Using 141 CME-interplanetary shock (CME-IPS) events and foF2 from eight ionosonde stations from January 2000 to September 2005, from the statistical results we find that there is a “same side?–?opposite side effect” in ionospheric negative storms, i.e., a large portion of ionospheric negative disturbances are induced by the same-side events (referring to the CMEs whose source located on the same side of the heliospheric current sheet (HCS) as the Earth), while only a small portion is associated with the opposite-side events (the CMEs source located on the opposite side of the HCS as the Earth); the ratio is 128 vs. 46, and it reaches 41 vs. 14 for the intense ionospheric negative storms. In addition, the ionospheric negative storms associated with the same-side events are often more intense. A comparison of the same-side event (4 April 2000) and the opposite-side event (2 April 2001) shows that the intensity of the ionospheric negative storm caused by the same-side event is higher than that by the opposite-side event, although their initial conditions are quite similar. Our preliminary results show that the HCS has an “impeding” effect to CME-IPS, which results in a shortage of energy injection in the auroral zone and restraining the development of ionospheric negative perturbations. 相似文献
Taking transfer orbits of a collinear libration point probe, a lunar probe and an interplanetary probe as examples, some applications of stable and unstable invariant manifolds of the restricted three-body problem are discussed. Research shows that transfer energy is not necessarily conserved when invariant manifolds are used. For the cases in which the transfer energy is conserved, the cost is a much longer transfer time. 相似文献
Relative dynamics between the chief satellite and the deputy ones in formation flying is crucial to maintaining the formation. A good choice of the formation usually requires a lower control frequency or less control energy. For formation flying missions in highly elliptic orbits, the well-known C-W equation is not accurate enough. Instead, Lawden’s equation is often used. First, the solution to Lawden’s equation with a very simple form is deduced. Then the J2 perturbation is added. It is found that Lawden’s solution is not necessarily valid when the J2 perturbation is considered. Completely discarding Lawden’s solution and borrowing the idea of mean orbit elements, two rules to initialize the formation are proposed. The deviation speed is greatly reduced. Different from previous studies on the J2 perturbation, except for the relatively simple expression for the semi-major axis, the tedious formulae of the long period terms and the short period terms of other orbital elements are not used. In addition, the deviation speed is further reduced by compensation of the nonlinear effects. Finally, a loose control strategy of the formation is proposed. To test the robustness of this strategy, a third body perturbation is added in numerical simulations. 相似文献
Based on the partial differential equation governing the effect of atmospheric pressure on water level of confined well, deriving
the boundary condition and considering the seepage water between well and aquifer, the author obtained the analytical solution
of water level change in time domain under the action of an atmospheric pressure history with the Laplace transform method.
This solution is composed of two terms:stable and retarded terms. The stable term is the multiplication of barometric efficiency
and simultaneous atmospheric pressure, and it implies the value of water level after infinite time when the atmospheric pressure
is a constant from the time in question. The retarded term is the transient process due to the time lag of water exchange
between well and aquifer. From the solution, it is obtained that the interference of atmospheric pressure on water level is
the integral superimposition of the contribution of all atmospheric pressure changes before the time in question. So that,
we further found out the response function of pulsive atmospheric pressure history. Calculation shows: (1) The pulsive response
function starts from zero and tends to a steady value, which is proportional to the barometric efficiency, when the time tends
to infinity; (2) The retarded time depends on the mechanical property of aquifer and the radius of well. The larger the seepage
coefficient, the smaller the radius of well and the thicker the aquifer, then the shorter the retarded time gets. This solution
can be used as the theoretical basis for further analysis of the atmospheric effect and practical correcting method in the
future. 相似文献
Dated isotopic ages for 15 alkaline intrusives in the Yanliao-Yinshan area, ranging from 268 to 190 Ma, ten of which are from
250 to 208 Ma, indicate that most of them were formed in the Triassic Epoch. All the ENd(t) ratios from - 17.19 to -3.21 averaging -7.09, the ESr(t) ratios fmm 11.7 to71.5 averaging 36.63, and the Isr(t) ratios from 0.705 0 to 0.709 3 averaging 0.706 8, show their characteristics of enrichment. On the ENd(t) virus ESr(t) correlation diagram, the samples from these intmsives were plotted within the enriched mantle trend lines and just outside,
demonstrating their close connection to materials from the enriched mantle reservoir, taking into account the same Pb isotopic
composition as that of the mantle. 相似文献