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Short-Term Variation of Cosmic Ray Diurnal Anisotropy and Solar Activity

机译:宇宙射线日各向异性和太阳活动的短期变化

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摘要

A correlative analysis has been made between cosmic ray intensity and solar activity (sunspot numbers) during high amplitude days for the period 1991-1995. The high amplitude days with the time of maximum in the corotational/azimuthal direction do not indicate any significant correlation with solar activity. The diurnal amplitude significantly remains constant and high (0.5%) during the entire period. Our observations suggest that the direction of the anisotropy of high amplitude anisotropic wave train events contribute significantly to the short-term behavior of the cosmic ray diurnal anisotropy. The correlation coefficient is found to remain positive during solar activity maximum for all the high amplitude anisotropic wave train events.
机译:在1991-1995年期间的高振幅天期间,宇宙射线强度与太阳活动(太阳黑子数)之间进行了相关分析。在方向/方位角方向上具有最大时间的高振幅天数并不表示与太阳活动有任何显着相关性。在整个周期中,昼夜振幅明显保持恒定且较高(0.5%)。我们的观察结果表明,高振幅各向异性波列事件的各向异性方向对宇宙射线昼夜各向异性的短期行为有重大贡献。发现在所有高振幅各向异性波列事件的太阳活动最大值期间,相关系数保持正值。

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