Propagation of type II associated CME using SHEBA and solar wind properties from ACE
This workflow firstly selects the fastest CME from the wind_typeii_soho_cme catalogue of the heliophysics event catalogue (HEC). It then finds properties of this CME from soho_lasco_cme and properties of the associated flare from goes_sxr_flare. The CME and flare properties are used to run the SHEBA propagation model to find an ETA range at Earth. The average solar wind speed at this time range is then used to re-define the CME speed (this accounts for solar wind drag). The new CME speed is then used in a second run of the SHEBA propagation model to find an ETA at Earth (or any chosen destination). This workflow is based on the design of
when_do_the_fastest_type_ii_cme_should_be_detected_throughout_all_the_heliosphere___returns_single_values__not_a_list__777405.t2flow
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When do the Fastest type II CME should be ...
(2)
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
When do the Fastest type II CME should be ...
(1)
Created: 2013-03-21
Credits:
Gab
Anja Le Blanc
David PS
Attributions:
When did the fastest type II CME happened?
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