User: Shanem

Avatar

Name: Shanem

Joined: Thursday 06 September 2012 08:41:54 (UTC)

Last seen: Thursday 06 September 2012 15:20:56 (UTC)

Email (public): Not specified

Website: Not specified

Location: Not specified

Shanem has been credited 1 time

Shanem 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: Not specified

Occupation/Role(s): Not specified

Organisation(s):

Not specified
 

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

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

What is this?

Linked Data

Non-Information Resource URI:


Alternative Formats

HTML
RDF
XML