solar observation 中文意思是什麼

solar observation 解釋
太陽觀測
  • 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...
  • observation : n 1 觀察，注意；觀察力；?望。2 觀測，實測；【航海】測天；【軍事】觀測，監視，偵察。3 （觀察得的）...
  1. Space environment threaten orbited spacecraft " s safe functioning and astronaut " s health, influence greatly communication depended on based - space way, airmanship orientation, military detection, aim identification, weather observation and source exploration and so on by all sorts of function ( magnetic storm, solar proton event and so on )

    空間環境通過各種效應（如磁暴、太陽質子事件等）對在軌航天器的安全運行及航天員的健康構成了嚴重的威脅，對依賴于天基手段的通信、導航定位、軍事偵察、目標識別、氣象觀測、資源勘探等等均有重要影響。
  2. Abstract : according to the observation of the number concentration spectrum and the mass concentration of atmospheric aerosol, tsp and its particle size distribution, micrometeorology, and the solar spectroscopic radiation, even the neutron activation treatment of sand dust samples in helan mountainous area, the formation law of sandstrom, dust and sand blowing weather and the characteristics of climatic variation in this area and the influence of helan mountain are counted and analysed

    文摘:利用賀蘭山地區沙塵暴歷史資料和綜合觀測資料，對大氣背景、浮塵、揚沙和沙塵暴發生期間的大氣氣溶膠數濃度譜、質量譜、大氣總懸浮顆粒（ tsp ）及粒徑分佈、微氣象、分光日射觀測以及沙塵樣品進行中子活化處理，分析了該地區浮塵、揚沙和沙塵暴形成規律，氣候變化特徵和賀蘭山的影響。
  3. According to the observation of the number concentration spectrum and the mass concentration of atmospheric aerosol, tsp and its particle size distribution, micrometeorology, and the solar spectroscopic radiation, even the neutron activation treatment of sand dust samples in helan mountainous area, the formation law of sandstrom, dust and sand blowing weather and the characteristics of climatic variation in this area and the influence of helan mountain are counted and analysed

    利用賀蘭山地區沙塵暴歷史資料和綜合觀測資料，對大氣背景、浮塵、揚沙和沙塵暴發生期間的大氣氣溶膠數濃度譜、質量譜、大氣總懸浮顆粒（ tsp ）及粒徑分佈、微氣象、分光日射觀測以及沙塵樣品進行中子活化處理，分析了該地區浮塵、揚沙和沙塵暴形成規律，氣候變化特徵和賀蘭山的影響。
  4. In chapter one, we make a review of particle acceleration theory and the use in solar corona. in chapter two, first we get the spectrum of synchrotron radiation then obtain the electron energy spectrum. in last chapter, we select the typical solar active region parameter to compare our result to the observation and discuss the acceleration mechanism

    本文第一章對粒子加速理論以及目前各種加速理論在太陽日冕中的應用作了介紹；第二章通過理論計算得到同步加速輻射譜以及電子能譜；第三章選取太陽日冕中典型參數，對同步加速輻射加速日冕快電子作了簡單討論。
  5. In contrast with the measurement of backscattered ultraviolet solar radiation onboard satellites, ir radiance measurements in 9. 6m spectral channel at various instruments onboard meteorological / environmental satellites allow ozone estimates during both day and night. in this paper, we use ir radiance measurements within 9. 6 im spectral channels from moderate resolution spectral radiometer ( modis ) and advanced tiros operational vertical sounder ( atovs ) to retrieve total column ozone based on the operational retrieval system of national satellite meteorological center. for validating retrieval results, both ground based observation and total ozone mapping spectrometers ( toms ) ozone measurements are used and atovs retrieval results are corrected after the validation

    本文利用美國noaa衛星上的先進的大氣垂直探測器業務系統（ atovs ）儀器和地球觀測系統衛星（ eos ）上的中解析度成像光譜儀（ modis ）上的9 . 6 m臭氧探測通道的輻射測值，在國家衛星氣象中心業務反演軟體系統基礎上，反演出了兩種儀器探測的大氣臭氧總量，並且利用中國五個常規臭氧觀測站的資料和美國研製的臭氧總量測繪光譜儀（ toms ）反演的臭氧資料對兩種反演結果進行驗證分析，對atovs反演結果進行了訂正。
  6. Join the solar eclipse observation activities organized by the hong kong space museum or local astronomical organizations

    一參加太空館或各大天文學會的觀測日食活動
  7. The simulations of ground temperature and earth absorbed net solar radiation are lower than the observation. sensible heat and latent heat are also lower than the observation

    由於模式模擬的地溫偏低，凈的短波輻射偏小，則模擬的感熱和潛熱值偏小。
  8. Based on the data of surface ozone, carbon dioxide, solar radiation, total ozone, climate observation as well as the boundary layer meteorological elements in 1994. 11 - 2002. 7, the characteristics of surface ozone and carbon dioxide are analyzed over waliguan by statistic method

    本文利用瓦里關1994年11月2002年7月地面臭氧、二氧化碳、太陽輻射、臭氧總量以及邊界層氣象要素和氣候觀測資料，通過統計分析的方法，對瓦里關地區二氧化碳和地面臭氧變化特徵進行了初步的分析。
  9. 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。
  10. Observation of meteors throws light on our understanding of the motion of the celestial bodies in our solar system, physical properties of the earths upper atmosphere and the spatial distribution of meteoroids which helps choosing safe and proper trajectories for launch vehicles such as artificial satellites

    觀測研究流星對研究太陽系天體的運動地球高空大氣物理性質了解流星體分佈這項資料對選擇航天器如人造衛星的運行軌跡十分重要等都有重要的意義。
  11. The main research contents of the operational design include : working out the in - orbit experiment scheme and optimizing the in - orbit control and observation scheme for solar x - euv imaging telescope ; analyzing the requirements to the mounting platform of telescope ; implementing the rudimental mechanical, electronic, thermal interface design

    在軌運行方案的主要研究內容包括：針對靜止軌道衛星應用平臺，制訂和優化瞭望遠鏡在軌試驗方案；完成望遠鏡的機電熱初步介面設計。
  12. 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。
  13. In this paper, the solar and land - atmosphere radiation rates are calculated by modtran3 model and satellite observation as well as surface data, solar direct irradiance infrared irradiance solar heating rate and infrared cooling rate were calculated from 43 samples of sunshine day and 5 samples of cloudy day 3 samples of rainy day of different latitudes in 12 stations. the paper analyzed solar heating rate and infrared cooling rate in sunshine day, the factors such as zenith angle, water vapor and latitude were found out correlating with solar heating rate and infrared cooling rate. solar heating rate and infrared cooling rate change on the same day and at the same station

    在對晴空大氣的計算中，本文對太陽的直接輻射與地氣系統的紅外輻射狀況進行了分析，並討論在不同的大氣狀況下太陽加熱率和紅外冷卻率的情況，找出與太陽加熱率和紅外冷卻率變化相關較大的因子?太陽天頂角和水汽條件、緯度；本文還進一步分析了不同緯度樣本的太陽加熱率與紅外冷卻率日變化及有雲、有雨情況下太陽加熱率和紅外冷卻率的變化情況：另外，文中通過改變二氧化碳在大氣中含量的方法，討論了它對太陽加熱率與紅外冷卻率的影響。
  14. In addition, china has participated in multilateral cooperative projects, such as " committee on earth observation satellites, " " world weather monitoring, " " un decade of disaster mitigation, " and " international solar - terrestrial physics.

    中國還參加了諸如「國際對地觀測委員會」 、 「世界天氣監測」 、 「聯合國減災十年」 、 「國際日地能量計劃」等多邊合作項目。
  15. In addition, china has participated in multilateral cooperative projects, such as " committee on earth observation satellites, " " world weather monitoring, " " un decade of disaster mitigation, " and " programme on international solar - terrestrial energy.

    中國還參加了諸如"國際對地觀測委員會" 、 "世界天氣監測" 、 "聯合國減災十年" 、 "國際日地能量計劃"等多邊合作項目。
  16. In this paper, we introduce a recently finished image - processing system for the high - resolution observation of solar magnetic field in the huairou solar observing station ( hsos )

    摘要文章介紹了懷柔太陽觀測基地最近完成的一套實時高分辨太陽磁場觀測系統。
  17. By the weather data of typical year from meteorological observation, the building facing correction factors of heating load of 27 cities in china are listed. not only the effect of direct solar radiation on the building facing correction factor, but also that of diffuse solar radiation is considered. this paper also analysis the effect of different building facing correction factors on the calculation of heating load

    以各氣象臺站實測典型年氣象資料為基礎，綜合考慮了直射輻射和散射輻射兩種情況，給出了全國27個城鎮的各朝向修正系數，並對採用不同修正系數對房間負荷計算的影響進行了對比分析。
  18. The correlation tracking ( ct ) method is used in this system to improve the spatial resolution, and the algorithm of ct is optimized to improve the temporal resolution for the purpose of routine observation of solar magnetic field

    系統採用局部相關跟蹤演算法來提高磁場觀測數據的空間解析度，同時對相關跟蹤演算法的實現程序進行了優化以滿足常規太陽磁場觀測的要求。
  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. The past twenty years saw the significant progress in astronomical observation when new instruments have come online to explore the distant universe across the electromagnetic spectrum and spacecraft have flown to probe the nearby members of the solar system, bringing a new understanding of our universe

    過去二十年，天文探測的發展一日千里。由射電波至伽瑪射線等不同波段的儀器相繼啟用，而各類型的太陽系探測器也帶來豐富的成果，使人類對宇宙有了新的認識。
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