Coronal Mass Ejections in September 2017 from Monitoring of Interplanetary Scintillations with the Large Phased Array of the Lebedev Institute of Physics


Cite item

Full Text

Open Access Open Access
Restricted Access Access granted
Restricted Access Subscription Access

Abstract

Results of monitoring of interplanetary scintillations with the Large Phased Array of the Pushchino Radio AstronomyObservatory at 111 MHz during a period of flare activity of the Sun in the first ten days of September 2017 are presented. Enhancements of scintillations associated with interplanetary coronal mass ejections propagating after limb flares have been recorded. The propagation velocities are estimated to be about 2000 km/s for an ejection on September 7 and about 1000 km/s for an ejection on September 6. It is shown that, during the propagation from the Sun, the lateral part of the ejections decelerates faster than its leading part. Night-time enhancements of second-timescale scintillations during periods of high geomagnetic activity have an ionospheric origin.

About the authors

I. V. Chashei

Pushchino Radio Astronomy Observatory, Astro Space Center, Lebedev Physical Institute

Author for correspondence.
Email: chashei@prao.ru
Russian Federation, Pushchino, Moscow oblast’, 142290

S. A. Tyul’bashev

Pushchino Radio Astronomy Observatory, Astro Space Center, Lebedev Physical Institute

Email: chashei@prao.ru
Russian Federation, Pushchino, Moscow oblast’, 142290

V. I. Shishov

Pushchino Radio Astronomy Observatory, Astro Space Center, Lebedev Physical Institute

Email: chashei@prao.ru
Russian Federation, Pushchino, Moscow oblast’, 142290

I. A. Subaev

Pushchino Radio Astronomy Observatory, Astro Space Center, Lebedev Physical Institute

Email: chashei@prao.ru
Russian Federation, Pushchino, Moscow oblast’, 142290

Supplementary files

Supplementary Files
Action
1. JATS XML

Copyright (c) 2018 Pleiades Publishing, Ltd.