Abstract
Initial spectropolarimetric observations at the Irkutsk Institute of Solar and Terrestrial Physics were influenced by the fact that, in the 1970s, a large amount of research was undertaken on turbulent electric fields in plasmas under laboratory conditions(227,228) Since most theories and models of solar flares rely on the concept of the turbulent state of a flare plasma, the Irkutsk group made some initial attempts to study plasma turbulence with the upper chromospheric layers of a solar flare by different spectroscopic techniques, in particular by the Berange—Mozer method, based on satellites of the forbidden Hel line(228,229) and estimates of linear polarization,(194)
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
