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31.
M.O. Riazantseva G.N. Zastenker J.D. Richardson 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2005,35(12):2147-2151
We investigate properties of large (>20%) and sharp (<10 min) solar wind ion flux changes using INTERBALL-1 and WIND plasma and magnetic field measurements from 1996 to 1999. These ion flux changes are the boundaries of small-scale and middle-scale solar wind structures. We describe the behavior of the solar wind velocity, temperature and interplanetary magnetic field (IMF) during these sudden flux changes. Many of the largest ion flux changes occur during periods when the solar wind velocity is nearly constant, so these are mainly plasma density changes. The IMF magnitude and direction changes at these events can be either large or small. For about 55% of the ion flux changes, the sum of the thermal and magnetic pressure are in balance across the boundary. In many of the other cases, the thermal pressure change is significantly more than the magnetic pressure change. We also attempted to classify the types of discontinuities observed. 相似文献
32.
利用武汉、广州、泉州和琼中等4个低纬地磁站连续多年的地磁资料,计算了各月5个磁静日Z分量日均值与中午1100---1300时段平均值之差(Dz),对每年12个Dz采用多元回归分析方法,得到各年的半年变化幅度和相位.结果表明:4个站的Dz每年都有半年变化现象;半年变化幅度与太阳活动有关,一般来说,太阳活动高年Dz半年变化幅度明显大于太阳活动低年;太阳活动本身的半年变化,对Dz半年变化幅度有显著的调制作用;Dz半年变化的相位在3—4月(或9—10月),即极大值出现在分季;低纬地区地磁Z分量存在显著的半年变化,能够反映赤道电急流也有明显的半年变化,这再一次证明,赤道电急流幅度的半年变化,通过“喷泉效应”使得电离层,f0F2产生半年变化,其是产生,f0F2半年变化的一个主要因素. 相似文献
33.
神舟2号大气密度探测器的探测结果(Ⅰ)日照和阴影区域热层大气密度变化 总被引:1,自引:2,他引:1
选用了神舟2号(SZ-2)大气密度探测器在2001年2—4月间的探测数据,进行日照和阴影区域热层大气密度变化的探讨.结果表明:在高度410km附近,日照和阴影区域大气密度变幅为2—3倍,变幅的大小与地磁活动程度呈负相关关系.日照面大气密度峰区位于星下点地方时1400—1500LT的纬度处,峰值大小与太阳活动程度呈正相关关系.阴影面大气密度谷区位于星下点地方时0400-0500的纬度处,同时在±10°纬度区域中还出现了阴影面峰区. 相似文献
34.
太阳质量损失对行星轨道的影响 总被引:5,自引:0,他引:5
本文利用Gylden-Meshcherskii方程和Eddington-Jeans定律,讨论太阳质量损失对行星轨道的影响,结果表明由于太阳质量损失会产生轨道半长径α的一阶周期项和二阶混合项;近日点角距ω的一阶周期项、二阶长期项和混合项,行星轨道半长径的长期变化会影响太阳系的稳定性。 相似文献
35.
S.V. Chalov 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2005,35(12):2106-2114
It may not be doubted anymore that anomalous cosmic rays (ACRs) are produced in the heliosphere from interplanetary pick-up ions through their acceleration at the solar wind termination shock. However, there is no general agreement in the community of heliospheric researchers concerning the mechanism of injection of the pick-up ions into the shock acceleration. We discuss here three possible ways for pick-up ions to be involved into the acceleration process at the termination shock: (1) preacceleration of pick-up ions in the whole region from the Sun up to the termination shock by solar wind turbulences and interplanetary shock waves, (2) local preacceleration of pick-up ions in a vicinity of the termination shock by shock surfing, and (3) formation of high-velocity tails in pick-up ion spectra consisting of secondary pick-up ions which are produced in the supersonic solar wind due to ionization of energetic neutral atoms entering from the inner heliosheath. 相似文献
36.
Noise in wireless systems from solar radio bursts 总被引:1,自引:0,他引:1
L.J. Lanzerotti D.E. Gary G.M. Nita D.J. Thomson C.G. Maclennan 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2005,36(12):2253-2257
Solar radio bursts were first discovered as result of their interference in early defensive radar systems during the Second World War (1942). Such bursts can still affect radar systems, as well as new wireless technologies. We have investigated a forty-year record of solar radio burst data (1960–1999) as well as several individual radio events in the 23rd solar cycle. This paper reviews the results of a portion of this research. Statistically, for frequencies f 1 GHz (near current wireless bands), there can be a burst with amplitudes >103 solar flux units (SFU; 1 SFU = 10−22 W/m2) every few days during solar maximum conditions, and such burst levels can produce problems in contemporary wireless systems. 相似文献
37.
利用MF雷达对耀斑期间电离层D区电子密度的观测研究 总被引:1,自引:0,他引:1
利用MF雷达观测资料对X级别耀斑爆发期间在66-80km高度之间的电子密度进行了研究,观测到了耀斑爆发期间电子密度的突然增加,在较低高度上的电子密度的时间变化趋势与耀斑的软X射线辐射通量相关.电子密度的变化强度依赖于具体的耀斑参数,有些耀斑引起的电子密度增加高达400cm^-3,有些仅为100cm^-3左右.但耀斑期间在这一高度区间增加的总电子含量增量仅占耀斑辐射引起的整个电离层总电子含量增量的千分之一左右.最后,利用恢复阶段电子密度的时间变化过程估算了1997年11月4日耀斑期间部分高度上的有效复合系数. 相似文献
38.
David J. Helfand 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1984,3(10-12)
“With all reserve, we advance the view that a supernova represents the transition of an ordinary star into a neutron star.”This conclusion, reached just 50 years ago in a classic paper by Walter Baade and Fritz Zwicky (1934), was published three decades before the first direct observational evidence for the existence of neutron stars was uncovered. It still informs the standard picture of neutron star production in the Galaxy. We examine herein some recent evidence bearing on this question which has been derived from
Observatory X-ray observations of supernova remnants and radio pulsars. In particular, the discovery that X-ray synchrotron nebulae are found surrounding most young ( 106 yr) pulsars observed to date is discussed. We explore the implications of the lack of such nebulae in the majority of supernova remnants (SNR) for the properties and frequency of neutron star formation in supernova events. 相似文献
39.
Luciano Nobili Roberto Turolla Silvia Zane 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
The huge potential drop between the footpoints of the closed field lines in the twisted magnetospheres of magnetars may accelerate electrons up to very high energies, γ ? 106. On the other hand, the comparison between the observed spectra of magnetars and spectra obtained by accurate theoretical models seems to favor of a picture in which the magnetosphere is filled by “slow” electrons (v ? 0.8c), rather than by ultra-relativistic particles. 相似文献
40.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2020,65(3):1070-1082
Solar sail halo orbits designed in the Sun-Earth circular restricted three-body problem (CR3BP) provide inefficient reference orbits for station-keeping since the disturbance due to the eccentricity of the Earth’s orbit has to be compensated for. This paper presents a strategy to compute families of halo orbits around the collinear artificial equilibrium points in the Sun-Earth elliptic restricted three-body problem (ER3BP) for a solar sail with reflectivity control devices (RCDs). In this non-autonomous model, periodic halo orbits only exist when their periods are equal to integer multiples of one year. Here multi-revolution halo orbits with periods equal to integer multiples of one year are constructed in the CR3BP and then used as seeds to numerically continue the halo orbits in the ER3BP. The linear stability of the orbits is analyzed which shows that the in-plane motion is unstable while the out-of-plane motion is neutrally stable and a bifurcation is identified. Finally, station-keeping is performed which shows that a reference orbit designed in the ER3BP is significantly more efficient than that designed in the CR3BP, while the addition of RCDs improve station-keeping performance and robustness to uncertainty in the sail lightness number. 相似文献