solar flare 中文意思是什麼

solar flare 解釋
耀斑。

  • 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...
  • flare : n 1 搖曳的火焰，閃爍的火光，閃光（信號）；曳光管；照明彈；（太陽的）耀斑，色球爆發。2 （突然）燒...
  1. Theoretical researches on solar activity, solar flare and cme were involved in many fields of foundational physics such as plasma astrophysics, magnetohydrodynamics ( mhd ) and so on. the forecast of solar activity, a main branch of space weather, was becoming more and more significant for preventing space disaster and for many aspects of space science

    探索太陽活動的規律、太陽耀斑及其伴隨cme的先兆、觸發過程及能量傳播機制等等，從理論上推動了等離子體天體物理、磁流體力學等諸多基礎理論的發展，有著重要的理論意義；而對太陽活動的預報，是國際前沿科學?空間天氣學的重要組成部分，對避免空間災害、為航空航天科學提供服務等方面，具有重大的實際應用價值。
  2. Solar flare is a violent solar activity

    太陽耀斑是一種劇烈的太陽活動現象。
  3. What is a " solar flare "

    什麼是太陽耀斑？
  4. Origin of solar flare

    太陽耀斑的由來
  5. One possibility is that the blast was like an ultra - powerful solar flare

    一種可能的原因是這種爆炸很像有超級能量的太陽耀斑。
  6. Impulsive solar flare

    脈沖太陽耀斑
  7. The most powerful solar flare as observed by satellite instrumentation is recorded

    2003年的今天，由衛星儀器觀測到的最強的一次太陽耀斑被記錄。
  8. During its lifetime, the xd recorded a total of 664 triggers. the research team identified and recorded lightcurves of near one hundred solar flare events data taken during half of the orbit when the shenzhou - ii orbiter faces the sun and 30 candidates of gamma ray bursts. many of these observations were verified by similar results taken by other orbiting satellites

    探測器在運作期間，共錄得664次撞擊，研究小組由此識別並記錄了近百次太陽耀斑的變光曲線當神舟二號在軌道上面向太陽時和約30次伽瑪射線爆發，大部分觀測結果跟其他人造衛星所測得的類似。
  9. The advantages of the new method of calculating the vtec including : ( 1 ) because the instrumental bias is considered, the vtec ' s change going with time is closer to their real change. ( 2 ) with the precision of calculated the vtec improved, the vtec can reflect the increase of the vtec resulted from the solar flare

    新的求解vtec的方法具有以下優點：考慮了gps衛星和接收機的儀器偏差的影響，計算的電子總量隨時間的變化更接近電離層的實際情況；提高了求解電子總量的精度，計算出的vtec值更能反映耀斑引起的電子總量的增加情況。
  10. According to the present status of studying the solar flare using gps, a new algorithm of processing gps data studying the solar flare is brought forward : after the instrumental bias has been determined, with the data of dual - frequency gps code and phase and navigation message, the vtec at the satellite ' s epp can be worked out

    根據現在研究太陽耀斑的實際情況，提出了利用gps研究太陽耀斑的數據處理方法：利用雙頻觀測值確定出儀器偏差后，再利用碼和相位觀測值，結合導航電文就可以求出電離層交叉點的沿天頂方向上的電子總量vtec值。
  11. 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。
  12. An exception to the above pattern occurs during solar flare activity, which takes place on an occasional basis during periods of high solar activity

    例外情況然而亦有，這就是在太陽活躍期偶發的閃焰爆發。
  13. In the present thesis, we summarized the current observation means, taxonomy and theoretic study of the solar flare. then, we introduce our research work of the well - known solar flare of april 27, 1981

    本文綜述了太陽耀斑的觀測和理論研究現狀，詳細介紹本人在攻讀碩士學位期間針對1981年4月27日在太陽西邊緣爆發的一個典型的耀斑后環所作分析的研究工作。
  14. Solar flare a sudden eruption of hydrogen gas on the surface of the sun, usually associated with sunspots and accompanied by a burst of ultraviolet radiation that is often followed by a magnetic disturbance

    太陽耀斑，太陽表面氫氣的突然爆發，經常和太陽黑子有關並伴有紫外線輻射的爆發，從而導致磁干擾。
  15. Operated by the united states is capable of monitoring solar flare events. an explosive development of solar flare on 20 january 2005 can be seen below

    下圖顯示發生於二零零五年一月二十日的太陽耀斑爆發過程。
  16. 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。
  17. The method of calculating the change rate of the vtec using phase data is introduced. with the help of this efficient method, the solar flare is analyzed in this thesis

    介紹了利用載波相位觀測值求解電子總量變化率的方法，並利用這種方法的計算結果對耀斑進行了分析。
  18. The advantages and disadvantages of this method with calculating vtec are compared. the results show that the effects of even smaller class solar flare can be reflected using this method

    比較了這種數據處理方法和求解vtec方法各自的優缺點，指出利用這種方法可以監測到級別更小的耀斑爆發。
  19. The theory and method of monitoring the solar flare using dual - frequency gps receiver observation data are discussed in details. the main work contains : the factors influencing the vertical total electron contents ( vtec ) of the ionosphere are summarized, and some knowledge about the solar flare is introduced. besides these, the effects of the solar flare on the ionosphere and of the flare burst on the gps measurements are clarified

    本文探討了利用雙頻gps接收機的觀測值監測太陽耀斑的有關理論和方法，主要工作包括：總結了影響電離層電子總量的因素，介紹了太陽耀斑的有關知識，闡明了太陽耀斑對電離層的影響及耀斑爆發對gps測量的影響。
  20. Furthermore the " microflare theory " tried to discuss and find the elementary flares in small space and time scale which might form and trigger the whole solar flare. the detection of radio fine structures showed many observational evidences of " microflare ". the observations and theoretical researches on radio fine structure have been developed fast recently and played an important role in solar radio astrophysics

    著名的「微耀斑理論」 ，試圖從較小的時間、空間尺度范圍探究太陽耀斑形成和觸發的基本單元，而射電精細結構是微耀斑理論的重要觀測基礎，對射電精細結構的觀測和理論研究已成為太陽射電天文學中快速發展的領域，對揭示太陽活動源區的物理本質具有重要的意義。
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