We present the first evidence for occurrences of magnetic interactions between a jet, a filament and coronal loops durin......

We present a new method for automatically forecasting the occurrence of solar flares based on photospheric magnetic meas......

We present a statistical study of decimetric type Ⅲ radio bursts,coronal mass ejections(CMEs),and Hα flares observed i......

在分析了近年来对太阳射电爆发与高能质子观测的基础上指出，既非Ⅱ型也非米波ＩＶ型而是强微汉爆发几乎总是同高能质子共生的，这一结果否......

论述了太阳二维光谱观测和研究的重大意义，综述了二维光谱观测技术和仪器的进展，特别介绍了应用ＣＣＤ的成像光谱仪的最近发展。文中还介绍......

太阳无黑子耀斑是太阳耀斑的特殊表现，无黑子耀斑的研究是太阳耀斑研究的重要组成部分。在本文中总结了太阳无黑子耀斑观测研究的以......

在太阳耀斑区磁场和电流研究方面，文中将着重介绍太阳横向磁场方位的确定，太阳活动区磁场的非热性表示、太阳耀斑前后的活动区磁场变......

对近年来的紫外空间观测仪器（包括在研项目）作了扼要介绍，并对一些关键问题如烃基污染致使仪器灵敏度迅速下降，镜面紫外反射率低下及改......

We present multi-wavelength observations of an M-class flare(M3.9) that occurred on 2014 June 11.Our observations were c......

The Advanced Space-based Solar Observatory(ASO-S)is a mission proposed for the 25 th solar maximum by the Chinese solar ......

一根塑造 S 的细丝的节在 sigmoidal 经历了爆发有塑造 S 的花冠的活跃区域(AR 8027 ) 组织细丝的结束，它被出现在 NW 下面的双性人......

As one of the payloads for the Advanced Space-based Solar Observatory(ASO-S)mission,the Lyman-alpha(Lyα)Solar Telescope......