Variations of the Cosmic Ray Intensity During Magnetic Storms
نویسندگان
چکیده
منابع مشابه
Time and other Variations in the Intensity of Cosmic Ray Neutrons
We have measured the barometer coefficient of cosmic ray neutron production at sea level and find the value —9,25% ± 0,20/cmHg. We have shown that there is no diurnal variation of neutron production of amplitude greater than about 0,4 %. The effects of the large solar flare of November 19th, 1949 on cosmic ray neutrons were much greater than on ionising cosmic rays at sea level; the maximum fac...
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[1] Differential intensity measurements of interplanetary H, He, and O ions made with the Low-Energy Charged Particle (LECP) instruments aboard the Voyager 1 (V1) and Voyager 2 (V2) deep space probes and the Low-Energy Ion Composition Analyzer (LICA) aboard the near-Earth Solar Anomalous Magnetospheric Particle Explorer (SAMPEX) satellite provide a comprehensive perspective on the transport of ...
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Cosmic Rays (CR) travel at speeds essentially indistinguishable from the speed of light. However whilst travelling through magnetic fields, both regular and turbulent, they are delayed behind the light since they are usually charged particles and their paths are not linear. Those delays can be so long that they are an impediment to correctly identifying sources which may be variable in time. Fu...
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ژورنال
عنوان ژورنال: Tellus
سال: 1954
ISSN: 0040-2826,2153-3490
DOI: 10.3402/tellusa.v6i3.8738