Workflows

Get image mimetype (1)

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Returns the mimetype of an image.

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

Credits: Markus Plangg

RAWverna Image evaluation - Read images (R... (1)

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Reads images for evaluation by RAWverna. The read parameters depend on the type of the images.

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

Credits: Markus Plangg

RAWverna Image evaluation - Read Image (RAW) (1)

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Reads an image from the given path using dcraw for image comparison.

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

Credits: Markus Plangg

RAWverna image evaluation - Read images (RAW) (1)

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Reads RAW images for evaluation by RAWverna.

Created: 2012-02-21

Credits: Markus Plangg

RAWverna Image Evaluator - Evaluate Equals (1)

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Takes two images as byte array and compares them for equality using the RAWverna Image Evaluator.

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

Credits: Markus Plangg

RAWverna Image Evaluator - Evaluate relative (1)

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Takes two images as byte array and compares them using the RAWverna Image Evaluator.

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

Credits: Markus Plangg

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

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

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

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

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

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

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 Characterisation - Fits (Simple) (1)

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Extracts metadata from images.

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

Credits: Markus Plangg

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

Disability estimates by year (1)

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Uses census and health survey for england together with R to estimate disability for districts in the UK

Created: 2012-02-28

Credits: Ian Dunlop

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

Example of interaction via HTML page (1)

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No description

Created: 2012-03-05 | Last updated: 2012-03-05

Credits: Alan Williams

RISE Atomic Service: Create Account (1)

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 This workflow create an new user account on the RISE server

Created: 2012-03-05 | Last updated: 2012-03-05

Credits: Jribault

RISE Atomic Service: Create Framework (1)

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 This workflow create a new framework on the RISE Server

Created: 2012-03-05 | Last updated: 2012-03-05

Credits: Jribault

RISE Atomic Service: Delete Framework (1)

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 This workflow delete an existing framework on the RISE Server.

Created: 2012-03-05 | Last updated: 2012-03-05

Credits: Jribault

RISE Atomic Service: Execute Simulation (1)

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 This workflow execute a simulation on the RISE server, and wait for its completion.

Created: 2012-03-05 | Last updated: 2012-03-05

Credits: Jribault

RISE Atomic Service: Get Simulation Result (1)

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 This workflow get the simulation result of an existing simulation on the RISE server.

Created: 2012-03-05 | Last updated: 2012-03-05

Credits: Jribault

RISE Atomic Service: Upload ZIP Model File (1)

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 This workflow upload a ZIP file of the simulation model on the RISE server.

Created: 2012-03-05 | Last updated: 2012-03-05

Credits: Jribault

RISE UI: Ask Framework Name (2)

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  This workflow ask the user to enter a new framework name.

Created: 2012-03-05 | Last updated: 2012-03-22

Credits: Jribault