-
With the rapid development of space technology, human activities into space are increasing, thereby producing lots of space debris. And the space debris impact is the major cause for the mechanical damage to the space crafts and the main factor affecting the service life; it even endangers the life safety of the astronauts working outside the spacecraft and pose a threat to the astronomical observation and studies. Thus, the monitoring and early warning of space debris are gradually attracting wide attention. Obviously, laser detection as a good-directivity and strong anti-jamming active detecting means has a unique advantage in terms of a round-the-clock detection. Therefore, the developing of debris-detecting laser beam source becomes the most direct and effective means for increasing the space debris detection accuracy. The laser detecting ability is restricted by the laser beam quality, the pulse energy and the repetition frequency at the same time. The beam quality could affect the ability to detect and recognize space target. The bigger the laser pulse energy, the higher the repetition frequency and the smaller the detectable debris, the stronger the detecting ability will be. A good detection effect could be achieved at 80-100 Hz laser pulse repetition frequency. A further increase of the repetition frequency will greatly increase the difficulty and cost accordingly but the improvement of the detection performance is not obvious at all. Thus, repetition frequency around 100 Hz becomes the best choice for laser space debris detection. Based on the laser diode side-pumped rod-shaped amplifier, a high-repetition-frequency and high-beam-quality of joule level Nd:YAG nanosecond laser for space debris detection is developed in this work. The laser adopts MOPA structure, mainly including single longitudinal mode, pre-amplifier unit, SBS phase-conjugate beam control unit and energy extraction unit. In the energy extraction unit, beam splitting-amplifying-combining is adopted for reducing the thermal effect on beam quality by reducing the working current of the amplifier. Under the condition of 100 Hz high repetition frequency and 10.73 J single pulse energy injected by the single longitudinal mode seed, 3.31 J output energy is gained. The output laser beam has a 4.58 ns pulse width, far field beam spot of 2.12 times the value of the diffraction limit, and 0.87% energy stability (RMS).
-
Keywords:
- diode-pumped /
- high repetition /
- nanosecond laser /
- high beam quality
[1] Dong J H, Hu Q Q 2007Chin.Opt.Lett. 5 S176
[2] Nalezyty M, Majczyna A, Wawrzaszek R, Sokolowski M 2010Proc.SPIE 7745 S178
[3] Ma X, Wang J, Zhou J, Zhu X, Chen W 2010Appl.Phys.B 103 809
[4] Zhang Z P, Yang F M, Zhang H F, Wu Z B, Chen J P, Li P, Meng W D 2012Res.Astron.Astrophys. 12 212
[5] Yang H L, Meng J Q, Ma X H, Chen W B 2014Chin.Opt.Lett. 12 96
[6] Yu H H, Gao P Q, Shen M, Guo X Z, Yang D T, Zhao Y 2016Astronomical ResearchTechnology 14 416(in Chinese)[于欢欢, 高鹏骐, 沈鸣, 郭效忠, 杨大陶, 赵有2016天文研究与技术14 416]
[7] Biro E, Weckman D C, Zhou Y 2002Metall.Mater.Trans.A 33 2019
[8] Andrebe Y, Behn R, Duval B P, Etienne P, Pitzschke A 2011Fusion Eng.Des. 86 1273
[9] Kim Y G, Lee J H, Lee J W, An Y H, Dang J J, Jo J M, Lee H Y, Chung K J, Hwang Y S, Na Y S 2015Fusion Eng.Des. 96-97 882
[10] Yoshida H, Nakatsuka M, Hatae T, Kitamura S, Sakuma T, Hamano T 2004Jpn.J.Appl.Phys. 43 L1038
[11] Yang X D, Bo Y, Peng Q J, Zhang H L, Geng A C, Cui Q J, Sun Z P, Cui D F, Xu Z Y 2006Opt.Commun. 226 39
[12] Sun W N, Wang W L, Bi G J, Zhu C, Yang W S 2006Chinese J.Lasers 33(suppl.) 20(in Chinese)[孙维娜, 王伟力, 秘国江, 朱辰, 杨文是2006中国激光33(suppl.) 20]
[13] Qiu J S, Tang X X, Fan Z W, Wang H C 2016Opt.Commun. 368 1
[14] Qiu J S, Tang X X, Fan Z W, Wang H C, Liu H 2016Appl.Opt. 55 21
[15] Qiu J S, Tang X X, Fan Z W, Chen Y Z, Ge W Q, Wang H C, Liu H 2016Acta Phys.Sin. 65 154204(in Chinese)[邱基斯, 唐熊忻, 樊仲维, 陈艳中, 葛文琦, 王昊成, 刘昊2016物理学报65 154204]
[16] Hasi W L J, Qiao Z, Cheng S X, Wang X Y, Zhong Z M, Zheng Z X, Lin D Y, He W M, Lu Z W 2013Opt.Commun. 311 375
-
[1] Dong J H, Hu Q Q 2007Chin.Opt.Lett. 5 S176
[2] Nalezyty M, Majczyna A, Wawrzaszek R, Sokolowski M 2010Proc.SPIE 7745 S178
[3] Ma X, Wang J, Zhou J, Zhu X, Chen W 2010Appl.Phys.B 103 809
[4] Zhang Z P, Yang F M, Zhang H F, Wu Z B, Chen J P, Li P, Meng W D 2012Res.Astron.Astrophys. 12 212
[5] Yang H L, Meng J Q, Ma X H, Chen W B 2014Chin.Opt.Lett. 12 96
[6] Yu H H, Gao P Q, Shen M, Guo X Z, Yang D T, Zhao Y 2016Astronomical ResearchTechnology 14 416(in Chinese)[于欢欢, 高鹏骐, 沈鸣, 郭效忠, 杨大陶, 赵有2016天文研究与技术14 416]
[7] Biro E, Weckman D C, Zhou Y 2002Metall.Mater.Trans.A 33 2019
[8] Andrebe Y, Behn R, Duval B P, Etienne P, Pitzschke A 2011Fusion Eng.Des. 86 1273
[9] Kim Y G, Lee J H, Lee J W, An Y H, Dang J J, Jo J M, Lee H Y, Chung K J, Hwang Y S, Na Y S 2015Fusion Eng.Des. 96-97 882
[10] Yoshida H, Nakatsuka M, Hatae T, Kitamura S, Sakuma T, Hamano T 2004Jpn.J.Appl.Phys. 43 L1038
[11] Yang X D, Bo Y, Peng Q J, Zhang H L, Geng A C, Cui Q J, Sun Z P, Cui D F, Xu Z Y 2006Opt.Commun. 226 39
[12] Sun W N, Wang W L, Bi G J, Zhu C, Yang W S 2006Chinese J.Lasers 33(suppl.) 20(in Chinese)[孙维娜, 王伟力, 秘国江, 朱辰, 杨文是2006中国激光33(suppl.) 20]
[13] Qiu J S, Tang X X, Fan Z W, Wang H C 2016Opt.Commun. 368 1
[14] Qiu J S, Tang X X, Fan Z W, Wang H C, Liu H 2016Appl.Opt. 55 21
[15] Qiu J S, Tang X X, Fan Z W, Chen Y Z, Ge W Q, Wang H C, Liu H 2016Acta Phys.Sin. 65 154204(in Chinese)[邱基斯, 唐熊忻, 樊仲维, 陈艳中, 葛文琦, 王昊成, 刘昊2016物理学报65 154204]
[16] Hasi W L J, Qiao Z, Cheng S X, Wang X Y, Zhong Z M, Zheng Z X, Lin D Y, He W M, Lu Z W 2013Opt.Commun. 311 375
Catalog
Metrics
- Abstract views: 5475
- PDF Downloads: 315
- Cited By: 0
下载:
