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Items tagged with "helio event catalog" (9)

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Workflows (9)

Workflow Find common events in HEC tables which use... (5)

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Use only tables which provide lat_hg and long_hg. Inputs: table names of two HEC tables; time interval in which the search is being conducted; delta for time and location to enlarge the search space. Output: VOTable which combines the resultset of the HEC by the common event.

Created: 2011-08-03 | Last updated: 2012-02-03

Credits: User Anja Le Blanc

Workflow 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: User Anja Le Blanc

Workflow 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: User Anja Le Blanc

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

Workflow Radio lists search over time period (2)

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This workflow searches the wind stereo II IV radioburst list, wind tyhpe II soho cme list, hfc radioburst type III list, tsrs solar radio event list and combines the return of these lists chronologically. Only time_start, time_end, and comment sections are preserved in the result list.

Created: 2012-02-13 | Last updated: 2012-02-14

Credits: User Anja Le Blanc

Workflow Filter CME events to events which could ha... (1)

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This workflow uses the initial time period to search for time periods where Earth and Mars are not further appart than 80 degrees. These time periods are used to find Halo CME events. The CME events are forward propagated to Earth and Sun. Only events were the propagation model predicts that both planets are on the propagation path will be included in the final VOTable

Created: 2012-02-29 | Last updated: 2012-02-29

Credits: User Anja Le Blanc

Workflow Monthly counts for event occurences betwee... (1)

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This workflow provides monthly counts of events in HEC between the beginning of year_start and the end of year_end. Returns the result as comma separated file (csv) and as list of lists.

Created: 2012-08-23

Credits: User Anja Le Blanc

Attributions: Workflow Counts number of events per month in HEC table Workflow Split VOTable into its values

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Workflow 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: User David PS User Eoincar

Attributions: Workflow Extract content of columns from VOTables

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

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

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Workflow 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: User David PS User Anja Le Blanc User Nadia Cerezo User Gab

Attributions: Workflow find events in xray and radio

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Non-Information Resource URI: http://alpha.myexperiment.org/tags/2897


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