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Planning Overview (Scp, Migration, Charact... (1)

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Copies an image from a remote path using scp. Then starts a migration action on the image and extracts properties from the original and migrated image. The properties are compared and on the image data itself, QA algorithms are started.

Created: 2012-02-28

Credits: Markus Plangg

Image Characterisation - Fits (Simple) (1)

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Extracts metadata from images.

Created: 2012-02-27 | Last updated: 2012-02-27

Credits: Markus Plangg

Image QA (RAW/NonRAW, Ssim, Equals) (1)

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Reads images either by reading the file directly or using dcraw depending on the image mimetype. Then runs QA algorithms to compare the images.

Created: 2012-02-27 | Last updated: 2012-02-27

Credits: Markus Plangg

Image QA - Read image (RAW/NonRAW) (1)

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Reads an image for evaluation. How the file is read depends on the image type (RAW, NonRAW) of the current image and the image to compare with.

Created: 2012-02-27 | Last updated: 2012-02-27

Credits: Markus Plangg

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

VAMDC VALD query with SME processing (2)

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VAMDC workflow that queries the VALD Atomic database in Moscow and runs SME (Spectroscopy Made Easy) VAMDC Taverna Plugin: http://voparis-twiki.obspm.fr/twiki/bin/view/VAMDC/TavernaUserGuide

Created: 2012-02-24 | Last updated: 2012-09-12

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 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: 2012-02-22 | Last updated: 2012-02-22

Credits: Anja Le Blanc

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DALEC

Created: 2012-02-22 00:55:52

License: Creative Commons Attribution-Share Alike 3.0 Unported License

File type: Trident (Package)

Comments: 0 | Viewed: 22 times | Downloaded: 18 times

Find protein identifications in PRIDE (2)

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Find protein identifications information in the PRIDE database using a protein accession as input.

Created: 2012-02-21 | Last updated: 2012-02-22

Credits: Rafael C. Jimenez