Results 11 to 20 of about 1,156 (218)
Implications of Solar Wind Disturbances on Forbush Decrease [PDF]
Physics AccessThis study investigated the role of solar wind disturbances on variations in cosmic ray intensity. To conduct the study, use was made of the data on cosmic rays from the SOPO, CLMX, and MOSC neutron stations, as well as solar wind speed data from 2000 ...
Ogochukwu C Nwuzor +5 more
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Model of optical response of marine aerosols to Forbush decreases [PDF]
Atmospheric Chemistry and Physics, 2010 In order to elucidate the effect of galactic cosmic rays on cloud formation, we investigate the optical response of marine aerosols to Forbush decreases – abrupt decreases in galactic cosmic rays – by means of modeling. We vary the nucleation rate of new
T. Bondo, M. B. Enghoff, H. Svensmark
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The 1 June 2025 Forbush Decrease Measured over a Range of Primary Cosmic Ray Energies
UniverseThe 1 June 2025 Forbush decrease in the terrestrial ground-level flux of cosmic ray secondaries was recorded by many cosmic ray systems. This was the deepest such decrease from the quiescent value of the flux, which has been observed over the past two ...
Roger Clay
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Neutron monitor yield function: improved spectral computations of the Forbush decrease of June 2015 [PDF]
, 2023 In this work a new improved coupling function by Xaplanteris et al. (2021) based on Quantum Field Theory is applied for spectral analysis of cosmic rays.
Xaplanteris, Loukas +3 more
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Magnetic Cloud and Its Interplanetary Shock Sheath as a Modulator of the Cosmic Ray Intensity [PDF]
Journal of Astronomy and Space Sciences, 2008 Forbush Decreases (FDs) are representative events of abrupt decrease in galactic cosmic ray intensity. They are known to be strongly associated with solar wind events such as interplanetary shock (IP shock) and magnetic cloud (MC).
Su Yeon Oh
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Spectral features of Forbush Decrease during Geomagnetic Storms [PDF]
, 2023 Geomagnetic storms and Forbush decreases (FD) on Earth are primarily caused by interplanetary coronal mass ejections (ICMEs) and stream/corotating interaction regions (SIRs/CIRs) originating in the Sun, which are propagated as a low-energy plasma ...
Baral, Rabin +9 more
core +1 more source
Forbush-storm classification of the events as a device for the solar wind diagnostics [PDF]
E3S Web of Conferences, 2020 The geoeffectiveness of the solar wind is usually determined on Earth by such phenomena in the geomagnetic field as storms and substorms. The second, no less significant effect is a sharp decrease in the intensity of galactic cosmic rays (GCR) Forbush ...
Shadrina Lyudmila P.
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Earth and Planetary Physics, 2020 Forbush decreases are depressions in the galactic cosmic rays (GCRs) that are caused primarily by modulations of interplanetary coronal mass ejections (ICMEs) but also occasionally by stream/corotating interaction regions (SIRs/CIRs).
Jingnan Guo +4 more
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Space Weather, 2022 High‐energetic charged particles, such as solar protons, and phenomena such as Forbush decreases are eligible candidates to affect the global electric circuit.
J. Tacza +6 more
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SOLAR ACTIVITY AND EARTH SEISMICITY
Solar-Terrestrial Physics, 2021 Using the results of continuous long-term observations over 50 years (including solar cycles 20–24), we study the relationship between Earth’s seismicity and solar activity.
V.L. Yanchukovsky
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