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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

Comments: 0 | Viewed: 39 times | Downloaded: 216 times

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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

Comments: 0 | Viewed: 44 times | Downloaded: 30 times

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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

Unique name: helio
Created: Thursday 14 August 2008 13:06:20 (UTC)

88 shared items   |   1 announcements

Latest announcement:: Registry of HELIO services

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ICS Use Case Solutions

Created: 2010-07-12 13:54:16 | Last updated: 2010-07-13 10:57:46

1 item in this pack

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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

retrieving solar monitor urls for votable ... (1)

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No description

Created: 2009-11-12 | Last updated: 2009-11-12

Credits: Anja Le Blanc

Retrieve all data for all instruments for ... (3)

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This workflow looks up all instruments known to have worked during the requested periode of time (ICS), restructures results to make them fit instruments.xsd and requests data for this periode from DPAS. Result: VOTable with list of URLs to data.

Created: 2010-04-15 | Last updated: 2010-08-09

Credits: Anja Le Blanc

Attributions: Extracting data from VOTable format by using XPath query

DPAS general query (1)

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general query to DPAS; it gets a list of instruments and lists for start and stop times; for a query hessiEC, phoenix2; start times 2001-01-01 00:00:00, 2005-04-01 00:00:00; stop times 2001-01-05 00:00:00, 2005-05-1 00:00:00 it would perform to queries: hessiEC from 2001-01-01 00:00:00 to 2001-01-05 00:00:00 and phoenix2 from 2005-04-01 00:00:00 to 2005-05-1 00:00:00 There is only one output file with the results from both queries.

Created: 2010-04-19 | Last updated: 2010-04-19

Credits: Anja Le Blanc

DPAS general query with sorted field (1)

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same as DPAS general query. Calling the DPAS sortedQuery web service. additional input: partialSorting input boolean true or false false all result entries are sorted by start measurementTime true each request is sorted by measurement time; no overall time order, but queries stay in the order they there asked.

Created: 2010-04-19 | Last updated: 2010-04-19

Credits: Anja Le Blanc

retrieve data for all instruments for even... (1)

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This workflow uses the HEC to retrieve events for a time spane given by the user from a HEC table given by the user as well. It uses all instruments available in the DPAS to retrieve data for the events Output: XML as returned by the DPASThis workflow uses the HEC to retrieve events for a time spane given by the user from a HEC table given by the user as well. It uses all instruments available in the DPAS to retrieve data for the events; empty results are filtered out, the data is combind wi...

Created: 2010-04-21

Credits: Anja Le Blanc

Attributions: DPAS general query HEC standard query Retrieve all data for all instruments for a given periode of time

Extracting data from VOTable format by usi... (1)

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Input VOTable and 'name' of a Output corrosponding data of that field in an arrayInput VOTable and 'name' of a Field

Created: 2010-07-01 | Last updated: 2010-07-01

Credits: Anja Le Blanc Donal Fellows

Call VSO web service with HELIO input data (1)

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  date transformation from 2000-10-02T23:00:00 to 20001002230000 HELIO instrument names as in http://helio-dev.i4ds.ch/xsd/instruments.xsd spitt into source and instrument names; if these pair don't exist only first part (source) is tried.

Created: 2010-08-04 | Last updated: 2010-08-04

Credits: Anja Le Blanc

instruments in sxr and euv spectrum (1)

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ICS use case 5

Created: 2010-08-20 | Last updated: 2010-08-20

Credits: Anja Le Blanc

retrive dpas data for all ics instruments ... (1)

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This workflow demonstrates the standard query there events for a period of time are requested from the HEC service, available instruments for this time come from the ICS and data only for the times of the events are requested from the DPAS.

Created: 2010-09-14 | Last updated: 2010-09-14

Credits: Anja Le Blanc

Attributions: Extracting data from VOTable format by using XPath query Retrieve all data for all instruments for a given periode of time

retrive dpas data for all ics instruments ... (1)

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This workflow demonstrates the standard query where events for a period of time are requested from the HEC service, available instruments for this time come from the ICS and data only for the times of the events are requested from the DPAS. In this version data from only 3 random events (out of the HEC list) will be requested from the DPAS.

Created: 2010-09-14 | Last updated: 2010-09-14

Credits: Anja Le Blanc

Attributions: retrive dpas data for all ics instruments for HEC event data

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: HFCout is a modified VOTable where a field is added with the number of associated hessi flares. combined_output 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: 2011-02-11 | Last updated: 2011-10-24

Credits: Anja Le Blanc

Converting from heliocentric coordinate sy... (1)

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Converting from heliocentric coordinate system with coordinates in arcsec to coordinates in longitude latitude Based on the IDL script xy2lonlat.pro http://hesperia.gsfc.nasa.gov/ssw/gen/idl/solar/xy2lonlat.pro Stonyhurst Heliographic Coordinate System to Helioprojective-Cartesian Coordinate System

Created: 2011-02-18 | Last updated: 2011-02-18

Credits: Anja Le Blanc

Associate goes X ray flares with active r... (1)

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This workflow is querying the HFC ActiveRegions list and HEC goes_xray_flare list. It requires a time periode and a search radius arround the centre of an Active Region as inputs It produces two outputs: HFCout is a modified VOTable where a field is added with the number of associated hessi flares. combined_output 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: 2011-02-18 | Last updated: 2011-02-18

Credits: Anja Le Blanc

Associate flares with active regions (1)

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This workflow is querying the HFC ActiveRegions list and HEC flare lists (names retrieved from the ontlogoy) It requires a time periode and a search radius arround the centre of an Active Region as inputs It produces two outputs: HFCout is a modified VOTable where a field per flare list is added with the number of associated flares. combined_output is a 2 dimensional list with an VOTable for each Active region and each one with an VOTable for all associated flares for that Active Region.

Created: 2011-02-22 | Last updated: 2011-08-24

Credits: Anja Le Blanc

Attributions: Associate goes X ray flares with active regions Associate hessi flares with active regions

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

Converting from coordinates in longitude l... (1)

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Based on lonlat2xy.pro Converts from Helioprojective-Cartesian Coordinate System to Stonyhurst Heliographic Coordinate SystemBased on lonlat2xy.pro http://hesperia.gsfc.nasa.gov/ssw/gen/idl/solar/lonlat2xy.pro Converts from Helioprojective-Cartesian Coordinate System to Stonyhurst Heliographic Coordinate System

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

Credits: 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

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: Anja Le Blanc

Find instruments of a special type in a se... (1)

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This workflow takes a type of isnstrument as input and the minimum and maxium coordinates in HCI as input. Cadence for the location service is for defining the 'continues' presence. Output is a VOTable based on the ICS return where two columns are added for the time this instrument has entered and exited the Region of Interest.

Created: 2011-08-24 | Last updated: 2011-08-24

Credits: Anja Le Blanc

Find instruments of a special type in a se... (1)

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This workflow takes a type of isnstrument as input and the minimum and maxium coordinates in HCI as input. Cadence for the location service is for defining the 'continues' presence. Output is a VOTable based on the ICS return where two columns are added for the time this instrument has entered and exited the Region of Interest.

Created: 2011-08-24 | Last updated: 2011-08-24

Credits: Anja Le Blanc

Attributions: Find instruments of a special type in a section of space described in HCI coordinates

Find periods of time where two ILS objects... (2)

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Inputs: name of target_obj of ILS of two objects and a number of degrees which these obejcts are allowed to be appart in hci longitude coordinates. Output VOTable of time periods where these two objects are closer than +/- input angle together.

Created: 2011-11-04 | Last updated: 2011-11-18

Credits: Anja Le Blanc

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

Propagation of the Co-roationg interaction... (2)

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use of the processing service to calculate time delays to the planets Inputs: time when propagation should start longitude of starting point on the sun speed of the solar wind error speed of the solar wind

Created: 2011-12-13 | Last updated: 2012-02-03

Credits: Anja Le Blanc

Propagation of the Solar Energetic Particl... (2)

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use of the processing service to calculate time delays to the planets Inputs: time when propagation should start longitude of starting point on the sun speed of the solar wind error value of solar wind speed traveling speed of energetic particals as percentage of the speed of light

Created: 2011-12-13 | Last updated: 2012-02-03

Credits: Anja Le Blanc HELIO

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: 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

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: 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

Co-rotating Interaction Regions backwards ... (1)

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Run the cir backwards propagation code on the HELIO processing service. Required inputs: time start of backwards propagation, the object (planet/spacecraft) from where the propagation should start, assumed solar wind speed at the time, assumed error of solar wind speed Output: VOTable with times at different points in solar system

Created: 2012-03-14 | Last updated: 2012-03-14

Credits: Anja Le Blanc

Split VOTable into its values (1)

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This workflow takes a single VOTable and splits it up in a vector for the names of fields, a vector for the UCDs of the fields, a vector for the UTypes of the fields, and a two dimensional vector for the values.

Created: 2012-03-14 | Last updated: 2012-03-14

Credits: Anja Le Blanc

Check in UOC which instruments were observ... (2)

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Query of the UOC to find the instrument_observatory keys for instruments which were observing at a given time period and a given location.

Created: 2012-03-15 | Last updated: 2012-03-15

Credits: Anja Le Blanc

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

ACE Average Speed (1)

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No description

Created: 2012-09-06

Credits: 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?

Propagation of type II associated CME usin... (3)

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No description

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?

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