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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

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HELIO Presentation at IEEE eScience 2011

Created: 2011-12-12 14:16:54

Credits: Donal Fellows

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

File type: PowerPoint 2007 presentation

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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

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HELIO Ontology

Created: 2012-03-05 11:25:21

Credits: Anja Le Blanc

License: Creative Commons Attribution 3.0 Unported License

File type: ZIP archive

Comments: 0 | Viewed: 53 times | Downloaded: 35 times

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HELIO Taverna Tutotial

Created: 2012-04-19 08:36:41 | Last updated: 2012-04-19 08:36:42

Credits: Anja Le Blanc

License: Creative Commons Attribution-Share Alike 3.0 Unported License

File type: PowerPoint presentation

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Introduction to Taverna and HELIO presentation

Created: 2012-04-19 09:00:18

Credits: Anja Le Blanc

License: Creative Commons Attribution-Share Alike 3.0 Unported License

File type: PowerPoint presentation

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HELIO Service List for Taverna 2.4

Created: 2012-08-30 09:45:06

Credits: Anja Le Blanc

License: BSD License

File type: XML

Comments: 0 | Viewed: 45 times | Downloaded: 32 times

Basic Call of HELIO Coordinate Transformat... (1)

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Transforms an input VOTable Coordinate set to a specified output VOTable Coordinate set. This workflow performs some remote computation and may take some time to complete.

Created: 2011-11-08 | Last updated: 2011-11-08

Credits: Anja Le Blanc

Basic Call of HELIO Coordinate Transformat... (2)

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Transforms an input VOTable Coordinate set to a specified output VOTable Coordinate set. This workflow performs some remote computation and may take some time to complete.

Created: 2011-11-09 | Last updated: 2012-07-09

Credits: Anja Le Blanc

Attributions: Basic Call of HELIO Coordinate Transformation Service

Find source at Sun of SW events on Earth (5)

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Try to detect the solar wind source on the Sun. Use backpropagation, ILS, HEC and HFC.

Created: 2011-11-15 | Last updated: 2012-05-24

Credits: Anja Le Blanc David PS

Connect flare events with proton events on... (4)

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This 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.

Created: 2011-11-15 | Last updated: 2012-05-15

Credits: 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.

Created: 2011-11-15 | Last updated: 2012-07-20

Credits: Anja Le Blanc David PS

Connect flare events with proton events on... (2)

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This workflow uses flares listed in any HELIO HEC flare catalogue (using the semantic mapping service), checks whether these flares are 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 are combinded into a list of VOTable outputs (one VOTable per flare catalogue with results).

Created: 2011-12-09 | Last updated: 2011-12-13

Credits: Anja Le Blanc

Attributions: Connect flare events with proton events on Earth via propagation model

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 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

Associate SEP events at Earth with flare, ... (1)

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This is the implementation of a use case worked on during CDAW3 of the HELIO project. SEP events propagated backward from Earth to the Sun. We allow for +- 30 min around the predicted time to search for flare events. The timing of the flare event informs the search time for Type III radio event (time_start to time_peak) and for the CME event (time_start to time_start+1h). Results are presented in a mulitlayered VOTable.

Created: 2012-03-13 | Last updated: 2012-03-13

Credits: Anja Le Blanc Rositsa

Attributions: Propagation of the Solar Energetic Particles to the Sun Extract content of columns from VOTables

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: 2012-03-13 | Last updated: 2012-03-13

Credits: 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

Get data and images for a date +/- 12 hour... (1)

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From the date as input date +/- 12 hours of data from the MLSO web page is collated. Images for up to three images (closest to date; -1; +1) are created via autoplot

Created: 2012-05-24 | Last updated: 2012-05-24

Credits: Anja Le Blanc

Check registry for wrongly registed and un... (2)

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HELIO registry contains a list of tables available in the HEC. The HEC contains a table with available talbes itself. This workflow shows the differences between these two lists.

Created: 2012-07-24 | Last updated: 2012-07-24

Credits: Anja Le Blanc

Check the content of the Registry for mism... (1)

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This workflow check for tables which are registered in the HELIO registry but not available in the UOC and for tables which are in the UOC but which are not registred.

Created: 2012-07-25

Credits: Anja Le Blanc

Check the content of the Registry for mism... (1)

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This workflow check for tables which are registered in the HELIO registry but not available in the HFC and for tables which are in the UOC but which are not registred.

Created: 2012-07-26

Credits: Anja Le Blanc

LASCO_CME_QUERY (1)

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This workflows queries the LASCO CME list and returns a VOTable with the following fields pa, pa_width, v_final and v_diff which is abs(v_init-v_final)/2

Created: 2012-09-05

Credits: Gab Eoincar Anja Le Blanc

Get SecchiRH composites images (1)

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 This workflow extracts the composite image from the http://secchirh.obspm.fr survey page.

Created: 2012-09-06 | Last updated: 2012-09-06

Credits: Baptiste Cecconi

Goes Flare Check WF (3)

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No description

Created: 2012-09-06 | Last updated: 2012-09-06

Credits: Baptiste Cecconi HELIO

Attributions: Extract content of columns from VOTables

WIND/Waves radio quicklook from CDAWeb WSD... (1)

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No description

Created: 2012-09-06

Credits: Baptiste Cecconi HELIO

Ulysses/URAP radio quicklook from CDAWeb W... (1)

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No description

Created: 2012-09-06

Credits: Baptiste Cecconi HELIO

When did the fastest type II CME happened? (1)

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Simple query to the HELIO Event Catalogue to extract the start and end time of the fastest CME from the Wind Type II catalogue. Also it extracts the Xray Class from the flare associated to the CME

Created: 2012-10-21

Credits: David PS Eoincar

Attributions: Extract content of columns from VOTables

When do the Fastest type II CME should be ... (2)

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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: 2012-10-21 | Last updated: 2013-03-20

Credits: David PS Eoincar Gab Baptiste Cecconi Shanem Jbyrne Florian Mayer Natasha A lynnyk

Attributions: LASCO_CME_QUERY LASCO_CME_QUERY MDES simple execution timeToTimeRange Forward CME propagation model (SHEBA) - defined outputs When did the fastest type II CME happened? Goes Flare Check WF 100CME_task1 Extract average Solar wind speed from ACE data

Solar Wind properties and plot (1)

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Using HELIO-MDES this workflow provides some properties of the solar wind from an input date and a mission and the plot +/-1 day for context.

Created: 2012-10-25

Credits: David PS

Attributions: MDES simple execution

HFC Synoptic map from date (1)

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query the HELIO Feature Catalogue, and retrieves the image with all the features catalgued for certain date.

Created: 2012-11-05

Credits: David PS

CDAW CME movie from date (1)

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generates the url for the input date to visualize CMEs and GOES xray light curve produced by CDAW at GSFC

Created: 2012-11-05

Credits: David PS

Attributions: HFC Synoptic map from date

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

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?

Produce vo table from helio catalogue (Cat... (1)

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A simple query of the Helio Event Catalogue (http://msslkz.mssl.ucl.ac.uk/helio_hec/HelioTavernaService?wsdl). User can enter catalogue name, time start, time end and desired paramter(s).

Created: 2014-01-13

Credits: Eoincar

Produce vo table from helio catalogue (Cat... (1)

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A simple query of the Helio Event Catalogue (http://msslkz.mssl.ucl.ac.uk/helio_hec/HelioTavernaService?wsdl). User can enter catalogue name, time start, time end, the desired parameter, parameter to order by, and limit on the search result.

Created: 2014-01-13

Credits: Eoincar

Produce vo table from helio catalogue (Cat... (1)

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A simple query of the Helio Event Catalogue (http://msslkz.mssl.ucl.ac.uk/helio_hec/HelioTavernaService?wsdl). User can enter catalogue name, time start, time end, and an SQL condition on the query.

Created: 2014-01-13

Credits: Eoincar

Invocation of instrument capability service (1)

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Simple invocation of the instrument capability service (ICS). Also shows what tables and table fields are available for searching.

Created: 2014-02-27

Credits: Eoincar

Instrument Capability Service Invocation w... (1)

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This workflow is an invocation ofthe Instrument Capability Service using the HELIO plugin built by Kevin Benson

Created: 2014-02-27