
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David PS shared Find data from a list of instruments and a time range where flares of certain intensity have happenedFor 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 …Wednesday 20 March 2013 17:33:38 (UTC)
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Nadia Cerezo shared Finding the origins of Solar Wind events at EarthThis 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 s …Friday 16 November 2012 12:52:01 (UTC)
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Workflow
Propagation of type II associated CME usin...
(3)
Created: 2014-02-11 | Last updated: 2014-02-17
Credits:
Eoincar
Anja Le Blanc
David PS
HELIO
Attributions:
When did the fastest type II CME happened?
Workflow
Ulysses/URAP radio quicklook from CDAWeb W...
(1)
Created: 2012-09-06
Credits:
Baptiste Cecconi
HELIO
Workflow
WIND/Waves radio quicklook from CDAWeb WSD...
(1)
Created: 2012-09-06
Credits:
Baptiste Cecconi
HELIO
Workflow
100CME_task1
(1)
Created: 2012-09-06 | Last updated: 2012-09-06
Credits:
Baptiste Cecconi
HELIO
Attributions:
Extract content of columns from VOTables
Workflow
Created: 2012-09-06 | Last updated: 2012-09-06
Credits:
Baptiste Cecconi
HELIO
Attributions:
Extract content of columns from VOTables
Workflow
Propagation of the Solar Energetic Particl...
(2)
Created: 2011-12-13 | Last updated: 2012-02-03
Credits:
Anja Le Blanc
HELIO
Linked Data
Non-Information Resource URI: http://www.myexperiment.org/groups/101
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