Small-Scale Brightenings in the UV Continuum of an M9.1 Solar Flare     

Lin Wang Cheng Fang Ming-De Ding 《中国天文和天体物理学报》2007,7(5):721-732

We analyze an M9.1 two-ribbon solar flare which occurred on 2004 July 22 us- ing the TRACE white-light and 1700A~。images,the RHESSI,and the SOHO/MDI data.We find many small-scale fast-varying brightenings that appeared in the white-light and 1700A~。images along the flare ribbons.Some of them underwent rapid motions in weak magnetic field regions.We identify these short-lived brightenings as UV continuum enhancement.Our preliminary result shows that the brightenings are closely related to the HXR emission.They have a lifetime of 30-60 s and a typical size of about 1″-2″.The intensity enhancement is about 150-200 times the mean value of the quiet-Sun.According to previous works,we infer that the 1700A~。enhancement may be dominated by the increased emission of 1680 A con- tinuum coming from the temperature minimum region.The impulsive feature in the 1700 A~。light curves of the small-scale brightenings may be due to the irradiation of the impulsive CIV line intensity caused by the bombardment of non-thermal electron beams.  相似文献   

Impact of Suspended Particles and Enhancement Techniques on Ultraviolet Disinfection of a Secondary Effluent   总被引：1，自引：0，他引：1  

WANG Jianling WANG Lin WANG Baozhen ZHANG Jinsong ZOU Oixian 《中国海洋大学学报(英文版)》2006,5(4):381-386

The concentration of suspended solids in the secondary effluent often varies widely, leading to frequent adjustment of the UV dosage to meet the disinfection criterion. In addition, a desired disinfection rate is difficult to achieve sometimes. The authors studied the particle size distribution, contribution of particle-associated Fecal Coliform （F. C. ）, and their influences on UV disinfection. A combined disinfection process （chlorination with a subsequent UV disinfection） was tested to improve the disinfection effect. The results indicated that the content of suspended solids, especially that of large particles, has a strong impact on UV disinfection efficiency; D〉 10 μm particles associated F.C. are difficult to be disinfected and are the main part of the tailings of F.C. inactivation curves. Pre-chlorination could decrease the number of particles in the secondary effluent and transform the large particles into small ones, reducing the influence of particles on UV disinfection and enhancing the resistance ability of the combined process to particle loading.  相似文献   

The Ultraviolet Coronagraph Spectrometer for the solar and heliospheric observatory     

《Solar physics》1995,162(1-2):313-356

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UV and optical spectral properties in early-type galaxies     

Stefan J. Kautsch  Werner W. Zeilinger 《Astrophysics and Space Science》2003,284(2):929-932

We investigate UV and optical spectra of a sample of nearby early-type galaxies with evidence of nuclear line emission. The spectral signatures of various contributors to the UV, such as the interstellar medium and various stellar populations are analyzed and compared with the optical spectral properties. We discuss the impact of these effects on the observational properties of galaxy evolution. This revised version was published online in August 2006 with corrections to the Cover Date.  相似文献   

Transition region and coronal plasmas: instrumentation and spectral analysis     

Klaus Wilhelm  Ingolf E. Dammasch  Donald M. Hassler 《Astrophysics and Space Science》2002,282(1):189-207

The plasma conditions in the solar atmosphere and, in particular, in coronal holes are summarized, before space-borne instrumentation for observing these regions in vacuum-ultraviolet light is briefly introduced with the Solar Ultraviolet Measurements of Emitted Radiation (SUMER) spectrometer on the Solar and Heliospheric Observatory (SOHO) as example. Spectroscopic measurements of small plasma jets are then analyzed in detail. Magnetic reconnection is thought to be responsible for heating the corona of the Sun as well as accelerating the solar wind by converting magnetic energy into thermal and kinetic energies. The continuous outflow of the fast solar wind from coronal holes on ‘open’ field lines, which reach out into interplanetary space, then requires many reconnection events of very small scale sizes – most of them probably below the resolution capabilities of present-day instruments. Our observations of such an event have been obtained with the Solar and Heliospheric Observatory (SOHO) providing both high-resolution imaging and spectral information for structural and dynamical studies. We find whirling or rotating motions as well as jets with acceleration along their propagation paths in close spatial and temporal vicinity to the coronal jet. This revised version was published online in July 2006 with corrections to the Cover Date.  相似文献   

Non-radial pulsation of the δ Scuti star UV Trianguli     

Ai-Ying Zhou  Zong-Li Liu  E. Rodríguez 《Monthly notices of the Royal Astronomical Society》2002,336(1):73-80

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In-flight Performance of the Advanced Camera for Surveys CCDs     

Mark Clampin  Marco Sirianni  George F. Hartig  Holland C. Ford  Garth D. Illingworth  Bill Burmester  William Koldewynd  Andre R. Martel  Adam Riess  Ronald J. Schrein  Pamela C. Sullivan 《Experimental Astronomy》2002,14(2):107-115

The Advanced Camera for Surveys (ACS), installed in the Hubble Space telescope in March 2002, will significantly extend HST's deep, survey imaging capabilities. ACS has met, or exceeded, all of its key performance specifications. In this paper we briefly review the in-flight performance of the instrument's CCD detectors and preview early ACS science observations. This revised version was published online in July 2006 with corrections to the Cover Date.  相似文献   

On the Station-Keeping and Control of the World Space Observatory/Ultraviolet     

Xi-Yun Hou  Hai-Hong Wang  Lin Liu Department of Astronomy  Nanjing University  Nanjing : Institute of Space Environment  Astronautics  Nanjing University  Nanjing 《中国天文和天体物理学报》2006,6(3):372-378

Collinear libration points play an important role in deep space exploration because of their special positions and dynamical characteristics. Since motion around them is unstable, we need to control the spacecraft if we wish to keep them around such a libration point for a long time. Here we propose a continuous low-thrust control strategy, illustrated with numerical simulations combined with the orbit design and control of the World Space Observatory/UltraViolet (WSO/UV).  相似文献   

CSRH阵列设计研究及馈源设计的初步考虑     

王威  颜毅华  张坚  姬国枢  陈志军 《天文研究与技术》2006,3(2):128-134

介绍频谱日像仪天线阵排列及实验馈源设计的研究工作。基于CSRH设计指标,模拟了天线阵T型排列、Y型排列、不规则型和螺旋型排列,给出了每种排列的UV覆盖图像,并在成图质量上对各种排列方式做了分析。最后综合考虑提出建议采用自相似螺旋型排列。  相似文献   

非常规气象要素在紫外线预报中的应用     

谢静芳  应爽  刘海峰  陈雷 《气象科技》2020,48(2):248-253

利用吉林省业务运行的WRF模式,计算了与紫外线指数相关的气温、湿度、云量、风速等常规气象要素和地表向下的短波辐射通量、地面热通量、反照率等非常规气象要素,利用长春市紫外线观测资料,分析了紫外线辐射与常规和非常规气象要素的相关性。基于长春市紫外线观测实况,以常规气象要素、非常规气象要素、混合气象要素为因子,利用相同的统计建模方法,分别建立紫外线预报模型。结果表明:大气短波辐射等非常规气象要素与紫外线指数的相关性,明显高于气温、云量、比湿、风速等常规气象要素;应用非常规气象要素和混合气象要素的紫外线预报方程,显著优于常规气象要素;基于混合气象要素的紫外线预报方程,与基于非常规气象要素的预报方程比较,预报性能差异不大。此外,应用常规气象要素建立的分季节紫外线预报方程,其预报效果明显优于全年预报方程。应用非常规气象要素建立的分季节紫外线预报方程,与全年预报方程相比,预报效果差异不大。  相似文献