Cosmic-ray data taken during the period of a solar flare and the magnetic storm that followed 26.5 hours later during July, 1946, are reported. The results following the flare agree with those of other investigators and, in addition, serve to establish the fact that the start of the cosmic-ray effect and the visual part of the solar flare were simultaneous. It is pointed out that increases of cosmic rays during solar flares suggest a mode of origin of the rays. The lack of effect of most solar flares on cosmic-ray intensity is noted and differences in intensity of the flares given as a possible reason. A high altitude balloon flight with an electroscope during the magnetic storm gave results in agreement with the current-sheet hypothesis of...
Shocks driven by energetic coronal mass ejections (CME's) and other interplanetary (IP) transie...
The present International Geophysical Year was chosen to include the most likely period of maximum a...
We investigate the trend of the nucleonic intensity of the cosmic rays during the large geomagnetic ...
The small effects produced by solar flares on cosmic ray intensity has been investigated.In the firs...
Five large cosmic ray bursts in connection with solar flares have been observed till now. Two of the...
The small effects produced by solar flares on cosmic ray intensity has been investigated.In the firs...
Among the upper air observations of cosmic ray intensity, Pomerantz after a preliminary choice selec...
179-182Ground based worldwide network of neutron monitors (Kiel, Oulu, Moscow and Norilsk) recorded...
This review attempts to present an integrated view of the several types of solar cosmic ray phenomen...
Seven examples of the observation of intense fluxes of ≈10-Mev charged particles associated with dis...
The amplitudes of geomagnetic sudden commencements are examined in ion to the optical, energetic par...
Observations of the cosmic radiation generated by solar flares are used to study the propagation of ...
The observation of solar flares in visual light is mostly made in the light of hydrogen-α, which sho...
The observation of solar flares in visual light is mostly made in the light of hydrogen-α, which sho...
Geomagnetic storms are initiated by organized magnetic structures of the solar wind. The intensity o...
Shocks driven by energetic coronal mass ejections (CME's) and other interplanetary (IP) transie...
The present International Geophysical Year was chosen to include the most likely period of maximum a...
We investigate the trend of the nucleonic intensity of the cosmic rays during the large geomagnetic ...
The small effects produced by solar flares on cosmic ray intensity has been investigated.In the firs...
Five large cosmic ray bursts in connection with solar flares have been observed till now. Two of the...
The small effects produced by solar flares on cosmic ray intensity has been investigated.In the firs...
Among the upper air observations of cosmic ray intensity, Pomerantz after a preliminary choice selec...
179-182Ground based worldwide network of neutron monitors (Kiel, Oulu, Moscow and Norilsk) recorded...
This review attempts to present an integrated view of the several types of solar cosmic ray phenomen...
Seven examples of the observation of intense fluxes of ≈10-Mev charged particles associated with dis...
The amplitudes of geomagnetic sudden commencements are examined in ion to the optical, energetic par...
Observations of the cosmic radiation generated by solar flares are used to study the propagation of ...
The observation of solar flares in visual light is mostly made in the light of hydrogen-α, which sho...
The observation of solar flares in visual light is mostly made in the light of hydrogen-α, which sho...
Geomagnetic storms are initiated by organized magnetic structures of the solar wind. The intensity o...
Shocks driven by energetic coronal mass ejections (CME's) and other interplanetary (IP) transie...
The present International Geophysical Year was chosen to include the most likely period of maximum a...
We investigate the trend of the nucleonic intensity of the cosmic rays during the large geomagnetic ...