The relationship between the backscattering coefficient and the biomass of narrow and broad leaf crops

2001 ◽  
Vol 39 (4) ◽  
pp. 873-884 ◽  
Author(s):  
G. Macelloni ◽  
S. Paloscia ◽  
P. Pampaloni ◽  
F. Marliani ◽  
M. Gai
Author(s):  
Kendall L. Carder ◽  
David K. Costello

Two important problems facing the ocean optics research community in the coming decade concern optical model closure and inversion (see Chapter 3). We obtain model closure if we can describe the measured light environment by combining elementary measurements of the optical properties of the medium with radiative transfer theory. If we can accurately deduce the concentration of various constituents from a combination of measures of the submarine light field and inverse model calculations, we term this process model inversion. The most elementary measurements of the optical properties of the sea are those that are independent of the geometry of the light field, the inherent optical properties (Preisendorfer, 1961). Optical properties that are dependent on the geometry of the light field are termed apparent optical properties (AOP). Models of the submarine light field typically relate apparent optical properties to inherent optical properties (see Chapter 2). Examples include the relationship between the AOP irradiance reflectance R and a combination of inherent optical properties (backscattering coefficient bb and absorption coefficient a), and the relationship between the AOP downwelling diffuse attenuation coefficient kd and a combination of the absorption coefficient, backscattering coefficient, and downwelling average cosine μd (e.g., Gordon et al., 1975; Morel and Prieur, 1977; Smith and Baker, 1981; Morel, 1988; Kirk, 1984a). Under some circumstances these relationships work well enough that the absorption coefficient can be derived indirectly. This is important since measurement of the absorption coefficient by direct means has been difficult. Derived values for the absorption coefficient by model inversion methods are not easily verified by independent measurements, however, because of the difficulty of measuring the absorption coefficient. Model closure and model inversion both become more tenuous when the following phenomena are present: 1. Transpectral or inelastic scattering such as fluorescence (e.g., Gordon, 1979; Carder and Steward, 1985; Mitchell and Kiefer, 1988a; Spitzer and Dirks, 1985; Hawes and Carder, 1990) or water Raman scattering (Marshall and Smith, 1990; Stavn, 1990; Stavn and Weidemann, 1988a,b; Peacock et al, 1990; Chapter 12 this volume). 2. Particles that are large relative to the measurement volume for inherent optical property meters such as beam transmissometers, light-scattering photometers, fluorometers, and absorption meters.


Author(s):  
J. Zhao ◽  
D. Floricioiu

Synthetic Aperture Radar (SAR) has been widely used in many different fields, such as geoscience, climate monitoring, security-related applications. However, over natural terrain the radar signal has the ability to penetrate the ground surface which can cause the bias in the elevation measurements. The aim of the paper is to assess the SAR signal penetration effect on the TanDEM-X absolute elevation over ice and snow covered areas and it presents the results concerning the X-band SAR signal penetration effect on dry snow areas and blue ice region. Additionally, the relationship between SAR signal penetration depth and backscattering coefficient is exploited and discussed. In this paper, two study sites, Schirmacher area and Recovery Ice Stream are selected and it is found that the general X-band SAR signal penetration depth is around 3–7 meter on dry snow area while no penetration depth is expected on the blue-ice region.


2013 ◽  
Vol 310 ◽  
pp. 366-374 ◽  
Author(s):  
Dominik Seidel ◽  
Christoph Leuschner ◽  
Christoph Scherber ◽  
Friderike Beyer ◽  
Tobias Wommelsdorf ◽  
...  

2018 ◽  
Vol 25 (02) ◽  
pp. 1850047
Author(s):  
A. G. XIE ◽  
H. Y. LIU ◽  
Y. YU ◽  
Y. Q. XIA ◽  
T. Y. WAN

Based on the experimental maximum escape depth [Formula: see text], [Formula: see text] of rediffused electrons from atomic number [Formula: see text] metal at incident energy of primary electron [Formula: see text], the relationship among [Formula: see text], [Formula: see text], [Formula: see text] and [Formula: see text] in the energy range of 9.3[Formula: see text]keV[Formula: see text]40[Formula: see text]keV was obtained and proved to be true by experimental data. According to the experimental results of rediffused electrons, the characteristics of secondary electron emission, relationships among parameters of rediffused electrons and the main processes of rediffused electrons emission, the formula for [Formula: see text] backscattering coefficient [Formula: see text], [Formula: see text], [Formula: see text] of [Formula: see text] metal films with film thickness [Formula: see text] as a function of [Formula: see text], Z and was deduced, and the results were analyzed. It is concluded that the deduced formula for [Formula: see text], [Formula: see text], [Formula: see text] can be used to calculate [Formula: see text], [Formula: see text], [Formula: see text] in the energy range of 9.3[Formula: see text]keV[Formula: see text]40[Formula: see text]keV. The secondary electron yield [Formula: see text] from thin films are applied in more and more fields such as electronic information technology, accelerator and space flight, and [Formula: see text], Z, [Formula: see text] is an important parameter of [Formula: see text] from [Formula: see text] metal films. So deducing the formula for [Formula: see text], [Formula: see text], [Formula: see text] in this study is necessary.


1967 ◽  
Vol 31 ◽  
pp. 239-251 ◽  
Author(s):  
F. J. Kerr

A review is given of information on the galactic-centre region obtained from recent observations of the 21-cm line from neutral hydrogen, the 18-cm group of OH lines, a hydrogen recombination line at 6 cm wavelength, and the continuum emission from ionized hydrogen.Both inward and outward motions are important in this region, in addition to rotation. Several types of observation indicate the presence of material in features inclined to the galactic plane. The relationship between the H and OH concentrations is not yet clear, but a rough picture of the central region can be proposed.


Paleobiology ◽  
1980 ◽  
Vol 6 (02) ◽  
pp. 146-160 ◽  
Author(s):  
William A. Oliver

The Mesozoic-Cenozoic coral Order Scleractinia has been suggested to have originated or evolved (1) by direct descent from the Paleozoic Order Rugosa or (2) by the development of a skeleton in members of one of the anemone groups that probably have existed throughout Phanerozoic time. In spite of much work on the subject, advocates of the direct descent hypothesis have failed to find convincing evidence of this relationship. Critical points are:(1) Rugosan septal insertion is serial; Scleractinian insertion is cyclic; no intermediate stages have been demonstrated. Apparent intermediates are Scleractinia having bilateral cyclic insertion or teratological Rugosa.(2) There is convincing evidence that the skeletons of many Rugosa were calcitic and none are known to be or to have been aragonitic. In contrast, the skeletons of all living Scleractinia are aragonitic and there is evidence that fossil Scleractinia were aragonitic also. The mineralogic difference is almost certainly due to intrinsic biologic factors.(3) No early Triassic corals of either group are known. This fact is not compelling (by itself) but is important in connection with points 1 and 2, because, given direct descent, both changes took place during this only stage in the history of the two groups in which there are no known corals.


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