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Chinese Academy of Sciences Institutional Repositories Grid
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CAS IR Grid
机构
地理科学与资源研究所 [7]
成都山地灾害与环境研... [3]
长春光学精密机械与物... [2]
化学研究所 [1]
数学与系统科学研究院 [1]
遥感与数字地球研究所 [1]
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OAI收割 [16]
内容类型
期刊论文 [7]
会议论文 [6]
SCI/SSCI论文 [3]
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2024 [1]
2021 [2]
2020 [1]
2014 [2]
2013 [2]
2008 [1]
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Multidisci... [1]
摄影测量与遥感技术 [1]
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Spatial patterns of light response parameters and their regulation on gross primary productivity in China
期刊论文
OAI收割
AGRICULTURAL AND FOREST METEOROLOGY, 2024, 卷号: 345, 页码: 11
作者:
Lin, Yong
;
Chen, Zhi
;
Yu, Guirui
;
Yang, Meng
;
Hao, Tianxiang
  |  
收藏
  |  
浏览/下载:28/0
  |  
提交时间:2024/01/22
Light response parameter
Apparent quantum yield (alpha)
Maximum gross photosynthetic rate ( A max )
Spatial heterogeneity
Eddy covariance
Identification of Multiscale Spatial Structure of Lunar Impact Crater: A Semivariogram Approach
期刊论文
OAI收割
IEEE JOURNAL OF SELECTED TOPICS IN APPLIED EARTH OBSERVATIONS AND REMOTE SENSING, 2021, 卷号: 14, 页码: 2731-2739
作者:
Wang, Jiao
;
Ming, Dongping
;
Cheng, Weiming
  |  
收藏
  |  
浏览/下载:20/0
  |  
提交时间:2021/06/10
Spatial resolution
Moon
Image segmentation
Geology
Remote sensing
Periodic structures
Mathematical model
Lunar impact crater
multiscale spatial structure
optimum resolution
scale parameter
semivariogram
Identification of Multiscale Spatial Structure of Lunar Impact Crater: A Semivariogram Approach
期刊论文
OAI收割
IEEE JOURNAL OF SELECTED TOPICS IN APPLIED EARTH OBSERVATIONS AND REMOTE SENSING, 2021, 卷号: 14, 页码: 2731-2739
作者:
Wang, Jiao
;
Ming, Dongping
;
Cheng, Weiming
  |  
收藏
  |  
浏览/下载:22/0
  |  
提交时间:2021/06/10
Spatial resolution
Moon
Image segmentation
Geology
Remote sensing
Periodic structures
Mathematical model
Lunar impact crater
multiscale spatial structure
optimum resolution
scale parameter
semivariogram
Quantitative spatial distribution model of site-specific loess landslides on the Heifangtai terrace, China
期刊论文
OAI收割
LANDSLIDES, 2020, 页码: DOI: 10.1080/15569543.2020.1780615
作者:
Zhou Qi
;
Xu Qiang
;
Peng Dalei
;
Fan Xuanmei
;
Ouyang Chaojun
  |  
收藏
  |  
浏览/下载:165/0
  |  
提交时间:2020/11/18
Loess landslide
Numerical simulation
Maximum likelihood estimation
Parameter probability
Spatial distribution
Debris-flows scale predictions based on basin spatial parameters calculated from Remote Sensing images in Wenchuan earthquake area
会议论文
OAI收割
35th International Symposiumon Remote Sensing of Environment (ISRSE35), Beijing, 2013.4.22-26
作者:
Jianrong Fan
;
Fan Jianrong
收藏
  |  
浏览/下载:33/0
  |  
提交时间:2014/12/12
Remote Sensing
Debris flow
spatial parameter
prediction
Hybrid Optimal Design of the Eco-Hydrological Wireless Sensor Network in the Middle Reach of the Heihe River Basin, China
SCI/SSCI论文
OAI收割
2014
作者:
Ge Y.
收藏
  |  
浏览/下载:35/0
  |  
提交时间:2014/12/24
eco-hydrological wireless sensor network
spatial sampling
hybrid
optimization criterion
unconditional stochastic simulation
constrained optimization
parameter-estimation
spatial prediction
soil
observatories
variogram
Concomitant flow and space variations of evapotranspiration due to changes in LUCC under seawater intrusion in a coastal region
会议论文
OAI收割
Remote Sensing and Modeling of Ecosystems for Sustainability X, San Diego, CA, United states, August 26, 2013 - August 29, 2013
Gao, Zhiqiang(1,3)
;
Ning, Jicai(1)
;
Cao, Xiaoming(2)
;
Shi, Runhe(3)
;
Gao, Wei(3)
收藏
  |  
浏览/下载:140/0
  |  
提交时间:2015/08/10
Salt water intrusion
Background effects
Land surface parameters
Land use and land cover
Landsat satellite
Pattern identification
Spatial distribution patterns
Surface parameter
Thermal infrared bands
Predicting Volume and Runout of Single Gully Debris-Flow Using Hypsometric Integral Value in the Wenchuan Earthquake Area
会议论文
OAI收割
Proceedings of the International Symposium on Earthquake-Induced Landslides, Japan, 2012
作者:
Zhang, Huaizhen
;
Fan, Jianrong
;
Liu, Qing
收藏
  |  
浏览/下载:21/0
  |  
提交时间:2016/12/05
Debris-flow
Runout zone
Wenchuan earthquake
Hypsometric integral
Spatial parameter
Improved best tradeoff for high-resolution image fusion based on spectral reflection function
会议论文
OAI收割
International Conference on Earth Observation Data Processing and Analysis, ICEODPA,, Wuhan, China, December 28, 2008 - December 30,2008
Wang, Zhongwu
;
Zhao, Zhongming
收藏
  |  
浏览/下载:23/0
  |  
提交时间:2014/12/07
This paper extended the best tradeoff fast intensity-hue-saturation (BTFIHS) fusion to a more general model. Firstly
based-on the methods proposed by previous researches
we integrated injecting strategy of spatial detail information into the fusion model and also adopted the idea of BTFIHS to keep the intensity unchanged with the corresponding pixel in panchromatic (PAN) image
while the hue and saturation of every pixel using BTFIHS were equal to them using tradeoff fast intensity-hue-saturation (TFIHS). Then we got a general formula of the improved best tradeoff for high-resolution image fusion based-on getting injecting parameter by spectral reflection function (SRF). At last
several experiments were carried on to analysis and discuss the quality of the new methods compared with their originals. Results show that the new method could yield a "true" high-resolution multispectral (MS) image
with vast improvement in blue band and nearly 3.3% improvement in Q4 for all bands. 2008 SPIE.
Research on the support structure of the primary mirror of large-aperture telescope (EI CONFERENCE)
会议论文
OAI收割
3rd International Symposium on Advanced Optical Manufacturing and Testing Technologies, AOMATT 2007: Large Mirrors and Telescopes, July 8, 2007 - July 12, 2007, Chengdu, China
Yang W.
;
Jingxu Z.
收藏
  |  
浏览/下载:27/0
  |  
提交时间:2013/03/25
Large-aperture telescope can be used in surveying battlefield
researching landform
searching object
real-time monitoring
imaging
detecting and identifying spatial targets and so on. A large-aperture telescope for achieving high resolution power is designed to monitor spatial target and image in real time. Real-time monitoring plays an important role in military conflicts. The orbit parameter of object
quantity
geometrical shape parameter and so on can be obtained by detect spatial target. With the development of optical technology
people require larger aperture in optics-electronic (OE) system. By increasing optical aperture
the ability of collecting light and resolution power in the system can be enhanced. But the support structure of the primary mirror of large-aperture telescope will be a very difficult problem. With the increase of primary mirror aperture
the weight of the primary mirror will become larger than before. The root mean square (rms) of the primary mirror is affected by many factors
such as deadweight
deformation of heat
environment and so on. Due to the primary mirror of telescope is an important component of telescope system. By reducing the weight of primary mirror
precision of the system is ensured. During the designing phase
one can consider the supporting project of the primary mirror synthetically and analyze it roundly according to technical requirement of optical system and the effect factors. The final structural design can be reasonable. In an astronomical telescope
the surface of reflector is an important part for collecting dark radiation of celestial bodies. Its surface shape will have an effect on collecting efficiency of telescope radiant energy directly. So the rms must be very high. Optical system of large aperture
small wavelength and small focus can receive maximal light intensity. For ground-based optical astronomical telescope
the design proposed in the paper can satisfy the requirement of the possible minimum atmosphere seeing at astronomical observatory site and exert the use efficiency of the telescope adequately. So the accuracy of the traditional surface of reflector can assure that 90% of all the light energy can be focused on within the angle diameter range of the minimum atmosphere seeing
then 100% of light energy should be focused on the angle diameter range of minimum atmosphere seeing. Because the rms of mirror is very high
precise surface machining and accurate the support of mirror are very important tasks during designing and manufacturing the telescope. In the paper
various support techniques of a large-aperture telescope primary mirror are discussed and a 3.5 meter telescope system at the Starfire Optical Range (SOR) overviewed simply
which was operated by the Directed Energy Directorate of the Air Force Research Laboratory
Kirtland AFB
NM
USA from the ground-based O-E system for the observations of spatial target. We also analyze Theoretical elastic deformation of the Steward Observatory 2.3 meter mirror is analyzed.