Cosmic ray fluxes in present and past times

被引:11
作者
Stozhkov, YI [1 ]
Okhlopkov, VP
Svirzhevsky, NS
机构
[1] Russian Acad Sci, PN Lebedev Phys Inst, Moscow, Russia
[2] Moscow MV Lomonosov State Univ, Skobeltsyn Inst Nucl Phys, Moscow, Russia
关键词
Atmosphere; Atom Concentration; Solar Activity; Ground Level; Sunspot Number;
D O I
10.1007/s11207-005-5193-1
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The data on primary cosmic ray fluxes at the top of the atmosphere are given for the period since 1937 till the present time. These data have been obtained from the regular cosmic ray flux measurements in the stratosphere and on the ground level. They have been used to find the relationship of cosmic ray fluxes with solar activity (sunspot number). On the basis of the deduced relationship the cosmic ray fluxes in the past have been recovered, as the sunspot number is known since 1500. The link between the smoothed data on Be-10 atom concentrations and cosmic ray fluxes is established which gives a possibility to calculate cosmic ray fluxes in the far past.
引用
收藏
页码:323 / 333
页数:11
相关论文
共 19 条
[1]   On galactic cosmic ray flux decrease near solar minima and imf intensity [J].
Ahluwalia, HS .
GEOPHYSICAL RESEARCH LETTERS, 2000, 27 (11) :1603-1606
[2]   USE OF BE-10 IN POLAR ICE TO TRACE THE 11-YEAR CYCLE OF SOLAR-ACTIVITY [J].
BEER, J ;
BLINOV, A ;
BONANI, G ;
FINKEL, RC ;
HOFMANN, HJ ;
LEHMANN, B ;
OESCHGER, H ;
SIGG, A ;
SCHWANDER, J ;
STAFFELBACH, T ;
STAUFFER, B ;
SUTER, M ;
WOLFLI, W .
NATURE, 1990, 347 (6289) :164-166
[3]  
BEER J, 2003, P 28 INT COSM RAY C, V7, P4147
[4]  
Beer J., 1994, SUN VARIABLE STAR SO, P291
[5]  
BLINOV AV, 1997, THESIS ST PETERSBURG
[6]  
CHARAKHCHYAN AN, 1976, T FIAN, V88, P3
[7]  
CHARAKHCHYAN AN, 1981, P 17 ICRC PAR, V3, P223
[8]   COSMIC-RAY INTENSITY VARIATIONS DURING 2 SOLAR CYCLES [J].
FORBUSH, SE .
JOURNAL OF GEOPHYSICAL RESEARCH, 1958, 63 (04) :651-669
[9]   WORLD-WIDE COSMIC-RAY VARIATIONS, 1937-1952 [J].
FORBUSH, SE .
JOURNAL OF GEOPHYSICAL RESEARCH, 1954, 59 (04) :525-542
[10]   Group Sunspot Numbers: A new solar activity reconstruction [J].
Hoyt, DV ;
Schatten, KH .
SOLAR PHYSICS, 1998, 179 (01) :189-219