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71.
1 IntroductionThesolaractivecycleisusuallydescribedwiththerelativesunspotnumbers.Analysesofhis toricaldataontherelativesunspotnumbershaverevealedawealthofinformationaboutthesolaractivecycle (HongQinfang 1 990 ,1 994;ZhongShuhua 1 991 ,1 995 ) .Theso called 1 1 yearpe rio… 相似文献
72.
依据太阳光子辐射产生的光压理论,作者揭示出了自然界存在有如下两种自然现象:(1)揭示了日-地闻天然形成的能量(动量)相耦舍的"轧制"式和"摇摆"式物理机制及其存在的证据.阐明了包括地壳运动、地震和火山活动在内的地球内动力地质作用所需要的能源(力源)不是传统地质学所理解的仅来自于地球内部,而主要是来自于太阳.太阳与其系内行星之间不单是先前人们所理解的靠万有引力作用所维系的那种家族式的首领关系,而且也是靠太阳辐射的斥力作用形成的"母子"关系.地球自生成以来,主要是靠太阳光子的能量(动量)的"哺育"才"活"下来的,地球目前还生机勃勃地"活着".地球的自转与公转及赤、黄交角的存在,不是先前人们所理解的只具有行星运动几何学上的意义,它在日一地之间能量(动量)相耦合转换机制中还起着更为关键的作用,它是整个地球能有效地、连续不断地获得太阳辐射能量(动量)使其能"活"下去而必须具有的最为简单的天然条件.(2)揭示了自然界任一恒星系内部恒星与行星或星际物质间的斥力作用普遍存在.众所周知,太阳是一颗质量较小的恒星,在银河星云系中类似太阳的发光恒星大约就有4000亿颗,在宇宙更是不计其数.这说明宇宙中的任一恒星系内恒星与它系内的行星及星际物质(除暗物质外)之间的能量(动量)耦合与交换主要是靠光子来实现的.光予是宇宙中既普遍存在又具有特殊性能的一种物质.光子不带电,其电荷、电偶极矩和磁矩皆为零,它是一种稳定的粒子,其寿命为无限大.宇宙中任一恒星辐射出的光子可以对外任何可见物体起作用.光子对受体的作用方式是碰撞,它不但把自身的能量传递给受体,还把自身的动量(以光压斥力的形式)传递给受体,其斥力方向与恒星与受体之间的引力方向恰恰相反,以阻止行星或星际物质在万有引力作用下向恒星内部凝聚,保持恒星系基本空间构架的相对稳定.由此推知,宇宙中物质之间的(光)斥力作用是普遍存在的,它与万有引力作用构成了相互依存的两个对立面,它们之闻的对立与统一构成了和谐一致的自然界.日一地间天然形成的能量(动量)相耦合的"轧制"式和"摇摆"式物理机制的发现与证实,为自然界星际(恒星与行星)尺度间的斥力作用普遍存在提供了有力的证据.这是自牛顿发现万有引力之后,首次对宇宙中星际间存在的"反引力"作用这一宏观自然现象的揭示. 相似文献
73.
74.
稻城圆环阵太阳射电望远镜(Daocheng Solar Radio Telescope, DSRT)作为子午工程二期太阳-行星际探测子系统的重要部分, 工作在150--450MHz频段, 可提供高空间、高时间分辨率的太阳爆发亮温图像. 针对DSRT天线的高精度指向测量以及对指向误差批量标定和校正的需求, 首先根据DSRT独有的三轴座架系统, 通过四元数旋转变换法建立了天线3参数编码器零点误差模型; 然后提出了基于射电源的漂移扫描法获得16个单元天线功率方向图, 并根据2维方向图确定波束中心的方法精确测量了DSRT天线指向误差; 最后用最小二乘法拟合得到模型参数, 并通过天线控制软件重新调整各个轴的零点, 后对调整结果进行验证. 结果表明指向校正方法可靠有效, 校正后16个天线的指向精度为0.5$^\circ$之内, 明显优于校正前3.5$^\circ$的指向误差, 满足误差小于DSRT天线最高工作频率下的1/10波束范围内的要求. 相似文献
75.
TNA–1500 radio telescope observations data of radio emission from local sources of different types have been examined. The established quantitative peculiarities of spectral and integral characteristics of fluctuations can be used for forecasting flare activity by means of pattern recognition technique. 相似文献
76.
77.
J. Kar 《Earth, Moon, and Planets》1996,73(2):187-192
Recently, the possibility of strong mass loss from an early sun has been proposed in connection with the lithium depletion problem along with early solar system problems. However, the time scale for this enhanced mass loss is uncertain. Using an empirical relation for the dependence of the Martian surface temperature on solar luminosity and surface pressure, we find that the mass loss time scale for a 1.1 M sun should be about 1 × 109 years or longer if Mars had liquid water on its surface 3.8 billion years ago. The minimum surface pressure on early Mars should be about 5 bars of CO2. 相似文献
78.
The probability distribution of the sea surface slope has been estimated using sun glitter images derived from the visible
wavelength radiometer on the Geostationary Meteorological Satellite (GMS) and surface vector winds observed by spaceborne
scatterometers. The brightness of the visible images is converted to the probability of wave surfaces which reflect the sunlight
toward GMS in grids of 0.25° × 0.25° (latitude × longitude). The slope and azimuth angle required for the reflection of the
sun's rays toward GMS are calculated for each grid from the geometry of GMS observation and location of the sun. The GMS images
are then collocated with surface wind data observed by three scatterometers. Using the collocated data set of about 30 million
points obtained in a period of 4 years from 1995 to 1999, the probability distribution function of the surface slope is estimated
as a function of wind speed and azimuth angle relative to the wind direction. The results are compared with those of Cox and
Munk (1954a). The surface slope estimated by the present method shows a narrower distribution and much less directivity relative
to the wind direction than that reported by Cox and Munk. It is expected that their data were obtained under conditions of
growing wind waves. In general, wind waves are not always developing, and the slope distribution might differ from the results
of Cox and Munk. Most of our data are obtained in the subtropical seas under clear-sky conditions. This difference in the
conditions may be the reason for the difference of slope distribution.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
79.
80.
I. CHARVÀTOVÀ 《Surveys in Geophysics》1997,18(2-3):131-146
The time series of solar and volcanic activities have been processed to show, mostly by means of statistical characteristics, the exceptional and recurring pattern of these phenomena in the intervals of the exceptional and recurring pattern of solar motion, i.e. in the intervals of the Sun's motion along the trefoils which reoccur in steps of 178.7 years. Nearly the same sets of five sunspot cycles have been found in the latest trefoil intervals (1730–1780 and 1910–1960), their length being constant and equal to 10 years (cycles No. 15–19). The steadily attenuated volcanic activity have been pointed out in the three latest trefoil intervals. The long-term maxima of surface air temperature occured in the central decades of the trefoil intervals. The results indicate a primary role of solar motion in a causal chain of ST-relations and a need of taking the Solar System as a whole into account to explain climatic changes. The solar motion can be computed in advance. Predictive assesments, so far in form of analogies, have been made: Because the solar motion in the next decades will be chaotic, lower and longer solar cycles (with irregular length), ocurrence of huge volcanic events and a decrease of global surface air temperature can be expected. 相似文献