solar particle 中文意思是什麼
solar particle
解釋
太陽粒子-
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。 -
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。 -
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。 -
Solar - ray photocatalysis characteristics of nano - titania particle doped with gadolinia made in different ways
2納米粒子的自然光催化活性的研究 -
Solar flares and energetic particle events also complicate matters by interrupting satellite and shortwave radio communications
太陽耀斑和高能粒子則會干擾人造衛星及短波廣播通訊系統運作。 -
The varieties, amount and particle size of reflective materials are the key factor for control of reflecting solar heat of coatings
反射材料的種類、數量和粒徑是決定塗層太陽熱反射能力的關鍵因素。 -
This kind of new particle is the neutrino, and scientists believe they exist in large number in the universe. take the solar neutrinos, for example, every second about one million billions 10
科學家相信，中微子在宇宙中的數目相當多，就以太陽製造的中微子為例，它們到達地球的數目確實是天文數字：每秒約有一百萬億10 -
The event gave us a good opportunity to discuss the processes of magnetic change, energy release and particle acceleration in the corona during the preflare, especially using decimetric and microwave fine structure data. in this thesis, we report the solar type iv bursts and its associated fiber fine structures recorded on 14 july 2000
中國國家天文臺懷柔觀測站的寬帶頻譜射電望遠鏡，觀測到了來自內日冕區的射電爆發及其精細結構，攜帶著耀斑爆發初期磁場變化、能量釋放的豐富信息，很有必要對其進行深入的理論分析和計算。 -
Radiation of solar particle and nontidal acceleration of earth
太陽粒子輻射與地球自轉非潮汐加速度 -
The space energetic particle environment inducing seu includes galactic cosmic ray, solar cosmic ray and high - energy trapped protons and heavy ions. these particles have enough energy and can deposit energy and generate charge in the sensitive volume ( sv ) of device
這些粒子有足夠的能量，能在器件的靈敏區中沉積足夠的能量和產生足夠的電荷，當沉積的電荷超過臨界電荷時，電路就產生了翻轉，即單粒子翻轉發生。 -
Was launched in 1997 by the united states. it is capable of measuring the composition of charged particle from the sun and the interplanetary magnetic field. it gives us important information on the materials released during solar events
於一九九七年由美國發射，它能分析從太陽釋放出來帶電荷粒子的物質組合及行星間的磁場，為我們提供太陽活動事件中釋出物質的重要資料。
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