activity
20102022
most citedOrigin and Ion Charge State Evolution of Solar Wind Transients during 4 -- 7 August 2011

32 citations · 118 across the 8 of their papers we have counts for

collaborators

8 papers

physics.space-ph2022

Formation of Coronal Mass Ejection and Post-eruption Flow of Solar Wind on 2010 August 18 event

Vladimir Slemzin, Farid Goryaev, Denis Rodkin

The state of the space environment plays a significant role for forecasting of geomagnetic storms produced by disturbances of the solar wind (SW). Coronal mass ejections (CMEs) pas…

physics.atom-ph2020

Verification of atomic data for He- and Li-like ions employing K-spectra from the tokamak plasma

F. Goryaev, A. Urnov

X-ray emission K-spectra of highly charged He- and Li-like argon ions recorded with high spectral, spatial, and temporal resolution at the TEXTOR tokamak were employed to develop a…

astro-ph.SR2020

Observations of Ray-Like Structures in Large-Scale Coronal Dimmings Produced by Limb CMEs

F. Goryaev, V. Slemzin, D. Rodkin

Observations of the off-limb corona with the SWAP wide-field telescope in the 174\,Å passband onboard the PROBA2 mission provide an opportunity to study post-eruptive processes in…

physics.space-ph2018★ 21 cited

Single ICMEs and Complex Transient Structures in the Solar wind in 2010 -- 2011

D. Rodkin, V. Slemzin, A. N. Zhukov +3

We analyzed statistics, solar sources and properties of interplanetary coronal mass ejections (ICMEs) in the solar wind. In comparison with the first eight years of Cycle 23, durin…

physics.space-ph2016★ 32 cited

Origin and Ion Charge State Evolution of Solar Wind Transients during 4 -- 7 August 2011

D. Rodkin, F. Goryaev, P. Pagano +5

We present study of the complex event consisting of several solar wind transients detected by Advanced Composition Explorer (ACE) on 4 -- 7 August 2011, that caused a geomagnetic s…

astro-ph.SR2012★ 28 cited

Signatures of the slow solar wind streams from active regions in the inner corona

V. Slemzin, L. Harra, A. Urnov +3

Some of local sources of the slow solar wind can be associated with spectroscopically detected plasma outflows at edges of active regions accompanied with specific signatures in th…