1.Geomagnetic solar flare effect on February 4and 6, 1986 at the china Antarctic Great wall Station
Geomagnetic solar flare effect on February 4 and 6，1986 at the china Antarctic Great wall Station
2.THE HEATING MECHANISM AND STABILITY OF THE GIANT POST FLARE ARCH OF 21-22 MAY, 1980
1980年5月21日—22日耀斑后冕拱(Post-flare coronal arch)的加热机制和稳定性
3.In television, an unwanted component in the picture signal output from a camera, caused by the scattering of light in the optical system. Flare is often described in terms of its position in the picture, e. g., edge flare, bottom flare.
电视中来自摄象机的图象信号输出中不希望出现的组成部分，它是由光学系统中光散射引起的。光斑常按照它在图象中的位置来描述，例如，边沿光斑、底部光斑。
4.Flare is often described in terms of its position in the picture, e. g., edge flare, bottom flare.
光斑常按照它在图象中的位置来描述，例如，边沿光斑、底部光斑。
5.These data bring to light the general picture of the distribution of the internal motion and the macroscopical motion of the flare Joop prominence with time and space in the course of its eruption and ascension:1. The southern leg system of the flare loop had the right-handed motion before the maximum brightness, and after the maximum brightness the two leg systems rotated at the same direction at the angular velocity of about 4×10-3 arc/sec.
这些资料揭示了该耀斑环在爆发上升过程中内部运动和宏观运动随时空分布的大致图象: 1.亮度极大前耀斑环南腿系出现右螺旋运动,亮度极大后发展为两腿系的同向旋转运动,角速度约为4×10~(-3)弧度/秒。
6.In chapter two, we researched a Ml. 3 X-ray flare and associated CME occurred in Active Region 10537 and found that CME and flare were likely two different manifestations of the same magnetic eruption process in the corona.
第二章对2004年1月8曰活动区NOAA AR 10537内发生的一个耀斑及相关CME进行了观测研究，发现耀斑和CME极可能是相同磁场过程在日冕中的不同表现。
7.Flare has a small radius and as soon as you get out of it you can COS the flare effect and vanish.
照明弹的范围很小,所以你一旦脱离(指陷阱还是照明弹不知道)你就可以[暗影斗篷]掉[闪光弹效果],然后[消失].
8.In electro-optical countermeasure environment, the variation of radiant energy of IR flare is very acute. The ant jamming IR seeker demands the dynamitic change of radiant energy of IR flare to be reflected in real time to meet the requirements of amplitude discrimination and amplitude correlation.
在光电干扰环境中，红外干扰弹辐射能量变化剧烈，抗干扰红外导引头要求实时表征红外干扰弹辐射能量动态变化，以满足幅度鉴别和幅度相关的需要。
9.The flare showed good temporal and spatial relationships with a quick partial halo CME (coronal mass Ejections) observed by SOHO/LASCO, and it is very likely that they are two different manifestations of the same magnetic eruption process in the corona. Therefore,we identify that the flare and the associated coronal dimmings are just the on-disk source region of the CME on solar disk.
该耀斑爆发与LASCO观测到的一个快速partialhaloCME在空间和时间上具有密切的关系,它们极可能是相同磁场过程在日冕的不同表现,故我们将此耀斑及与之伴随的日冕dimming认证为这一CME的日面源区。
10.The statistical studies between the flare activities and the different types of magnetic disturbance during the years 1936-1958 confirm further our earlier finding of the N-S and E-W asymmetries in the solar-geomagnetic relationship. Also, there are evidences that the characteristics of magnetic disturbance show some relation to the magnetic types of solar active region producting flare, and to the propagation velocity of solar disturbance in the interplanetary space.
对1936—1958年期间各类磁扰与耀斑活动的统计关系,进一步证实作者以前发现的太阳活动与磁扰关系之间的南北及东西不对称性,也有证据表明,磁扰特性与活动区磁场类型及太阳扰动产物在行星际空间的传播速度有关。
