共查询到20条相似文献，搜索用时 343 毫秒
1.
Tlatov(2007)研究认为,太阳活动和太阳磁场变化的22年周期,可能与太阳自转速度的变化有关.可是关于太阳自转速度为什么呈现出22年的变化周期,尚未见到有说服力的解释.本文通过对行星会合指数、行星系质心绕太阳系质心的运动、太阳绕太阳系质心运动以及太阳自转角动量变化的分析,发现行星系统的会合与相互背离,导致了太阳系质心与太阳质心的背离和靠近,从而引发太阳绕太阳系质心旋转角动量与太阳自转角动量的分离与叠加.由此认为,这两种角动量间的转换是太阳自转角速度呈现22年周期性变化的原因.太阳自转速度极小值对应于行星会合指数极大值;而太阳自转速度极大值对应行星会合指数极小值.其中平均11年左右为太阳自转加速期,另外11年则为太阳自转减速期.这一发现,可能为太阳活动与太阳磁场变化22年周期的成因机制的解释提供一个新的线索. 相似文献
2.
基于之前创建的行星会合指数运动学方程,发现太阳质心具有平均准22年向太阳系质心靠近(有时近似重合)的轨道运动周期.在整个太阳系角动量守恒的前提下,推出太阳自转角动量和太阳绕转角动量之和守恒.二者角动量转换造成太阳自转角动量变化和太阳绕转角动量变化具有互为反向的准22年变化规律.太阳自转角速度变化(dω/dt)图像与太阳黑子磁性指数图像具有一致对应关系,这种对应关系可以从物理机制上对太阳活动周相位变化和太阳活动强弱变化进行解释,这为预测太阳活动提供了一种有效方法.本研究为太阳活动替代性指标指代的双世纪周期和2403年哈尔斯塔(Hallstatt)周期规律找到了理论根据. 相似文献
3.
4.
运用刘复刚和王建(2013a)创建的行星会合指数K指代太阳绕太阳系质心运动时,一般情况,行星系质心是和木星位于太阳一侧.当其它3颗大质量行星(或其它7颗行星)和木星分居在太阳两侧,并且这4颗大质量行星(或8颗行星)与太阳近似排成直列的状态时,行星系质心则处在木星相反一侧,这时造成了太阳绕太阳系质心顺时针旋转的假象.本文对这一认识进行了澄清,并通过图示的方法定性地解释了太阳在一个行星系统平均轨道会合周期内角速度的变化特征.相当太阳系质心(C)从太阳本体旋出直到C再次旋进太阳本体这一时段,太阳轨道运动是处在减速期;而当C旋进直到旋出太阳本体这一时段,太阳轨道运动处在加速期.并将其运动特征与太阳轨道角动量的变率进行了对比,这将为揭示太阳活动规律的动力学机制提供了一种可能途径和新的思想方法. 相似文献
5.
日心说是一种思想革命,它将太阳系坐标原点从地心移到日心.但这种革命并不彻底,因为日心又在绕太阳系质心运动.其实,太阳系的其他天体都是绕太阳系质心运动.类比行星轨道运动特征,本文将太阳轨道运动概括为三个基本定律:第1定律,太阳和行星系质心相对太阳系质心同步运动,其运行轨迹近似为绕太阳系质心旋进和旋出的连续变化的叶形曲线.第2定律,太阳轨道运动具有平均准22.13年方向周期.第3定律,太阳绕太阳系质心运动,当其边缘到达太阳系质心时,太阳轨道运动角速度处于减速状态;当太阳后部边缘即将离开太阳系质心时,太阳轨道运动角速度处于加速状态. 相似文献
6.
基于太阳系质心坐标系论证了太阳和行星系质心同步绕太阳系质心运动的命题.对K指数的研究发现,太阳系结构演变可导致选定的太阳质心坐标系的性质具有周期性变化的特征.太阳系结构变化可以从K指数的量值上予以区分.当行星系统处在K=Kmax和K=Kmin分布状态时,所揭示的正是整个太阳系结构演变的两种性质相反的极端状态.太阳轨道运动的复杂性主要是指太阳轨道运动具有向太阳自转运动转变的周期性变化特征.K指数除了具有指代太阳轨道运动极半径的变化特征之外,还近似具有与木星同步绕转的方向周期.理论分析获得:太阳轨道运动角动量的变化可导致太阳自转角动量和行星系统轨道角动量的变化,这对进一步探讨地球轨道运动扣自转运动的变化机制具有重要的参考价值. 相似文献
7.
地球自转角速度的季节性和年变化的成因已达成基本共识,但更长时间尺度的周期性变化成因尚无定论,它们或归因于太阳活动、日月引潮力、地壳反弹、大气圈波动或行星摄动的影响等.直至目前,地球自转变化的规律和机制还没有完全弄清楚.研究发现:根据行星会合指数(K)标定太阳轨道运动特征的方法是可行的.通过对行星会合指数(K)的FFT检测发现太阳轨道运动周期与前人研究的地球自转日长(LOD)变化周期具有极强的相关性.太阳轨道运动在受到行星系统力矩作用的同时,致使近日行星轨道运动受到太阳引力作用的波动影响而产生扰动.受太阳巨大引力作用的牵制,导致地球轨道角动量和太阳轨道角动量的变化具有正相关关系.根据地球轨道角动量和自转角动量之和守恒,进而推断地球自转角速度的变化对太阳轨道运动特征的响应,这在思想方法上是一种突破. 相似文献
8.
Tlatov(2007)研究表明太阳自转具有准22年振荡周期,并认为是太阳系自引力造成的.根据刘复刚和王建(2013)创建的行星会合指数KP(令KP=K是为了和其他指数的表现形式相统一)和获得的修正系数发现:太阳轨道运动具有平均准22.1826年运动周期,认为太阳轨道角动量和太阳自转角动量的周期性叠加致使太阳自转角速度具有准22.20年周期性变化.基于行星会合指数KP同时标定了太阳质心S相对于一个无法观测到的太阳系质心C位置关系的变化规律,进而通过太阳轨道运动指数KS、速率指数Kv、加速度指数Kα对太阳轨道运动特征进行了系统描述,这使得从行星系统之视角分析、揭示太阳运动和太阳活动成为可能,并对太阳自转运动的准11年和22年周期振荡受控于太阳轨道运动的调控进行了分析,这从探索途径和思想方法上是一种突破.依K_P表达式给出的太阳轨道运动轨迹与Jose(1965)、杨志根等(1988)、Scafetta(2014)、Mc Cracken等(2014)给出的图像不但形态特征相同而且图像的相位也完全一致.行星会合指数KP更重要的作用是标定了行星系统质心距离太阳位置关系的变化.本文从行星系统质心出发,根据行星系统质心P与太阳质心S绕太阳系质心C同步运动这一基本原理来进一步揭示太阳轨道运动规律.由于研究问题的出发点和视角不同,按这一途径可根据8大行星公开的天文数据分析太阳轨道运动规律.这种方法不但把纷繁复杂的行星系统统一起来,呈现出行星系统固有的整体运动规律,而且在整个太阳系中建立了与太阳处于相同子系统地位的行星系统质心.在此基础上,通过行星系统质心P与太阳S间位置关系变化,系统分析了太阳S和太阳系质心C的统一与分野规律.其重要意义是通过行星系质心运动规律发现它与太阳轨道运动特征间的本质联系,这使得从行星系统质心的运动特征对太阳运动与太阳活动关系的探寻成为可能. 相似文献
9.
《地球物理学进展》2015,(1)
基于创建的行星会合指数(K)运动学方程,得到太阳绕太阳系质心绕转的真正周期为准22.1826年.在整个太阳系角动量守恒前提下,根据K指数所指代的太阳绕太阳系质心运动轨迹推出:太阳绕转和太阳自转各自角动量虽不守恒,但二者角动量之和守恒.当行星系统处于最大相背离状态,太阳自转角动量增加,太阳自转受到逆时针方向旋转切向力的作用;当行星系统处于最大会合状态,太阳自转角动量减小,太阳自转受到顺时针方向旋转切向力的作用.行星系统远日4颗大质量行星和近日4颗小质量行星对太阳引力的合力沿太阳绕转轨道半径垂直方向的分力,具有准22年周期变化,而且该力的方向就是沿太阳旋转运动轨迹的切向方向.该分力11年与太阳自转方向同向,另11年与太阳自转方向反向,且分别对应太阳自转角动量11年增大和11年减小的变化.这为研究太阳22年磁周期动力学机制探寻到一种新的思想方法. 相似文献
10.
太阳轨道运动长周期性韵律的成因 总被引：2，自引：0，他引：2
太阳轨道运动具有双世纪(约200年)和哈尔斯塔(约2500年)长周期规律.这两个周期可以通过行星会合指数方程获得.根据图像获知,这两个太阳轨道运动周期都是由太阳最基本的22年轨道运动周期集合而成.太阳轨道运动的22年周期和太阳活动的22年磁周期是一一对应的.本文通过行星会合指数图像与太阳轨道运动角动量变率(Jose,1965)图像和树木年轮-珊瑚综合指标所指代的太阳活动图像(Charvátová,2000)的比对,以及对太阳轨道运动角动量与太阳自转角动量呈负相关关系的分析,认为太阳的自转运动规律决定着太阳自身的活动规律.从而得出,行星会合指数不但可以指代太阳的轨道运动规律,同时也可指代太阳的活动规律. 相似文献
11.
12.
In this paper, we examine the nature of the main source of the sporadic solar wind on the Sun: coronal mass ejections (CMEs).
Analysis of data from Mark 3 and Mark 4, the Digital Prominence Monitor (MLSO), and STEREO (EUVI) spacecraft has revealed
the existence of two types of CMEs: gradual and impulse. They differ in the place, velocity, and angular size at the instant
of their emergence. The source of gradual CMEs is located in the corona, at a distance of 1.1 R
0 < R ≤ 1.7 R
0 from the center of the Sun. They start moving from a state of rest, having an angular size ≈15–65° (in the heliographic coordinate
system). Impulse CMEs are probably formed under the Sun’s photosphere. This may be due to the supersonic emergence of magnetic
tubes (ropes) from the convective zone. The possibility of this phenomenon has been demonstrated earlier in theory. The radial
velocity of such tubes at the photospheric level may be 100 km/s or higher; the minimum angular size is ∼1°. 相似文献
13.
《Journal of Atmospheric and Solar》2003,65(4):469-482
Solar radiation (both total and in various wavelengths) varies at different time scales—from seconds to decades or centuries—as a consequence of solar activity. The energy received from the Sun is one of the natural driving forces of the Earth's atmosphere and since this energy is not constant, it has been argued that there must be some non-zero climate response to it. This response must be fully specified in order to improve our understanding of the climate system and the impact of anthropogenic activities on it. However, despite all the efforts, if and how subtle variations of solar radiation affect climate and weather still remains an unsolved puzzle. One key element that is very often taken as evidence of a response, is the similarity of periodicities between several solar activity indices and different meteorological parameters. The literature contains a long history of positive or negative correlations between weather and climate parameters like temperature, rainfall, droughts, etc. and solar activity cycles like the 27-day cycle, the prominent 11-year sunspot cycle, the 22-year Hale cycle and the Gleissberg cycle of 80–90 years. A review of these different cycles is provided as well as some of the correlative analyses between them and several stratospheric parameters (like stratospheric geopotential heights, temperature and ozone concentration) and tropospheric parameters (like temperature, rainfall, water level in lakes and river flooding, clouds) that point to a relationship of some kind. However, the suspicion on these relationships will remain as long as an indisputable physical mechanism, which might act to produce these correlations, is not available. 相似文献
14.
D. V. Erofeev 《Geomagnetism and Aeronomy》2012,52(8):1097-1106
The behavior of correlation tensors of fluctuations in the solar wind magnetic field and velocity is studied during different phases of a solar cycle on the basis of a 45-year measurement series of solar wind parameters. It is found that the orientation of fluctuations in the magnetic field and velocity is approximately axisymmetric relative to the direction of a local magnetic field during high solar activity. This symmetry is violated significantly during periods of low solar activity, and deviations from the symmetry are regular and oppositely directed during minima of even and odd 11-year cycles, which is probably connected with variations in the orientation of the Sun??s magnetic field. The dependence of the power of fluctuations on the local magnetic field direction reveals significant deviations from local symmetry during all phases of a solar cycle, especially for velocity fluctuations. 相似文献
15.
Hiroko Miyahara Kentaro Nagaya Kimiaki Masuda Yasushi Muraki Hiroyuki Kitagawa Toshio Nakamura 《Quaternary Geochronology》2008,3(3):208-212
In this paper, we review the variation of the 11-year solar cycle since the 15th century revealed by the measurement of radiocarbon content in single-year tree-rings of Japanese cedar trees. Measurements of radiocarbon content in absolutely dated tree-rings provide a calibration curve for accurate dating of archaeological matters, but at the same time, enable us to examine the variations of solar magnetic activity in the pre-historical period. The Sun holds several long-term quasi-cyclic variations in addition to the fundamental 11-year sunspot activity cycle and the 22-year polarity reversal cycle, and it is speculated that the property of the 11-year and the 22-year solar cycle varies in association with such long-term quasi-cycles. It is essential to reveal the details of solar variations around the transition time of solar dynamo for illuminating the mechanisms of the long-term solar variations. We therefore have investigated the property of the 11-year and 22-year cycles around the two grand solar minima; the Maunder Minimum (1645–1715 AD) and the Spoerer Minimum (1415–1534 AD), the periods of prolonged sunspot minima. As a result, slight stretching of the “11-year” and the “22-year” solar cycles was found during these two grand solar activity minima; continuously during the Maunder Minimum and only intermittently during the Spoerer Minimum. On the contrary, normal or slightly shortened 11-year cycles were detected during the interval period of these two minima. It suggests the inverse correlation between the solar cycle length and solar magnetic activity level, and also the change of meridional flow during the grand solar activity minima. Further measurements for the beginning of the grand solar minima will provide a clue to the occurrence of such prolonged sunspot disappearance. We also discuss the effect of solar variations to radiocarbon dating. 相似文献
16.
The effect of the 11-year solar cycle on the response of planetary wavenumbers 1 and 2 at 10 and 30 hPa in winter to solar activity oscillations on the time scale of the Sun's rotation (27.2 day) is discussed in terms of statistical spectral analysis. The three oscillations studied are the 27.2 d (period of the Sun's rotation), 25.3 d (periodicity caused by modulation of the 27.2 d stratospheric response by annual atmospheric variation), and 54.4 d (doubled period of the solar rotation). A significant effect of the 11-year solar cycle is found for the 54.4 d periodicity in planetary wavenumber 1, and for the 27.2 and 25.3 d periodicities in planetary wavenumber 2. The effect of the 11-year solar cycle is expressed in the evident differences between the amplitudes of responses of planetary waves at maximum and minimum of the solar cycle: the amplitudes are much larger at high than at low solar activity. The 11-year modulation of planetary wave activity is most pronounced at mid-latitudes, mainly at 40–60°N, where the observed variability of planetary waves is large. The results obtained are in good agreement with results of the recent modeling study by Shindell et al. (Science 284 (1999) 305). 相似文献
17.
《Journal of Atmospheric and Solar》1999,61(1-2):15-24
Total solar irradiance has been monitored from space for nearly two decades. These space-borne observations have established conclusively that total solar irradiance changes over a wide range of periodicities—from minutes to the 11-year solar cycle. Since the total energy flux of the Sun is the principal driver for all Earths atmospheric phenomena, the accurate knowledge of the solar radiation received by the Earth and its variations is an extremely important issue. In this paper we review the long-term variations of total solar irradiance during solar cycles 21 and 22. We conclude that, within the current accuracy and precision of the measurements, the minimum level of total solar irradiance is about the same for both solar cycles 21 and 22. 相似文献
18.
Time variations in strong and weak photospheric magnetic fields have been considered based on synoptic maps from the Kitt Peak observatory for 1976?C2003. The magnetic fields of positive and negative polarities of the Northern and Southern hemispheres of the Sun and their imbalance were studied. It has been indicated that different groups of magnetic fields vary with 11-or 22-year periods depending on their values. The difference between positive and negative fluxes for each hemisphere always varies with a 22-year period. For weak fields, the 22-year cycle is related to the manifestation of the global solar magnetic field. For strong fields, the imbalance between positive and negative fluxes reflects the predominant role of leading sunspots in a given solar hemisphere. It has been detected that the total magnetic flux over the entire solar disk varies with an 11-year period in antiphase with the solar activity cycle for the weakest magnetic fields (0?C5 G). 相似文献
19.
Yu. A. Nagovitsyn 《Geomagnetism and Aeronomy》2014,54(6):673-679
Prolonged variations in the duration of the Schwabe-Wolf (～11 years) and Suess (～200 years) cycles have been analyzed using different experimental data. It was shown that the duration of the Schwabe-Wolf cycle on a 2000-year time scale varied monotonically (on average, increasing) and cyclically (with a period of several hundred years); periods of 10.4, 11.0, and 11.4 years predominate on the occurrence frequency histogram. The Suess cycle duration was 200–290 years during the Holocene and tended to increase in the past. This was accompanied by cyclic variations with a period of 2300–2500 years corresponding to the Hallstatt cycle. Arguments for the assumption that the Suess cycle duration decreased by a factor of more than 1.5 over the past half billion years are presented. This may indicate that the solar rotation characteristics and convection zone parameters varied on long time scales during the Sun’s evolution on the main sequence. 相似文献
20.
Summary It is proposed that gravitational torques can furnish a mechanism for the radial outward transport of angular momentum in the solar nebula. For this effect to be present the disc of the nebula must have a spiral structure with trailing arms. A mathematical model is constructed with the main object of seeing whether purely advective inward eddy transports of angular momentum could offset the gravitational torques. It is found that for a protosun much more massive than the disc the eddy transport is small, allowing the gravitational effects of predominate. In such a case convergence of angular momentum is to be expected at the outer edge of the disc. The possibility exists that matter could be shed to large distances perhaps giving rise to the cloud of comets surrounding the solar system as proposed byJ. H. Oort. 相似文献