A hydromagnetic model of the solar eclipse effect on the diurnal variation of the geomagnetic field

1964 ◽  
Vol 8 (3) ◽  
pp. 314-316
Author(s):  
Jacoclv Taueb ◽  
A. Zátopek
Keyword(s):  
Diurnal Variation ◽  
Solar Eclipse ◽  
Geomagnetic Field ◽  
Eclipse Effect

Solar Eclipse Effect on Shelter Air Temperature

1996 ◽  
Vol 77 (1) ◽  
pp. 89-99 ◽  
Author(s):  
M. Segal ◽  
R. W. Turner ◽  
J. Prusa ◽  
R. J. Bitzer ◽  
S. V. Finley
Keyword(s):  
Air Temperature ◽  
Solar Eclipse ◽  
Eclipse Effect

Possible Influence of the Solar Eclipse on the Global Geomagnetic Field

2017 ◽  
Vol 13 (S335) ◽  
pp. 167-170
Author(s):  
Jung-Hee Kim ◽  
Heon-Young Chang
Keyword(s):  
Solar Activity ◽  
Solar Cycle ◽  
Solar Eclipse ◽  
Geomagnetic Field ◽  
Geomagnetic Observatory ◽  
Geomagnetic Disturbances ◽  
Solar Eclipses ◽  
A Site

AbstractWe investigate the geomagnetic field variations recorded by INTERMAGNET geomagnetic observatories. We confirm that the effect of solar eclipse can be seen over an interval of 180 minutes centered at the time of maximum eclipse on a site of a geomagnetic observatory. It is found that the effect of the solar eclipse on the geomagnetic field becomes conspicuous as the magnitude of a solar eclipse becomes larger. The effect of solar eclipses is more evident in the second half of the path of Moon’s shadow. We also find that the effect can be overwhelmed, more sensitively by geomagnetic disturbances than by solar activity of solar cycle.

Possible solar eclipse effect 23 October 1976

Nature ◽  
1978 ◽  
Vol 271 (5640) ◽  
pp. 91-92 ◽  
Author(s):  
G. L. M. SCHEEPERS
Keyword(s):  
Solar Eclipse ◽  
Eclipse Effect

On the nature of some anomalies in the cosmic-ray distribution

1968 ◽  
Vol 46 (10) ◽  
pp. S614-S616 ◽  
Author(s):  
N. P. Chirkov ◽  
G. F. Krymsky ◽  
A. I. Kuzmin
Keyword(s):  
Magnetic Field ◽  
Diurnal Variation ◽  
Interplanetary Magnetic Field ◽  
Equatorial Plane ◽  
Geomagnetic Field ◽  
Cosmic Ray ◽  
Neutron Monitors ◽  
Vector Method ◽  
Worldwide Network ◽  
Northern And Southern Hemispheres

Diurnal and semidiurnal variations of the data from the worldwide network of neutron monitors during 1958 are analyzed using the receiving-vector method. It is shown that there exists an "antisymmetric" diurnal variation, i.e., a variation with opposite phases in the northern and southern hemispheres. After correction for the distortion due to the geomagnetic field, it is found that this variation has an amplitude of 0.03% and an hour of maximum at 21.5 hours in the northern hemisphere. If the variation is due to cosmic-ray screening in the interplanetary magnetic field, this field must have a slope of 7° with respect to the solar equatorial plane.

Geomagnetic Field Variations during the Total Solar Eclipse of 2 July 2019 in La Serena, Chile

2021 ◽  
Vol 61 (2) ◽  
pp. 287-292
Author(s):  
P. Vega-Jorquera ◽  
J. A. Lazzús ◽  
L. Tamblay ◽  
L. Palma-Chilla ◽  
I. Salfate ◽  
...  
Keyword(s):  
Solar Eclipse ◽  
Geomagnetic Field ◽  
Total Solar Eclipse
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