CAJ | 학술논문

2004年11月9日WIND飞船探测到一个典型的行星际激波.激波前行星际磁场为持续约50 min的弱南向磁场,越过激波面,磁场发生北向偏转且太阳风动压脉冲增强.在此强动压脉冲增强结构作用下,磁层被压缩至一个很小的区域.激波作用于磁层时引起地球同步轨道各区域高能粒子通量的响应,但是不同磁地方时的高能粒子通量的响应不同,表现出双模式扰动,即在晨昏两侧各能段的电子和质子通量显著增强,在子夜侧发生类似于亚暴的无色散粒子注入现象.扰动从向阳面传输到背阳面,向阳面粒子通量最先增强,随后背阳面靠近晨昏两侧,粒子通量开始增强,最后子夜侧粒子通量表现出无色散高能粒子注入的特点,另外,在靠近正午侧,质子通量先于电子通量发生响应,在子夜侧电子通量则先于质子通量发生响应.利用位于向阳面正午两侧的GOES-10和GOES-12卫星观测数据发现,激波作用于磁层时靠近晨侧的磁场变化表现出简单压缩效应,而靠近昏侧的磁场变化则显然不同,B_x分量减弱,B_z分量几乎减为零,而B_y分量则显著增强,此外,位于近地磁尾低纬尾瓣区的TC-1卫星观测到激波触发的尾瓣SI现象.
2004년11월9일WIND비선탐측도일개전형적행성제격파.격파전행성제자장위지속약50 min적약남향자장,월과격파면,자장발생북향편전차태양풍동압맥충증강.재차강동압맥충증강결구작용하,자층피압축지일개흔소적구역.격파작용우자층시인기지구동보궤도각구역고능입자통량적향응,단시불동자지방시적고능입자통량적향응불동,표현출쌍모식우동,즉재신혼량측각능단적전자화질자통량현저증강,재자야측발생유사우아폭적무색산입자주입현상.우동종향양면전수도배양면,향양면입자통량최선증강,수후배양면고근신혼량측,입자통량개시증강,최후자야측입자통량표현출무색산고능입자주입적특점,령외,재고근정오측,질자통량선우전자통량발생향응,재자야측전자통량칙선우질자통량발생향응.이용위우향양면정오량측적GOES-10화GOES-12위성관측수거발현,격파작용우자층시고근신측적자장변화표현출간단압축효응,이고근혼측적자장변화칙현연불동,B_x분량감약,B_z분량궤호감위령,이B_y분량칙현저증강,차외,위우근지자미저위미판구적TC-1위성관측도격파촉발적미판SI현상.
On November 9, 2004, the WIND spacecraft detected a typical interplanetary shock. Before the shock, there is a sustaining weak southward magnetic field lasting about 50 nun. Across the shock front, the magnetic field turns northward, and the solar wind dynamic pressure is abruptly enhanced, i.e., the shock is a strong Dynamic Pressure Pulse (DPP). The magnetosphere is compressed to a rather small region upon the impact of the DPP. During the impingement of the shock, the magnetospheric compression causes two-mode disturbances of the energetic particle at the geosynchronous orbit, i.e., particle fiux enhancement due to the compression near dawn and dusk and dispersionless particle injection similar to substorm. The disturbances propagate from the dayside to the nightside. The energetic particle fiuxes on the dayside first increase, and then after about 1 min,the particle fluxes near dawn and dusk on the nightside begin to increase. Finally, dispersionless particle injection is seen near the midnight, Furthermore, near the noon the responses of electron are prior to those of proton. Contrarily, near the midnight the responses of proton are prior to those of electron. By using GOES-10 and GOES-12 observations on two sides of the noon, it is found that the magnetic field on the dawn-noon sector is simply compressed, while for the magnetic field on the noon-dusk sector, B_x and B_z component decreases, but B_y component notably increases. The TC-1 spacecraft located at near-Earth low-latitude lobe region observes the shock-induced lobe SI phenomena.