The latitudinal behavior of intensities and multiplicities was registered by the neutron monitor 2 NM and the lead-free neutron monitor 3 SND (slow-neuron detector) in the equator-Kaliningrad line in the Atlantic Ocean. Coupling coefficients for 3 SND show the sensitivity of this detector to primary particles of cosmic rays of energies on the average lower than for 2 NM. As multiplicities increase, the coupling coefficients shift towards higher energies
Recordings on relativistic solar flare protons observed at Sanae, Antarctic, show that the percentag...
The main objective is to check whether the periodicities observed in the cosmic rays in the interval...
DOMC and DOMB neutron monitors (NM) operate at the Concordia research station (Dome C on the Antarct...
In 1981-1985 the neutron component of cosmic rays was recorded, the effect of cosmic ray multiplicat...
Multiplicity measurements using the NM-64 neutron monitor have been carried out continuously at Syow...
Thesis (Ph.D. (Physics))--North-West University, Potchefstroom Campus, 2006.The propagation of high-...
Sixty element 3He neutron multiplicity detector systems were designed, constructed and tested for us...
Neutron monitors are integral detectors of secondary cosmic rays. Since each of them has its own det...
Evaluation of barometer coefficients of neutron monitors located at high latitudes has been performe...
Modulation of cosmic-ray energy spectrum was studied by using the Turku double neutron monitor. The ...
In order to examine the stability of neutron monitor observation, each of the monthly average counti...
Two Bonner sphere spectrometers (BSSs) have recently been installed to measure secondary neutrons fr...
An introduction to the demography of cosmic ray neutrons including a detailed description of neutron...
Neutron monitors of standard design (IGY or NM64) are employed worldwide to study variations in the ...
The Sayan cosmic ray (CR) spectrograph recorded an SCR flare that occurred on 16 February 1984. Data...
Recordings on relativistic solar flare protons observed at Sanae, Antarctic, show that the percentag...
The main objective is to check whether the periodicities observed in the cosmic rays in the interval...
DOMC and DOMB neutron monitors (NM) operate at the Concordia research station (Dome C on the Antarct...
In 1981-1985 the neutron component of cosmic rays was recorded, the effect of cosmic ray multiplicat...
Multiplicity measurements using the NM-64 neutron monitor have been carried out continuously at Syow...
Thesis (Ph.D. (Physics))--North-West University, Potchefstroom Campus, 2006.The propagation of high-...
Sixty element 3He neutron multiplicity detector systems were designed, constructed and tested for us...
Neutron monitors are integral detectors of secondary cosmic rays. Since each of them has its own det...
Evaluation of barometer coefficients of neutron monitors located at high latitudes has been performe...
Modulation of cosmic-ray energy spectrum was studied by using the Turku double neutron monitor. The ...
In order to examine the stability of neutron monitor observation, each of the monthly average counti...
Two Bonner sphere spectrometers (BSSs) have recently been installed to measure secondary neutrons fr...
An introduction to the demography of cosmic ray neutrons including a detailed description of neutron...
Neutron monitors of standard design (IGY or NM64) are employed worldwide to study variations in the ...
The Sayan cosmic ray (CR) spectrograph recorded an SCR flare that occurred on 16 February 1984. Data...
Recordings on relativistic solar flare protons observed at Sanae, Antarctic, show that the percentag...
The main objective is to check whether the periodicities observed in the cosmic rays in the interval...
DOMC and DOMB neutron monitors (NM) operate at the Concordia research station (Dome C on the Antarct...