All content

Search filter terms
Filter by category
Filter by type
Filter by tag
Filter by user
Filter by licence
Filter by group
Filter by wsdl
Results per page:
Sort by:
Showing 5 results. Use the filters on the left and the search box below to refine the results.
Tag: sep Group: HELIO Wsdl: http://cagnode58.cs.tcd.ie:8080/helio-hps-server/hpsService?wsdl

Workflow Propagation of the Solar Energetic Particl... (1)

Thumb
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: 2012-03-13 | Last updated: 2012-03-13

Credits: User Anja Le Blanc

Workflow Associate SEP events at Earth with flare, ... (1)

Thumb
This is the implementation of a use case worked on during CDAW3 of the HELIO project. SEP events propagated backward from Earth to the Sun. We allow for +- 30 min around the predicted time to search for flare events. The timing of the flare event informs the search time for Type III radio event (time_start to time_peak) and for the CME event (time_start to time_start+1h). Results are presented in a mulitlayered VOTable.

Created: 2012-03-13 | Last updated: 2012-03-13

Credits: User Anja Le Blanc User Rositsa

Attributions: Workflow Propagation of the Solar Energetic Particles to the Sun Workflow Extract content of columns from VOTables

Workflow Propagation of the Solar Energetic Particl... (1)

Thumb
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: User Anja Le Blanc

Workflow Propagation of the Solar Energetic Particl... (2)

Thumb
use of the processing service to calculate time delays to the planets Inputs: time when propagation should start longitude of starting point on the sun speed of the solar wind error value of solar wind speed traveling speed of energetic particals as percentage of the speed of light

Created: 2011-12-13 | Last updated: 2012-02-03

Credits: User Anja Le Blanc Network-member HELIO

Workflow Connect flare events with proton events on... (4)

Thumb
This workflow uses flares listed in the goes_sxf_flare list, checks wether this flare is connected to Earth via the Parker spiral, and looks for proton events at earth listed in the goes_proton_event list. The flare listing and the proton listing is combinded into a VOTable output.

Created: 2011-11-15 | Last updated: 2012-05-15

Credits: User Anja Le Blanc

Results per page:
Sort by: