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哈尔滨工业大学 可调谐激光技术国家级重点实验室, 黑龙江 哈尔滨 150001
[ "马晶(1956-),男,教授,博士生导师,现为空间光通信技术研究中心主任,可调谐激光技术国家级重点实验室副主任,卫星激光通信技术国防重点学科实验室副主任,主要研究方向为卫星光通信、激光干涉计量、光学信息处理和激光全息。E-mail:majing@hit.edu.cn" ]
朱福南(1991-),女,硕士研究生,2014年于哈尔滨工业大学获得学士学位,主要研究方向为卫星光通信。E-mail:zjjxzfn@sina.com E-mail:zjjxzfn@sina.com
收稿日期:2016-04-14,
录用日期:2016-5-30,
纸质出版日期:2016-08-25
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马晶, 朱福南, 周彦平, 等. 星地两用光学表面污染检测装置[J]. Editorial Office of Optics and Precision Engineeri, 2016,24(8):1878-1883.
Jing MA, Fu-nan ZHU, Yan-ping ZHOU, et al. Detection device of optical surface pollution for satellite and ground[J]. Optics and precision engineering, 2016, 24(8): 1878-1883.
马晶, 朱福南, 周彦平, 等. 星地两用光学表面污染检测装置[J]. Editorial Office of Optics and Precision Engineeri, 2016,24(8):1878-1883. DOI: 10.3788/OPE.20162408.1878.
Jing MA, Fu-nan ZHU, Yan-ping ZHOU, et al. Detection device of optical surface pollution for satellite and ground[J]. Optics and precision engineering, 2016, 24(8): 1878-1883. DOI: 10.3788/OPE.20162408.1878.
针对光通信终端的光学表面污染,研制了10 MHz镀铝石英晶体微天平(QCM),用于实时检测真空试验中的污染量以保证光通信的可靠性。该装置通过引入参考晶体消除环境因素的影响,并降低对其控温精度的要求,其理论质量灵敏度可达10
-9
g/cm
2
。经过绝对标定实验后,其实际质量灵敏度为10
-8
g/cm
2
,满足应用需求,且成本低,实用性好,可用于星上或地面污染检测。文中依据不同的污染源工作温度,分别在32 ℃高温恒温段,32 ℃~-27 ℃降温段,低温保持段及-2 ℃~32 ℃升温段进行了污染沉积量的检测。结果表明:在试验初期的高温恒温段,污染源与敏感表面温差高于0 ℃,15.75 h内单位面积污染沉积量为1.68×10
-4
g/cm
2
;在低温保持段,温差一直低于-22 ℃,23.37 h内单位面积污染解吸附量为1.08×10
-4
g/cm
2
;真空试验的总污染沉积量为2.7×10
-5
g/cm
2
。得到的结果证实了该QCM用于污染量检测的有效性。文中还初步分析了真空试验下的污染沉积过程,为光学表面污染的预估与防护提供了依据。
For the surface pollution of an optical communication terminal
a 10 MHz Aluminized Quartz Crystal Microbalance (QCM) is developed to detect the amount of deposited pollution in real time during a vacuum test. By introducing a reference crystal
the QCM eliminates the influence of environmental factors substantially
and reduces the requirements for temperature accuracy and its theoretical mass sensitivity is up to 10
-9
g/cm
2
. Through an absolute calibration experiment
the practical mass sensitivity of the QCM is 10
-8
g/cm
2
shows a lower cost and good practicability and can be used both in satellites and on the ground. According to different operating temperatures of pollution sources
the test is divided into 32 ℃ constant temperature segment
32 ℃ to -27 ℃ cooling segment
cryostat segment and -2 ℃ to 32 ℃ heating segment. The results show that in the high temperature segment at begin
the temperature difference between pollution source and sensitive surface is above 0 ℃
and the amount of pollution deposition per unit area is 1.68×10
-4
g/cm
2
in 15.75 h. In the cryostat segment
the temperature difference is below -22 ℃
the amount of desorption per unit area is 1.08×10
-4
g/cm
2
in 23.37 h. Moreover
the total amount of deposition is 2.7×10
-5
g/cm
2
in the vacuum test. These results confirm the validity of the QCM for detecting the amount of pollution deposition
analyze the deposition process under vacuum test preliminarily and provide a gist for predicting and preventing the pollution of optical surfaces.
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