A copy of this work was available on the public web and has been preserved in the Wayback Machine. The capture dates from 2018; you can also visit the original URL.
The file type is application/pdf.
Polar jet kinetics and energetics analysed from STEREO/COR data
2012
Proceedings of the International Astronomical Union
Preserved Fulltext
We analyze coronagraph observations of a polar jet eruption observed by SECCHI/STEREO. The brightness distribution of the jet in white-light coronagraph images is compared with a kinetic particle model. In this first application, we consider only gravity as the dominant force on the jet particles along the magnetic field. The kinetic model explains well the observed brightness evolution. The initial particle velocity distribution is fitted by Maxwellian distributions and we find deviations of
doi:10.1017/s1743921313003177
fatcat:styxpzgftfgv3j5q54yi4ymszy