40 citations · 201 across the 20 of their papers we have counts for
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Full orbital solution for the binary system in the northern Galactic disc microlensing event Gaia16aye
Łukasz Wyrzykowski, P. Mróz, K. A. Rybicki +182
Gaia16aye was a binary microlensing event discovered in the direction towards the northern Galactic disc and was one of the first microlensing events detected and alerted to by the…
On existence of two different mechanisms for forming coronal mass ejections
V. Eselevich, M. Eselevich, V. Romanov +2
We confirm the principal difference of the initiation phase between the impulsive and gradual CME motion trajectory revealed earlier in preliminary studies. Based on studying the d…
A formation mechanism for the type II radio emission in the solar corona unrelated to shock waves
V. G. Eselevich, M. V. Eselevich
Mark 4, COR1/STEREO and LASCO/SOHO data analysis shows that at least a portion of type II radio bursts observed in the corona occurs in the presence of a CME, but in the absence of…
Coronal Shock Waves, EUV Waves, and Their Relation to CMEs. III. Shock-Associated CME/EUV Wave in an Event with a Two-Component EUV Transient
V. V. Grechnev, A. N. Afanasyev, A. M. Uralov +5
On 17 January 2010, STEREO-B observed in extreme ultraviolet (EUV) and white light a large-scale dome-shaped expanding coronal transient with perfectly connected off-limb and on-di…
Estimated relations at a shock driven by a coronal mass ejection
M. Eselevich, V. Eselevich
Analysis of SOHO/LASCO C3 data reveals a discontinuity, interpreted as a shock wave, in plasma density radial profiles in a restricted region ahead of each of ten selected coronal…
On The Possible Mechanism Of Energy Dissipation In Shock-Wave Fronts Driven Ahead Of Coronal Mass Ejections
M. Eselevich, V. Eselevich
Analysis of Mark 4 and LASCO C2, C3 coronagraph data shows that, at the distance R from the center of the Sun, the thickness of a CME-generated shock-wave front…