CMEchaser looks for the occultation of background astronomical sources by CMEs to enable measurement of effects such as variations in the ionized content and the associated Faraday rotation of polarized signals along the line of sight to the background source. The code transforms a given Galactic coordinate to its concordant point in the Helioprojective, Sun-centered plane and estimates the point at which the line of sight from the source to the Earth passes through it. It then searches a user selected database to detect if any CMEs which launched before the observation date would have crossed the line of sight at the epoch of observation, and produces a number of useful plots. CMEchaser can run as a flat script orcan be installed as a package....

Shaifullah, G., Tiburzi, C., Zucca, P. (2020). CMEchaser: Coronal Mass Ejection line-of-sight occultation detector [Software].

CMEchaser: Coronal Mass Ejection line-of-sight occultation detector

Shaifullah, Golam
Primo
;
2020

Abstract

CMEchaser looks for the occultation of background astronomical sources by CMEs to enable measurement of effects such as variations in the ionized content and the associated Faraday rotation of polarized signals along the line of sight to the background source. The code transforms a given Galactic coordinate to its concordant point in the Helioprojective, Sun-centered plane and estimates the point at which the line of sight from the source to the Earth passes through it. It then searches a user selected database to detect if any CMEs which launched before the observation date would have crossed the line of sight at the epoch of observation, and produces a number of useful plots. CMEchaser can run as a flat script orcan be installed as a package....
Software
Software
English
2020
https://bitbucket.org/golamshaifullah/cme_chaser/wiki/Home
2020ascl.soft08015S
Shaifullah, G., Tiburzi, C., Zucca, P. (2020). CMEchaser: Coronal Mass Ejection line-of-sight occultation detector [Software].
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/10281/400614
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