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[ascl:1805.005] 3DCORE: Forward modeling of solar storm magnetic flux ropes for space weather prediction

3DCORE forward models solar storm magnetic flux ropes called 3-Dimensional Coronal Rope Ejection (3DCORE). The code is able to produce synthetic in situ observations of the magnetic cores of solar coronal mass ejections sweeping over planets and spacecraft. Near Earth, these data are taken currently by the Wind, ACE and DSCOVR spacecraft. Other suitable spacecraft making these kind of observations carrying magnetometers in the solar wind were MESSENGER, Venus Express, MAVEN, and even Helios.

Code site:
https://doi.org/10.6084/m9.figshare.5450341 https://github.com/cmoestl/3DCORE
Appears in:
http://adsabs.harvard.edu/abs/2018SpWea..16..216M
Bibcode:
2018ascl.soft05005M

ascl:1805.005
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