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19942026
most citedCosmic-ray propagation and interactions in the Galaxy

1.2k citations

Showing 2017Show all

28 papers · 1 filter

astro-ph.SR2017★ 3 cited

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…

astro-ph.SR2017★ 16 cited

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…

hep-ph2017★ 3 cited

Generation of the relic neutrino asymmetry in a hot plasma of the early Universe

Victor B. Semikoz, Maxim Dvornikov

The neutrino asymmetry in the early universe plasma, , is calculated both before and after the electroweak phase transition (EWPT). In the Standard Model before EW…

hep-ph2017

Magnetic field generation in dense gas of massive electrons with anomalous magnetic moments electroweakly interacting with background matter

Maxim Dvornikov

We describe the generation of the electric current flowing along the external magnetic field in the system of massive charged fermions, possessing anomalous magnetic moments and el…

math.AT2017

Local coefficients and the Herbert Formula

Petr M. Akhmet'ev, Theodore Yu. Popelenskii

We discuss a generalisation of the Herbert formula for double points, when the normal bundle of an immersion admits an additional structure, and an application.

physics.ins-det2017★ 4 cited

The STM32 microcontroller based pulse intensity registration system for the neutron monitor

Alexander Shepetov, Alexander Chubenko, Olga Kryakunova +3

We present the outlines of a new microcontroller based data acquisition system which is aimed for reliable operation in a typical cosmic ray particle registration experiment. The s…

nucl-th2017★ 5 cited

Neutrino emission from Cooper pairs at finite temperatures

Lev B. Leinson

A brief review is given of the current state of the problem of neutrino pair emission through neutral weak currents caused by the Cooper pairs breaking and formation (PBF) in super…

astro-ph.HE2017★ 25 cited

Cosmic ray acceleration in magnetic circumstellar bubbles

V. N. Zirakashvili, V. S. Ptuskin

We consider the diffusive shock acceleration in interstellar bubbles created by powerful stellar winds of supernova progenitors. Under the moderate stellar wind magnetization the b…

physics.plasm-ph2017

Long-lived plasma formations in the atmosphere as an alternative energy source

Maxim Dvornikov, G. Sh. Mekhdieva, L. A. Agamalieva

A model of a stable plasma formation, based on radial quantum oscillations of charged particles, is discussed. The given plasmoid is described with the help of the nonlinear Schröd…

astro-ph.SR2017★ 1 cited

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…

astro-ph.CO2017

Cosmological magnetic fields in turbulent matter

Maxim Dvornikov

We study the evolution of magnetic fields in turbulent hot plasma of the early Universe accounting for the chiral magnetic effect. The magnetohydrodynamic turbulence is modeled by…

physics.plasm-ph2017★ 10 cited

Calculations for the Practical Applications of Quadratic Helicity in MHD

Petr M. Akhmet'ev, Simon Candelaresi, Alexandr Yu Smirnov

For the quadratic helicity we present a generalization of the Arnol'd inequality which relates the magnetic energy to the quadratic helicity, which poses a lower bound. W…

hep-ph2017

Neutrino spin oscillations in curved space-time under the influence of external fields

Maxim Dvornikov

We study neutrino spin oscillations in background matter under the influence of strong electromagnetic and gravitational fields. The neutrino spin evolution is treated quasiclassic…

physics.plasm-ph2017★ 11 cited

Thomson scattering in inhomogeneous plasmas: The Role of the Fluctuation-Dissipation Theorem

V. V. Belyi

A self-consistent kinetic theory of Thomson scattering of an electromagnetic field by a non-uniform plasma is derived. We draw the readers' attention to the inconsistency in recent…

astro-ph.SR2017★ 2 cited

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…

astro-ph.SR2017★ 18 cited

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…

cond-mat.mes-hall2017★ 3 cited

Magnetization reversal of thin ferromagnetic elements with surface anisotropy

N. A. Usov, O. N. Serebryakova

The magnetization reversal process in thin-film ferromagnetic elements with surface anisotropy of various shapes and sizes is investigated by means of numerical simulation. The dep…

cond-mat.mes-hall2017★ 91 cited

Interaction effects in assembly of magnetic nanoparticles

N. A. Usov, O. N. Serebryakova, V. P. Tarasov

A specific absorption rate of a dilute assembly of various random clusters of iron oxide nanoparticles in alternating magnetic field has been calculated using Landau- Lifshitz stoc…

astro-ph.SR2017★ 48 cited

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…

astro-ph.HE2017★ 10 cited

Nonlinear approach to the entrainment matrix of superfluid nucleon mixture at zero temperature

Lev B. Leinson

The superfluid drag effect, in hydrodynamics of pulsating neutron stars, is conventionally described with the aid of the entrainment matrix relating the mass currents with the velo…

astro-ph.SR2017★ 11 cited

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…

astro-ph.SR2017★ 21 cited

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…

astro-ph.SR2017★ 35 cited

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).…

astro-ph.SR2017

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…