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31.
An improved formula for the green-to-red line intensity ratio in the solar corona is proposed. The results are compared with those given by the previous expression.  相似文献   
32.
Autoionization rate coefficients for some ions found in solar corona have been computed in the temperature range 105–108 K semiempirically. In each case the coefficients decrease as we go from less to more ionized ones and have a typical temperature dependence.  相似文献   
33.
The common Indian freshwater catfish, Heteropneustes fossilis, was exposed to the 96 h-LC50 (0.007-0.013 ppm) of the organochloride thiodan (endosulfan) for 4 days. The stressed fishes showed various histopathological changes. In the liver, extensive degeneration of cytoplasm, pycnosis of nuclei, and loss of glycogen was observed most commonly. Stasis of circulation and constriction of bile duct lumen was also seen frequently. In the kidney, shrinkage of glomeruli, cytoplasmic damage and epithelial desquamation in tubules, and extensive degeneration of hemopoietic stroma was commonly observed. In the intestine, the damage was comparatively negligible, the most common effect was an increased mucus cell activity leading to accumulation of mucoid exudates in the lumen.  相似文献   
34.
Summary The equation for density perturbation induced by plane hydromagnetic waves (responsible for geomagnetic secular variation) has been derived based on -plane formulation. It is deduced that for the usual physical properties of the earth's core such a density perturbation would be small and would not be, in the main, responsible for the recently discovered correlation between gravitation and geomagnetic potentials.  相似文献   
35.
Summary Different results have been obtained by Negi and Wait in connection with the effect of overburden in electromagnetic exploration by assuming different definitions of screening factor. Both definitions are based on frequency domain considerations. We shall describe the screening characteristics for a transient field with a two-concentric shell model with screening factor=(magnetic field of target and screen-magnetic field of screen alone)/(field of target alone). It is found that the screening factor does become more than one in some situations which means that the EM response of target is more in some cases when the screen is present than when it is absent.Presented at the fifty-second Annual Meeting of AGU during April 12–16, 1971, Washington, D.C.  相似文献   
36.
Summary A matrix formalism is developed to facilitate computation of temperature distribution in the steady state in the interior of a multi-layered earth. The idealized model consists of homogeneous and isotropic layers of constant (but arbitrary) values of heat production as well as thermal conductivities. The known surface data is continued by this method to define the thermal structure at any desired point of the interior for planar and spherical stratification. Extension of the problem to the unsteady flow conditions has been presented.  相似文献   
37.
38.
Summary. The conventional assumption of the equality of the slope of the empirical linear heat flow/heat generation relation and the logarithmic decrement in the exponential model of the heat production is not valid. The rigorous analysis of the heat flow equation shows that, with the increase of the magnitude of the slope, the invalidity becomes significant. In the Indian shield region, the available estimate of the slope is 14.8 km, while the corresponding logarithmic decrement value is 17.2 km, However, it may be emphasized that in the step model the slope is rightly interpreted as the thickness of the radioactive layer.  相似文献   
39.
Summary The paper describes a theoretical investigation of heat transfer in stratified horizontal slab and spherical shell containing temperature dependent heat sources. The desired expressions of temperatures contain only ordinary functions suitable for high speed computation. The results can find applications in defining the local and global temperature distributions in the earth's crust.  相似文献   
40.
We have investigated some properties such as speed, apparent width, acceleration, latitude, mass and kinetic energy, etc. of all types of coronal mass ejections (CMEs) observed during the period 1996–2007 by SOHO/LASCO covering the solar cycle 23. The results are in satisfactory agreement with previous investigations.  相似文献   
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