1.2k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Russian Academy of SciencesRU133 papers
- Lomonosov Moscow State UniversityRU72 papers
- National Research Tomsk State UniversityRU34 papers
- Institute of Solar-Terrestrial PhysicsRU32 papers
- Universitat de ValènciaES27 papers
- Troitsk Institute for Innovation and Fusion ResearchRU23 papers
- Universidade de São PauloBR21 papers
- Chinese Academy of SciencesCN20 papers
- Instituto de Física CorpuscularES19 papers
- Institute for High Energy PhysicsES18 papers
- National Astronomical ObservatoriesCN18 papers
- Kurchatov InstituteRU17 papers
11 papers · 2 filters
Kinematics of CMEs and associated shock waves as deduced from LASCO data: comparative analysis
V. G. Fainshtein, Ya. I. Egorov, Yu. S. Zagainova
From data by LASCO C2 and C3 coronagraphs, depending on time (distance), we have determined positions and velocities of the front for fast limb CMEs' body with their sources near t…
Two-step solar filament eruptions
Boris Filippov
Coronal mass ejections (CMEs) are closely related to eruptive filaments and usually are the continuation of the same eruptive process into the upper corona. There are failed filame…
Development of Solar Flares and Features of the Fine Structure of Solar Radio Emission
G. P. Chernov, V. V. Fomichev, Y. Yan +3
The reason for the occurrence of different elements of the fine structure of solar radio bursts in the decimeter and centimeter wavelength ranges has been determined based on all a…
Long- and Mid-Term Variations of the Soft X-ray Flare Type in Solar Cycles
I. M. Chertok, A. V. Belov
Using data from the Geostationary Operational Environmental Satellites (GOES) spacecraft in the 1-8 Å wavelength range for Solar Cycles 23, 24, and part of Cycles 21 and 22, we com…
Can superflares occur on the Sun? A view from dynamo theory
M. M. Katsova, L. L. Kitchatinov, M. A. Livshits +3
Recent data from the Kepler mission has revealed the occurrence of superflares in sun-like stars which exceed by far any observed solar flares in release of energy. A natural idea…
Order out of Randomness : Self-Organization Processes in Astrophysics
Markus J. Aschwanden, Felix Scholkmann, William Bethune +13
Self-organization is a property of dissipative nonlinear processes that are governed by an internal driver and a positive feedback mechanism, which creates regular geometric and/or…
Catalog of Hard X-ray Solar Flares Detected with Mars Odyssey/HEND from the Mars Orbit in 2001-2016
M. A. Livshits, I. V. Zimovets, D. V. Golovin +7
The study of nonstationary processes in the Sun is of great interest, and lately, multiwavelength observations and registration of magnetic fields are carried out by means of both…
Temporal and Periodic Variations of Sunspot Counts in Flaring and Non-flaring Active Regions
A. Kilcik, V. Yurchyshyn, B. Donmez +3
We analyzed temporal and periodic behavior of sunspot counts (SSCs) in flaring (C, M, or X class flares), and non-flaring active regions (ARs) for the almost two solar cycles (1996…
Two Step Filament Eruption During 14-15 March 2015
R. Chandra, B. Filippov, R. Joshi +1
We present here an interesting two-step filament eruption during 14-15 March 2015. The filament was located in NOAA AR 12297 and associated with a halo Coronal Mass Ejection (CME).…
Latitudinal profiles of the photospheric magnetic field for solar cycles 19-21
Elena Vernova, Marta Tyasto, Dmitrii Baranov
For groups of photospheric magnetic fields differing in strength the time averaged synoptic maps were obtained on the basis of the National Solar Observatory Kitt Peak data (1976-2…
An Early Diagnostics of the Geoeffectiveness of Solar Eruptions from Photospheric Magnetic Flux Observations: The Transition from SOHO to SDO
I. M. Chertok, V. V. Grechnev, A. A. Abunin
In our previous articles (Chertok et al.: 2013, Solar Phys. 282, 175, and 2015, Solar Phys. 290, 627), we presented a preliminary tool for the early diagnostics of the geoeffective…