Theory and modeling of galactic cosmic rays: Trends and prospects
J Kóta - Space Science Reviews, 2013 - Springer
We address past and future trends in the theory and modeling of galactic cosmic rays in the
heliosphere, and select some of the outstanding issues where future progress is anticipated …
heliosphere, and select some of the outstanding issues where future progress is anticipated …
Global muon detector network used for space weather applications
M Rockenbach, A Dal Lago, NJ Schuch… - Space Science …, 2014 - Springer
In this work, we summarize the development and current status of the Global Muon Detector
Network (GMDN). The GMDN started in 1992 with only two muon detectors. It has consisted …
Network (GMDN). The GMDN started in 1992 with only two muon detectors. It has consisted …
Monitoring short-term cosmic-ray spectral variations using neutron monitor time-delay measurements
Neutron monitors (NMs) are ground-based detectors of cosmic-ray showers that are widely
used for high-precision monitoring of changes in the Galactic cosmic-ray (GCR) flux due to …
used for high-precision monitoring of changes in the Galactic cosmic-ray (GCR) flux due to …
The temperature effect in secondary cosmic rays (muons) observed at the ground: Analysis of the global muon detector network data
The analysis of cosmic ray intensity variation seen by muon detectors at Earth's surface can
help us to understand astrophysical, solar, interplanetary and geomagnetic phenomena …
help us to understand astrophysical, solar, interplanetary and geomagnetic phenomena …
Determination of interplanetary coronal mass ejection geometry and orientation from ground‐based observations of galactic cosmic rays
T Kuwabara, JW Bieber, P Evenson… - Journal of …, 2009 - Wiley Online Library
We have developed a method for determining interplanetary coronal mass ejection (ICME)
geometry from galactic cosmic ray data recorded by the ground‐based muon detector …
geometry from galactic cosmic ray data recorded by the ground‐based muon detector …
Corrections for temperature effect for ground-based muon hodoscopes
AN Dmitrieva, RP Kokoulin, AA Petrukhin… - Astroparticle …, 2011 - Elsevier
Influence of atmospheric temperature on muon flux at sea level is considered. Results of
calculations of muon spectrum for normal atmospheric conditions, differential temperature …
calculations of muon spectrum for normal atmospheric conditions, differential temperature …
[PDF][PDF] On energetic particles in space
K Kudela - acta physica slovaca, 2009 - physics.sk
Particles energized above the Earth's atmosphere provide unique informations about
specific physical processes in the outer space. This is an attempt to present a short review of …
specific physical processes in the outer space. This is an attempt to present a short review of …
Global Analysis of the Extended Decreases in Cosmic Rays Observed with Worldwide Networks of Neutron Monitors and Muon Detectors: Temporal Variation of the …
K Munakata, Y Hayashi, M Kozai, C Kato… - The Astrophysical …, 2024 - iopscience.iop.org
This paper presents the global analysis of two extended decreases in the galactic cosmic-
ray intensity observed by worldwide networks of ground-based detectors in 2012. This …
ray intensity observed by worldwide networks of ground-based detectors in 2012. This …
Long-term variation of the solar diurnal anisotropy of galactic cosmic rays observed with the Nagoya multi-directional muon detector
K Munakata, M Kozai, C Kato, J Kota - The Astrophysical Journal, 2014 - iopscience.iop.org
We analyze the three-dimensional anisotropy of the galactic cosmic ray (GCR) intensities
observed independently with a muon detector at Nagoya in Japan and neutron monitors …
observed independently with a muon detector at Nagoya in Japan and neutron monitors …
Measurement and simulation of neutron monitor count rate dependence on surrounding structure
Neutron monitors are the premier instruments for precise measurements of time variations
(eg, of solar origin) in the galactic cosmic ray (GCR) flux in the range of∼ 1–100 GeV …
(eg, of solar origin) in the galactic cosmic ray (GCR) flux in the range of∼ 1–100 GeV …