2003 Vol. 23, No. 1

Display Method:
SINGLE FLUID 2D MAGNETOHYDRODYNAMIC SIMULATION OF SOLAR WIND STRUCTURE
XUE Jintao, WANG Jingfang, QIAN Xin, DENG Xiaohua
2003, 23(1): 1-6. doi: 10.11728/cjss2003.01.20030101
Abstract(2226) PDF 567KB(996)
Abstract:
In this paper, single fluid 2D MagnetoHydroDynamic (MHD) equations with a momentum addition is used to simulate the solar wind structure on the meridian plane. With the comparison between the simulation results and observations by Ulysses, it is found that the form and deposited location of the momentum addition have great effect on solar wind velocity and density far away from the Sun. An appropriate momentum addition is adopted to calculate the solar wind velocity and density and obtained similar results with the Ulysses observations. It is found that the acceleration process simulated near the Sun agrees well with the data observed. The momentum addition should be deposited on 3.5-10 solar radii as a conclusion of the paper, and the result provides some clues for the problem of the solar wind acceleration mechanism.
A STUDY ON THE Bs EVENTS IN INTERPLANETARY SPACE AND THE ASSOCIATED CMEs IN 2000
YE Pinzhong, WANG Yuming
2003, 23(1): 7-17. doi: 10.11728/cjss2003.01.20030102
Abstract(2520) PDF 848KB(1021)
Abstract:
According to the observations from WIND spacecraft, the events of southward magnetic field (Bs events) occurred in 2000 are studied. Among these 12 events, there were 11 events associated with the coronal mass ejections (CMEs). Using the data from WIND, SOHO/LASCO, and SOHO/EIT, we identified the associated CMEs, which were all halo type. All of these CMEs were moving outward with fast speeds and caused shocks ahead. The initial sites of these CMEs on the solar disc were in an asymmetrical region. By studing 5 strong Bs events (Bs ≥ 20 nT), it is found that the energy of the associated CMEs was high, or the associated CMEs just directed to the Earth, or there were several CMEs, which caused one same Bs event combinationally. In addition, during the solar maximum, the relationship between the intense disturbances in interplanetary space and the high-speed streams seem to be weak.
THE INFLUENCE OF ION’S NONLINEAR POLARIZATION DRIFT ON THE CHARACTER OF SOLITARY KINETIC ALFVÉN WAVE
DUAN Suping, LI Zhongyuan
2003, 23(1): 18-24. doi: 10.11728/cjss2003.01.20030103
Abstract(2578) PDF 598KB(951)
Abstract:
Considering the influence of ion's nonlinear polarization drift on Solitary Kinetic Alfvér Wave (SKAW), the character of the low-frequency dip SKAW in the magnetic plasma is investigated with the two-fluid mode. The derived results indicate that two kinds of dip SKAW both exist in a wide range in magnetosphere (for the pressure parameter β-10-6-0.1, where β is the ratio of thermal pressure to magnetic pressure, i.e. β = 2μ0 nT/B02). They propagate at Sub- Alfvéric speed or Super-Alfvéric speed. And ion's nonlinear polarization drift has great effect on the SKAW when the value of β is smaller (β-10-6-10-4). It can not be neglected. But it has weak effect on the SKAW when the value of β is bigger (β - 0.1). Because of the SKAW having the parallel electric field, the solitary wave is important for the acceleration and energy transmission of charged particles in magnetic plasma. And the SKAW is also put effects on the transverse ion transverse acceleration. The SKAW makes a novel kind of mechanism of energy transmission possible.
QUASI-COLLISIONLESS MAGNETIC RECONNECTION EVENTS IN THE NEAR-EARTH MAGNETOTAIL
ZHOU Guocheng, CAI Chunlin, CAO Jinbin, WANG Deju, HenriReme, AndreBalogh
2003, 23(1): 25-33. doi: 10.11728/cjss2003.01.20030104
Abstract(2367) PDF 865KB(743)
Abstract:
Hot ion (- 5 eV/e-32 keV/e) and magnetic field data observed by Cluster Ⅱ-C1 CIS/HIS and FGM during the magnetotail plasma sheet crossing on September 15, 2001 are analyzed in this paper. In the interval of 0340-0440 UT, fast tailward ion flows (VXGSM < 0) were observed, which were associated with the enhancements of southward and dusk-downward magnetic fields (BZGSM < 0 and BYGSM < 0 or > 0). It can be inferred from these observations that magnetic reconnection events took place at XGSE > -18.6 Re within the plasma sheet in the interval of 0340-0440 UT on September 15, 2001. The characteristics for these events are consistent with the physical pictures of theory for a quasi-collisionless magnetic reconnection. Hence these events should be called as quasi-collisionless magnetic reconnection events.
THE ABNORMAL FLUCTUATIONS OF GPSP SEUDO-RANGE MEASUREMENTS AFTER LOCAL SUNSET
CHEN Zhiyu, ZHANG Donghe, XIAO Zuo
2003, 23(1): 34-41. doi: 10.11728/cjss2003.01.20030105
Abstract(2853) PDF 749KB(965)
Abstract:
Using GPS signals to deduce the ionospheric TEC as a tool to study the ionospheric physical processes has been widely conducted. For a duel frequency GPS receiver, both pseudo-range and phase measurements are used. Phase measurement is not sensitive to so-called multi-path effect so it is less affected by scattered or reflected signals and is more useful in determining the exact TEC value, including the signals' scintillation due to the fast fluctuations of electron density. In this paper, an observational phenomenon is introduced to show that the pseudo-range fluctuates asymmetrically day and night. During the nighttime, especially, one to three hours after the local sunset, fluctuations of pseudo-range values often appear and last for several hours. The magnitudes of these fluctuations are much larger than that observed at daytime. Some examples are given and their observational features are analyzed. Both examinations of the environments around the receiver and the asymmetrical features of the phenomenon itself show that these fluctuations can not be produced by any ground objects, but instead, may be due to some ionospheric structures. By comparing with the theoretical and observational characteristics of ionospheric Spread-F at mid- and low latitudes, particularly with its occurring time after local sunset, it is suggested that the nighttime fluctuations of GPS pseudo-range measurements is a kind of multi-path effects, which is produced due to the scattering of GPS signals by large scaled ionospheric structures such as Spread-F. Thus, GPS may provide a way to study the ionospheric irregularities.
DISCOVERY OF WATER ICE ON THE MOON SURFACE AND ITS SIGNIFICANCE
XU Lin, LIU Jianzhong, ZOU Yongliao, LI Chunlai
2003, 23(1): 42-49. doi: 10.11728/cjss2003.01.20030106
Abstract(2719) PDF 765KB(1078)
Abstract:
This paper presents a review of the discovery of water ice on the Moon surface, the surveying techniques, the occurring forms, distribution and amount of water resources, and the migration of water on the Moon surface and its prospects in utilization. The surveying data available have shown that the water resources on the Moon are distributed mainly in the permanently shadowed areas of both lunar poles and water reserves amount approximately to 6.6× 109t. The dominant distribution of Moon surface water ice in the permanently shadowed areas of both lunar poles is attributed to the fact that water on the Moon surface may migrate gradually by way of elastic jumping to the temperature-low areas. This study holds that whether there exists water on the Moon would exert no influence on the construction of any moon base by mankind. It is simple and economic to acquire water by making use of ilmenite reactions in lunar basalts. Depends on new explorating data, if we produce 1t water we need use ilmenite 8.5m3, but we should consume regiolith 80m3.
PRIMARY RESEARCH ON PREDICTION METHOD OF 10.7cm SOLAR RADIO FLUX
MIAO Juan, LIU Siqing, XUE Bingsen, GONG Jiancun, WANG Jialong
2003, 23(1): 50-54. doi: 10.11728/cjss2003.01.20030107
Abstract(2831) PDF 433KB(1104)
Abstract:
In this paper, "Similar Cycle" method is introduced and smoothed monthly mean F10.7 flux of cycle 23 is predicted in two approaches and then the prediction is tested. In the first one smoothed monthly mean sunspot numbers of cycle 23 is obtained by "Similar Cycle" method and then smoothed monthly mean F10.7 flux is predicted according to statistical relationship between sunspot numbers and F10.7 flux. In the second approach the "Similar Cycle" method is directly applied to predict smoothed monthly mean F10.7 flux of cycle 23 by using historical data of past solar cycles. From the prediction, three results are obtained: 1) Both of these two prediction results are close to observations, both having double. 2) The second prediction is closer to the observation than the first one, which shows that F10.7 flux has similar varing trend with sunspot numbers, but still has its own local varing characters. This can be proved by the second peak of observed F10.7 flux in cycle 23. 3) Using "Similar Cycle" method, the "Shape" of F10.7 flux in a solar cycle can be described well, which is difficult to get by other methods.
MICRO-SATELLITE ATTITUDE DETERMINATION USING GPS CARRIER PHASES
HE Xiufeng, LIU Jianye
2003, 23(1): 55-59. doi: 10.11728/cjss2003.01.20030108
Abstract(2254) PDF 329KB(959)
Abstract:
The GPS carrier phase measurements are used to determine the attitude of a vehicle. A technique based on the attitude cost function is proposed for attitude determination assuming that the cycle integer ambiguities are known. The method that minimizes the cost function is discussed. To verify the method proposed, the experiments have been conducted, and the testing results are given in this paper.
COMPOSITE ADAPTIVE CONTROL OF SPACE MANIPULATOR SYSTEM WITH PRISMATIC JOINT
CHEN Li
2003, 23(1): 60-67. doi: 10.11728/cjss2003.01.20030109
Abstract(2196) PDF 666KB(1183)
Abstract:
In this paper, the control problem of free-floating space manipulator system with prismatic joint was studied. It is shown that the Jacobian matrix and the dynamic equations of the system could not easily be linearly parameterized, if we deduced it by use of the conservation relationship of the momentum and the angular momentum of the system. With the augmentation approach, we got the augmented generalized Jacobi matrix and the dynamic equation of the system that could be linearly dependent on a group of inertial parameters. Based on the results, the composite adaptive control scheme for free-floating space manipulator system with prismatic joint and unknown inertial parameters to track the desired trajectory in inertia space is proposed. The advantages of the control scheme proposed are that it needs not to measure the position, velocity and acceleration of the base. A two-link planar space manipulator system is simulated to verify the proposed control scheme.
EXPERIMENTAL RESEARCH OF FIRST FEED-SUPPORT SYSTEM OF FAST
YU Liming, SUO Shuangfu, JI Linhong, REN Gexue
2003, 23(1): 68-73. doi: 10.11728/cjss2003.01.20030110
Abstract(2140) PDF 544KB(917)
Abstract:
The first feed-support system, which is one of the key techniques of FAST, is introduced in this paper. Systemic experimental research with the scaled model, which is one of thirtieth of actual structures, is made. In the experiment, the position deflection of the feed-car was analyzed when the feed-car ran along the part of a circle. Furthermore, the equivalent rigidity of the system was measured and the position deflection of the feed-car resulting from wind was computed. The research results confirmed that the first feed-support system meets the required position control precision. Also, the results are very helpful to the precise position control of the large span cable structures.
CALCULATING IMAGE MOTION OF AEROSPACE CAMERA BASED ON DYNAMIC OBJECT-IMAGE CONJUGATE RELATION
ZHOU Qingcai, WANG Zhijian
2003, 23(1): 74-79. doi: 10.11728/cjss2003.01.20030111
Abstract(2145) PDF 407KB(994)
Abstract:
In this paper, the coordinate system of aerospace camera is established. The geometry relation between object and image vectors is made clear. Then operation matrix in aerospace camera is denned. Finally, based on the static and dynamic object-image conjugate relation, image motion in aerospace camera was analysed. The result shows the concise concept and simple expression of this method, which is consistent with uniform coordinate transform method.