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1.
A garnet-omphacite-kyanite-coesite geothermobarometer is constructed to estimate the peak metamorphic pressure of ultrahigh-pressure
(UHP) eclogites. For this we use a quaternary regular solution model for garnet, and propose a new model for sodic pyroxene
that assumes double site solid-solution (Na,Ca)M2(Al,Fe3+,Fe2+,Mg)M1Si2O6, where cations in the M2- and the M1-sites mix randomly but with inter-site interactions, not only between nearest neighboring
cations but also between next nearest neighboring cations. In the new model, overall excess interaction parameters are quantitatively
deduced from the previous experimental data and critical temperature, and the activity of the jadeite component agrees reasonably
with that based on the Landau theory. Furthermore, the relations of the calculated order parameter to temperature and composition
are consistent with other experimental works. These facts support the usefulness of the new model. Application of our geothermobarometer
to kyanite eclogite gave metamorphic conditions around 3.4 GPa and 800 ∘C for both samples from the Dora Maira Massif, Western Alps, and from Rongcheng County, in the Su-Lu region of eastern China.
Received: 30 December 1996 / Accepted: 25 August 1997 相似文献
2.
Two types of biotite isograd are defined in the low-grade metamorphism of the Wazuka area, a Ryoke metamorphic terrain in the Kii Peninsula, Japan. The first, BI1, is defined by the reaction of chlorite+K-feldspar= biotite+muscovite+quartz+H2O that took place in psammitic rocks, and the second, BI2, by the continuous reaction between muscovite, chlorite, biotite and quartz in pelitic rocks. The Fe/Mg ratios of the host rocks do not significantly affect the reactions. From the paragenesis of pelitic and psammitic metamorphic rocks, the following mineral zones were established for this low-pressure regional metamorphic terrain: chlorite, transitional, chlorite-biotite, biotite, and sillimanite. The celadonite content of muscovite solid solution in pelitic rocks decreases systematically with the grade of metamorphism from 38% in the chlorite zone to 11% in the biotite zone. Low pressure does not prohibit muscovite from showing the progressive change of composition, if only rocks with appropriate paragenesis are chosen. A qualitative phase diagram of the AKF system relevant to biotite formation suggests that the higher the pressure of metamorphism, the higher the celadonite content of muscovite at BI1, which is confirmed by comparing the muscovites from the Barrovian and Ryoke metamorphism. 相似文献
3.
We investigate a possibility that non-thermal X-ray emission in a supernova remnant(SNR) is produced by jitter radiation,
which is the analogue of synchrotron radiation in small-scale random magnetic fields. We can fit the multi-wavelength data
of SNRs RX J1713.7-3946 (G347.3-0.5) and RX J0852.0-4622 (G266.6-1.2) by constructing pure jitter and inverse Compton (IC)
emission models. We find that the physical fit parameters of random magnetic fields take values of several tens of μG strength
and of the order of ∼107 cm correlation length. These properties of random magnetic fields in collisionless shock of SNRs are discussed.
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4.
The structure of the cosmic ray electron halo of a starburst galaxy depends strongly on the nature of galactic wind and the
configuration of the magnetic field. We have investigated these dependencies by solving numerically the propagation of electrons
originating in starburst galaxies, most likely in supernova remnants. The calculations are made for several models for the
galactic winds and for the configuration of the magnetic fields for comparison with observations. Our simulation of a quasi-radio
halo reproduces both the extended structure of ∼9 kpc and the subtle hollow structure near the polar region of the radio halo
that are observed in the starburst galaxy NGC 253. These findings suggest the existence of strong galactic wind in NGC 253.
相似文献
5.
The abundance of extinct radioactive nucleus202Pb trapped in chondrites is calculated from the anomalous isotopic ratio202Hg/196Hg, assuming the isotopic anomalies are only due to the decay of202Pb. The magnitude of nonuniformity of the distribution of202Pb inferred from the excess isotopic abundance of202Hg is the same order of magnitude suggested by anomalous isotopic abundances of the other chemical elements found in meteoritic materials. 相似文献
6.
Y. Mizumura J. Kushida K. Nishijima G.V. BicknellR.W. Clay P.G. EdwardsS. Gunji S. HaraS. Hayashi S. KabukiF. Kajino A. KawachiT. Kifune R. KiuchiK. Kodani Y. MatsubaraT. Mizukami Y. MizumotoM. Mori H. MuraishiT. Naito M. OhishiV. Stamatescu D.L. SwabyT. Tanimori G. ThorntonF. Tokanai T. ToyamaS. Yanagita T. YoshidaT. Yoshikoshi 《Astroparticle Physics》2012,35(9):563-572
We have searched for very high energy (VHE) gamma rays from four blazars using the CANGAROO-III imaging atmospheric Cherenkov telescope. We report the results of the observations of H 2356-309, PKS 2155-304, PKS 0537-441, and 3C 279, performed from 2005 to 2009, applying a new analysis to suppress the effects of the position dependence of Cherenkov images in the field of view. No significant VHE gamma ray emission was detected from any of the four blazars. The GeV gamma-ray spectra of these objects were obtained by analyzing Fermi/LAT archival data. Wide range (radio to VHE gamma-ray bands) spectral energy distributions (SEDs) including CANGAROO-III upper limits, GeV gamma-ray spectra, and archival data, even though they are non-simultaneous, are discussed using a one-zone synchrotron self-Compton (SSC) model in combination with a external Compton (EC) radiation. The HBLs (H 2356-309 and PKS 2155-304) can be explained by a simple SSC model, and PKS 0537-441 and 3C 279 are well modeled by a combination of SSC and EC model. We find a consistency with the blazar sequence in terms of strength of magnetic field and component size. 相似文献
7.
山东海阳所麻粒岩向过渡榴辉岩转化的变质动力学过程及其构造意义 总被引：8，自引：3，他引：5
在山东半岛东南端的乳山海阳所,角闪岩和长英质片麻岩呈互层产出.在某些角闪岩层的中心残留有弱变形的麻粒岩和强变形的过渡榴辉岩(斜长石榴辉岩)团块.在弱变形的麻粒岩团块中发育有窄的(<1cm)剪切条带.沿着这些剪切条带和在强变形过渡榴辉岩团块中,原麻粒岩被转化为含斜长石的过渡榴辉岩.变形和流体在这一转化过程中加速了元素扩散和迁移的速度,在变形强和有流体加入的部位麻粒岩向榴辉岩转化的程度明显增强.麻粒岩相矿物组合(Cpx-Ⅰ+Opx+Pl-Ⅰ+ Hbl-Ⅰ + Grt-Ⅰ+ Ilm)及其花岗变晶结构被完好地保存于弱变形的麻粒岩中,其矿物成分显示出0.8～0.9 GPa和780℃～830℃的麻粒岩相变质条件.榴辉岩相叠加在麻粒岩中形成了一系列的环边状矿物和结构:环边状石榴石(Grt-Ⅱ)形成于麻粒岩相斜长石(Pl-Ⅰ)和暗色矿物(如Cpx-Ⅰ、Opx和Hbl-Ⅰ)的交界处,细粒石榴石(Grt-Ⅱ)、富钠单斜辉石(Cpx-Ⅱ)和石英形成于麻粒岩相角闪石(Hbl-Ⅰ)的外缘.同时榴辉岩相叠加造成麻粒岩相单斜辉石边缘钙契尔马克组份的降低和硬玉组份的升高.但在弱变形的麻粒岩中,麻粒岩相单斜辉石(Cpx-Ⅰ)的外缘并无榴辉岩相单斜辉石形成.沿着弱变形麻粒岩中的剪切条带和在过渡榴辉岩中,榴辉岩相矿物[Grt-Ⅱ+ Omp/Di(Cpx-Ⅱ)+ Ab(Pl-Ⅱ)+ Qtz + Hbl-Ⅱ+ Ky + Zo + Rut]广泛发育,它们的定向排列形成了明显的面理.其形成的温压条件为1.0～1.4 GPa和560℃～680℃,为过渡榴辉岩相变质.虽然其中仍然残留有被拉长的麻粒岩相单斜辉石,但它们含有很高的硬玉组份,且其外缘环绕有细粒的钠质透辉石或绿辉石(Cpx-Ⅱ).海阳所榴辉岩相变质的温压条件远远低于位于海阳所东南和东北的苏鲁超高压变质带中柯石英榴辉岩变质的温压条件.因此海阳所地区代表一条不同于超高压变质带的冷榴辉岩带,它可能与大别山南部的冷榴辉岩带相当.苏鲁超高压变质带的南部边界位于海阳所以北. 相似文献
8.
9.
Garnet-orthopyroxene and orthopyroxene-clinopyroxene relationships in simple and complex systems 总被引：10，自引：2，他引：10
Use of simple mixing models of orthopyroxene and garnet solid solutions enables extrapolation of experimentally determined equilibria in the MgSiO3-Al2O3 system to uninvestigated parts of pressure-temperature-composition space. Apparent discrepancies in the experimental data for simple and multicomponent systems may be explained by considering the effect of CaO and FeO on reducing pyrope activity in the garnet solid solutions. Equilibration pressures of natural garnet-orthopyroxene assemblages may be calculated, provided temperatures are known, from a combination of the experimental data on the MgSiO3-Al2O3 system and analyses of coexisting natural phases.Despite the presence of a compositional gap in the system, the solubility of enstatite in diopside coexisting with orthopyroxene can also be approximately treated by an ideal solution model. An empirical approach has been developed to take account of Fe2+ on the orthopyroxene-clinopyroxene miscibility gap in natural systems in order to calculate equilibration temperatures of 2-pyroxene assemblages. The model presented reproduces almost all of the available experimental data for multicomponent systems to within 60° C. 相似文献
10.
In pelitic schists of the Sanbagawa metamorphic belt, sphene, rutile, and ilmenite occur as discrete grains, in composite aggregates, and as inclusions in garnets. Textural relationships, disposition of inclusions in garnet, and the compositions of ilmenites suggest that the titanium-bearing accessories stable at the peak metamorphic conditions were as follows: sphene in the chlorite zone, sphene plus rutile in the garnet zone, and ilmenite in the highest grade of the belt, the biotite zone. Rutile appears in the garnet zone as a consequence of Ca incorporation into garnet and a progressive increase in
.Retrograde reactions were responsible for the composite aggregates of rutile, sphene and ilmenite and these must be carefully evaluated before prograde relationships between titanium-bearing accessories can be properly understood. 相似文献