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tamerstorfer/ELEvoHI: ELEvoHI_v2.0.0.0

integration_instructionsResearch softwarekeyboard_double_arrow_right Software 02 Jun 2020Publisher:Zenodo
Authors: Amerstorfer, Tanja; Jürgen, H.;

doi: 10.5281/zenodo.3873419 , 10.5281/zenodo.3873420 , 10.5281/zenodo.5045415

tamerstorfer/ELEvoHI: ELEvoHI_v2.0.0.0

Abstract

ELEvoHI relies on heliospheric imagers (HI) observations to obtain the kinematics of a CME. With the newly developed deformable front, the model is able to react to the ambient solar wind conditions during the entire propagation and along the whole front of the CME. To get an estimate of the ambient solar wind conditions, we make us of ambient solar wind models.

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citations
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
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