Skip to main content

and
  1. No Access

    Article

    Measurement of the large-scale anisotropy of cosmic rays in the PAMELA experiment

    Large-scale anisotropy or so-called sidereal-diurnal wave has been detected in the PAMELA satellite experiment in the time interval of 2006–2014. The magnitude of anisotropy has been measured simultaneously fo...

    A. V. Karelin, O. Adriani, G. C. Barbarino, G. A. Bazilevskaya, R. Bellotti in JETP Letters (2015)

  2. No Access

    Article

    Detection of a change in the North-South ratio of count rates of particles of high-energy cosmic rays during a change in the polarity of the magnetic field of the Sun

    A change in the ratio of the intensities of particles of high-energy cosmic rays arriving from the North and South in the time interval of 2010–2014 has been detected with a calorimeter entering into the exper...

    A. V. Karelin, O. Adriani, G. C. Barbarino, G. A. Bazilevskaya, R. Bellotti in JETP Letters (2015)

  3. No Access

    Article

    Measurement of the flux of primary cosmic ray antiprotons with energies of 60 MeV to 350 GeV in the PAMELA experiment

    It is interesting to measure the antiproton galactic component in cosmic rays in order to study the mechanisms by which particles and antiparticles are generated and propagate in the Galaxy and to search for n...

    O. Adriani, G. A. Bazilevskaya, G. C. Barbarino, R. Bellotti, M. Boezio in JETP Letters (2013)

  4. No Access

    Article

    Upper limit on the antihelium flux in primary cosmic rays

    The explanation of the observed baryon asymmetry, i.e., the almost complete absence of antimatter in the visible part of the universe, is one of the most important problems in cosmology. The real asymmetry val...

    A. G. Mayorov, A. M. Galper, O. Adriani, G. A. Bazilevskaya, G. Barbarino in JETP Letters (2011)