photosphere n.【天文學】光球;光球層。
n. 【天文學】光球;光球層。 “extended photosphere“ 中文翻譯: 延伸光球“stellar photosphere“ 中文翻譯: 恒星光球“photospheric abundance“ 中文翻譯: 光球豐度“photosource of neutron“ 中文翻譯: 光中子源“photospheric activity“ 中文翻譯: 光球活動“photosource“ 中文翻譯: 光源“photospheric eruption“ 中文翻譯: 光球爆發“photosilver“ 中文翻譯: 感光銀“photospheric facula“ 中文翻譯: 光球光斑“photosignal“ 中文翻譯: 光電信號; 光信號“photospheric granulation“ 中文翻譯: 米粒組織“photoshostyle photoshop“ 中文翻譯: 樣式
photostat |
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The two sunspots of a pair have different polarities , one would be a magnetic north and the other is a magnetic south . thus , we believe that there are magnetic field lines joining the two sunspots of a pair . the strong magnetic field locks the gas of the photosphere in places and inhibits the hotter gas below to rise at the sunspots 黑子經常成雙成對出現,每對皆由極性相反的黑子組成,若一個為磁北,另一個必為磁南,由此我們估計每對黑子皆由磁力線所連系,強大的磁場牽制著光球層上的氣體,并阻止了下層較熾熱的氣體上升至黑子范圍,結果黑子比太陽表面其他地方溫度較低。 |
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Sunspots are dark regions on the sun s surface , where their temperatures are lower than the average temperature of the photosphere 6 , 000 degrees celsius , and are presumably associated with the strong magnetic field . the strength of the magnetic fields is thousands times stronger than earth s . such strong magnetic field keeps sunspots at 4 , 500 degree celsius and also serves as a reservoir of energy for explosive events like solar flares 太陽黑子是太陽表面的暗黑區域,溫度較光球層的平均溫度攝氏6 , 000度低,而區域內的磁場比地球的磁場還要高出數千倍,這強大的磁場除了令黑子處于攝氏4 , 500度外,更為爆發性現象如太陽耀斑提供了能量。 |
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Her affection for him was now the breath and life of tess s being ; it enveloped her as a photosphere , irradiated her into forgetfulness of her past sorrows , keeping back the gloomy spectres that would persist in their attempts to touch her - doubt , fear , moodiness , care , shame 她對他的愛現在達到了極點,成了她生命的存在它像一團靈光把她包圍起來,讓她眼花繚亂,忘記了過去的不幸,趕走了那些企圖向她撲來的憂郁的幽靈疑慮恐懼郁悶煩惱羞辱。 |
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The amount of sunspots on the photosphere is periodic with a period of about 11 years . at the beginning of the period , sunspots will appear at higher latitudes i . e . far away from the equator of the sun . then , the number of sunspots will increase and they will appear at lower latitudes 太陽黑子的多寡變化有一個十一年的周期,在周期之始,黑子基本上出現在緯度較高的地方即離太陽赤道較遠,接著太陽黑子數目會不斷增多,并且會向赤道靠攏。 |
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Nothing can be cooler than 0k . the gas below the photosphere has a higher temperature and so will rise up to the photosphere . after releasing its energy , the gas will become cooler and darker 光球層之下的氣體溫度比光球層高,就好像沸騰的水,底層的氣體會向上升,當這些熾熱氣體把能量釋放后,便會變冷變暗,然后沉降回光球層之下,這種對流運動產生了稱為 |
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The density of the gas in the photosphere is just right that below it , the gas is very dense and light cannot directly get through . while above it , the gas is thin enough to allow us seeing through 我們可以看見光球層,原因是它的氣體密度剛剛好,在它之下的氣體密度太大,光線不能通過在它之上的氣體則足夠稀薄,能讓光球層發出的光線順利通過。 |
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Are dark small regions on the sun . their temperature is only 4000k compared to 6000k elsewhere in the photosphere . since they are cooler , less light is produced and they appear as black spots 是太陽的黑暗區域,溫度只有約4000度,由于相對來說它們比光球層其他地方冷,產生的光亦較少,所以看來較暗。 |
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It turns out that zinc , gallium , and copper are very difficult to measure precisely in the solar photosphere so our measurements of the sun may not be quite right 其結果是在太陽光球層中的鋅、鎵、銅恰好是很難測定的,那么我們對太陽的測量方法可能不是很正確。 |
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Her hopes mingled with the sunshine in an ideal photosphere which surrounded her as she bounded along against the soft south wind 迎著溫柔的南風,她一路跳躍著向前走去,她的希望同陽光融合在一起,似乎幻化成了一道環繞著她的光環。 |
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The visible surface of the sun ( the photosphere ) has a granular appearance with a typical dimension of a granule being 1000 kilometers 有形的太陽表面(光球) ,有顆粒狀的外觀與一個典型的維某顆粒被1000公里。 |
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K . we still cannot completely explain why the temperature of the chromosphere and corona can be higher than the photosphere 度。為甚么日冕和色球層的溫度可以比光球層更高,仍是天文學上一個未解之謎。 |
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K . it is much fainter than the photosphere , so we can see it usually only during a total solar eclipse 度。有趣的是,它相對來說比光球層暗,所以通常只能在日全食時才能看見它。 |
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Thus , the photosphere defines the surface of the sun . its temperature is about 6000k 所以,光球層界定了肉眼可見的太陽表面,它的溫度約為絕對溫度6000度。 |
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Above the photosphere is another layer of gas , about 2 , 000km thick , called the 在光球層之上,是一層約為二千公里厚的 |
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There is no sharp break between the photosphere and the outer atmosphere of the sun on one side and the solar interior on the other . 無論在光球與它上面的太陽大氣之間,或是在光球層與它下面的太陽本體之間,都沒有明顯的突變。 |
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A continuous flow of energy is supplied to the photosphere to make good the prodigious losses by radiation . 有一種連續不斷的能流供給光球,以彌補輻射造成的巨大損耗。 |
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The chromosphere is a frothy layer churned up by gases in the photosphere . 色球層在光球層氣體的攪拌下是個多泡層。 |