The nature of seismic noise

When seismic signals from impulsive sources are reflected or refracted by discrete inhomogeneities in the seismic medium, ‘arrivals’ are recorded. If, however, the number of inhomogeneities becomes large and the distance between them becomes small, then interference among the arrivals takes place and source-caused ‘noise ’ is recorded. If the spacing between observatories is large compared with the spacing between and dimensions of the scatterers, the source-caused noise is incoherent. If the number of scatterers is large enough for the problem to be treated statistically, the noise has a random character. The properties of the noise can be computed by averaging statistically over all the signals due to the scattering from the ensemble of scatterers. Single scattering only is treated here. There are ‘local’ or ‘end’ effects corresponding to scattering near the source or the receiver which cannot be taken into account in the calculations. The main problem which has been treated is that of the scattering of body waves of P and S types in an unbounded inhomogeneous medium. The magnitudes of the scattered waves of all types— PP, PS, SP, SS —have been computed. In addition the phase shifts (time delays or advances) in incident P and S can be computed. It is found that body waves of either P or S type convert into scattered S waves with considerably greater ease than into scattered P waves. The comparative efficiency of these processes is about two orders of magnitude. Thus P waves show small phase shifts; S waves show large phase shifts. The waves between P and S are most likely of the character of S . The approximations in the calculations involve the assumptions of wavelength long compared with the dimensions of the scatterer and the dimensions of the scattering region long compared with wavelength. Under these conditions the approximations are those for Rayleigh scattering. Hence, in all the results, the scattering varies as the fourth power of the frequency and the mean square scattered energy is proportional to the linear dimension of the scattering region. At higher frequencies, the scattering changes from a fourth power dependence upon frequency to a second power dependence. This is a result which is obtained only for scattering by elastic media; it is not found in media without shear modulus. Experimental evidence for this high frequency effect has been found.

2003 ◽  
Vol 285 (4) ◽  
pp. R917-R925 ◽  
Author(s):  
R. E. Mistlberger ◽  
M. C. Antle ◽  
I. C. Webb ◽  
M. Jones ◽  
J. Weinberg ◽  
...  

Circadian rhythms in the Syrian hamster can be markedly phase shifted by 3 h of wheel running or arousal stimulation during their usual daily rest period (“subjective day”). Continuous wheel running is predictive but not necessary for phase shifts of this “nonphotic” type; hamsters aroused by gentle handling without running can also show maximal shifts. By contrast, physical restraint, a standard stress procedure and thus presumably arousing, is ineffective. To resolve this apparent paradox, phase-shifting effects of 3-h sessions of restraint or other stress procedures were assessed. In a preliminary study, phase shifts to arousal by gentle handling were significantly potentiated by the cortisol synthesis inhibitor metyrapone, suggesting that stress-related cortisol release may inhibit phase shifts to arousal. Next, it was confirmed that restraint in the subjective day does not induce phase shifts, but behavioral observations revealed that it also does not sustain arousal. Restraint combined with noxious compressed air blasts did sustain arousal and induced a significant cortisol response compared with arousal by gentle handling but did not induce shifts. Restraint combined with continuous horizontal rotation was also ineffective, as was EEG-validated arousal via confinement to a pedestal over water. However, 3 h of resident-intruder interactions (an intense psychosocial stress) or exposure to an open field (a mild stress) did induce large shifts that were positively correlated with indexes of forward locomotion. The results indicate that large phase shifts associated with arousal in the usual sleep period are neither induced nor prevented by stress per se, but are dependent on the expression of at least low levels of locomotor activity. Sustained arousal alone is not sufficient.


1991 ◽  
Vol 69 (8-9) ◽  
pp. 1166-1174 ◽  
Author(s):  
Jacek W. Kaminski ◽  
John C. McConnell

In a planetary atmosphere the J value is determined by the angular-averaged radiance, or the average density of photons in an element of volume. The average density may be enhanced by multiple scattering of photons in a conservative, or near-conservative scattering atmosphere. We show that in a conservative semi-infinite medium this enhancement will be a factor of 5, for optical depths greater than about 20 for coherent scattering. We investigate the modification of the J values owing to multiple scattering in an optically thick medium of various optical depths, various single-scattering albedos of the scattering medium, and a range of surface albedos. We have applied the results to the calculation of J values in clouds in the terrestrial atmosphere and in the Rayleigh-scattering atmosphere of Uranus. We note that J values in a realistic atmosphere may be enhanced by as much as a factor of 5 throughout a large fraction of the atmosphere over those calculated without multiple scattering and surface reflection.


1965 ◽  
Vol 87 (3) ◽  
pp. 381-387 ◽  
Author(s):  
L. B. Evans ◽  
C. M. Chu ◽  
S. W. Churchill

Numerical values are presented for the reflection and transmission of radiation falling obliquely on finite slabs of absorbing and anisotropically scattering material. The angular distribution for single scattering was represented by a finite series of Legendre polynomials. The method of Chandrasekhar was used to reduce the representation of radiant transport from an integrodifferential equation to a set of integral equations. This set of equations was solved reiteratively on a digital computer. Previous solutions have been limited to isotropic and Rayleigh scattering or infinite media. The results for different phase functions for single scattering can be interpreted reasonably well in terms of only the forward-scattered fraction.


2005 ◽  
Vol 30 (19) ◽  
pp. 2605 ◽  
Author(s):  
Yinlan Ruan ◽  
Barry Luther-Davies ◽  
Weitang Li ◽  
Andrei Rode ◽  
Vesslin Kolev ◽  
...  

Author(s):  
J.H Hannay

Daylight, or sky light, is sunlight Rayleigh scattered by the atmosphere onto the ground. This random scattering propagation through clear air is governed by ‘radiative transfer’. Beyond the single-scattering approximation, the famous virtuoso analysis of Chandrasekhar formulated the problem and offered exact, but rather involved, and ultimately numerical, algorithms for its solution. However, there is no real difficulty in writing down directly the exact Rayleigh scattering series in integrals. Its practical utility is limited to fairly small thicknesses T of atmosphere (compared with the mean free path), but the Earth has just such. Here even the next order beyond single scattering (error order T 2 ) supplies a formula for the brightness and partial polarization of daylight across the sky, which captures the essential topology of the polarization pattern, and also remains uniformly valid in the small thickness limit, for all elevations of the Sun and viewing angles. The status of the mathematical polarization direction pattern invented by Berry, Dennis and Lee as the simplest fit to the required topology is clarified.


1971 ◽  
Vol 49 (11) ◽  
pp. 1536-1539 ◽  
Author(s):  
H. Stocker ◽  
E. H. Berkowitz

Charge state fractions, 5+, 6+, 7+, and 8+, of high energy 16O ions between 18.7 and 59.7 MeV were measured and ratios of charge state fractions differing by one charge unit were found to follow an inverse fourth power dependence. The average ionic charge of a 16O beam varies from 6.4 to 7.6 over this range.


1977 ◽  
Vol 67 (5) ◽  
pp. 1277-1290
Author(s):  
L. Martel ◽  
M. Munasinghe ◽  
G. W. Farnell

abstract The transmission and reflection of a Rayleigh wave through a step on a homogeneous half-space of Poisson's ratio σ = 0.253 have been investigated by a seismic models method. The experimental results show good agreement with numerical ones obtained by finite-difference calculations when the wave is incident onto a downward step. Phase shifts are given both for the upward and downward steps. The characteristics of the transmitted wave do not depend much on the direction of propagation but those of the reflected wave are clearly direction-dependent. In each case the transmission and reflection coefficients and phase shifts depend on the ratio of step height to wavelength. The group delays are calculated and they are positive or negative depending on the period. About 80 per cent of the incident energy is converted into body waves when the step is higher than 0.3 times the wavelength of the Rayleigh wave.


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