氣象觀測塔 的英文怎麼說
中文拼音 [qìxiàngguāncètǎ]
氣象觀測塔
英文
weather (instrumentation) tower- 氣 : Ⅰ名詞1 (氣體) gas 2 (空氣) air 3 (氣息) breath 4 (自然界冷熱陰晴等現象) weather 5 (氣味...
- 觀 : 觀名詞1. (道教的廟宇) taoist temple2. (姓氏) a surname
- 測 : 動詞1. (測量) survey; fathom; measure 2. (測度; 推測) conjecture; infer
- 氣象 : 1. (大氣現象) meteorological phenomena2. (氣象學) meteorology3. (情景) atmosphere; scene
- 觀測 : observe; observation; viewing
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Should all automatic observing systems fail, essential meteorological elements will be measured manually on site and reported to amo for onward transmission to air traffic control every half an hour via trunk mobile radio or other available radio communication means such as mobile phones
倘若所有自動觀測系統失靈,必須的氣象資料可用人手量度,再報給機場氣象所,然後每半小時經由集群無線電通話系統或其他無線電通訊渠道例如行動電話,發送給航空交通管制塔。Conventional meteorological equipment such as thermometers, barometers and raingauges are set up in a meteorological enclosure near the air trafficcontrol tower
在航空交通指揮塔附近的氣象觀測園內,設置了溫度計氣壓計及量雨計等常規氣象儀器。From the past research work, it has been known that the main mechanisms of spectral lines broadening in the atmospheres of stars are doppler broadening, spectral lines broadening by rotation and expending, pressure broadening ( stark broadening ), natural broadening, spectral lines broadening in magnetic field, sonic waves and alfv e n waves broadening, etc. but it is not enough to explain the recent observation phenomena by above theories of spectral lines broadening
以往的研究已經判明,在恆星大氣內譜線致寬的主要機制是多普勒致寬、自轉源或膨脹源引起的致寬、壓力致寬(斯塔克致寬) 、自然致寬、磁場引起的加寬、聲波及阿爾文波致寬等。然而,已有的譜線致寬理論不足以解釋最近的一些觀測現象,仍存在觀測值與理論值之間的差異。
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