activity
20082017
most citedCoronal Shock Waves, EUV waves, and Their Relation to CMEs. I. Reconciliation of "EIT waves", Type II Radio Bursts, and Leading Edges of CMEs

66 citations · 210 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2017★ 11 cited

Development and Parameters of a Non-Self-Similar CME Caused by Eruption of a Quiescent Prominence

I. V. Kuzmenko, V. V. Grechnev

The eruption of a large quiescent prominence on 17 August 2013 and associated coronal mass ejection (CME) were observed from different vantage points by Solar Dynamics Observatory…

astro-ph.SR2016★ 30 cited

A Tiny Eruptive Filament as a Flux-Rope Progenitor and Driver of a Large-Scale CME and Wave

V. V. Grechnev, A. M. Uralov, A. A. Kochanov +5

A solar eruptive event SOL2010-06-13 observed with SDO/AIA has been discussed in the contexts of the CME gebesis and an associated EUV transient in terms of a shock driven by the a…

astro-ph.SR2014★ 28 cited

Responsibility of a Filament Eruption for the Initiation of a Flare, CME, and Blast Wave, and its Possible Transformation into a Bow Shock

V. V. Grechnev, A. M. Uralov, I. V. Kuzmenko +3

Multi-instrument observations of two filament eruptions on 24 February and 11 May 2011 suggest the following updated scenario for eruptive flare, CME and shock wave evolution. An i…

astro-ph.SR2013★ 11 cited

Microwave Negative Bursts as Indications of Reconnection between Eruptive Filaments and Large-Scale Coronal Magnetic Environment

V. Grechnev, I. Kuzmenko, A. Uralov +2

Low-temperature plasma ejected in solar eruptions can screen active regions as well as quiet solar areas. Absorption phenomena can be observed in microwaves as 'negative bursts' an…

astro-ph.SR2011★ 66 cited

Coronal Shock Waves, EUV waves, and Their Relation to CMEs. I. Reconciliation of "EIT waves", Type II Radio Bursts, and Leading Edges of CMEs

V. V. Grechnev, A. M. Uralov, I. M. Chertok +5

We show examples of excitation of coronal waves by flare-related abrupt eruptions of magnetic rope structures. The waves presumably rapidly steepened into shocks and freely propaga…

astro-ph.SR2010★ 9 cited

Solar flare-related eruptions followed by long-lasting occultation of the emission in the He II 304 A line and in microwaves

V. V. Grechnev, I. V. Kuzmenko, I. M. Chertok +1

Plasma with a temperature close to the chromospheric one is ejected in solar eruptions. Such plasma can occult some part of emission of compact sources in active regions as well as…