activity
20122016
most citedInvestigation of Hot X-ray Points (HXPs) Using Spectroheliograph Mg XII Experiment Data From CORONAS-F/SPIRIT

24 citations · 88 across the 5 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2016★ 11 cited

Breakout Reconnection Observed by the TESIS EUV Telescope

Anton Reva, Artem Ulyanov, Sergey Shestov +1

We present experimental evidence of the coronal mass ejection (CME) breakout reconnection, observed by the TESIS EUV telescope. The telescope could observe solar corona up to 2 $R_…

astro-ph.SR2015★ 21 cited

EUV Spectra of Solar Flares from the EUV Spectroheliograph SPIRIT aboard CORONAS-F satellite

Sergey Shestov, Anton Reva, Sergey Kuzin

We present detailed EUV spectra of 4 large solar flares: M5.6, X1.3, X3.4, and X17 classes in the spectral ranges 176-207 Å and 280-330 Å. These spectra were obtained {by the slitl…

astro-ph.SR2015★ 23 cited

Wave-like Formation of Hot Loop Arcades

Anton Reva, Sergey Shestov, Ivan Zimovets +2

We present observations of hot arcades made with the Mg XII spectroheliograph onboard the CORONAS-F mission, which provides monochromatic images of hot plasma in the Mg XII 8.42 A…

astro-ph.SR2015★ 9 cited

Initiation and early evolution of the Coronal Mass Ejection on May 13, 2009 from EUV and white-light observations

Anton Reva, Artem Ulyanov, Sergey Bogachev +1

We present the results of the observations of a coronal mass ejection (CME), which occurred on May 13, 2009. The most important feature of these observations is that the CME was ob…

astro-ph.SR2015★ 24 cited

Investigation of Hot X-ray Points (HXPs) Using Spectroheliograph Mg XII Experiment Data From CORONAS-F/SPIRIT

Anton Reva, Sergey Shestov, Sergey Bogachev +1

Observations in the Mg XII 8.42 AA line onboard the CORONAS-F satellite have revealed compact high temperature objects-hot X-ray points (HXP)-and their major physical parameters we…

astro-ph.SR2014

Sparkling EUV bright dots observed with Hi-C

S. Regnier, C. E. Alexander, R. W. Walsh +12

Observing the Sun at high time and spatial scales is a step towards understanding the finest and fundamental scales of heating events in the solar corona. The Hi-C instrument has p…