A. S. Lidvansky

Transient variations of secondary cosmic rays due to atmospheric electric field and evidence for pre-lightning particle acceleration

We present the data on short-term variations of the intensity of secondary cosmic rays during thunderstorm periods. The effect is studied separately for the soft (electrons) and hard (muons) components of cosmic rays, their intensities being correlated with the near-earth electric field using a second-order polynomial. It is shown that the linear and quadratic terms are dominant for the soft and hard components, respectively. In addition, some irregular enhancements of the soft component just before lightning discharges are observed giving evidence in favor of some particle acceleration process. They can be considered as an experimental confirmation of the runaway breakdown theory developed for the process of lightning initiation.

Investigating the separatrices for the runaway threshold of cosmic ray electrons in a thunderstorm atmosphere

Using a modified GEANT4 code, we calculated the probabilities for cosmic ray electrons to become runaway particles in an electric field with a strength ranging from 0 to 5 kV/cm. About 10 million trajectories were calculated for particles with initial energies of 0.1 to 100 MeV. Instead of a single separatrix determining the region of runaway electrons, a set of curves connecting points with equal probabilities of a runaway regime (from 0 to 100%) was obtained. It was shown that not only is the threshold for a runaway regime probabilistic in character, but the critical field as well. This must be considered when calculating variations in the intensity of cosmic rays during thunderstorms.

Studying the muon and hadron components of extensive air showers with the Carpet-2 array

The method of separating muons and hadrons recorded by the Muon Detector of the Carpet-2 air shower array of Baksan Neutrino Observatory (Institute for Nuclear Research, Russian Academy of Sciences) is described. The results of studying characteristics of the muon and hadron components of extensive air showers (EAS) with Ne ≥ 105 are presented. For the range of distances 40–55 m from shower axes the numbers of hadrons with energies higher than 30 GeV and muons with energies above 1 GeV are obtained as functions of the shower size Ne.

Strong variations of cosmic ray muons during thunderstorms

Experimental data about a strong decrease of the intensity of cosmic ray muons are presented. The event occurred during a thunderstorm on September 24, 2007 in Baksan Valley (North Caucasus). The threshold energy of muons is 100 MeV. In comparison with other events of this type detected previously, this event is remarkable by a longer duration (more than an hour and a half) and by the fact that well-pronounced correlations with lightning strokes are observed for the first time.

Reconstruction of the direction of the true anisotropy of galactic cosmic rays

A method of reconstructing the declination of galactic cosmic ray anisotropy is described, and its results are presented. The method is based on analysis of delay distributions in symmetrically arranged detectors of an air shower array, and it represents a modification of the crossed telescopes method. It is shown that the declination of the true anisotropy vector is close to 60° (i.e., this vector lies approximately within the galactic plane). Because of this, the true degree of anisotropy of galactic cosmic rays is severalfold higher than the first harmonic of intensity in the sidereal time (the quantity measured directly), and it equals about 0.2%.

The Carpet-3 experiment to search for diffuse gamma rays with energies of more than 100 TeV

An experiment for measuring the flux of cosmic diffuse gamma rays with energies above 100 TeV (the Carpet-3 air shower array) is now being prepared at the Baksan Neutrino Observatory, Institute for Nuclear Research, Russian Academy of Sciences. The preparations entail a substantial increase of the areas of both the muon detector and the surface air shower array. The experiment’s sensitivity to showers generated by primary gamma rays is estimated for different configurations of the array. In addition, preliminary estimates of the upper limit on the flux of diffuse gamma rays with energies higher than 1.3 PeV, derived using experimental data from the old Carpet-2 array, are presented for a net exposure time of 9.2 years.

Lateral distribution function of charged particles in EAS near the axis

High-precision measurements of the lateral distribution function (LDF) of charged particles near the axis of extensive air showers (EASes) were performed with the CARPET air shower array of the Baksan Neutrino Observatory for several ranges of Ne, including the knee region. For the sake of comparison with the experiment, calculations for primary protons and iron nuclei were made using the CORSIKA code (the QGSJET01C model of interaction). The measured experimental LDF is compared with our calculations.

Direction of the anisotropy vector of TeV cosmic rays

The preliminary results of measuring the direction of the stellar anisotropy vector of cosmic rays with the Carpet array at the Baksan Neutrino Observatory (Institute for Nuclear Research, Russian Academy of Sciences) are presented. The direction of the anisotropy vector is determined by analyzing the distribution of time delays of the signal from distant detectors of the array with respect to its central part. It is shown that the anisotropy vector has the direction α0 (R.A.) ≈ 1.5 h, δ0 ≈ 62° in the equatorial coordinate system. At such a direction, the CR anisotropy measured with the Baksan Underground Scintillation Telescope and the Andyrchi array is ≈0.2%.

Variations in cosmic rays during thunderstorms and new geophysical effects

Processes that occur during thunderstorms accompanied by anomalous disturbances in cosmic rays are comprehensively investigated using the Carpet air shower array at the Baksan Neutrino Observatory. The data collected so far indicate the discovery of a new type of electric discharge: runaway electron break-down in the near-threshold regime. A glow in the stratosphere corresponding to this discharge is detected, as is stabilization of geomagnetic micro-pulsations. Both are demonstrated using one event as an example.

Comprehensive study of energetic particle processes in thunderclouds

In the course of an experiment studying variations of cosmic rays during thunderstorms at the Baksan Neutrino Observatory evidence has been obtained in favor of existence of a new type of large-scale electric discharge in thunderstorm atmosphere: a slow runaway electron breakdown in the near-threshold regime. Continuous glow of the stratosphere region above thunderclouds is discovered, correlating with anomalous disturbances in intensity of secondary cosmic rays detected on the ground.