User: David PS

XPath From VOTable (1)

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A XPath From text version for VOTables. This is useful to extract certain information from the header of the VOTables but it could work for any XPath.

Created: 2014-03-12

Credits: David PS Anja Le Blanc

Attributions: Extracting data from VOTable format by using XPath query

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?

Plane cut on planetary models provided und... (1)

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This is a simple workflow using one of the webservice provided by IMPEx. It calculates the value of a plane for different variables for a particular planetary model.

Created: 2013-09-11

Credits: David PS

Get Particle trajectories from starting po... (1)

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This is a workflow that uses 2 different services from IMPEx to calculate different variables at a certain radius for a particular planetary model.

Created: 2013-09-10

Credits: David PS

Attributions: Sphere lan-lot random points Particle trajectories in the planetary models provided under IMPEx VOTable on the net maker for IMPEx Interpolate n-randon points in a sphere on a planetary models provided under IMPEx

Interpolate n-randon points in a sphere on... (1)

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This is a workflow that uses 2 different services from IMPEx to calculate different variables at a certain radius for a particular planetary model.

Created: 2013-09-10

Credits: David PS

Attributions: Interpolate values on planetary models provided under IMPEx VOTable on the net maker for IMPEx Sphere lan-lot random points

Sphere lan-lot random points (1)

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It gest n lat-lon coordinates pairs as comma separated values. It uses a a random generator from http://www.random.org

Created: 2013-09-10

Credits: David PS

Vector field lines in the planetary models... (1)

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This is a simple workflow using one of the webservice provided by IMPEx. It calculates the field lines for the vector field requested for the starting points provided for a particular planetary model.

Created: 2013-09-10

Credits: David PS

Particle trajectories in the planetary mod... (1)

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This is a simple workflow using one of the webservice provided by IMPEx. It calculates the particle trajectories for the defined particle (initial position, velocity, mass and charge) for a particular planetary model.

Created: 2013-09-10

Credits: David PS

Interpolate values on planetary models pro... (2)

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This is a simple workflow using one of the webservice provided by IMPEx. It calculates the value of different variables, at the cordinates that a spacecraft pass through for the time range provided, for a particular planetary model. The orbital values of the spacecraft are obtained by AMDA.

Created: 2013-09-10 | Last updated: 2013-09-10

Credits: David PS

Interpolate values on planetary models pro... (1)

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This is a simple workflow using one of the webservice provided by IMPEx. It calculates the value of different variables, at the cordinates provided, for a particular planetary model.

Created: 2013-09-10

Credits: David PS

VOTable on the net maker for IMPEx (1)

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This simple workflow is a way to create a simple votable that uses the standards from IMPEx and provides an URL for the created VOTable enabling re-use of it through the IMPEx services

Created: 2013-09-10

Credits: David PS

Venus: Compare VEX data with HYB model (1)

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It compares data from VEX from a certain date range with what HYB has modeled in the coordinates where VEX spacecraft is at that moment.

Created: 2013-04-07

Credits: David PS Natasha

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?

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: 2013-03-21

Credits: Nadia Cerezo Anja Le Blanc David PS

Attributions: Monthly counts for event occurences between beginning of year_start and end of year_end

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: David PS Anja Le Blanc Nadia Cerezo Gab

Attributions: find events in xray and radio

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

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

Finding the origins of Solar Wind events a... (6)

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This gives a comprenhensive overview of high speed solar wind events (CME or CIR) seen at Eart, by obtaining the maximum in-situ measure velocity from the data evaluation service (DES), propagating the even backwards to Earth using the HELIO processing service (HPS) and SHEBA propagation model, and search whether halo CMEs or CHs were observed on that time, and retrieves, besides all the previous information, a context solar wind plot (+/- 1 day) and a URL linking to a context movie for CMEs...

Created: 2012-11-16 | Last updated: 2013-03-21

Credits: David PS

Attributions: CME backwards propagation Co-rotating Interaction Regions backwards propagation HFC Synoptic map from date CDAW CME movie from date Solar Wind properties and plot Back CIR-CME propagation model LASCO_CME_QUERY

CDAW CME movie from date (1)

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generates the url for the input date to visualize CMEs and GOES xray light curve produced by CDAW at GSFC

Created: 2012-11-05

Credits: David PS

Attributions: HFC Synoptic map from date

HFC Synoptic map from date (1)

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query the HELIO Feature Catalogue, and retrieves the image with all the features catalgued for certain date.

Created: 2012-11-05

Credits: David PS

Solar Wind properties and plot (1)

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Using HELIO-MDES this workflow provides some properties of the solar wind from an input date and a mission and the plot +/-1 day for context.

Created: 2012-10-25

Credits: David PS

Attributions: MDES simple execution

Back CIR-CME propagation model (1)

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With a observing time at an object and the type of PM that you want to run executes it and provides the plots and the time and longitude where it should be seen the origin of the event.

Created: 2012-10-24

Credits: David PS Anja Le Blanc

Attributions: CME backwards propagation Co-rotating Interaction Regions backwards propagation

Forward CME propagation model (SHEBA) - de... (1)

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Extract Objects, HitOrMiss, ETAs and plots for a selected run of the SHEBA forward CME.

Created: 2012-10-21

Credits: David PS

Attributions: CME backwards propagation

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: David PS Eoincar

Attributions: Extract content of columns from VOTables

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

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