www.eettaiwan.com|基于98个网页 3. 太阳活动峰 每11年,太阳经历一个叫做“太阳活动峰(solar maximum)”的活动期,紧接着一个叫做“太阳活动谷(solar minimum)”的宁静期。 … haohz-lhp.blog.163.com|基于50个网页 更多释义 例句
CONSECUTIVE SOLAR MINIMUM AND MAXIMUM PERIODSElBorie, M A
solar maximum 太阳活动极大期；太阳极大期；太阳活动峰；太阳最大值 双语例句 1. The primary cosmic radiation that reaches the earth is minimum at periods of maximum solar activity.在极大的太阳活动时期,到达地球的初级宇宙辐射是极小值.来自辞典例句 2. The inner box is painted black to ab...
Superposed epoch analyses of 549 storms are performed to make a comparison of solar wind features of geomagnetic storm events at solar minimum (July 1974 to June 1977; July 1984 to June 1987; July 1994 to June 1997) and solar maximum (January 1979 to December 1981; January 1989 to December...
In winter (December to February), SLP composite differences between solar maximum and solar minimum phases at lag 0 years (see the Methods section and Supplementary Fig. 1) for the SOL experiment (Fig. 1a) show a statistically significant decrease of 2 hPa over the Arctic region, and a ...
During solar maximum,geomagnetic stormsoccur more often, with the majority driven by CMEs. During solar minimum, storms are mainly driven by CIRs (though CIR storms are more frequent at solar maximum than at minimum). Geomagnetic storm effects ...
suggest that for the Ariel 4 epoch $(Z\\approx 70)$ the behaviour is more appropriate to periods of maximum, rather than minimum, solar activity. Stu... C.,V.,Goodall,... - 《Proceedings of the Royal Society A Mathematical Physical & Engineering Sciences》 被引量: 4发表: 1975年 Sola...
(b) the SOHO/VIRGO TSI over solar cycle 23—the thick vertical dashed line marks the start of the SOHO/VIRGO record used. In both cases, the thick red lines are the 50-day running average over the measurements. While the mean solar minimum to solar maximum change in TSI is∼1 Wm...
and a half years, sunspot activity gets weaker and weaker, and then this builds for the next five and a half years. The peak of each cycle is the actual point of Solar Minimum, and Solar Maximum, however we refer to each five and a half period as Solar Minimum and Solar maximum too...
The research deals mainly with Very Large Array and Solar Maximum Mission observations of the ubiquitous coronal loops that dominate the structure of the low corona. As illustrated, the observations of thermal cyclotron lines at microwave wavelengths provide a powerful new method of accurately specifying...