Correlation of Pc 3, 4, and 5 activity with solar wind speed
Correlation of Pc 3, 4, and 5 activity with solar wind speed
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Pc 3、4、5活动与太阳风速的相关性
DOI：
10.1029/ja084ia11p06694
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发表时间：
1979
影响因子：
--
通讯作者：
C. Russell
中科院分区：
文献类型：
--
作者：
E. Greenstadt;J. Olson;Philip D. Loewen;H. Singer;C. Russell
发现在卡尔加里和勒杜克的Pc 3，4和5的磁脉动振幅与太阳风速度的正相关性。1970年9月和10月获得的数据证实并扩展了仅在卡尔加里发现的Pc 3，4早期间隔中的类似结果，从而为速度控制的贡献（如开尔文-亥姆霍兹不稳定性）提供了进一步的证据。
Positive correlations of magnetic pulsation amplitude with solar wind speed are found for Pc 3, 4, and 5 at both Calgary and Leduc. The data, obtained in September and October 1970, confirm and extend similar results found in an earlier interval for Pc 3, 4 at Calgary alone, thus adding further evidence for a velocity-controlled contribution, such as the Kelvin-Helmholtz instability, to pulsation activity.