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11.
本文对第22太阳周(1987年1月至1992年12月)中发生过M级以上的X射线耀斑(Hα耀斑级别≥M级,并伴有X射线的耀斑)对应的395个活动区资料进行了耀斑指数的统计,得到的结果:1.22太阳周M级以上X射线耀斑级别综合指数表,2.22太阳周M级以上X射线耀斑总指数表,3.第22太阳周M级以上X射线耀斑总指数随时间的变化曲线,4.第22太阳周M级以上X射线濯斑总指数直方图,该图表明第22太阳周活动的极大年分别是1989和1991年,为第23周太阳活动预报提供了可用参数。 相似文献
12.
我们对第12周至第22周的太阳黑子月平均面积数进行统计分析,并与相应的太阳黑子月平均数相比较,结果表明太阳黑子月平均面积数活动周与太阳黑子月平均数活动周有一定的关系。在多数情况下,太阳黑子出现最大值的时间与太阳黑子面积数出现最大值的时间上不一致;太阳黑子平滑月平均数活动周上升期与太阳黑子平滑月平均面积数上升期在大多数情况下不相同;太阳黑子平滑月平均数活动周平均效果的瓦德迈尔效应(Waldmeiereffect)一般要比太阳黑子平滑平均面积数的活动周明显;文中还对太阳黑子平滑月平均面积数活动周的特征进行了分析。 相似文献
13.
Interplanetary field enhancements were first discovered in the vicinity of Venus. These events are characterised by an increase in the magnitude of the heliospheric magnetic field with a near-symmetrical, sometimes thorn-shaped profile, and last from minutes to hours. Surveys of the events near Venus and Earth indicated clustering of the events in inertial space, which suggested that their sources were Solar System objects other than the Sun. A survey is presented of strong events of this type detected by the Ulysses spacecraft from 1990 to late 2001. Most of the events are accompanied by a discontinuity in the field direction near the events' centres. Other discontinuities are often symmetrical about the enhancement. The majority of events last less than two hours. When examined as a whole, the events tend to be accompanied by subtle changes in some plasma parameters. The majority of the enhancements are accompanied by magnetic holes on their fringes. The enhancements' occurrence rate increases with decreasing heliocentric distance. Possible formation mechanisms are discussed. No link was found with solar, or solar wind sources. Several aspects of the survey results are consistent with an origin related to cometary dust trails. Possible processes associated with a dust-solar wind interaction are discussed. 相似文献
14.
Wolfram Neutsch Herbert Kalisch Horst Fichtner S. Ranga Sreenivasan Maurice Shevalier 《Astrophysics and Space Science》2003,288(3):391-408
The study of the expansion of the solar wind out of a system of coronal holes is continued. To this end, we consider the numerical
integration of partial differential equations for problems with icosahedral symmetry, in general. First, employing Weyl theory,
orbifold coordinates are introduced. Second, the icosahedral coordinates are discussed in detail. Third, following an analysis
of the properties of these coordinates and the derivation of a few expressions useful for grid construction, various alternatives
for the distribution of lattice points required for numerical integration are considered. A comparison of these numerical
grids motivates the choice of a specific grid optimized for the numerical integration carried out in the accompanying paper
by Kalish et al.(2002).
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
15.
本文简要地介绍了云南天文台太阳射电快速记录系统PIN调制器的运用,描述了该器件的结构原理和性能检测,并给出了测试结果 相似文献
16.
Memorial landscapes: analytic questions and metaphors 总被引:1,自引:0,他引:1
Over the past two decades, geographers have probed the intersection of collective memory and urban space. Their sustained
interest in the subject reflects an understanding of the social condition of commemoration and the important role that space
plays in the process and politics of collective memory. Along with other critical social scientists, geographers envision
these public symbols as part of larger cultural landscapes that reflect and legitimate the normative social order. A review
of the extant literature indicates that geographers scrutinize memorial landscapes through three conceptual lenses that may
be understood via the metaphors of ‘text,’ ‘arena,’ and ‘performance.’ These metaphors are in turn mobilized through a series
of analytic questions that serve to identify the interests served and denied by landscape ‘texts,’ the ‘arenas’ in which they
are produced, and the ways in which they are enacted via ‘performance.’ This article’s synopsis of the subfield’s predominant
metaphors and its attendant questions contributes to the ongoing cultural geographic project of articulating and implementing
methods for interpreting landscapes as open-ended symbolic systems.
相似文献
Derek H. AldermanEmail: |
17.
Farn Parungo Clarence Nagamoto Cecilia M. I. R. Girz Jeff Torgerson Zhou Mingyu 《海洋学报(英文版)》1995,14(2):201-207
ObservationofcloudsandsolarradiationoverthePacificOceanasrelationtoglobalclimate¥FarnParungo;ClarenceNagamoto;CeciliaM.I.R.Gi... 相似文献
18.
气溶胶光学厚度的时空变化 总被引:2,自引:0,他引:2
在大气中气溶胶微粒是一种重要的大气微量成分。气溶胶光学厚度也是大气校正所需的重要大气参数,同时也是海洋水色卫星主要的数据产品。由于气溶胶光学厚度的时空变化较大,所以如何准确获取大气校正和卫星数据产品真实性检验所需的气溶胶光学厚度则是至关重要的。在简述气溶胶光学性质的基础上,并结合2002年6月HY—1南海实验数据来阐述现场气溶胶光学厚度的准确获取。 相似文献
19.
20.
We discuss the winding of a force-free axisymmetric magnetic field rooted on a heavy conductor onz=0. In quadrupolar symmetry the field expands in the half-spacez>0 and the toroidal flux concentrates on a conical surface. After a mean twist of 208°, the conical layer hosts large toroidal current loops with reversal of the magnetic flux on either side. The evolution of the field structure is described by scale-free static solutionsBr
–(p+2), withp taking values between 0 and 2. The large expansion factor of the field structure is suggestive of flaring originating on the solar photosphere. 相似文献