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11.
J. F. Prieto P. J. González A. Seco G. Rodríguez-Velasco L. Tunini P. A. Perlock A. Arjona A. Aparicio A. G. Camacho J. B. Rundle K. F. Tiampo J. L. G. Pallero S. Pospiech J. Fernández 《Pure and Applied Geophysics》2009,166(8-9):1461-1484
We review the results of the geodetic and structural studies carried out on La Palma Island using geodetic and geophysical data during the period 1992–2007. InSAR and GPS observation techniques were applied to study the existence of deformation on the island and gravity observations were carried out for structural studies. Gravity data were inverted using a nonlinear three-dimensional gravity inversion approach to obtain the geometry of the anomalous bodies constructed in a random growth process with respect to an exponentially stratified background. The main structural feature is a large central body (under the Caldera de Taburiente) with high density, which was interpreted as the Pliocene-age uplifted seamount and a relatively dense intrusive plutonic complex/magma body. The Cumbre Vieja series is characterized by elongated minima distributed according to the rift structure. InSAR results show a clear subsidence located on the Teneguía volcano, where the last eruption took place in 1971. A thermal source is the most probable origin for this deformation. A GPS network composed of 26 stations covering the total island surface was set up. Vertical displacements determined comparing the GPS coordinates obtained in 2007 with coordinates determined in 1994 are consistent with the InSAR results obtained in the southern part of the island. This is not the case for the northern part. From the comparison of 2006 and 2007 coordinates it is clear that more time is needed to obtain significant displacements, but observed trends are also consistent with InSAR results. All the observed significant displacements are in stations located outside of the large high-density central body. 相似文献
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Alfredo Aparicio Colombo C.G. Tassinari Roberto García Vicente Araña 《Journal of Volcanology and Geothermal Research》2010,189(1-2):143-150
The lavas produced by the Timanfaya eruption of 1730–1736 (Lanzarote, Canary Islands) contain a great many sedimentary and metamorphic (metasedimentary), and mafic and ultramafic plutonic xenoliths. Among the metamorphosed carbonate rocks (calc-silicate rocks [CSRs]) are monomineral rocks with forsterite or wollastonite, as well as rocks containing olivine ± orthopyroxene ± clinopyroxene ± plagioclase; their mineralogical compositions are identical to those of the mafic (gabbros) and ultramafic (dunite, wherlite and lherzolite) xenoliths. The 87Sr/86Sr (around 0.703) and 143Nd/144Nd (around 0.512) isotope ratios of the ultramafic and metasedimentary xenoliths are similar, while the 147Sm/144Nd ratios show crustal values (0.13–0.16) in the ultramafic xenoliths and mantle values (0.18–0.25) in some CSRs. The apparent isotopic anomaly of the metamorphic xenoliths can be explained in terms of the heat source (basaltic intrusion) inducing strong isotopic exchange (87Sr/86Sr and 143Nd/144Nd) between metasedimentary and basaltic rocks. Petrofabric analysis also showed a possible relationship between the ultramafic and metamorphic xenoliths. 相似文献
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E. Banda E. Suriñach A. Aparicio J. Sierra E. Ruiz de la Parte 《Geophysical Journal International》1981,67(3):779-789
Summary. Quarry blasts recorded along three lines on the central Iberian Meseta are used in an attempt to interpret the crustal structure. The results of the interpretation of the data, together with published surface wave and earthquake data, suggest a layered structure of the crust having the following features: the basement, in some areas covered by up to 4 km of sediments, has a P -velocity of 6.1 km s−1 ; a low-velocity layer, between 7 and 11 km depth, seems to exist on the basis of both P and S interpretation of seismic data; a thick middle crust of 12 km has a P -velocity of 6.4 km s−1 and overlies a lower crust with a mean P -velocity of 6.9 km s−1 and a possible slight negative gradient; the mean v p / v s ratio for the crust is about 1.75; the Moho is reached at about 31 km depth and consists of a transition zone at least 1.5 km thick. The P -velocity of the upper mantle is close to 8.1 km s−1 and the S -velocity about 4.5 km s−1 , which gives a v p /v s ratio of 1.8 for the uppermost mantle. A tentative petrological interpretation of the velocities and composition of the layers is given. 相似文献
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J. López Ruiz A. Aparicio L. García Cacho 《International Journal of Earth Sciences》1980,69(1):94-106
Muscovites in metapelites belonging to the Chloritoid, Staurolite, Kyanite, Sillimanite-K feldspar and Sillimanite-K feldspar-Cordierite zones of the Sierra de Guadarrama metamorphic area, have a chemical composition close to the end member Ms (mean value around Ms 92); nevertheless, they show definite variations in Al2O3, K2O and Na2O contents and, to a lesser extent, in FeO and MgO.These chemical variations (i. e., a progressive decrease of celadonite content, a increase followed by a decrease in paragonite solid solution towards compositions close to the endmember muscovite) may be regarded as in a close relationship with metamorphic grade in the upper metamorphic zones (Chloritoid, Staurolite and Kyanite zones), but the corresponding variations in the remaining lower zones (that is, a slight increase in Fe and Mg coupled with a slight increase in AlVI and Ti, and more or less abrupt changes in Na and K contents) can only be explained considering the interference of anatectic phenomena, which modificate the normal trends due to changes in metamorphic grade.As a consequence of these observations, it has been concluded that muscovite composition in metapelites can only be used as an indicator of metamorphic grade in conditions where partial melting phenomena are absent.
Zusammenfassung Muskovite in Metapeliten, die zu den Chloritoid, Staurolit, Cyanit, Sillimanit-K-Feldspat und Sillimanit-K-Feldspat-Cordierit Zonen der Sierra Guadarrama Metamorphgebiet gehören, zeigen einen Chemismus, der sich dem Endglied Muskovit nähert (Durchschnitt etwa Ms 92). Es wurden trotzdem bestimmte Veränderungen in den Gehalten von hauptsächlich Al2O3, K2O und Na2O und in geringerem Ausmaß in FeO und MgO festgestellt.Diese chemischen Veränderungen (d. h. ein progressives Abnehmen des Keladonitgehaltes, gefolgt von einer Abnahme der Paragonitmischungsreihe in einer Richtung, die sich dem Endglied Muskovit annähert) können in einem engen Zusammenhang mit der höher metamorphen Zone (Chloritoid-, Staurolit- und Cyanitzonen) gesehen werden. Die entsprechenden Veränderungen in den tieferen Zonen (d. h. eine minimale Abnahme von Fe und Mg begleitet von einer ebenfalls geringen Abnahme von Al und Ti und einer mehr oder weniger abrupten Veränderung im Na- und K-Gehalt) können jedoch nur unter Berücksichtigung der Interferenz von anatektischen Phänomenen gesehen werden. Solche Phänomene modifizieren den normalen Trend durch eine Veränderung des Metamorphosegrades.Daraus folgt, daß die Muskovitzusammensetzung als Indikator des Metamorphosegrades nur in Abwesenheit von partiellen Schmelzphenomen gebraucht werden kann.
Résumé Les muscovites des métapélites de la Sierra de Guadarrama, appartenant aux zones à chloritoïde, staurotide, disthène, sillimanite-feldspath potassique et sillimanite-feldspath potassique-cordierite, ont une composition chimique très proche de la valeur theorique (valeur moyenne Ms 92); néanmoins elles présentent une certaine variation dans les teneurs en Al2O3, K2O et Na2O et, à une moindre échelle, en FeO et MgO.Ces variations chimiques (diminution progressive en céladonite, augmentation suivie d'une diminution de la paragonite vers des compositions proches de la muscovite sensu stricto) que présentent les muscovites des zones à chloritoïde, staurotide et disthène sont étroitement liées aux zones métamorphiques superieures. Au contraire, les variations (legère augmentation des teneurs en Fe et Mg, legère diminution en AlVI et Ti, et plus ou moins brusques variations en Na et K, respectivement) correspondantes des muscovites des zones de la sillimanite-feldspath potassique et de la sillimanite-feldspath potassiquecordiérite, ne peuvent s'expliquer que si l'on admis que, dans les niveaux plus métamorphiques, les muscovites souffrent une série de changements chimiques dûs au début de l'anatexie, laquelle modifie les tendances normales liées à l'intensité du metamorphisme.En conséquence, seules les muscovites des métapélites situées au-dessus de l'isograde du feldspath potassique, en dehors de toute fusion partielle peuvent être utilisées pour déterminer le degré de métamorphisme des roches qui les contiennent.
, , , , -K- -- - , , 92 % . 23, K2 Na2O FeO MgO. (.. , , , ) — , . (.. , ) , . . , .相似文献
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M. Hernandez W. P. S. Meikle A. Aparicio C. R. Benn M. R. Burleigh A. C. Chrysostomou A. J. L. Fernandes T. R. Geballe P. L. Hammersley J. Iglesias-Paramo D. J. James P. A. James S. N. Kemp T. A. Lister D. Martinez-Delgado A. Oscoz D. L. Pollacco M. Rozas S. J. Smartt P. Sorensen R. A. Swaters J. H. Telting W. D. Vacca N. A. Walton M. R. Zapatero-Osorio 《Monthly notices of the Royal Astronomical Society》2000,319(1):223-234
We present first-season infrared (IR) and optical photometry and spectroscopy of the Type Ia Supernova 1998bu in M96. We also report optical polarimetry of this event. SN 1998bu is one of the closest type Ia supernovae of modern times, and the distance of its host galaxy is well determined. We find that SN 1998bu is both photometrically and spectroscopically normal. However, the extinction to this event is unusually high, with We find that SN 1998bu peaked at an intrinsic Adopting a distance modulus of 30.25 (Tanvir et al.) and using Phillips et al.'s relations for the Hubble constant, we obtain Combination of our IR photometry with those of Jha et al. provides one of the most complete early-phase IR light curves for a SN Ia published so far. In particular, SN 1998bu is the first normal SN Ia for which good pre- t B max IR coverage has been obtained. It reveals that the J , H and K light curves peak about 5 days earlier than the flux in the B -band curve. 相似文献
19.
A. J. P. Aparicio J. M. Vaquero V. M. S. Carrasco M. C. Gallego 《Solar physics》2014,289(11):4335-4349
The solar program of the Astronomical Observatory of Madrid started in 1876. Observations were made in this institution to determine sunspot numbers and areas for ten solar cycles. The program was completed in 1986 and the resulting data have been published in various Spanish scientific publications. Four periods of this program (with different observers and instruments) were identified with the aid of the interesting metadata that has been made available. In the present work, the published data were retrieved and digitized. Their subsequent analysis showed that most of these data could be considered reliable given their very high correlation with reference indices (international sunspot number, group sunspot number, and sunspot area). An abrupt change emerged in the sunspots/groups ratio in 1946, which lasted until 1972. 相似文献
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Sebastian L. Hidalgo Antonio Aparicio David MartÍnez-Delgado 《Astrophysics and Space Science》2003,284(2):595-598
The surface brightness profile in the V band of the Phoenix dwarf galaxy shows two stellar components: an inner one, which
contains all the young stars of the galaxy, and an outer one predominantly populated by red stars. Deep color-magnitude diagrams
(CMDs), based on Hubble Space Telescope (HST) observations and reaching the oldest turn-offs, are used to analyze the inner
and outer stellar components. Results show that, together with an old stellar population, the outer field contains also an
intermediate-age population. These results are compatible with a scenario in which star forming regions are shrinking with
time (the shrinking scenario). It seems more difficult to support a halo-disk scenario, which would require extended structures
populated only by really old stars.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献