User: David PS

XPath From VOTable (1)

• Download

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

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

• Download

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)

• Download

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)

• Download

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)

• Download

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)

• Download

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)

• Download

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)

• Download

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)

• Download

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)

• Download

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)

• Download

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

Find data from a list of instruments and a... (1)

• Download

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

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

• Download

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)

• Download

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)

• Download

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)

• Download

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)

• Download

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

When do the Fastest type II CME should be ... (2)

• Download

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

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

• Download

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)

• Download

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