Evolution of cosmic ray fluxes during the rising phase of solar cycle 23: ULYSSES EPAC and COSPIN/KET observations

2000 ◽  
Author(s):  
B. Heber
Keyword(s):  
Solar Cycle ◽  
Cosmic Ray ◽  
Solar Cycle 23

scholarly journals Investigation of the relation between space-weather parameters and Forbush decreases automatically selected from Moscow and Apatity cosmic ray stations during solar cycle 23

2021 ◽  
Vol 21 (11) ◽  
pp. 273
Author(s):  
Jibrin Adejoh Alhassan ◽  
Ogbonnaya Okike ◽  
Augustine Ejikeme Chukwude
Keyword(s):  
Solar Cycle ◽  
Space Weather ◽  
Cosmic Ray ◽  
Computer Code ◽  
Weather Data ◽  
Forbush Decreases ◽  
Two Samples ◽  
Solar Cycle 23 ◽  
Weather Parameters ◽  
Galactic Cosmic Ray

Abstract We present the results of an investigation of the relation between space-weather parameters and cosmic ray (CR) intensity modulation using algorithm-selected Forbush decreases (FDs) from Moscow (MOSC) and Apatity (APTY) neutron monitor (NM) stations during solar cycle 23. Our FD location program detected 408 and 383 FDs from MOSC and APTY NM stations respectively. A coincident computer code employed in this work detected 229 FDs that were observed at the same Universal Time (UT) at the two stations. Out of the 229 simultaneous FDs, we formed a subset of 139 large FDs(%) ≤ − 4 at the MOSC station. We performed a two-dimensional regression analysis between the FD magnitudes and the space-weather data on the two samples. We find that there were significant space-weather disturbances at the time of the CR flux depressions. The correlation between the space-weather parameters and decreases in galactic cosmic ray (GCR) intensity at the two NM stations is statistically significant. The implications of the present space-weather data on CR intensity depressions are highlighted.

scholarly journals Long-Term Cosmic Ray Variability and the CME-Index

2012 ◽  
Vol 2012 ◽  
pp. 1-8 ◽  
Author(s):  
Helen Mavromichalaki ◽  
Evangelos Paouris
Keyword(s):  
Standard Deviation ◽  
Solar Cycle ◽  
Cosmic Ray ◽  
Heliospheric Current Sheet ◽  
Angular Width ◽  
Cosmic Ray Intensity ◽  
Cosmic Ray Modulation ◽  
Solar Cycle 23 ◽  
Solar Cycle 24 ◽  
Cycle 24

The cosmic ray modulation in relation to solar activity indices and heliospheric parameters during the period January 1996–October 2011, covering the solar cycle 23 and the ascending phase of solar cycle 24, is studied. The new perspective of this contribution is that the CME-index, obtained from only the CMEs with angular width greater than 30 degrees, gives much better results than in previous works. The proposed model for the calculation of the modulated cosmic ray intensity obtained from the combination of solar indices and heliospheric parameters gives a very satisfactory value of the standard deviation. The best reproduction of the cosmic ray intensity is obtained by taking into account solar and interplanetary indices such as sunspot number, interplanetary magnetic field, CME-index, and heliospheric current sheet tilt. The standard deviation between the observed and calculated values is about 6.63% for the solar cycle 23 and 4.13% for the ascending part of solar cycle 24.

Study of Cosmic Ray Intensity in Relation to the Interplanetary Magnetic Field and Geomagnetic Storms for Solar Cycle 23

Solar Physics ◽  
2016 ◽  
Vol 291 (2) ◽  
pp. 603-611 ◽  
Author(s):  
Hema Kharayat ◽  
Lalan Prasad ◽  
Rajesh Mathpal ◽  
Suman Garia ◽  
Beena Bhatt
Keyword(s):  
Magnetic Field ◽  
Solar Cycle ◽  
Interplanetary Magnetic Field ◽  
Geomagnetic Storms ◽  
Cosmic Ray ◽  
Cosmic Ray Intensity ◽  
Solar Cycle 23
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