Add to ORKGWe report on the comparison of time variations observed in the gamma ray component of cosmic radiation as measured by our detectors for Environmental Radiation operated in different locations at different time of the solar activity cy-cle. We study the response of these detectors in the occasion of Forbush decreases and ground level events, and compare our observation with those reported by the neutron monitor network
Since data-taking began in January 2004, the Pierre Auger Observatory has been recording the count r...
The Forbush effect is one of the striking examples of irregular variations in the cosmic ray (CR) fl...
Long-term instrumental measurements of the 1-100GeV/nucleon cosmic radia-tion intensity commenced in...
Three decades of research have shown that the cosmic ray intensity varies with time. Some of the va...
Since data-taking began in January 2004, the Pierre Auger Observatory has been recording the count r...
Since data-taking began in January 2004, the Pierre Auger Observatory has been recording the count r...
The Forbush effect is one of the striking examples of irregular variations in the cosmic ray (CR) fl...
Long-term instrumental measurements of the 1-100GeV/nucleon cosmic radia-tion intensity commenced in...
Three decades of research have shown that the cosmic ray intensity varies with time. Some of the va...
Since data-taking began in January 2004, the Pierre Auger Observatory has been recording the count r...
Since data-taking began in January 2004, the Pierre Auger Observatory has been recording the count r...
The Forbush effect is one of the striking examples of irregular variations in the cosmic ray (CR) fl...
Long-term instrumental measurements of the 1-100GeV/nucleon cosmic radia-tion intensity commenced in...