Ie User: David PS

2577?size=160x160

Name: David PS

Joined: Friday 25 February 2011 12:32:43 (UTC)

Last seen: Monday 22 January 2018 09:19:10 (UTC)

Email (public): Not specified

Website: Not specified

Location: Dublin, Ireland

David PS has been credited 25 times

David PS has an average rating of:

0.0 / 5

(0 ratings in total)

for their items

Description/summary not set


Other contact details:

Not specified

Interests:

Not specified

Field/Industry: Solar Physics/Space Weather

Occupation/Role(s): Research

Organisation(s):

TCD

 

Note: some items may not be visible to you, due to viewing permissions.

Workflow

Uploader

Workflow XPath From VOTable (1)

Thumb
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: User David PS User Anja Le Blanc

Attributions: Workflow Extracting data from VOTable format by using XPath query

Workflow

Uploader

Workflow Propagation of type II associated CME usin... (3)

Thumb
No description

Created: 2014-02-11 | Last updated: 2014-02-17

Credits: User Eoincar User Anja Le Blanc User David PS Network-member HELIO

Attributions: Workflow When did the fastest type II CME happened?

Workflow

Uploader

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

Thumb
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: User David PS

Workflow

Uploader

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

Thumb
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: User David PS

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

Workflow

Uploader

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

Thumb
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: User David PS

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

Workflow

Uploader

Workflow Sphere lan-lot random points (1)

Thumb
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: User David PS

Workflow

Uploader

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

Thumb
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: User David PS

Workflow

Uploader

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

Thumb
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: User David PS

Workflow

Uploader

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

Thumb
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: User David PS

Workflow

Uploader

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

Thumb
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: User David PS

Workflow

Uploader

Workflow VOTable on the net maker for IMPEx (1)

Thumb
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: User David PS

Workflow

Uploader

Workflow Venus: Compare VEX data with HYB model (1)

Thumb
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: User David PS User Natasha

Workflow

Uploader
3463?size=60x60 Gab

Workflow When do the Fastest type II CME should be ... (1)

Thumb
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: User Gab User Anja Le Blanc User David PS

Attributions: Workflow When did the fastest type II CME happened?

Workflow

Workflow Monthly counts for event occurences betwee... (1)

Thumb
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: User Nadia Cerezo User Anja Le Blanc User David PS

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

Workflow

Uploader

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

Thumb
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: User David PS User Anja Le Blanc User Nadia Cerezo User Gab

Attributions: Workflow find events in xray and radio

Workflow

Uploader

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

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

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

Workflow

Uploader

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

Thumb
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: User David PS

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

Workflow

Uploader

Workflow CDAW CME movie from date (1)

Thumb
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: User David PS

Attributions: Workflow HFC Synoptic map from date

Workflow

Uploader

Workflow HFC Synoptic map from date (1)

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

Created: 2012-11-05

Credits: User David PS

Workflow

Uploader

Workflow Solar Wind properties and plot (1)

Thumb
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: User David PS

Attributions: Workflow MDES simple execution

Workflow

Uploader

Workflow Back CIR-CME propagation model (1)

Thumb
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: User David PS User Anja Le Blanc

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

Workflow

Uploader

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

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

Created: 2012-10-21

Credits: User David PS

Attributions: Workflow CME backwards propagation

Workflow

Uploader

Workflow When did the fastest type II CME happened? (1)

Thumb
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: User David PS User Eoincar

Attributions: Workflow Extract content of columns from VOTables

Workflow

Workflow Associate a Shock at Earth with Flare and ... (2)

Thumb
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: User Anja Le Blanc User David PS

Workflow

Workflow Find source at Sun of SW events on Earth (5)

Thumb
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: User Anja Le Blanc User David PS

What is this?

Linked Data

Non-Information Resource URI:


Alternative Formats

HTML
RDF
XML