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31.
Olga K. Sil’chenko 《Astrophysics and Space Science》2011,335(1):171-176
I review the origin of UV-radiation in galaxies of different morphological types. UV-excess in spectra of massive elliptical
galaxies which have predominantly old stellar populations is traditionally explained by the contribution of low-mass stars
at very late, poorly known stages of evolution—by so called ‘AGB-manqué’ stars or by the population of extended horizontal
branch. However recent results from the GALEX survey of a large sample of nearby ellipticals have also demonstrated probable
traces of recent star formation in a third of all ellipticals observed. In spiral galaxies extended UV-disks have been discovered
by the GALEX; they are certainly illuminated by the current star formation, but what has provoked star formation in the areas
of very low gas density, beyond the distribution of older stars, is a puzzle yet. The UV-spectra of starburst galaxies or
starforming galactic nuclei are characterized by weak emission lines, if any, quite dissimilar to their optical spectra. 相似文献
32.
Anthropogenic subsidence in the Mexicali Valley,Baja California,Mexico, and slip on the Saltillo fault 总被引:2,自引:1,他引:1
Ewa Glowacka Olga Sarychikhina Francisco Suárez F. Alejandro Nava Robert Mellors 《Environmental Earth Sciences》2010,59(7):1515-1524
Deep fluid extraction in the Cerro Prieto geothermal field (CPGF) has caused subsidence and induced slip on tectonic faults
in the Mexicali Valley (Baja California, Mexico). The Mexicali Valley is located in the southern part of the Salton Trough,
at the boundary between the Pacific and North American plates. The Valley is characterized by being a zone of continuous tectonic
deformation, geothermal activity, and seismicity. Within the Cerro Prieto pull-apart basin, seismicity is concentrated mainly
in swarms, while strong earthquakes have occurred in the Imperial and Cerro Prieto transform faults, that are the eastern
and western bound of the basin. Since 1973, fluid extraction at the CPGF has influenced deformation in the area, accelerating
the subsidence and causing rupture (frequently as vertical slip or creep) on the surface traces of tectonic faults. Both subsidence
and fault slip are causing damage to infrastructure like roads, railroad tracks, irrigation channels, and agricultural fields.
Currently, accelerated extraction in the eastern part of CPGF has shifted eastwards the area of most pronounced subsidence
rate; this accelerated subsidence can be observed at the Saltillo fault, a southern branch of the Imperial fault in the Mexicali
Valley. Published leveling data, together with field data from geological surveys, geotechnical instruments, and new InSAR
images were used to model the observed deformation in the area in terms of fluid extraction. Since the electricity production
in the CPGF is an indispensable part of Baja California economy, extraction is sure to continue and may probably increase,
so that the problem of damages caused by subsidence will likely increase in the future. 相似文献
33.
Olga Popova 《Earth, Moon, and Planets》2004,95(1-4):303-319
The fate of entering meteoroids in atmosphere is determined by their size, velocity and substance properties. Material from
ablation of small-sized meteors (roughly R≤0.01–1 cm) is mostly deposited between 120 and 80 km altitudes. Larger bodies (up to meter sizes) penetrate deeper into the
atmosphere (down to 20 km altitude). Meteoroids of cometary origin typically have higher termination altitude due to substance
properties and higher entry velocity. Fast meteoroids (V>30–40 km/s) may lose a part of their material at higher altitudes due to sputtering. Local flow regime realized around the
falling body determines the heat transfer and mass loss processes. Classic approach to meteor interaction with atmosphere
allows describing two limiting cases: – large meteoroid at relatively low altitude, where shock wave is formed (hydrodynamical
models); – small meteoroid/or high altitudes – free molecule regime of interaction, which assumes no collisions between evaporated
meteoroid particles. These evaporated particles form initial train, which then spreads into an ambient air due to diffusion.
Ablation models should make it possible to describe physical conditions that occur around meteor body. Several self-consistent
hydrodynamical models are developed, but similar models for transition and free molecule regimes are still under study. This
paper reviews existing ablation models and discusses model boundaries. 相似文献
34.
35.
G. Beskin N. Borisov V. Komarova S. Mitronova S. Neizvestny V. Plokhotnichenko M. Popova 《Astrophysics and Space Science》1997,248(1-2):51-57
I summarize fully-sampled observations of the 3 mm emission from CO and HCN in the inner arcminute of NGC 1068. The CO emission
is distributed in the form of a molecular bar, coincident with the infrared bar, from which emanate two spiral arms. A relatively
weak concentration of CO line emission is found at the nucleus. By contrast, the HCN emission is strongly concentrated at
the center, with relatively weak emission in the region of the star-forming arms. The ratio of HCN to CO integrated intensities
is about 0.6 over the central r ≉ 175 pc and is the highest ratio measured in the center of any galaxy; the ratio reflects
the high thermal pressure (TK ~ 50 K, n[H2] ~ 4 × 106 cm-3) in the few hundred parsecs surrounding the nucleus.
The kinematics in the star-forming arms are well described by circular orbits, with ordered noncircular motions of < 30 km
s-1 that may be attributed to spiral density wave streaming. Interior to the bar, noncircular motions dominate the gas kinematics.
A model of the CO kinematics contrains any Inner Lindblad Resonance to be close to the location of the hundred-parsec scale
HCN ‘disk’. At the nucleus, the spatially unresolved CO emission shows a triplet velocity structure characteristic of kinematically
independent regions.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
36.
Ptichnikov A. V. Shvarts E. A. Popova G. A. Baibar A. S. 《Doklady Earth Sciences》2022,507(1):981-985
Doklady Earth Sciences - The potential role of forests in achieving carbon neutrality in the Russian Federation by 2060 is analyzed. It is shown that the key rate in the Strategy for the... 相似文献
37.
Javier Tomasella Patrícia F. Pinho Laura S. Borma José A. Marengo Carlos A. Nobre Olga R. F. O. Bittencourt Maria C. R. Prado Daniel A. Rodriguez Luz A. Cuartas 《Climatic change》2013,116(3-4):723-746
It is well known that most of the severe droughts in Amazonia, such as that of 1997, are El Niño-related. However, in 2005, the Amazon was affected by a severe drought that was not El Niño-related, as most of the rainfall anomalies that have happened in southwestern Amazonia are driven by sea surface temperature anomalies in the tropical North Atlantic. Earlier studies have analyzed both droughts in terms of their meteorological causes and impacts in terra firme (non-flooded) forests. This study compares the hydrological effects of both droughts on the Amazonian floodplain and discusses their potential ecological and human impacts based on an extensive literature review. The results revealed that the effects of the 2005 drought were exacerbated because rainfall was lower and evaporation rates were higher at the peak of the dry season compared to the 1997 drought. This induced a more acute depletion of water levels in floodplain lakes and was most likely associated with higher fish mortality rates. Based on the fact that the stem growth of many floodplain species is related to the length of the non-flooded period, it is hypothesized that the 1997 drought had more positive effects on floodplain forest growth than the 2005 drought. The fishing community of Silves in central Amazonia considered both droughts to have been equally severe. However, the 2005 drought was widely broadcasted by the press; therefore, the governmental mitigation efforts were more comprehensive. It is suggested that the availability of new communication technology and greater public awareness regarding environmental issues, combined with the new legal framework for assessing the severity of calamities in Brazil, are among the primary factors that explain the difference in societal response between the two droughts. 相似文献
38.
Recent high-resolution observations from the Solar Dynamics Observatory (SDO) have reawakened interest in the old and fascinating phenomenon of solar tornado-like prominences. This class of prominences was first introduced by Pettit (Astrophys. J. 76, 9, 1932), who studied them over many years. Observations of tornado prominences similar to the ones seen by SDO had already been documented by Secchi (Le Soleil, 1877). High-resolution and high-cadence multiwavelength data obtained by SDO reveal that the tornado-like appearance of these prominences is mainly an illusion due to projection effects. We discuss two different cases where prominences on the limb might appear to have a tornado-like behavior. One case of apparent vortical motions in prominence spines and barbs arises from the (mostly) 2D counterstreaming plasma motion along the prominence spine and barbs together with oscillations along individual threads. The other case of apparent rotational motion is observed in a prominence cavity and results from the 3D plasma motion along the writhed magnetic fields inside and along the prominence cavity as seen projected on the limb. Thus, the “tornado” impression results either from counterstreaming and oscillations or from the projection on the plane of the sky of plasma motion along magnetic-field lines, rather than from a true vortical motion around an (apparent) vertical or horizontal axis. We discuss the link between tornado-like prominences, filament barbs, and photospheric vortices at their base. 相似文献
39.
40.
We use data on open star clusters (OSCs) from the Homogeneous Catalog of OSC Parameters to determine some of the parameters of the spiral structure of our Galaxy: the pitch angle of the spiral arms \(i = 21\mathop .\limits^ \circ 5\), the pattern speed Ωp = 20.4 ± 2.5 km s?1 kpc?1, and the initial phase of the spiral θ0 = 206°. The spiral pattern of the Galaxy proves to have been virtually unchanged over the last billion years, and signatures of the concentration of objects toward the spiral arms can be traced back to this age. However, the number of spiral arms in the structure cannot be determined from OSCs. 相似文献