摘要: To facilitate the use of cosmic-ray intensity data from ionization chambers which are being sent to International Geophysical Year World Data Centers, and those have appeared in two publications Carnegie Institution Washington, an improved correction for instrumental drift at Huancayo is derived reliability corrections seasonal variations discussed. From chambers, decrease its maxima (near sunspot minima) shown lag a year or more behind increase solar activity following minima. This does not appear results obtained by Neher high altitude latitude, nor Rose neutron monitor Ottawa. The variability daily means (from monthly means) 1957 largest observed during complete cycles. Tables corrected wave included, together with graphs period 1954–1957.
harvard.edu
agu.org参考文章(6)
Scott E. Forbush, Isabelle Lange, Cosmic-ray results from Huancayo Observatory, Peru, June 1936-December, 1946 : including summaries from observatories at Cheltenham, Christchurch, and Godhavn through 1946 Carnegie Institution of Washington. ,(1948)
J. Bartels, Random fluctuations, persistence, and quasi-persistence in geophysical and cosmical periodicities Journal of Geophysical Research. ,vol. 40, pp. 1- 60 ,(1935) , 10.1029/TE040I001P00001
Scott E. Forbush, World‐wide cosmic ray variations, 1937–1952 Journal of Geophysical Research. ,vol. 59, pp. 525- 542 ,(1954) , 10.1029/JZ059I004P00525
H. V. Neher, V. Z. Peterson, E. A. Stern, Fluctuations and latitude effect of cosmic rays at high altitudes and latitudes Physical Review. ,vol. 90, pp. 655- 674 ,(1953) , 10.1103/PHYSREV.90.655
Peter Meyer, J. A. Simpson, Changes in the Low-Energy Particle Cutoff and Primary Spectrum of Cosmic Rays Physical Review. ,vol. 106, pp. 568- 571 ,(1955) , 10.1103/PHYSREV.106.568
H. V. Neher, Low-energy primary cosmic-ray particles in 1954 Physical Review. ,vol. 103, pp. 228- 236 ,(1956) , 10.1103/PHYSREV.103.228