光谱学与光谱分析
光譜學與光譜分析
광보학여광보분석
SPECTROSCOPY AND SPECTRAL ANALYSIS
2015年
5期
1432-1435
,共4页
谱仪%掠入射%平场谱仪%X射线和紫外
譜儀%掠入射%平場譜儀%X射線和紫外
보의%략입사%평장보의%X사선화자외
Spectrograph%Grazing-incidence%A flat-field spectrograph%Ray-trace%Soft X-rays
等离子体辐射的谱线中包含着等离子体状态的大量信息。因此,探测等离子体状态参数的最有效手段之一就是等离子体辐射的谱线测量。现有的软X射线掠入射平场谱仪由于受到已有掠入射变间距凹面反射光栅的限制,在保持平焦场的情况下,可测量波段范围只有5~40 nm。为了扩展掠入射X U V平场谱仪的测谱范围,首先编制了掠入射变间距凹面反射光栅的光路追踪程序。然后与文献[6]同样条件下的结果进行了数值比较,结果表明我们的程序计算结果与Harada等的结果符合的非常好,从而验证了所编制光路追踪程序的可信性。最后利用所编程序对不同掠入射条件下变间距凹面反射光栅的平焦场变化情况进行了详细的数值研究。通过计算和分析表明,在保持软X射线波段范围5~40 nm为平场不变的情况下,在45~80 nm的超紫外线波段范围内找到了一个满足平焦场条件的平场面直线方程为 y=-2.50 x+661.11的平场面,从而利用一块掠入射凹面光栅就可以将掠入射平场谱仪的波长范围从5~40 nm扩展到5~80 nm。这个结果即从理论上论证了将传统的掠入射平场谱仪从软X射线波段扩展到超紫外线(XUV)波段的可行性,也为提高了掠入射平场凹面光栅的使用性提出了新的设计思路。
等離子體輻射的譜線中包含著等離子體狀態的大量信息。因此,探測等離子體狀態參數的最有效手段之一就是等離子體輻射的譜線測量。現有的軟X射線掠入射平場譜儀由于受到已有掠入射變間距凹麵反射光柵的限製,在保持平焦場的情況下,可測量波段範圍隻有5~40 nm。為瞭擴展掠入射X U V平場譜儀的測譜範圍,首先編製瞭掠入射變間距凹麵反射光柵的光路追蹤程序。然後與文獻[6]同樣條件下的結果進行瞭數值比較,結果錶明我們的程序計算結果與Harada等的結果符閤的非常好,從而驗證瞭所編製光路追蹤程序的可信性。最後利用所編程序對不同掠入射條件下變間距凹麵反射光柵的平焦場變化情況進行瞭詳細的數值研究。通過計算和分析錶明,在保持軟X射線波段範圍5~40 nm為平場不變的情況下,在45~80 nm的超紫外線波段範圍內找到瞭一箇滿足平焦場條件的平場麵直線方程為 y=-2.50 x+661.11的平場麵,從而利用一塊掠入射凹麵光柵就可以將掠入射平場譜儀的波長範圍從5~40 nm擴展到5~80 nm。這箇結果即從理論上論證瞭將傳統的掠入射平場譜儀從軟X射線波段擴展到超紫外線(XUV)波段的可行性,也為提高瞭掠入射平場凹麵光柵的使用性提齣瞭新的設計思路。
등리자체복사적보선중포함착등리자체상태적대량신식。인차,탐측등리자체상태삼수적최유효수단지일취시등리자체복사적보선측량。현유적연X사선략입사평장보의유우수도이유략입사변간거요면반사광책적한제,재보지평초장적정황하,가측량파단범위지유5~40 nm。위료확전략입사X U V평장보의적측보범위,수선편제료략입사변간거요면반사광책적광로추종정서。연후여문헌[6]동양조건하적결과진행료수치비교,결과표명아문적정서계산결과여Harada등적결과부합적비상호,종이험증료소편제광로추종정서적가신성。최후이용소편정서대불동략입사조건하변간거요면반사광책적평초장변화정황진행료상세적수치연구。통과계산화분석표명,재보지연X사선파단범위5~40 nm위평장불변적정황하,재45~80 nm적초자외선파단범위내조도료일개만족평초장조건적평장면직선방정위 y=-2.50 x+661.11적평장면,종이이용일괴략입사요면광책취가이장략입사평장보의적파장범위종5~40 nm확전도5~80 nm。저개결과즉종이론상론증료장전통적략입사평장보의종연X사선파단확전도초자외선(XUV)파단적가행성,야위제고료략입사평장요면광책적사용성제출료신적설계사로。
The radiation spectrum from the plasmas contains a large amount of information of plasmas .Thus ,one of the most ef-fective methods to detecting the plasma parameters is measure the plasma radiation spectrum .Until now ,since the restriction of the Toshiba mechanically ruled aberration-corrected concave gratings ,the measurable wavelength range of the incidence flat-field grazing spectrometer in the soft X-ray range are only from 5 to 40 nm .In order to extend the wavelength rang of grazing inci-dence flat-field spectrometer ,first ,a grazing incidence concave reflection grating ray-trace code is written using optical path equation .Second ,under the same conditions with reference 6 ,we compare our numerical results with Harada’s results .The re-sults show that our results agree very well with the results of Harada .The results of comparison show that our ray-trace code is believable .Finally ,the variety of the flat-field curves are detailedly investigated using the ray-trace code with the different graz-ing incidence conditions .The results show that the measurable wavelength range of the incidence flat-field grazing spectrometer are extended to 5~80 nm from the soft X-ray wavelength range of 5~40 nm .This result theoretically demonstrates the possibil-ity of expanded the traditional band flat-field grazing incidence spectrometer from soft X-ray band to the extreme ultraviolet (XUV) ,and also bring a new design ideas for improving the use of grazing incidence flat field concave grating .