太赫兹大气遥感技术

胡伟东; 季金佳; 刘瑞婷; 王雯琦; LeoP.LIGTHART

doi:10.3788/CO.20171005.0656

Volume 10 Issue 5

Oct. 2017

Turn off MathJax

Article Contents

Chinese Optics > 2017 > 10(5): 656-665.

HU Wei-dong, JI Jin-jia, LIU Rui-ting, WANG Wen-qi, Leo P. LIGTHART. Terahertz atmosphere remote sensing[J]. Chinese Optics, 2017, 10(5): 656-665. doi: 10.3788/CO.20171005.0656

Citation:

HU Wei-dong, JI Jin-jia, LIU Rui-ting, WANG Wen-qi, Leo P. LIGTHART. Terahertz atmosphere remote sensing[J]. Chinese Optics, 2017, 10(5): 656-665. doi: 10.3788/CO.20171005.0656

HU Wei-dong, JI Jin-jia, LIU Rui-ting, WANG Wen-qi, Leo P. LIGTHART. Terahertz atmosphere remote sensing[J]. Chinese Optics, 2017, 10(5): 656-665. doi: 10.3788/CO.20171005.0656

Citation:

HU Wei-dong, JI Jin-jia, LIU Rui-ting, WANG Wen-qi, Leo P. LIGTHART. Terahertz atmosphere remote sensing[J]. Chinese Optics, 2017, 10(5): 656-665. doi: 10.3788/CO.20171005.0656

PDF( 3385 KB)

Terahertz atmosphere remote sensing

doi: 10.3788/CO.20171005.0656

1.
Beijing Institute of Technology, School of information and electronics, Beijing 100081, China
2.
Delft University of Technology, Delft 2628 CN, Netherlands

Funds:

Major Instrument Project of National Natural Science Fundation of China 61527805

Group Project of National Natural Science Fundation of China 61421001

Project of Innovation & Introduced Intelligence for colleges and universities of China B14010

More Information

Corresponding author: HU Wei-dong, E-mail:hoowind@bit.edu.cn
Received Date: 11 May 2017
Rev Recd Date: 13 Aug 2017
Publish Date: 01 Oct 2017

Abstract

Abstract

Terahertz waves play an increasingly important role in the field of atmosphere remote sensing due to its unique atmosphere sensitivity. Terahertz atmospheric remote sensing technology has been a research hotspot at the international level. In 2004, NASA launched AURA, which included 2.5THz radiometer with two polarization properties. In 2007, ESA developed the Marschals heterodyne spectrometer, which adopted limb scanning method to detect the hyperspectral spectra of gas components in sub-millimeter wave thermal radiation. Currently, China's in-orbit meteorological satellite Fengyun-Ⅲ is equipped with a millimeter-band radiometer, and Fengyun-Ⅳ is the world's first GEMS carrying terahertz remote sensing instrument. Based on the analysis of the application and technology of terahertz remote sensing at home and abroad, this paper puts forward the idea of developing remote sensing technology with independent intellectual property rights according to the current situation of atmospheric remote sensing in China.
- terahertz,
- atmosphere remote sensing,
- cloud particles,
- radiometer

FullText(HTML)

References(38)

References

[1]	YAO J Q, WANG J L, ZHONG K, et al.. Study and outlook of THz radiation atmospheric propagation[J]. Journal of Optoelectronics·Laser, 2010, 21(10):1582-1588.(in Chinese)
[2]	PETER H S. Terahertz technology[J]. IEEE Transactions on Microwave Theory and Techniques, 2002, 50(3):910-928. doi: 10.1109/22.989974
[3]	ZHANG J Q, XUE CH, GAO G, et al.. Development and trend of cloud and aerosol optical remote sensing instrument[J]. Chinese Optics, 2015, 8(5):679-698. doi: 10.3788/co.
[4]	HU X H, LIU S T, PAN ZH D, et al.. The development of spaceborne shimmer detection instrument and its data application[J]. Chinese Optics, 2015, 8(3):350-359. doi: 10.3788/co.
[5]	KLEIN U. Future satellite earth observation requirements and technology in millimetre and sub-millimetre wavelength region[C]. The 17th Int Symp on Space THz Technology, Paris, France, 2006:21-28.
[6]	SOHN B J, CHUNG E S, SCHMETZ J, et al.. Estimating upper-tropospheric water vapor from SSM/T-2satellite measurements[J]. J. Appl. Meteor, 2003, 42:488-504. doi: 10.1175/1520-0450(2003)042<0488:EUTWVF>2.0.CO;2
[7]	CLERBAUX C, TURQUETY S, COHEUR P. Infrared remote sensing of atmospheric composition and air quality:towards operational applications[J]. Comptes Rendus Geoscience, 2010, 342(4):349-356.
[8]	WANG W, DONG J H, MENG Q Y. Development and trend of visible light remote sensing camera for Mars exploration[J]. Chinese Optics, 2014, 7(2):208-214.
[9]	YING Y B, WANG J P, JIANG H Y. Inspecting diameter and defect area of fruit with machine vision[J]. Transactions of the CSAE, 2002, 18(5):216-220.
[10]	WATERS J W, READ W G, FROIDEVAUX L, et al.. The UARS and EOS microwave limb sounder(MLS) experiments[J]. Journal of the Atmospheric Sciences, 1998, 56:194-218.
[11]	WATERS J W, PECKHAM G E. The microwave limb sounder(MLS) experiments for UARS and EOS[J]. The International Society for Optical Engineering, 1991:543-546.
[12]	PUMPHREY H C, CLARK H L, HARWOOD R S. Lower stratospheric water vapor measured by UARS MLS[J]. Geophysical Research Letters, 2000, 27(12):1691-1694. doi: 10.1029/1999GL011339
[13]	BARATH F T, CHAVEZ M C, COFIELD R E, et al.. The upper atmosphere research satellite microwave limb sounder instrument[J]. J. Geophys Res, 1993, 98(10):751-762.
[14]	BARON P, RICAUD P, et al.. Studies for the Odin sub-millimetre radiometer.Ⅱ:Retrieval methodology[J]. Canadian Journal of Physics, 2002, 80(4):341-356. doi: 10.1139/p01-150
[15]	URBAN J, LAUTIE N, LE FLOCHMOEZ E, et al.. Odin/SMR limb observations of stratospheric trace gases:validation of N₂O[J]. Journal of Geophysical Research, 2005, 110:D09301-D09320. https://core.ac.uk/display/70561256
[16]	LI X Y, CHEN L F, SU L, et al.. Development of submillimeter wave edge detection[J]. Journal of Remote Sensing, 2013, 6:1325-1344.
[17]	YANG ZH D, LU N M, SHI J M, et al.. Overview of FY-3 satellite payload and ground application systems[J]. Meteorological Science and Technology, 2013, 4:6-12. http://www.sciencedirect.com/science/article/pii/B9780127999487000050
[18]	DONG Y H. FY-4 meteorological satellite and its application prospect[J]. Shanghai Aerospace, 2016, 2:1-8.
[19]	FRANKLIN E K, STEVEN J W, ANDREW J H, et al.. Submillimeter-wave cloud ice radiometer:simulations of retrieval algorithm performance[J]. Journal of Geophysical Research, 2002, 107(D3):4028-4048. doi: 10.1029/2001JD000709
[20]	VANEK M D, NOLT I G, TAPPAN N D, et al.. Far-infrared sensor for cirrus(FIRSC):an aircraft-based Fourier-transform spectrometer to measure cloud radiance[J]. Appl. Opt., 2001, 40(13):2169-2176. doi: 10.1364/AO.40.002169
[21]	EVANS K F, WANG J R, RACETTE P E, et al.. Ice cloud retrievals and analysis with the compact scanning submillimeter imaging radiometer and the cloud radar system during CRYSTAL FACE[J]. American Meteorological Society, 2005, 44:839-859. https://espo.nasa.gov/attrex/content/Ice_Cloud_Retrievals_and_Analysis_with_the_Compact_Scanning_Submillimeter_Imaging_Radiometer
[22]	MARAZITA S M, BISHOP W L, HESLER J L, et al.. Integrated Ga As Schottky mixers by spin on dielectric wafer bonding[J]. IEEE Transactions on Electron Devices, 2000, 47(6):1152-1157. doi: 10.1109/16.842956
[23]	MARSH S, ALDERMAN B, MATHESON D, et al. Design of low-cost 183 GHz subharmonic mixers for commercial applications[J]. IET Circuits, Devices and Systems, 2007, 1(1):1-6 doi: 10.1049/iet-cds:20060212
[24]	TESSMANN A, LEUTHER A, SEHWOERER C, et al. Acoplanar 94 GHz low-noise amplifier MMIC using 0.07μm. metamorphie cascode HEMTs[C]. IEEE MTT-S International Microwave Symposium Digest, IEEE, 2003:1581-1584.
[25]	BRYERTON E W, MEI X, KIM Y M, et al.. A W-band Low-Noise Amplifier with 22K noise temperature[C]. IEEE MTT-S International Microwave Symposium Digest, Boston, USA, 2009:681-684.
[26]	LU D R, HSU Y C, KAO J C, et al.. A 75.5-to-120.5-GHz, high-gain CMOS low-noise amplifier[C]. IEEE MTT-S International Microwave Symposium Digest, Montreal, Canada, IEEE, 2012:1-3.
[27]	HROBAK M, STERNS M, SCHRAMM M, et al.. Planar zero bias Schottky diode detector operating in the E-and W-band[C]. 2013 European Microwave Conference(EuMC), IEEE, 2013:179-182.
[28]	LI S. Development of millimeter wave geophone[D]. Chengdu:University of Electronic Science and technology of China, 2008:59-77.
[29]	XUE W. W band broadband direct detection receiving front-end[D]. Chengdu:University of Electronic Science and technology of China, 2013:39-50.
[30]	AUSTON D H, SMITH P R. Cherenkov radiation from femtosecond optical pulses in elect ro-optic media[J]. Appl. Phys. Lett., 1984, 53(16):1555-1558. doi: 10.1103/PhysRevLett.53.1555
[31]	FATTINGER CH, GRISCHKOWSKY D. Point source terahertz optics[J]. Appl. Phys. Lett., 1988, 53(16):1480-1482. doi: 10.1063/1.99971
[32]	LEITENSTORFER S, HUNSCHE J, SHAH M C, et al.. Detectors and sources for ultrabroadband electro-optic sampling:experiment and theory[J]. Appl. Phys. Lett., 1999, 74(11):1516-1518. doi: 10.1063/1.123601
[33]	KONO S, TANI M, GU P, et al.. Detection of up to 20 THz with a low-temperature-grown GaAs photoconductive antenna gated with 15 fs light pulses[J]. Appl. Phys. Lett., 2000, 77(25):4104-4106. doi: 10.1063/1.1333403
[34]	HAJENIUS M. Full characterization and analysis of a terahertz heterodyne receiver based on a NbN hot electron bolometer[J]. Phys. Rev. Lett., 2006, 100(7):074507. https://repository.tudelft.nl/islandora/object/uuid:3c930069-6427-4fb0-a113-88758172c003/?collection=research
[35]	SEMENOV A D, HUBERS H W, RICHTER H. Superconducting hot-electron bolometer mixer for terahertz heterodyne receivers[J]. IEEE Appl. Superconductivity, 2003, 13(2):168-171. doi: 10.1109/TASC.2003.813672
[36]	WHYBORN N D. Heterodyne instrument for FIRST(HIFI):preliminary design[J]. SPIE, 1998, 3357:336-347.
[37]	KOMIYAMA S, ASTAFIEV O, ANTONOV V V, et al.. A single-photon detector in the far-infrared range[J]. Nature, 2000, 403(6768):405-407. doi: 10.1038/35000166
[38]	ASTAFIEV O, KOMIYAMA S, KUT SUWA T, et al.. Single-photon detector in the microwave range[J]. Phys. Rev. Lett., 2002, 80(22):4250-4252.