S - solar wind 中文

solar wind 太陽風，日射微粒流。

太陽風，日射微粒流。 “solar“ 中文翻譯： adj. 太陽的，根據太陽運行測量的；因太陽作用產生的。 ...“wind“ 中文翻譯： wind3 vt. (wound , win ...“high-speed solar wind“ 中文翻譯：高速太陽風“interplanetary solar wind“ 中文翻譯：行星際太陽風“polar solar wind“ 中文翻譯：極區太陽風“quiet-time solar wind“ 中文翻譯：寧靜太陽風“scavenging solar wind“ 中文翻譯：凈化太陽風“solar polar wind“ 中文翻譯：極區太陽風“solar wind boundary“ 中文翻譯：太陽風邊界“solar wind dynamic pressure“ 中文翻譯：太陽風動壓“solar wind instrument“ 中文翻譯：太陽風測量儀器“solar wind interaction“ 中文翻譯：太陽風相互作用“solar wind power generator“ 中文翻譯：太陽能-風能發電裝置“solar wind properties“ 中文翻譯：太陽風性質“solar wind radial variation“ 中文翻譯：太陽風徑向變化“solar wind scavenging“ 中文翻譯：太陽風凈化“solar wind termination“ 中文翻譯：太陽風終端“solar wind geomagnetic field boundary“ 中文翻譯：太陽風地磁場邊界“solar“ 中文翻譯： 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 spot 太陽黑點。 solar light 日光。 solar energy 太陽能。 a solar battery 太陽能電池。 solar heat 太陽熱。 “by the wind“ 中文翻譯：頂風航行; 逆戧; 迎風航駛“in the wind“ 中文翻譯：乘著風; 居上風；頂風；上風船; 向上風航行; 在風中我只是一個英語專業的學生而已，過獎了。; 在進行“into the wind“ 中文翻譯：迎風“into wind“ 中文翻譯：迎風的“on a wind“ 中文翻譯：幾乎頂著風; 迎風航駛迎風航駛“on the wind“ 中文翻譯：幾乎頂風; 前舷風; 迎風, 在風中傳播; 迎風航駛迎風航駛

solar year
Solar wind , which consists mainly of protons and electrons flying away from the sun . at times of strong solar wind , we might see 的源頭，太陽風主要是飛離太陽的質子和電子，當太陽風強勁的時候，在地球兩極有可能看見
At the heart of the study of space weather is a question : how do changes in the solar wind affect conditions in the space surrounding the earth 太空氣象研究的中心課題是：太陽風的變化是如何影響地球周遭太空的？
Like a boat trying to cut through the ocean waves , the induced magnetic fields pile up where the solar wind meets venus ' s ionosphere 就像試圖穿越海浪的船，誘發的磁場積蓄在太陽風與金星的電離層的交匯處。
The sun emits solar wind ? plasma , containing electrically charged particles ? which travels out into space at fantastic speeds 太陽會發射出太陽風? ?一種帶電粒子流，它會以極快的速度奔入太空。
Explosions and solar storms on the surface of the sun send charged particles known as solar winds hurtling towards earth 太陽表面的爆炸和太陽風暴，把帶電粒子（即所謂的太陽風）猛烈射向地球。
Explosio and solar storms on the surface of the sun send charged particles known as solar winds hurtling towards earth 太陽表面的爆炸和太陽風暴，把帶電粒子（即所謂的太陽風）猛烈射向地球。
Auroras are most commonly visible at high latitudes . they are associated with geomagnetic activity brought about by solar wind 極光通常在高緯度的地區出現，它們與太陽風引致的地磁活動有關。
The observatory , in a cart called “ solar wind “ , took the gold award in the advance team category 在蕓蕓參賽隊伍中，天文臺憑著戰車太陽風出賽，脫穎而出，勇奪太陽慈善大獎高級組金獎。
The solar wind fluctuates in strength , but is prevented from entering both when it is strong and when it is weak 雖然太陽風的強度是波動的，電離層仍可以在太陽風強有力的時候阻止它穿過。
The observatory , in a cart called “ solar wind “ , took the gold award in the advance team category 在蕓蕓參賽隊伍中，天文臺憑著戰車太陽風出賽，脫穎而出，勇奪太陽慈善大獎高級組金獎。
It was the first time hko joined such activity . hko won the charity gold award with its cart - the “ solar wind “ 天文臺憑著戰車太陽風出賽，脫穎而出，勇奪太陽慈善大獎高級組金獎。
A geomagnetic storm occurs when a violent solar wind hits the earth and severely distorts the earth s magnetic field 地磁暴起因是由于猛烈太陽風沖擊地球，使地球磁場急速變形而造成的。
The solar wind has its own magnetic field , which travels with the outflowing plasma into interplanetary space 太陽風有它自己的磁場，這個磁場會隨著外流的太陽風電漿一起流入星際空間。
But in the magnetosphere , weather results from the interaction between the earth ' s magnetic field and the solar wind 但在磁層里，太空天氣卻是由地球磁場和太陽風的交互作用所造成。
The chapter 1 is about the basic knowledge about the coronal hole , the solar wind and the recurrent geomagnetic strom 以單個冕洞為研究對象，分析了該冕洞及其引發的地磁暴特征。
Are much more violent eruptions . they will emit strong x - ray , ultraviolet , visible light and solar wind 則是更猛烈的爆發，會放射出強烈的x射線紫外線可見光及太陽風。
This energy involves tons of charged particles , hurled our way in the so - called solar wind 該能量包括成千上萬噸帶電粒子，猛烈沖擊我們這里，這就是所謂的太陽風暴。
Study of the solar wind particles will help our understanding of the origin and evolution of the solar system 研究太陽風的粒子能讓我們了解太陽系的誕生及演變。
The genesis spacecraft was launched in 2001 to collect the solar wind particles 創始號（ genesis ）太空船于二零零一年升空，其任務是采集太陽風粒子樣本。

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solar wind

solar wind 太陽風，日射微粒流。

solar year

Solar wind , which consists mainly of protons and electrons flying away from the sun . at times of strong solar wind , we might see 的源頭，太陽風主要是飛離太陽的質子和電子，當太陽風強勁的時候，在地球兩極有可能看見

At the heart of the study of space weather is a question : how do changes in the solar wind affect conditions in the space surrounding the earth 太空氣象研究的中心課題是：太陽風的變化是如何影響地球周遭太空的？

Like a boat trying to cut through the ocean waves , the induced magnetic fields pile up where the solar wind meets venus ' s ionosphere 就像試圖穿越海浪的船，誘發的磁場積蓄在太陽風與金星的電離層的交匯處。

The sun emits solar wind ? plasma , containing electrically charged particles ? which travels out into space at fantastic speeds 太陽會發射出太陽風? ?一種帶電粒子流，它會以極快的速度奔入太空。

Explosions and solar storms on the surface of the sun send charged particles known as solar winds hurtling towards earth 太陽表面的爆炸和太陽風暴，把帶電粒子（即所謂的太陽風）猛烈射向地球。

Explosio and solar storms on the surface of the sun send charged particles known as solar winds hurtling towards earth 太陽表面的爆炸和太陽風暴，把帶電粒子（即所謂的太陽風）猛烈射向地球。

Auroras are most commonly visible at high latitudes . they are associated with geomagnetic activity brought about by solar wind 極光通常在高緯度的地區出現，它們與太陽風引致的地磁活動有關。

The observatory , in a cart called “ solar wind “ , took the gold award in the advance team category 在蕓蕓參賽隊伍中，天文臺憑著戰車太陽風出賽，脫穎而出，勇奪太陽慈善大獎高級組金獎。

The solar wind fluctuates in strength , but is prevented from entering both when it is strong and when it is weak 雖然太陽風的強度是波動的，電離層仍可以在太陽風強有力的時候阻止它穿過。

The observatory , in a cart called “ solar wind “ , took the gold award in the advance team category 在蕓蕓參賽隊伍中，天文臺憑著戰車太陽風出賽，脫穎而出，勇奪太陽慈善大獎高級組金獎。

It was the first time hko joined such activity . hko won the charity gold award with its cart - the “ solar wind “ 天文臺憑著戰車太陽風出賽，脫穎而出，勇奪太陽慈善大獎高級組金獎。

A geomagnetic storm occurs when a violent solar wind hits the earth and severely distorts the earth s magnetic field 地磁暴起因是由于猛烈太陽風沖擊地球，使地球磁場急速變形而造成的。

The solar wind has its own magnetic field , which travels with the outflowing plasma into interplanetary space 太陽風有它自己的磁場，這個磁場會隨著外流的太陽風電漿一起流入星際空間。

But in the magnetosphere , weather results from the interaction between the earth ' s magnetic field and the solar wind 但在磁層里，太空天氣卻是由地球磁場和太陽風的交互作用所造成。

The chapter 1 is about the basic knowledge about the coronal hole , the solar wind and the recurrent geomagnetic strom 以單個冕洞為研究對象，分析了該冕洞及其引發的地磁暴特征。

Are much more violent eruptions . they will emit strong x - ray , ultraviolet , visible light and solar wind 則是更猛烈的爆發，會放射出強烈的x射線紫外線可見光及太陽風。

This energy involves tons of charged particles , hurled our way in the so - called solar wind 該能量包括成千上萬噸帶電粒子，猛烈沖擊我們這里，這就是所謂的太陽風暴。

Study of the solar wind particles will help our understanding of the origin and evolution of the solar system 研究太陽風的粒子能讓我們了解太陽系的誕生及演變。

The genesis spacecraft was launched in 2001 to collect the solar wind particles 創始號（ genesis ）太空船于二零零一年升空，其任務是采集太陽風粒子樣本。