A solar tower, in the context of astronomy, is a structure used to support equipment for studying the Sun, and is typically part of solar telescope designs. Generically, the term solar tower has many more uses especially for a type of power production using Earth's Sun. Solar tower observatories are also called vacuum tower telescopes. The term has also been used to refer to other structures used for experimental purposes, such as the Solar Tower Atmospheric Cherenkov Effect Experiment (STACEE), which is being used to study Cherenkov radiation, and the Weizmann Institute solar power tower.
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| - Torre solare (it)
- Solar tower (astronomy) (en)
- 太阳塔 (zh)
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| - 太陽塔（英語：solar tower），又稱為塔式太陽望遠鏡，是專門用於觀測太陽的天文設備。 太陽塔的高度通常在20米以上，目的在避免受到地面被太陽能加熱產生的熱輻射造成的大氣擾動，塔的頂部安置觀測太陽的定天鏡，將太陽光垂直導入正下方安置的成像系統和觀測儀器。傳統的用於觀測的天文臺不需要安置在地面高度以上的位置，因為在晚上進行觀測時，地面的輻射已經降至最小值了。 在1904年，威爾遜山天文台建造了水平式的雪太陽觀測台，很快的就發現熱輻射會妨礙觀測的進行。幾乎就在雪觀測台開始運作的同時，60尺高的太陽塔就開始規劃，在1908年完成，是世界上最早建成的太陽塔。緊接著，150尺高的太陽塔也在1912年完成。 60尺的太陽塔現在仍用於日震學的研究工作，而150尺的高塔仍活躍於加州大學的太陽週期計畫中。 這個項目的觀測設備也用於其他的研究計畫，例如，太陽塔的契忍可夫效應實驗（），就是用來研究契忍可夫輻射；還有魏茨曼科學研究學院的。 (zh)
- A solar tower, in the context of astronomy, is a structure used to support equipment for studying the Sun, and is typically part of solar telescope designs. Generically, the term solar tower has many more uses especially for a type of power production using Earth's Sun. Solar tower observatories are also called vacuum tower telescopes. The term has also been used to refer to other structures used for experimental purposes, such as the Solar Tower Atmospheric Cherenkov Effect Experiment (STACEE), which is being used to study Cherenkov radiation, and the Weizmann Institute solar power tower. (en)
- Una torre solare è una struttura usata a supporto della strumentazione per lo studio del Sole. La radiazione solare viene raccolta alla sommità da specchi (generalmente due, l'eliostato e il celostato) che convogliano il fascio di luce verso la base della torre, dove sono posti strumenti in grado di studiarla, che comprendono il telescopio solare e lo spettroeliografo. (it)
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| - A solar tower, in the context of astronomy, is a structure used to support equipment for studying the Sun, and is typically part of solar telescope designs. Generically, the term solar tower has many more uses especially for a type of power production using Earth's Sun. Solar tower observatories are also called vacuum tower telescopes. Solar towers are used to raise the observation equipment above atmospheric turbulence caused by solar heating of the ground and the radiation of the heat into the atmosphere. Traditional observatories do not have to be placed high above ground level, as they do most of their observation at night, when ground radiation is at a minimum. The horizontal Snow solar observatory was built on Mount Wilson in 1904. It was soon found that heat radiation was disrupting observations. Almost as soon as the Snow Observatory opened, plans were started for a 60-foot-tall (18 m) tower that opened in 1908 followed by a 150-foot (46 m) tower in 1912. The 60-foot (18 m) tower is currently used to study helioseismology, while the 150-foot (46 m) tower is active in UCLA's Solar Cycle Program. The term has also been used to refer to other structures used for experimental purposes, such as the Solar Tower Atmospheric Cherenkov Effect Experiment (STACEE), which is being used to study Cherenkov radiation, and the Weizmann Institute solar power tower. (en)
- Una torre solare è una struttura usata a supporto della strumentazione per lo studio del Sole. La radiazione solare viene raccolta alla sommità da specchi (generalmente due, l'eliostato e il celostato) che convogliano il fascio di luce verso la base della torre, dove sono posti strumenti in grado di studiarla, che comprendono il telescopio solare e lo spettroeliografo. Esempi di tali strutture sono la torre solare dell'Osservatorio di Arcetri, parte dell'INAF, la torre Einstein di Potsdam costruita nel 1920, e le due torri da 46 e 18 metri dell'Osservatorio di Monte Wilson. La torre da 18 metri è usata per lo studio dell'eliosismologia. Il termine è stato usato anche per riferirsi ad altre strutture usate per scopi sperimentali, come la "Solar Tower Atmospheric Cherenkov Effect Experiment" (STACEE) di Albuquerque nel Nuovo Messico, che viene impiegata per lo studio della radiazione di Čerenkov, e la centrale solare a torre dell'Istituto Weizmann a Rehovot in Israele. (it)
- 太陽塔（英語：solar tower），又稱為塔式太陽望遠鏡，是專門用於觀測太陽的天文設備。 太陽塔的高度通常在20米以上，目的在避免受到地面被太陽能加熱產生的熱輻射造成的大氣擾動，塔的頂部安置觀測太陽的定天鏡，將太陽光垂直導入正下方安置的成像系統和觀測儀器。傳統的用於觀測的天文臺不需要安置在地面高度以上的位置，因為在晚上進行觀測時，地面的輻射已經降至最小值了。 在1904年，威爾遜山天文台建造了水平式的雪太陽觀測台，很快的就發現熱輻射會妨礙觀測的進行。幾乎就在雪觀測台開始運作的同時，60尺高的太陽塔就開始規劃，在1908年完成，是世界上最早建成的太陽塔。緊接著，150尺高的太陽塔也在1912年完成。 60尺的太陽塔現在仍用於日震學的研究工作，而150尺的高塔仍活躍於加州大學的太陽週期計畫中。 這個項目的觀測設備也用於其他的研究計畫，例如，太陽塔的契忍可夫效應實驗（），就是用來研究契忍可夫輻射；還有魏茨曼科學研究學院的。 (zh)
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