Principles Of A High Resolution Forest Imaging Model For Sar

Author(s):  
R.J. Miller ◽  
L.M.J. Brown ◽  
A.J. Siebert
Author(s):  
Mi Wang ◽  
Yufeng Cheng ◽  
Xiaoxiang Long ◽  
Bo Yang

The GaoFen-4 (GF-4) remote sensing satellite is China’s first civilian high-resolution geostationary optical satellite, which has been launched at the end of December 2015. To guarantee the geometric quality of imagery, this paper presents an on-orbit geometric calibration method for the area-array camera of GF-4. Firstly, we introduce the imaging features of area-array camera of GF-4 and construct a rigorous imaging model based on the analysis of the major error sources from three aspects: attitude measurement error, orbit measurement error and camera distortion. Secondly, we construct an on-orbit geometric calibration model by selecting and optimizing parameters of the rigorous geometric imaging model. On this basis, the calibration parameters are divided into two groups: external and internal calibration parameters. The external parameters are installation angles between the area-array camera and the star tracker, and we propose a two-dimensional direction angle model as internal parameters to describe the distortion of the areaarray camera. Thirdly, we propose a stepwise parameters estimation method that external parameters are estimated firstly, then internal parameters are estimated based on the generalized camera frame determined by external parameters. Experiments based on the real data of GF-4 shows that after on-orbit geometric calibration, the geometric accuracy of the images without ground control points is significantly improved.


Author(s):  
Mi Wang ◽  
Yufeng Cheng ◽  
Xiaoxiang Long ◽  
Bo Yang

The GaoFen-4 (GF-4) remote sensing satellite is China’s first civilian high-resolution geostationary optical satellite, which has been launched at the end of December 2015. To guarantee the geometric quality of imagery, this paper presents an on-orbit geometric calibration method for the area-array camera of GF-4. Firstly, we introduce the imaging features of area-array camera of GF-4 and construct a rigorous imaging model based on the analysis of the major error sources from three aspects: attitude measurement error, orbit measurement error and camera distortion. Secondly, we construct an on-orbit geometric calibration model by selecting and optimizing parameters of the rigorous geometric imaging model. On this basis, the calibration parameters are divided into two groups: external and internal calibration parameters. The external parameters are installation angles between the area-array camera and the star tracker, and we propose a two-dimensional direction angle model as internal parameters to describe the distortion of the areaarray camera. Thirdly, we propose a stepwise parameters estimation method that external parameters are estimated firstly, then internal parameters are estimated based on the generalized camera frame determined by external parameters. Experiments based on the real data of GF-4 shows that after on-orbit geometric calibration, the geometric accuracy of the images without ground control points is significantly improved.


Blood ◽  
2008 ◽  
Vol 112 (11) ◽  
pp. 647-647
Author(s):  
Judith Runnels ◽  
Alicia Carlson ◽  
Costas Pitsillides ◽  
Joel Spencer ◽  
Juwell Wu ◽  
...  

Abstract BACKGROUND: Imaging animal models that offer serial measurement of systemic tumor progression, such as the GFP+ or bioluminescence MM model, have been limited to low resolution, gross measurements of tumor progression that are insufficient to detect individual cells, and their interaction with their microenvironment. Therefore, the need exists for development of sensitive, high resolution three-dimensional imaging methods that identify the dynamic changes that occur during tumor initiation and progression. We here show the use of in vivo fluorescence confocal microscopy to follow MM tumor initiation and progression at the cellular level using stably GFP-transfected MM1S cells in a xenograft model of MM. METHODS: 5 × 10 6 MM1S-GFP-Luc cells were injected into the tail veins of non-irradiated SCID/Beige male mice. MM cell growth in the marrow of the calvarial bone was analyzed using in vivo flow cytometry and fluorescence confocal microscopy, as previously described (Sipkins et al 2005). High-resolution images with unprecedented cellular detail were obtained through the intact mouse skull at depths of up to 250μm. To visualize the bone marrow vasculature the mice were injected with a blood pool marker (Angiosense 680 or 750) immediately before imaging, and to delineate the surface of calvarial bone, a fluorescent hydroxyapatite tag (Osteosense) was used. The validity of the imaging data was established by sacrificing select mice, and analyzing the previously imaged tissues by standard histologic and immunohistologic techniques. After MM tumors became established in the fourth week following injection, 1 mg/kg Bortezomib was administered twice weekly to a subset of the mice, these were imaged following treatment along with controls that were not treated. For all mice imaged, the number and areas of the skull where GFP+ MM cells were found were recorded. Confirmation of homing and tumor progression was also performed using CD138+ selected primary tumor cells. RESULTS: Using this model, we were able to detect and monitor individual GFP+MM cells within the bone marrow microenvironment. We demonstrate that MM.1 S cells and primary CD138+ cells exit the systemic circulation within one hour of injection, followed by specific rolling and adhesion to the vasculature of the bone marrow microenvironment. Within 4 days post after injection, the MM cells were fully engrafted along the bone marrow sinusoids, which were surrounded by bisphosphonate-rich bone structures including ostoeoblasts. Within the second week, loose clusters of a few cells began to form around the blood vessels. Growth and expansion appeared to be closely associated with the vasculature. Tumor growth dramatically increased in the third week following cell injection when areas of the parasagittal regions became completely involved with MM cells. In contrast, standard bioluminescence imaging performed concurrently detected tumor initiation only at 4 weeks post-injection, indicating that confocal microscopy is a much more sensitive technique in detecting early tumor proliferation. Imaging of bortezomib-treated mice demonstrated that tumor size and density was reduced in the skull, but even more dramatically the number of sites containing GFP+MM was greatly reduced. CONCLUSIONS: Our imaging model differs from other models due to its unprecedented resolution. Therefore it is particularly useful for following small numbers of tumor cells either early in disease progression or after therapeutic treatment. This model offers a more sensitive spatial and temporal live imaging of MM cells in the BM microenvironment and can be used to explore the dynamic interaction of MM with different structures and environments of the BM. We anticipate that this model will allow for a better understanding of the biologic effects of therapeutic agents on the growth of MM cells within the bone marrow niches.


Author(s):  
Y. Zhu ◽  
S. Jin ◽  
Y. Tian ◽  
M. Wang

To meet the requirement of high accuracy and high speed processing for wide swath high resolution optical satellite imagery under emergency situation in both ground processing system and on-board processing system. This paper proposed a ROI-orientated sensor correction algorithm based on virtual steady reimaging model for wide swath high resolution optical satellite imagery. Firstly, the imaging time and spatial window of the ROI is determined by a dynamic search method. Then, the dynamic ROI sensor correction model based on virtual steady reimaging model is constructed. Finally, the corrected image corresponding to the ROI is generated based on the coordinates mapping relationship which is established by the dynamic sensor correction model for corrected image and rigours imaging model for original image. Two experimental results show that the image registration between panchromatic and multispectral images can be well achieved and the image distortion caused by satellite jitter can be also corrected efficiently.


1967 ◽  
Vol 31 ◽  
pp. 45-46
Author(s):  
Carl Heiles

High-resolution 21-cm line observations in a region aroundlII= 120°,b11= +15°, have revealed four types of structure in the interstellar hydrogen: a smooth background, large sheets of density 2 atoms cm-3, clouds occurring mostly in groups, and ‘Cloudlets’ of a few solar masses and a few parsecs in size; the velocity dispersion in the Cloudlets is only 1 km/sec. Strong temperature variations in the gas are in evidence.


2019 ◽  
Vol 42 ◽  
Author(s):  
J. Alfredo Blakeley-Ruiz ◽  
Carlee S. McClintock ◽  
Ralph Lydic ◽  
Helen A. Baghdoyan ◽  
James J. Choo ◽  
...  

Abstract The Hooks et al. review of microbiota-gut-brain (MGB) literature provides a constructive criticism of the general approaches encompassing MGB research. This commentary extends their review by: (a) highlighting capabilities of advanced systems-biology “-omics” techniques for microbiome research and (b) recommending that combining these high-resolution techniques with intervention-based experimental design may be the path forward for future MGB research.


1994 ◽  
Vol 144 ◽  
pp. 593-596
Author(s):  
O. Bouchard ◽  
S. Koutchmy ◽  
L. November ◽  
J.-C. Vial ◽  
J. B. Zirker

AbstractWe present the results of the analysis of a movie taken over a small field of view in the intermediate corona at a spatial resolution of 0.5“, a temporal resolution of 1 s and a spectral passband of 7 nm. These CCD observations were made at the prime focus of the 3.6 m aperture CFHT telescope during the 1991 total solar eclipse.


1994 ◽  
Vol 144 ◽  
pp. 541-547
Author(s):  
J. Sýkora ◽  
J. Rybák ◽  
P. Ambrož

AbstractHigh resolution images, obtained during July 11, 1991 total solar eclipse, allowed us to estimate the degree of solar corona polarization in the light of FeXIV 530.3 nm emission line and in the white light, as well. Very preliminary analysis reveals remarkable differences in the degree of polarization for both sets of data, particularly as for level of polarization and its distribution around the Sun’s limb.


1988 ◽  
Vol 102 ◽  
pp. 41
Author(s):  
E. Silver ◽  
C. Hailey ◽  
S. Labov ◽  
N. Madden ◽  
D. Landis ◽  
...  

The merits of microcalorimetry below 1°K for high resolution spectroscopy has become widely recognized on theoretical grounds. By combining the high efficiency, broadband spectral sensitivity of traditional photoelectric detectors with the high resolution capabilities characteristic of dispersive spectrometers, the microcalorimeter could potentially revolutionize spectroscopic measurements of astrophysical and laboratory plasmas. In actuality, however, the performance of prototype instruments has fallen short of theoretical predictions and practical detectors are still unavailable for use as laboratory and space-based instruments. These issues are currently being addressed by the new collaborative initiative between LLNL, LBL, U.C.I., U.C.B., and U.C.D.. Microcalorimeters of various types are being developed and tested at temperatures of 1.4, 0.3, and 0.1°K. These include monolithic devices made from NTD Germanium and composite configurations using sapphire substrates with temperature sensors fabricated from NTD Germanium, evaporative films of Germanium-Gold alloy, or material with superconducting transition edges. A new approache to low noise pulse counting electronics has been developed that allows the ultimate speed of the device to be determined solely by the detector thermal response and geometry. Our laboratory studies of the thermal and resistive properties of these and other candidate materials should enable us to characterize the pulse shape and subsequently predict the ultimate performance. We are building a compact adiabatic demagnetization refrigerator for conveniently reaching 0.1°K in the laboratory and for use in future satellite-borne missions. A description of this instrument together with results from our most recent experiments will be presented.


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