solar stream 中文意思是什麼
solar stream
解釋
太陽粒子流-
A continuous stream of charged particles, called the solar wind, impinges on the earth's magnetosphere.
稱作太陽風的連續帶電子流撞擊在地球的磁層上。 -
The engine, which uses electricity from the craft ' s solar panels to produce a stream of charged particles called ions, generates only small amounts of thrust but only needed 80 kilograms of xenon fuel
離子引擎將航天器太陽能面板所採集的太陽能轉化為電能，再生成帶電的離子流。太陽能離子引擎所產生的推動力並不大，但所需要的氙氣燃料也很少，只有80千克。 -
The planet and its neighbours are bathed in the solar wind, a stream of charged particles ejected from the upper atmosphere of the sun
地球與其鄰近的行星都處于太陽風（從太陽上層大氣層發射出的帶電粒子流）的勢力范圍之內。 -
It is important to find a precise and fast algorithm for solar radiative transfer in the atmosphere. in this paper, we present, based on stamnes " s discrete - ordinate - method, an analytical four - stream approximation algorithm
我們在knutstamnes的離散縱標法（ 1988 ）的基礎之上，提出了一種輻射傳輸四流近似計算方法，並且該演算法可以得到一個解析解。 -
Stardust collected these particles between february and may 2000, and again between august and december 2002, while passing through a stream of dust that flows into our solar system from interstellar space
「星塵」在2000年二月和五月以及2002年8月至12月穿越一股流入太陽系的星際氣體流時收集這些微粒。 -
A two stream model has been used to calculate the variation of optical depth and their effects to ultraviolet radiation of each extinction material. with the model, the relation among season, solar zenith angle and ultraviolet radiation has been discussed, and the variation of ultraviolet radiation under different clouds has also been studied. the comparative research of ultraviolet radiation among kunming, beijing and other abroad area at the same latitude has also been done
在已建立的計算昆明紫外輻射兩流模式改進的基礎上，進一步計算並討論了： 1各種消光物質的光學厚度變化規律及其對紫外輻射的影響2季節變化及太陽天頂角變化與紫外輻射的關系3不同雲的光學厚度下紫外輻射的變化4昆明與北京兩地模式計算結果比較，以及與國外相近緯度觀測結果進行了比較。
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