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CAS IR Grid
机构
青藏高原研究所 [1]
长春光学精密机械与物... [1]
上海光学精密机械研究... [1]
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OAI收割 [3]
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期刊论文 [2]
会议论文 [1]
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2011 [1]
2008 [1]
2007 [1]
学科主题
地理学::自然地理学 [1]
激光技术;激光物理与... [1]
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Allometric models for leaf area estimation across different leaf-age groups of evergreen broadleaved trees in a subtropical forest
期刊论文
OAI收割
PHOTOSYNTHETICA, 2011, 卷号: 49, 期号: 2, 页码: 219-226
Zhang L (张林)
;
Pan, L (Pan L.)
收藏
  |  
浏览/下载:17/0
  |  
提交时间:2012/05/10
LINEAR MEASUREMENTS
NONDESTRUCTIVE METHODS
WIDTH MEASUREMENT
L.
ACCURATE
REGRESSION
CITRUS
LENGTH
Accurate measurement of carrier-envelope phase drift for infrared femtosecond laser pulses
期刊论文
OAI收割
opt. express, 2008, 卷号: 16, 期号: 26, 页码: 21383, 21388
Song Liwei
;
Zhang Chunmei
;
Wang Jianliang
;
冷雨欣
;
李儒新
收藏
  |  
浏览/下载:803/79
  |  
提交时间:2009/09/18
Accurate measurements
Femtosecond pulses
Incident lasers
Incident pulses
Infrared femtosecond lasers
Interference fringes
Interference measurements
Measurement processes
Novel schemes
Phase drifts
Phase jitter
Second harmonics
Spectral interferences
Application of CMOS APS star tracker with large FOV in attitude and angular velocity determination (EI CONFERENCE)
会议论文
OAI收割
Advanced Sensor Systems and Applications III, November 12, 2007 - November 14, 2007, Beijing, China
Lu D.
;
Guang J.
;
Shaoju W.
;
Tao C.
收藏
  |  
浏览/下载:30/0
  |  
提交时间:2013/03/25
The paper deals with the spacecraft attitude determination problem using a new kind of star tracker with large FOV based on CMOS APS. Star tracker has been developed since 1970s and proved to be the most accurate sensor ever used in the spacecraft attitude determination systems. But the traditional CCD star tracker also has some disadvantages
such as small FOV
high power consumption
low sample rate and low working angular rate limit which prevent the use of CCD star tracker in attitude large angle maneuvering process. The new kind of star tracker based on CMOS APS has no such disadvantages and is more applicable on modern low-cost agile small satellites. Its higher sample rate and working angular rate limit over traditional CCD star tracker make it more adapt for spacecraft angular velocity determination. Because of the large FOV of the star tracker
the mathematical model of traditional CCD star tracker with a small FOV is not appropriate. So a new mathematical model was quoted to fit the star tracker with a large FOV. An alternative adaptive algorithm was also introduced in the paper. It can help the EKF algorithm work lacking of accurate covariance of the observation noise. An optimal estimation algorithm was used to estimate the angular velocity directly from the star tracker measurements. Mathematic simulation results indicate the CMOS APS star tracker can give accurate attitude information and estimated angular rate. The method can be used as the chief attitude determination system design of low-cost satellite without gyros
or be used as a backup strategy in the event of gyro failures to enhance the reliability of the attitude determination system.