Add to ORKGThe method of spectrographic global survey was used to study the time variations in parameters of cosmic ray (CR) pitch angle anisotropy and their relationship with the variations of some solar wind characteristics under different electromagnetic conditions in interplanetary space. A classification is made of the conditions that are accompanied by the increase in CR anisotropy
Two cosmic rays which pass through the same point going in opposite directions will, in the absence ...
Modulation model are discussed with more time spent on two current ideas: episodic modulation and dr...
It was demonstrated that an interplanetary magnetic field (IMF) sense dependent 2nd order anisotropy...
The distribution of galactic cosmic ray particles in the heliosphere is influenced (modulated) by t...
Cosmic ray intensity variations connected with recurrent high-speed fluxes (HSF) of solar wind are i...
It has been established, that the beginning of the change of vector of Solar-diurnal anisotropy of G...
The measurement of the anisotropy in the arrival direction of cosmic rays is complementary to the st...
In this review an attempt is made to present an integrated view of the solar modulation process that...
On the basis of the model and experimental investigations, the spatial distribution of cosmic ray an...
Observations of the cosmic radiation generated by solar flares are used to study the propagation of ...
Investigations of cosmic ray anisotropies and their relationship to concurrent magnetic field data a...
The measurement of the anisotropies of cosmic ray arrival direction provides important informations ...
Abstract. The measurement of the anisotropy in the cosmic ray (CR) arrival direction distribution pr...
The search for an anisotrophy in the penetrating component of the cosmic-ray flux is usually carried...
A unified theory of cosmic ray diurnal variations has been proposed in which the first 3 harmonics o...
Two cosmic rays which pass through the same point going in opposite directions will, in the absence ...
Modulation model are discussed with more time spent on two current ideas: episodic modulation and dr...
It was demonstrated that an interplanetary magnetic field (IMF) sense dependent 2nd order anisotropy...
The distribution of galactic cosmic ray particles in the heliosphere is influenced (modulated) by t...
Cosmic ray intensity variations connected with recurrent high-speed fluxes (HSF) of solar wind are i...
It has been established, that the beginning of the change of vector of Solar-diurnal anisotropy of G...
The measurement of the anisotropy in the arrival direction of cosmic rays is complementary to the st...
In this review an attempt is made to present an integrated view of the solar modulation process that...
On the basis of the model and experimental investigations, the spatial distribution of cosmic ray an...
Observations of the cosmic radiation generated by solar flares are used to study the propagation of ...
Investigations of cosmic ray anisotropies and their relationship to concurrent magnetic field data a...
The measurement of the anisotropies of cosmic ray arrival direction provides important informations ...
Abstract. The measurement of the anisotropy in the cosmic ray (CR) arrival direction distribution pr...
The search for an anisotrophy in the penetrating component of the cosmic-ray flux is usually carried...
A unified theory of cosmic ray diurnal variations has been proposed in which the first 3 harmonics o...
Two cosmic rays which pass through the same point going in opposite directions will, in the absence ...
Modulation model are discussed with more time spent on two current ideas: episodic modulation and dr...
It was demonstrated that an interplanetary magnetic field (IMF) sense dependent 2nd order anisotropy...