延误分析

D. Rohini, R. Chimmalgi
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引用次数: 0

摘要

: TSSA和CTSI相互延迟或滞后1,3,5。利用太阳周期数据(21,22,23)进行分析,得出了H α耀斑指数与延迟之间可能存在的相关关系,发现这两个参数呈反相关关系,相关系数为0.8 9427。27日太阳活动相关系数最高。定义了一个新的参数,称为延迟索引数(d1)。该参数在第21、22、23太阳活动周的时间跨度内,出现了延迟事件数的两个尖峰。峰值在1986年和1996年太阳平静期下降。因此,D I作为太阳相当相位(即太阳极小期)的指示器。急剧上升的可能原因正在调查中。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Delay Analysis
: TSSA and CTSI shows delay or lag wrt each other 1,3,5 . Solar cycle data (21,22,23) is used in the analysis and possible correlation between H alpha flare index and delay is worked out .It is found that these two parameters are anti correlated with a correlation factor of 0.8 9427 . The 27day solar activity shows heighest correlation factor. A new parameter called delay index number ( D I ) is defined.This paramter shows two sharp peaks wrt delay event number ,during the span of solar cycle 21,22,23. The peaks fall in soalr quite period 1986 and 1996. Thus D I acts as an indicator of quite phase (ie solar minima )of sun.The possible cause for sharp shoot up is under investigation.
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