activity
20172020
most citedCatalog of Hard X-ray Solar Flares Detected with Mars Odyssey/HEND from the Mars Orbit in 2001-2016

11 citations · 26 across the 3 of their papers we have counts for

collaborators

8 papers

astro-ph.SR20207 cited

Multiwavelength Stereoscopic Observation of the May 1, 2013 Solar Flare and CME

Erica Lastufka, Säm Krucker, Ivan Zimovets +7

A M-class behind-the-limb solar flare on 1 May 2013 (SOL2013-05-01T02:32), accompanied by a ( 400 km/s) CME was observed by several space-based observatories with different v…

astro-ph.HE2020

Gamma-ray flux depressions of the Crab nebula in the high-energy range

M. S. Pshirkov, B. A. Nizamov, A. M. Bykov +1

The giant gamma-ray flares of the Crab nebula discovered by AGILE and Fermi observatories came as a surprise and have challenged the existing models of pulsar wind nebulae. We have…

astro-ph.SR2019

Soft X-ray heating as a mechanism of optical continuum generation in solar-type star superflares

B. A. Nizamov

Superflares on the solar type stars observed by \textit{Kepler} demonstrate the contrast in the optical continuum of the order 0.1--1 per cent. The mechanism of formation of this r…

astro-ph.SR20188 cited

Properties of Kepler Stars with the Most Powerful Flares

M. M. Katsova, B. A. Nizamov

We analyze physical characteristics of late-type stars wherein the Kepler mission registered superflares. We use the revised stellar fundamental parameters, i.e. effective temperat…

astro-ph.SR2018

Radio, Hard X-Ray, and Gamma-Ray Emissions Associated with a Far-Side Solar Event

V. V. Grechnev, V. I. Kiselev, L. K. Kashapova +9

The SOL2014-09-01 far-side solar eruptive event produced hard electromagnetic and radio emissions observed with detectors at near-Earth vantage points. Especially challenging was a…

astro-ph.HE2018

Constraints on the AGN flares as sources of ultra-high energy cosmic rays from the Fermi-LAT observations

B. A. Nizamov, M. S. Pshirkov

It is well known that if the most energetic cosmic rays ( eV) were protons then their acceleration sites should possess some extreme properties, including gigantic lumin…