{"title":"A TRANSITION REGION EXPLOSIVE EVENT OBSERVED IN He ii WITH THE MOSES SOUNDING ROCKET","authors":"J. Fox, C. Kankelborg, R. Thomas","doi":"10.1088/0004-637X/719/2/1132","DOIUrl":null,"url":null,"abstract":"Transition region explosive events (EEs) have been observed with slit spectrographs since at least 1975, most commonly in lines of C iv (1548 Å, 1550 Å) and Si iv (1393 Å, 1402 Å). We report what we believe to be the first observation of a transition region EE in He ii 304 Å. With the Multi-Order Solar EUV Spectrograph (MOSES) sounding rocket, a novel slitless imaging spectrograph, we are able to see the spatial structure of the event. We observe a bright core expelling two jets that are distinctly non-collinear, in directions that are not anti-parallel. The jets have sky-plane velocities of order 75 km s−1 and line-of-sight velocities of +75 km s−1 (blue) and −30 km s−1 (red). The core is a region of high non-thermal Doppler broadening, characteristic of EEs, with maximal broadening 380 km s−1 FWHM. It is possible to resolve the core broadening into red and blue line-of-sight components of maximum Doppler velocities +160 km s−1 and −220 km s−1. The event lasts more than 150 s. Its properties correspond to the larger, long-lived, and more energetic EEs observed in other wavelengths.","PeriodicalId":22368,"journal":{"name":"The Astrophysical Journal Supplement Series","volume":"25 1","pages":"1132 - 1143"},"PeriodicalIF":0.0000,"publicationDate":"2010-07-27","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"17","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"The Astrophysical Journal Supplement Series","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1088/0004-637X/719/2/1132","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 17
Abstract
Transition region explosive events (EEs) have been observed with slit spectrographs since at least 1975, most commonly in lines of C iv (1548 Å, 1550 Å) and Si iv (1393 Å, 1402 Å). We report what we believe to be the first observation of a transition region EE in He ii 304 Å. With the Multi-Order Solar EUV Spectrograph (MOSES) sounding rocket, a novel slitless imaging spectrograph, we are able to see the spatial structure of the event. We observe a bright core expelling two jets that are distinctly non-collinear, in directions that are not anti-parallel. The jets have sky-plane velocities of order 75 km s−1 and line-of-sight velocities of +75 km s−1 (blue) and −30 km s−1 (red). The core is a region of high non-thermal Doppler broadening, characteristic of EEs, with maximal broadening 380 km s−1 FWHM. It is possible to resolve the core broadening into red and blue line-of-sight components of maximum Doppler velocities +160 km s−1 and −220 km s−1. The event lasts more than 150 s. Its properties correspond to the larger, long-lived, and more energetic EEs observed in other wavelengths.
至少从1975年开始,人们就用狭缝光谱仪观测到了过渡区爆炸事件(EEs),最常见的是在C iv (1548 Å, 1550 Å)和Si iv (1393 Å, 1402 Å)谱线上。我们报告了我们认为在He 304 Å中首次观察到的过渡区EE。利用多阶太阳极紫外探空火箭(Multi-Order Solar EUV Spectrograph, MOSES),一种新型的无缝隙成像光谱仪,我们能够看到事件的空间结构。我们观察到一个明亮的核心喷出两股明显非共线的喷流,它们的方向不是反平行的。这些喷气机的天机速度约为75 km s - 1,视距速度为+75 km s - 1(蓝色)和- 30 km s - 1(红色)。核心是非热多普勒展宽高的区域,具有EEs的特征,最大展宽为380 km s−1 FWHM。可以将核心的扩展分解为最大多普勒速度+160 km s - 1和- 220 km s - 1的红色和蓝色视线分量。事件持续时间超过150秒。它的性质与在其他波长中观察到的更大、寿命更长、能量更大的ee相对应。