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A. Kepa B. SylwesterM. Siarkowski J. Sylwester 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
X-ray spectrometer RESIK has observed spectra in the four wavelength bands from 3.3 Å to 6.1 Å. This spectral range contains many emission lines of H- and He-like ions for Si, S, Ar and K. These lines are formed in plasma of coronal temperatures (T > 3 MK). Analysis of their intensities allows studying differential emission measure distributions (DEM) in temperature range roughly between 3 MK and 30 MK. The aim of present study was to check whether any relationship exists between the character of DEM distribution, the event phase and the X-ray flare class. To do this we have calculated and analyzed the DEM distributions for a set of flares belonging to different GOES classes from the range B5.6–X1. The DEM distributions have been calculated using “Withbroe–Sylwester” multiplicative, maximum likelihood iterative algorithm. As the input data we have used absolute fluxes observed by RESIK in several spectral bands (lines + continuum). Respective emission functions have been calculated using the CHIANTI v. 5.2 atomic data package. 相似文献
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S. Sheridan M.W. Bardwell A.D. Morse G.H. Morgan 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
A novel ionisation source which uses commercially available Carbon Nano Tube devices is demonstrated as a replacement for a filament based ionisation source in an ion trap mass spectrometer. The carbon nanotube ion source electron emission was characterised and exhibited typical emission of 30 ± 1.7 μA with an applied voltage differential of 300 V between the carbon nanotube tips and the extraction grid. The ion source was tested for longevity and operated under a condition of continuous emission for a period of 44 h; there was an observed reduction in emission current of 26.5% during operation. Spectra were generated by installing the ion source into a Finnigan Mat ITD700 ion trap mass spectrometer; the spectra recorded showed all of the characteristic m/z peaks from m/z 69 to m/z 219. Perfluorotributylamine spectra were collected and averaged contiguously for a period of 48 h with no significant signal loss or peak mass allocation shift. The low power requirements and low mass of this novel ionisation source are considered be of great value to future space missions where mass spectrometric technology will be employed. 相似文献
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空心阴极的发射体在电子发射时会处于动态热平衡状态,这种发射热特性对发射体的利用率和工作寿命有重要意义。为研究空心阴极发射热特性及相关热设计方法,建立一种流-热耦合数值模型,将等离子体流场计算与组件热分布计算进行耦合,并采取一种逆向迭代方法来收敛计算,数值模型在验证试验下的计算误差低于11.3%。在此基础上,对发射体温差的机理以及阴极顶孔径对发射体温差的影响规律进行数值分析,主要结论为:羽状模式下的核心电离区较发散,导致发射体温差较点状模式高出50 K左右;适当增加阴极顶孔径可对发射体温差有降低作用。 相似文献
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论述了计算机电磁泄漏的危害及测试的意义,介绍了测试系统的组成,对某国产微型计算机进行了测试,并对其测试数据进行了分析,提出了行之有效的防护措施。 相似文献
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We investigate the possibility of observing the effects of magnetic reconnection inside a current sheet forming in a coronal streamer in the extended corona. In particular we study the possibility to observe with the UVCS of SOHO the excitation of the tearing instability in the current sheet. 相似文献