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11.
P. C. Lightfoot C. J. Hawkesworth J. Hergt A. J. Naldrett N. S. Gorbachev V. A. Fedorenko W. Doherty 《Contributions to Mineralogy and Petrology》1993,114(2):171-188
The Late Permian to Early Triassic Siberian Traps have been sampled by drill core (core SG-9) and from surface exposure (section 1F) in the Noril'sk region of the Siberian Platform, Russia. Combined major, trace element, and Nd-, Sr-, and Pb-isotope data on selected samples through the Siberia Trap, offer new chemostratigraphic criteria for the identification and characterisation of two fundamentally different magma types and 9 of the 11 formations of lava developed near Noril'sk. A Lower Sequence of sub-alkalic basalts, tholeiites, and picritic basalts (upwards these are the Ivakinsky, Syverminsky, and Gudchichinsky formations) are overlain by an Upper Sequence of picritic basalts and tholeiites interbedded with tuffs (upwards, these are the Khakanchansky, Tuklonsky, Nadezhdinsky, Morongovsky, Mokulaevsky and Kharayelakhsky formations).The Gudchichinsky and Tuklonsky formations contain both picritic and tholeiitic lavas. The Tuklonsky formation tholeiites and picrites have moderate Gd/Yb (1.6–1.8), low TiO2 (0.45–0.95 wt%), a significant negative Ta and Nb anomaly (Nb/La =0.42–0.57) and unradiogenic Nd (
Nd
CHUR
= to -4.6). In contrast, both the Gudchichinsky formation tholeiites and picrites have high Gd/Yb (2.3–3.1), and TiO2 (1.2–2.3 wt%), no significant Nb or Ta anomaly (Nb/La =0.8–1.1), and radiogenic Nd (
Nd
CHUR
= to 7.3). The low-Ti and Nb/La, high La/Sm, and unradiogenic Nd-isotope signatures of the picritic Tuklonsky formation lavas and the tholeiitic lavas of the Upper Sequence are characteristic of magmas strongly influenced by material from the continental lithosphere, whereas the high-Ti and Nb/La, low La/Sm and radiogenic Nd-isotope signatures of the Lower Sequence are more comparable to deeper asthenospheric mantle-plume generated lavas similar to oceanic island basalts. The lavas overlying the Tuklonsky formation have mg-numbers of 0.63 to 0.68, and are more evolved than the Tuklonsky (Mg-number < 0.62) and have more radiogenic
Nd
CHUR
(Tuklonsky:-0.03 to-4.66; Mokulaevsky: + 0.60 to + 1.61), but have many of the incompatible trace element features of the Tuklonsky sky type magma. These lavas show a progressive upwards decline in SiO2 (55–49 wt%), La/Sm (4.6–2.0), and
UR
Sr
( + 67 to + 13) which has previously been attributed to a decrease in the proportion of crustal material contributed to the magma. This paper explores and alternative model where a component of the crustal contribution might be derived from within an ancient region of the mantle lithosphere as recycled sediment rather than from the overlying continental crust. 相似文献
12.
V. N. Fedorenko 《Astrophysics and Space Science》1990,163(2):187-200
I give an interpretation of a result of Simpsonet al. (1988) on the variation with kinetic energyT
i
of the mean pathlengthX
m
(T
i
) of the galactic cosmic rays (CGRs) in the range 0.1T
i
10.0 GeV nucl–1. I argue that the data onX
m
(T
i
) may be interpreted in terms of a model of GCR diffusion on the one-dimensional Alfvén-wave turbulence, having a cutoff in the spectrum at frequencies
h
, where
h
is the proton gyrofrequency. The cutoff results in changing of the character of variation of the GCR diffusion coefficientD(T
i
)T
a
in the rangeT
i
1 GeV nucl–1 towards some more complicated variation at 0.1T
i
1.0 GeV nucl–1 due to the peculiarities of the pitch-angle scattering at 900. 相似文献
13.
The dependence of energy transport by acoustic gravity waves (AGWs) on their spectral properties is studied. On the basis
of the analysis of expressions for group velocities and energy fluxes of AGWs, it is shown that there exist separate frequencies
and wavelengths at which the energy transport in space is most efficient. Comparison of the obtained results with the data
of observations on board the Dynamic Explorer 2 satellite shows that, in the upper atmosphere of the Earth’s polar regions,
AGWs with spectral parameters corresponding to the maximum of energy transport predominate. 相似文献
14.
The peculiarities of the distribution of medium-scale acoustic gravity waves (AGWs) in polar regions according to the data
of measurements on board the Dynamics Explorer 2 satellite are studied. Over polar regions of both hemispheres at heights
of 250–400 km, wave variations in neutral atmospheric parameters were systematically registered. These variations were identified
as AGWs with horizontal wavelengths of 500–650 km. The relative amplitudes of polar AGWs in a neutral concentration reach
10%. Wave trains extend over the polar caps to thousands of kilometers and show a distinct spatial relationship with the auroral
oval. A systematic direction is found in AGW propagation from the nighttime sector of the oval into the day-time sector, where
wave activity is strictly limited. An assumption is formulated that this restriction is caused by dynamic interactions between
AGWs and the zonal wind in the daytime sector of the auroral oval. 相似文献
15.
16.
17.
The phenomenological model of condensation interaction between galactic cosmic rays (GCRs) and water vapor, which makes it possible to estimate atmospheric pressure variations at different altitudes with changing GCR flux, has been developed. It has been indicated that pressure should increase at all altitudes in the considered interval (0–5 km above sea level) during Forbush decreases. Therefore, the correlation between pressure and GCR flux under mountain conditions can be negative as near sea level. However, the performed calculation of the cross-correlation function of the series of daily data, obtained at Jungfraujoch station (3475 m) in 1968–1992, indicated that this correlation is positive and statistically significant with a maximum leading the GCR variation onset by two days. As usual, pressure increased during Forbush decreases due to the condensation mechanism. The obtained results can be explained by the manifestation of the optical mechanism related to solar flares, which operates together with the condensation mechanism and causes a decrease in pressure at high altitudes. It has been indicated that the effectiveness of this mechanism substantially changes with the phase of the quasibiennial cycle. 相似文献
18.
Some peculiarities of the use of a laser for the determination of the instrumental profile of the high-resolution spectrograph have been described. The results of the investigation of the instrumental profile of the Kiev-Golosejevo double-pass solar spectrograph are presented in graphs.The influence of the width of the slits of the double-pass spectrograph upon the main features of its instrumental profile is discussed briefly. 相似文献
19.
According to measurements on the Dynamic Explorer 2 satellite, features of the propagation of acoustic gravity waves (AGWs) in the multicomponent upper atmosphere have been investigated. In the altitude range 250–400 km in wave concentration variations of some atmospheric gases, amplitude and phase differences have been observed. Using the approach proposed in this paper, in different gases, AGW variations have been divided into components associated with elastic compression, adiabatic expansion, and the vertical background distribution. The amplitude and phase differences observed in different gases are explained on the basis of analyzing these components. It is shown how to use this effect in order to determine the wave propagation, the vertical displacement of the volume element, the wave frequency, and the spatial distribution of the wave energy density. 相似文献
20.
Manninen J. Kleimenova N. G. Gromova L. I. Fedorenko Yu. V. Nikitenko A. S. Lebed’ O. M. 《Geomagnetism and Aeronomy》2020,60(3):301-310
Geomagnetism and Aeronomy - This paper discusses the spectral and temporal features of the 7-h daytime VLF noise emission burst in the frequency band of 1‒10 kHz observed on the Earth’s... 相似文献