Improved Approach in the Coupling Function Between Primary and Ground Level Cosmic Ray Particles Based on Neutron Monitor Data

Solar Physics ◽  
2021 ◽  
Vol 296 (6) ◽  
Author(s):  
L. Xaplanteris ◽  
M. Livada ◽  
H. Mavromichalaki ◽  
L. Dorman ◽  
M. K. Georgoulis ◽  
...  
Keyword(s):  
Neutron Monitor ◽  
Cosmic Ray ◽  
Ground Level ◽  
Coupling Function ◽  
Neutron Monitor Data ◽  
Monitor Data

Modeling the solar cosmic ray event of 13 December 2006 using ground level neutron monitor data

2009 ◽  
Vol 43 (4) ◽  
pp. 474-479 ◽  
Author(s):  
C. Plainaki ◽  
H. Mavromichalaki ◽  
A. Belov ◽  
E. Eroshenko ◽  
V. Yanke
Keyword(s):  
Neutron Monitor ◽  
Cosmic Ray ◽  
Ground Level ◽  
Neutron Monitor Data ◽  
Monitor Data

The second spherical harmonic of the diurnal variation and the orientation of the interplanetary magnetic field

1968 ◽  
Vol 46 (10) ◽  
pp. S973-S975 ◽  
Author(s):  
G. V. Skeipin ◽  
P. A. Krivoshapkin ◽  
G. F. Krymsky ◽  
A. I. Kuzmin
Keyword(s):  
Magnetic Field ◽  
Diurnal Variation ◽  
Interplanetary Magnetic Field ◽  
Neutron Monitor ◽  
Spherical Harmonic ◽  
Cosmic Ray ◽  
Vector Information ◽  
Neutron Monitor Data ◽  
Distribution Vector ◽  
Monitor Data

The super neutron monitor data from Goose Bay and Deep River for 1965 have been analyzed to give month-to-month changes of the first and second harmonics of the solar-diurnal variation. Using these results together with various suppositions about the nature of the cosmic-ray distribution vector, information is obtained concerning the orientation of the interplanetary magnetic field.

scholarly journals Cosmic ray heliospheric transport study with neutron monitor data

2015 ◽  
Vol 120 (10) ◽  
pp. 8229-8246 ◽  
Author(s):  
H. S. Ahluwalia ◽  
R. C. Ygbuhay ◽  
R. Modzelewska ◽  
L. I. Dorman ◽  
M. V. Alania
Keyword(s):  
Neutron Monitor ◽  
Cosmic Ray ◽  
Transport Study ◽  
Neutron Monitor Data ◽  
Monitor Data

The enhanced daily variation in cosmic-ray intensity

1968 ◽  
Vol 46 (10) ◽  
pp. S794-S800 ◽  
Author(s):  
D. Venkatesan ◽  
T. Mathews
Keyword(s):  
Neutron Monitor ◽  
Daily Variation ◽  
Cosmic Ray ◽  
Cosmic Ray Intensity ◽  
Neutron Monitor Data ◽  
Monitor Data

The study of the super neutron monitor data from Calgary and Sulphur Mountain during January 1964 to May 1967 shows the importance of transient changes of intensity occurring over a few hours and its contribution to the daily variation. Trains of enhanced daily variation lasting a few days occur during recovery periods of fast Forbush and gradual decreases. The diurnal hour of maximum for a total of 250 days of enhanced daily variation during the period occurs at 17–18 h LT, which is the same as that for the rest of the period. The semidiurnal hour of maximum is distributed reasonably well over all hours, which points to its origin from transient changes in intensity.

Sign in / Sign up

Export Citation Format

Share Document