When do the Fastest type II CME should be detected throughout all the heliosphere?

Created: 2012-10-21 19:00:36      Last updated: 2013-03-20 12:21:55

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

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1. Jason Byrne, Florian Mayer, Gabriele Pierantoni, Andrii Lynnyk, Nataliya Bourrel, Baptiste Cecconi, David Pérez-Suárez, Eoin Carley, Shane Maloney., HELIO Use Case 2: The 100 CME Challenge, Poster, 02 November 2012, http://dx.doi.org/10.6084/m9.figshare.97156, Accessed at: 01 July 2012


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