1) spaghetti-shaped radio burst
条状射电爆发
2) radio bursts
射电爆发
1.
The main conclusions include: 1) Under the approximations of Dulk et al(1982),the parallel and perpendicular components of the magnetic field in the sources of radio bursts are calculated self-consistently,and 2-dimensional distribution was obtained firstly.
主要结论可归纳为:1)在Dulk等人(1982)的近似下自恰计算射电爆发源区磁场的平行和垂直分量,并首次得到该磁场在日面的两维分布。
2.
After analyzing 158 radio bursts observed from September 2000 to September 2001 with the 0.
5GHz太阳射电频谱仪2000年9月至2001年9月取得的158个射电爆发,发现其中约有65%存在4类不同类型的快速精细结构(FFS):毫秒尖峰辐射、Ⅲ型爆发、准周期脉动、慢漂移结构。
3.
It is shown in this paper that the solar radio bursts originate not only from flares but also from coronal mass ejections (CMEs) or CME flare combinations, based on the data of recent space and ground besed solar observations.
本文分析了近二十年来的地面和空间太阳有关观测资料，得出太阳射电爆发的起因为耀斑和／ 或日冕物质抛射（ＣＭＥ） 而不仅仅是耀斑，这将有利于更深刻地了解太阳射电爆发和共生高能现象的物理过
3) radio burst
射电爆发
1.
The analyses of characteristics of moving type Ⅳ dm burst and the starting sequence of radio bursts at multi-band may indicate that this accompanied white-light flare (WLF) and the radio bursts are activated by the same accelerated electrons from lower corona.
从射电运动Ⅳ型爆发的特征和多频射电爆发开始时序的分析可以看出这个伴生的白光耀斑（ Ｗ Ｌ Ｆ） 和射电爆发同是由低日冕的加速电子激活，可能通过非热电子沉降能量于色球层， 产生了色球层压缩波， 又经二步能量传输过程在上光球层导致 Ｗ Ｌ Ｆ。
2.
olar radio burst is a kind of manifestation of solar flare in radio wavelength band.
太阳射电爆发是太阳耀斑在无线电波段的一种表现，并相当敏感地反映了耀斑的能量释放过程。
3.
The exciter functions of the radio bursts observed on May 21, 1990 at 2840 MHz and 2640 MHz have been obtained by means of this method.
本文利用傅里叶变换解卷积积分的方法,分析了1990年5月21日北京天文台2840MHz和2640MHz的射电爆发资料,分别求出了它们的激励函数。
4) multi-emitter fingers
梳状发射极条
5) explosive electron emission
爆炸电子发射
1.
The electron gun can be divided into explosive electron emission (EEE), anode plasma (AP) and oriented magnetic field.
电子束产生部分由爆炸电子发射阴极、等离子体阳极及导向磁场构成。
6) solar radio burst
太阳射电爆发
1.
Besides,the relationship between solar radio bursts and SPA/SFA is analysed too.
同时还对SPA及SFA与太阳射电爆发之间的关系进行了分
2.
Finally the parameters of fine structures is calculated and analyzed so as to understand the physics of solar radio burst.
由此,可以计算精细结构的特征参数,并进行统计分析,从而揭示太阳射电爆发的本质。
3.
Solar radio bursts are usually accompanying with solar flares.
太阳射电爆发通常发生在太阳耀斑期间,它携带着爆发源区的物理环境以及辐射机制等诸多重要信息,尤其是微波爆发的精细结构,持续时间短、变化快、结构复杂,可以反映重联过程复杂的磁场结构、高能粒子运动等许多特征。
补充资料：条状
1.列举情状。
说明：补充资料仅用于学习参考，请勿用于其它任何用途。
参考词条