solar x ray 中文意思是什麼

solar x ray 解釋
射線
  • solar : adj 太陽的，根據太陽運行測量的；因太陽作用產生的。n ＝ solarium the solar system 太陽系。 a solar...
  • x : X2＝ （羅馬數字）10 XX ＝ 20 IX ＝ 9 XV ＝ 15 XL ＝ 40 LX ＝ 60 XC ＝ 90 DXL ＝ 540 MX ＝ 1010 ＝...
  • ray : n 雷〈姓氏，男子名， Raymond 的昵稱〉。n 1 光線，射線，熱線；〈詩〉光輝，閃爍，曙光，一線光明。2 ...
  1. From the x - ray eyes of the trace satellite to the projected images on the floor of the solar telescope observatory at kitt peak in arizona, " solarmax " examines man s changing perception of the sun throughout time

    本片帶你從追號星的x -光眼，到利用位於亞里桑那州基特峰天文臺上的太陽望遠鏡觀看太陽，藉此探索人類從古至今對太陽觀點的改變。
  2. At first, environment detection data is collected, modulated and emitted in the the system of fy - 2 and detectors. then data signal is magnified, demodulated and sent in the earth - based system of data receiving and demodulating. at last, data is received, processed, stored, displayed and judged to make alarm automatically by telephone for solar proton - events and x - ray flare in the system of data processing and alerting

    首先在fy - 2衛星及探測器系統中，環境探測數據被收集、調制並發射，接著由地基數據接收及解調系統將數據信號放大、解調還原並發送，最後由數據處理及警報系統將數據接收處理、保存顯示並對太陽質子事件、 x耀斑進行自動電話報警。
  3. Space explorers for charge - particles detecting and those for solar x - ray detecting are kernels of space environment monitoring systems for space charge - particles monitoring and space soft 、 hard x - ray monitoring respectively

    本文討論的x射線探測器標定分析系統，主要用於實現對x射線探測器的能譜標定。
  4. By means of 4 dual - frequency gps receivers over china, the tec in the ionosphere during solar flare on nov 22, 1998 is calculated. the results indicate that the flare, the x - ray level of which is x3. 7, cause obvious tec enhancements in the ionosphere, the largest tec enhancement caused by the flare is about 1. 25 tecu. the characteristic of this method to study such ionospheric disturbances caused by flares is analyzed. it is concluded that this method can be used to study the ionosphere disturbances caused by solar flare, and can get more ionospheric disturbances information because of the special satellite constellation

    此次耀斑爆發引起了設在北京的高頻多普勒長達15min左右的無線電短波中斷。通過對gps得到的電離層tec進行分析發現：此次耀斑造成了大面積的電離層tec的增加，耀斑爆發引起的最大tec增幅在1 . 25個tec單位左右利用高精度的gps數據處理方法可研究耀斑引起的電離層擾動。另外，還分析了由gps計算的tec的時空變化特點。
  5. Summarizing their result, we found the following results : ( 1 ) there are two x - ray sources in the active object the north one is much stronger than the southern, and the southern is higher than the former to the solar surface

    在前人的研究成果中，我們發現如下結論： （ 1 ）該耀斑爆發時出現兩個x射線源。較強的位於北面，距日面較近，出現的時間比南面的x射線源早，消失得晚。
  6. It is used in solar cells and semiconductor detectors for astrophysical research, for x - ray fluorescence ( xrf ) analysis, industrial gauging, nuclear proliferation treaty verifaction et. al, and also in laser window and infrared array technology as subtriate for hg1 - xcdxte

    同時它還可作為紅外探測器材料碲鎘汞（ hgcdte ）和外延襯底，以及激光窗口和太陽電池等。
  7. The main research contents of the technical design include : analyzing the necessary parts of the solar x - euv telescope and the method of imaging x and euv ray ; developing the optic, electronic and mechanical design of this instrument ; computing solar x - euv imaging telescope ' s response to different temperature plasma, analyzing combination application of telescope filters for reconstructing the plasma paramaters and apprasing the telescope ' s response to the solar activities

    技術設計的主要內容包括：分析瞭望遠鏡的系統組成及成像方式選擇；完成太陽x - euv成像望遠鏡光學、電子學、機械等方面的技術設計：計算分析了太陽x - euv成像望遠鏡對不同溫度的等離子體響應、反演高低溫等離子體參數的最佳過濾片組合利用及望遠鏡對不同太陽活動現象的響應。
  8. With x - ray " s erupting generated by solar proton flare, x - ray transmit toward earth with light speed and isn " t effected by magnetic field of earth. it arrive in earth earlier several decades minutes to hours than proton liquid. make use of the difference of time they spend on space spread, we make alarm for solar proton event by physical character of solar x - ray, which is a very valid means

    伴隨太陽質子耀斑產生的x射線爆發，它以光速向地球傳播而且不受地磁場的影響，它比質子流超前幾十分鐘甚至幾十小時到達地球，利用二者在空間傳播的時間差，以太陽x射線某些物理特徵警報太陽質子事件是一種十分有效的手段。
  9. At present we have made great efforts on radiation statistics of proton - flare " s x - ray, especially hard x - ray, and character of hard x - ray in the process of proton accelerating, and we have gotten solar x - ray " s character before proton event and bring forward forecasting method which is actualized and proved in fy - 2 satellite " s alarming system of proton event

    目前我們已經在質子加速過程中的硬x射線特徵、質子耀斑x射線輻射統計（特別是硬x射線特徵）等方面作了系統的工作，已獲得質子事件前兆的太陽x射線特徵，並提出了預報方法，已在fy - 2衛星質子報警系統中加以了實施和驗證。
  10. The space observation in soft x - ray and extreme ultraviolet ( euv ) region is an important portion of the space astronomy and an effective solar observation method developed increasingly. in this thesis we designed a euv multi spectrum space solar telescope ( eut ) based on the requirement of high angular resolution and wide field of view for solar observations ; investigated the transmission performance of eut ; invented a method of eut pointing calibration on the space orbit and solved the high precision pointing calibration problems ; constructed a prototype of 17. 1nm telescope, tested the possibility of eut design, and developed some cutting - edge techniques

    本文根據空間平臺上高解析度對日觀測的需要，設計出一種可以在四個極紫外波段對日同時成像多光譜太陽望遠鏡（ eut ） ；研究了極紫外（ euv ）波段太陽望遠鏡光學傳輸特性；提出了真空紫外波段在軌指向的標定方法，解決了高精度指向標定問題；研製出一臺17 . 1nm望遠鏡的地面樣機，驗證eut設計的可行性，攻克了部分關鍵的技術難關；為進一步的研究工作奠定了基礎。
  11. It is not only the satisfactory substrate used for the epitaxy growth of infrared detector material hgcdte, but also attractive candidates for the manufacture of high quality x - ray or y - ray detectors, photoelectronic modulator, solar cell, and laser windows etc. no matter what the crystal is used as detectors or epitaxy substrate, it is of vital importanteto obtain high quality cdznte crystals with perfect surface

    它不僅是生長紅外探測器材料hgcdte最理想的外延襯底，而且還被廣泛用於制備高性能x射線或射線探測器、光電調制器、太陽能電池和激光窗口等。獲得高性能、高質量的czt晶體是至關重要的。無論是作探測器還是作外延襯底等都要求它的表面質量要非常高，因為表面質量會直接影響到器件的性能。
  12. The xd recorded the biggest solar x - ray flare on record on april 2, 2001

    探測器於2001年4月2日錄得有記錄以來最強大的x射線耀斑。
  13. Such a process can take place in the low mass x - ray binary systems where the mass transfer from the companion to the neutron star can be larger than 0. 5 solar masses. if the neutron star in the low mass x - ray binary accretes the matter, the central densities can reach to a state that strange - matter seeds are formed in the interiors of the star

    在這個系統內，中子星可能會吞噬超過0 . 5個太陽質量的伴星物質，當中子星吸收了這些物質后，中心的密度會增加至足以產生奇異物質種子，這些種子會開始吞噬四周的中子物質，釋放出大量中微子和反中微子，令星體冷卻。
  14. The bastille - day flare of 14 july 2000, a great solar flare with x - ray / ha importance of x5. 7 / b3, was observed around 10 : 24 ut in the noaa 9077 ar at position n22w07. in this flare, very rich interesting radio bursts and fine radio spectral structures were detected, not only in metric wave band, but also in decimetric and microwave band ( 1. 0 - 7. 6 ghz by national astronomical observatories of chinese academy of sciences - naoc )

    2000年7月14日的太陽耀斑爆發? bastille事件，備受國際太陽物理學家關注，著名的sci刊物「 solarphysics 」特出版專輯研討該事件，從光球、色球、日冕、直至日地空間的廣闊空間尺度范圍內，對該事件的觀測資料進行了分析和理論研究。
  15. In this paper, we mainly discuss multilayer mirrors for x - ray solar telescope operating at 17. 1nm wavelength. the diameter of primary mirror for telescope is 130 millimeters and secondary mirror is 66mm. especially, we will engage in controllation of uniformity of period thickness

    本文主要針對工作波長為17 . 1nm的x射線空間望遠鏡中的主鏡與次鏡的膜厚分佈均勻性進行控制，其中主鏡直徑為130mm ，曲率半徑為7 . 5m 。
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