共查询到20条相似文献,搜索用时 0 毫秒
1.
K.T. Kriebel P. Moerl M.E. Reinhardt R. Schellhase T. Koenig W. Rattei 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1982,2(6):11-13
The determination of the cloud top height by means of satelliteborne IR-radiometers requires the conversion of the measured radiance to an equivalent blackbody temperature and the assignment of this temperature to a geometrical height. The latter is associated with errors which add up easily to several kilometers. DFVLR did a case study to compare satellite derived cloud top heights with those from airborne Lidar measurements. The difference of the radiosonde temperature from the standard temperature profile results in a 1.8 km difference in cloud top height. The achievable accuracy using actual radiosonde temperatures is ± 0.4 km for optical thick clouds and much less for optical thin clouds. 相似文献
2.
An attempt to determine the ideal psychological profiles for crews of long term space missions. 总被引:1,自引:0,他引:1
H Ursin B Comet C Soulez-Larivière 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1992,12(1):301-314
This paper reviews possible psychological criteria for selection at individual level (personality, psychological stability, competence, social skills) as well as at crew level (crew size, gender, compatability, group homeostasis). Once astronauts have been selected an important effort will have to be made pre-flight to prepare the crew to the autonomy necessary for a Mars trip. During the mission psychological support will be important, but probably limited by the mission constraints. At this stage, mission success will probably rely mainly on the capacity of the crew to prevent and manage crises internally. Post-flight psychological support is necessary to help astronauts to readapt to a normal way of life on Earth. 相似文献
3.
Rong-yu Sun Chang-yin Zhao 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
Optical survey is a main technique for observing space debris, and precisely measuring the positions of space debris is of great importance. Due to several factors, e.g. the angle object normal to the observer, the shape as well as the attitude of the object, the variations of observed characteristics for low earth orbital space debris are distinct. When we look at optical CCD images of observed objects, the size and brightness are varying, hence it’s difficult to decide the threshold during centroid measurement and precise astrometry. Traditionally the threshold is given empirically and constantly in data reduction, and obviously it’s not suitable for data reduction of space debris. Here we offer a solution to provide the threshold. Our method assumes that the PSF (point spread function) is Gaussian and estimates the signal flux by a directly two-dimensional Gaussian fit, then a cubic spline interpolation is performed to divide each initial pixel into several sub-pixels, at last the threshold is determined by the estimation of signal flux and the sub-pixels above threshold are separated to estimate the centroid. A trail observation of the fast spinning satellite Ajisai is made and the CCD frames are obtained to test our algorithm. The calibration precision of various threshold is obtained through the comparison between the observed equatorial position and the reference one, the latter are obtained from the precise ephemeris of the satellite. The results indicate that our method reduces the total errors of measurements, it works effectively in improving the centering precision of space debris images. 相似文献
4.
F. Rákóczi E. Kovács 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1981,1(4):133-137
A method for the determination of cloud motion vectors is proposed by calculating from METEOSAT images the displacement of characteristic formations in the brightness field. The claculations are made for a sector of the Atlantic Ocean (ψ = 48°?38°N, λ = 24°?12°W). The adaptability of the Soebel operator for such calculations is also shown. The calculated wind vectors are in a good agreement with wind data at 850 mb surface. 相似文献
5.
Xiaomin Zuo Weixing Wan Chunliang Xia Anshou Zheng 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
Strong positive correlation between sporadic E layers and the solar activity and the long-term declining trend of Es were found in this paper. Then the feed-forward back propagation neural networks (NNs) were used to simulate the long-term variation of Es at four stations and predict foEs yearly average values. The inputs used for NNs are the yearly mean values of foEs in the daytime of the past ten years and the yearly averaged data of solar 10.7 cm radio flux (F107) of the present year, and the output is the present yearly mean value of daytime foEs. The outputs of trained NNs have high correlation with the desired values and the foEs yearly mean values predicted by NNs have good agreement with the observed data. The results indicate that NNs can make full use of the observed data to simulate the long variation rule of Es. Also, the results confirm the effect of solar activity on Es. 相似文献
6.
D.R. Pick J.L. Brownscombe 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1981,1(4):247-260
TOVS (TIROS Operational Vertical Sounder) comprises the three radiometers HIRS-2 (High resolution Infra Red Sounder Mod 2), MSU (Microwave Sounding Unit) and SSU (Stratospheric Sounding Unit) mounted on the TIROS-N series of operational spacecraft. Data from these sounders have been available since October 1978 and the series should continue to beyond 1985. The derivation and assessment of stratospheric geopotential height fields from these sounders, with particular reference to the SSU, are described. Measurements of stratospheric diurnal temperature effects and plots of zonally meaned brightness temperatures over a 450 day period are also presented. 相似文献
7.
Jerzy Kostrowicki 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1982,2(8):209-215
The scope and degree of land transformation depends on the system of land use by man. Therefore research on land use systems is of considerable importance, both for better knowledge of resulting processes as well as for more rational land management. To start such research a classification of land use systems is necessary. The paper presents an attempt at such a classification, preceded by an information on the studies carried on in the past as well as an explanation of reasons why such an attempt has been made, followed by the discussion of possible criteria, methods and techniques of land use systems identification. 相似文献
8.
G. Sèze C. Belcour M. Desbois 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1985,5(6):165-168
New developments of a cloud classification scheme based on histogram clustering by a statistical method are studied. Use of time series of satellite pictures and of spatial variances is introduced and discussed. 相似文献
9.
Triloki Pant Dharmendra Singh Tanuja Srivastava 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2010
Unsupervised classification of Synthetic Aperture Radar (SAR) images is the alternative approach when no or minimum apriori information about the image is available. Therefore, an attempt has been made to develop an unsupervised classification scheme for SAR images based on textural information in present paper. For extraction of textural features two properties are used viz. fractal dimension D and Moran’s I. Using these indices an algorithm is proposed for contextual classification of SAR images. The novelty of the algorithm is that it implements the textural information available in SAR image with the help of two texture measures viz. D and I. For estimation of D, the Two Dimensional Variation Method (2DVM) has been revised and implemented whose performance is compared with another method, i.e., Triangular Prism Surface Area Method (TPSAM). It is also necessary to check the classification accuracy for various window sizes and optimize the window size for best classification. This exercise has been carried out to know the effect of window size on classification accuracy. The algorithm is applied on four SAR images of Hardwar region, India and classification accuracy has been computed. A comparison of the proposed algorithm using both fractal dimension estimation methods with the K-Means algorithm is discussed. The maximum overall classification accuracy with K-Means comes to be 53.26% whereas overall classification accuracy with proposed algorithm is 66.16% for TPSAM and 61.26% for 2DVM. 相似文献
10.
An ensemble deep learning based shoreline segmentation approach (WaterNet) from Landsat 8 OLI images
Firat Erdem Bulent Bayram Tolga Bakirman Onur Can Bayrak Burak Akpinar 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2021,67(3):964-974
Shorelines constantly vary due to natural, urbanization and anthropogenic effects such as global warming, population growth, and environmental pollution. Sustainable monitoring of coastal changes is vital in terms of coastal resource management, environmental preservation and planning. Publicly available Landsat 8 OLI (Operational Land Manager) images provide accurate, reliable, temporal and up-to-date information about coastal areas. Recently, the use of machine learning and deep learning algorithms have become widespread. In this study, we used our public Landsat 8 OLI satellite image dataset to create a majority voting method which is an ensemble automatic shoreline segmentation system (WaterNet) to obtain shorelines automatically. For this purpose, different deep learning architectures have been utilized namely as Standard U-Net, Dilated U-Net, Fractal U-Net, FC-DenseNet, and Pix2Pix. Also, we have suggested a novel framework to create labeling data from OpenStreetMap service to create a unique dataset called YTU-WaterNet. According to the results, IoU and F1 scores have been calculated as 99.59% and 99.79% for the WaterNet. The results indicate that the WaterNet method outperforms other methods in terms of shoreline extraction from Landsat 8 OLI satellite images. 相似文献
11.
H.C. Sweet J.R. Bagby D.L. DeVincenzi 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1983,3(8):23-26
A systems design study group jointly sponsored by the American Society for Engineering Education, Stanford University and NASA's Ames Research Center, was requested to develop a design for an orbiting quarantine facility. The proposed facility is constructed of Spacelab shells formed into five modules of different sizes, each compatible with missions of other objectives. Once placed in a low Earth orbit by the Space Shuttle, each component is linked via the international docking system. Radiating from the docking module are a replaceable logistics module which stores a thirty day supply of consumables and waste, a module providing living quarters for five crew members, a power system module, and a quarantine testing laboratory. Within the laboratory module is a primary barrier system of sealed cabinets in which the sample is assessed for life forms. These chambers isolate the sample from terrestrial contamination and protect the researchers. A combination of procedures and mechanisms separates the laboratory module from the remainder of the facility and provides a secondary barrier. The conditions of space provide a tertiary barrier protecting the Earth's biosphere. 相似文献
12.
G. Salamunićcar S. Lončarić 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
Crater Detection Algorithms (CDAs) applications range from estimation of lunar/planetary surface age to autonomous landing on planets and asteroids and advanced statistical analyses. A large amount of work on CDAs has already been published. However, problems arise when evaluation results of some new CDA have to be compared with already published evaluation results. The problem is that different authors use different test-fields, different Ground-Truth (GT) catalogues, and even different methodologies for evaluation of their CDAs. Re-implementation of already published CDAs or its evaluation environment is a time-consuming and unpractical solution to this problem. In addition, implementation details are often insufficiently described in publications. As a result, there is a need in research community to develop a framework for objective evaluation of CDAs. A scientific question is how CDAs should be evaluated so that the results are easily and reliably comparable. In attempt to solve this issue we first analyzed previously published work on CDAs. In this paper, we propose a framework for solution of the problem of objective CDA evaluation. The framework includes: (1) a definition of the measure for differences between craters; (2) test-field topography based on the 1/64° MOLA data; (3) the GT catalogue wherein each of 17,582 craters is aligned with MOLA data and confirmed with catalogues by N.G. Barlow et al. and J.F. Rodionova et al.; (4) selection of methodology for training and testing; and (5) a Free-response Receiver Operating Characteristics (F-ROC) curves as a way to measure CDA performance. The handling of possible improvements of the framework in the future is additionally addressed as a part of discussion of results. Possible extensions with additional test-field subsystems based on visual images, data sets for other planets, evaluation methodologies for CDAs developed for different purposes than cataloguing of craters, are proposed as well. The goal of the proposed framework is to contribute to the research community by establishing guidelines for objective evaluation of CDAs. 相似文献
13.
A. Shevyrnogov G. Vysotskaya A. Sukhinin O. Frolikova M. Tchernetsky 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(1):36-40
The paper shows the efficiency of an application of the vegetation index image time series to determine long-term vegetation dynamics. The influence of large industrial centers of Siberia on the near-by vegetation is demonstrated. The analysis of the data shows that the influence of industrial waste is stronger in the Siberian North. These regions are characterized by critical conditions for vegetation existence. In the south of the Krasnoyarsk region, human impact is also important, but the possibility of vegetation self-rehabilitation is higher. The present-day economic situation in Russia is unique, with a temporary abrupt fall of industrial production and its following increase. Thus, we managed to analyze the degree of human impact on the environment within a relatively short-time interval. 相似文献
14.
Jeongrae Kim Seung Woo Lee Hyung Keun Lee 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
An ionospheric spatial gradient represents the ionosphere delay difference between different locations, and its variation over a specific area is important for implementing differential GNSS systems. An estimation method for the ionospheric spatial gradient over a small regional area is proposed. A plate map model is implemented for the direct estimation of the gradients. Nine years of GPS data were processed to figure out the annual variation of the mean gradient at the mid-geomagnetic latitude of 30° N. Gradients along the north–south direction have a mean of 0.65 mm/km and follow solar-cycle variations. 相似文献
15.
平面度误差目标函数凸凹性的研究 总被引:2,自引:1,他引:2
证明了平面度误差最小区域评定法的目标函数是二维欧氏空间R2 中的连续、不可微的凸函数 ,从而证明了目标函数的全局极小值是唯一的。 相似文献
16.
直线度误差目标函数凸凹性的研究 总被引:1,自引:1,他引:1
证明了直线度误差最小区域评定法的目标函数是一维欧式空间R1中的连续、不可微的凸函数 ,从而证明了目标函数的全局极小值是唯一的。 相似文献
17.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2023,71(7):3076-3089
Applications including change detection, disaster management, and urban planning require precise building information, and therefore automatic building extraction has become a significant research topic. With the improvements in sensor and satellite technologies, more data has become available, and with the increased computational power, deep learning methods have emerged as successful tools. In this study, U-Net and FPN architectures using four different backbones (ResNet-50, ResNeXt-50, SE-ResNext-50, and DenseNet-121), and an Attention Residual U-Net approach were used for building extraction from high-resolution aerial images. Two publicly available datasets, Inria Aerial Image Labeling Dataset and Massachusetts Buildings Dataset were used to train and test the models. According to the results, Attention Residual U-Net model has the highest F1 score with 0.8154, IoU score with 0.7102, and test accuracy with 94.51% on the Inria dataset. On the Massachusetts dataset, FPN Dense-Net-121 model has the highest F1 score with 0.7565 and IoU score with 0.6188, and Attention Residual U-Net model has the highest test accuracy with 92.43%. It has been observed that, FPN with DenseNet backbone can be a better choice when working with small size datasets. On the other hand, Attention Residual U-Net approach achieved higher success when a sufficiently large dataset is provided. 相似文献
18.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2007,39(9):1439-1444
We present the analysis of the radio observations of December 1, 2004 from 07:00 UT to 07:40 UT in the 1.100–1.340 GHz band by Solar Broadband Radio Dynamic Spectrometer (SBRS) in Huairou Station. There are three groups of radio fine structures during the impulsive phase of this flare denoted by N1, Z2, and Z3. N1 has several emission lines with mixed fast and slow frequency drift rate which may reflect the conditions of flare loop and fast flows out from reconnection site; Z2 and Z3 are zebra patterns. The radio observations combined with hard X-ray and other observations show that the fine structures are connected with energetic particles. The information about magnetic field and energetic particle during the burst are also estimated based on our model. 相似文献
19.
A.J. Blustin G. Branduardi-Raymont M.L. Crawford A.A. Breeveld J.S. Kaastra S.M. Kahn 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2004,34(12):2540-2543
A large number of galaxies, both normal and active, have been observed in ultraviolet light by the Optical Monitor on XMM-Newton. These are some of the deepest wide-field ultraviolet images of these galaxies yet obtained, and in many cases the first collected in this waveband. We present images of five active galaxies, and discuss the potential uses of the ultraviolet surface brightness distribution and morphology, in association with X-ray data, for Active Galactic Nuclei, star formation and galaxy evolution studies. 相似文献
20.
Vincent Barra Véronique Delouille Jean-François Hochedez 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
The study of the variability of the solar corona and the monitoring of its traditional regions (Coronal Holes, Quiet Sun and Active Regions) are of great importance in astrophysics as well as in view of the Space Weather and Space Climate applications. Here we propose a multichannel unsupervised spatially constrained fuzzy clustering algorithm that automatically segments EUV solar images into Coronal Holes, Quiet Sun and Active Regions. Fuzzy logic allows to manage the various noises present in the images and the imprecision in the definition of the above regions. The process is fast and automatic. It is applied to SoHO–EIT images taken from February 1997 till May 2005, i.e. along almost a full solar cycle. Results in terms of areas and intensity estimations are consistent with previous knowledge. The method reveal the rotational and other mid-term periodicities in the extracted time series across solar cycle 23. Further, such an approach paves the way to bridging observations between spatially resolved data from imaging telescopes and time series from radiometers. Time series resulting form the segmentation of EUV coronal images can indeed provide an essential component in the process of reconstructing the solar spectrum. 相似文献