Workflows

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

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

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

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

VOTables from NED Web Services (1)

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Extraction of a sample of VOTables from all the NED Web Services present in paper 2007ASPC..382..165M Web-based Tools - NED VO Services (Mazzarella, J. M.; NED Team). The National Virtual Observatory: Tools and Techniques for Astronomical Research. ASP Conference Series, Vol. 382. Edited by M.J. Graham, M.J. Fitzpatrick, and T.A. McGlynn. San Francisco: Astronomical Society of the Pacific, 2007., p.165

Created: 2012-06-28 | Last updated: 2013-04-12

Credits: Jose Enrique Ruiz

Astronomical object name to equatorial coo... (1)

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 Resolve equatorial coordinates of a list of objects (names) with AstroTaverna plugin

Created: 2012-06-30 | Last updated: 2012-07-01

Credits: Jose Enrique Ruiz

VOTable of NED Images from a List of Objects (1)

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Extraction of metadata using NED Image Virtual Observatory Service into a single VOTable, providing a list of objects and the width for each field in arcmin. Among the most relevant metadata are the URL link to the FITS images. This Wf makes use of a Tool developed as an internal pyhton script file.

Created: 2012-07-01 | Last updated: 2012-07-01

Credits: Jose Enrique Ruiz

Attributions: Astronomical object name to equatorial coordinates Resolver