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901.
In this study we use a numerical simulation of an artificial coronal mass ejection (CME) to validate a method for calculating propagation directions and kinematical profiles of interplanetary CMEs (ICMEs). In this method observations from heliospheric images are constrained with in-situ plasma and field data at 1 AU. These data are used to convert measured ICME elongations into distance by applying the harmonic mean approach, which assumes a spherical shape of the ICME front. We used synthetic white-light images, similar to those observed by STEREO-A/HI, for three different separation angles between remote and in-situ spacecraft of 30°, 60°, and 90°. To validate the results of the method, the images were compared to the apex speed profile of the modeled ICME, as obtained from a top view. This profile reflects the “true” apex kinematics because it is not affected by scattering or projection effects. In this way it is possible to determine the accuracy of the method for revealing ICME propagation directions and kinematics. We found that the direction obtained by the constrained harmonic mean method is not very sensitive to the separation angle (30° sep: ?=W7; 60° sep: ?=W12; 90° sep: ?=W15; true dir.: E0/W0). For all three cases the derived kinematics agree relatively well with the real kinematics. The best consistency is obtained for the 30° case, while with growing separation angle the ICME speed at 1 AU is increasingly overestimated (30° sep: ΔV arr≈??50 km?s?1, 60° sep: ΔV arr≈+?75 km?s?1, 90° sep: ΔV arr≈+?125 km?s?1). Especially for future L4/L5 missions, the 60° separation case is highly interesting in order to improve space-weather forecasts. 相似文献
902.
T. Wiegelmann S. K. Solanki J. M. Borrero H. Peter P. Barthol A. Gandorfer V. Martínez Pillet W. Schmidt M. Knölker 《Solar physics》2013,283(2):253-272
Observations with the balloon-borne Sunrise/Imaging Magnetograph eXperiment (IMaX) provide high spatial resolution (roughly 100 km at disk center) measurements of the magnetic field in the photosphere of the quiet Sun. To investigate the magnetic structure of the chromosphere and corona, we extrapolate these photospheric measurements into the upper solar atmosphere and analyze a 22-minute long time series with a cadence of 33 seconds. Using the extrapolated magnetic-field lines as tracer, we investigate temporal evolution of the magnetic connectivity in the quiet Sun’s atmosphere. The majority of magnetic loops are asymmetric in the sense that the photospheric field strength at the loop foot points is very different. We find that the magnetic connectivity of the loops changes rapidly with a typical connection recycling time of about 3±1 minutes in the upper solar atmosphere and 12±4 minutes in the photosphere. This is considerably shorter than previously found. Nonetheless, our estimate of the energy released by the associated magnetic-reconnection processes is not likely to be the sole source for heating the chromosphere and corona in the quiet Sun. 相似文献
903.
Speeds and Arrival Times of Solar Transients Approximated by Self-similar Expanding Circular Fronts 总被引:1,自引:0,他引:1
The NASA Solar TErrestrial RElations Observatory (STEREO) mission offered the possibility to forecast the arrival times, speeds, and directions of solar transients from outside the Sun–Earth line. In particular, we are interested in predicting potentially geoeffective interplanetary coronal mass ejections (ICMEs) from observations of density structures at large observation angles from the Sun (with the STEREO Heliospheric Imager instrument). We contribute to this endeavor by deriving analytical formulas concerning a geometric correction for the ICME speed and arrival time for the technique introduced by Davies et al. (Astrophys. J., 2012, in press), called self-similar expansion fitting (SSEF). This model assumes that a circle propagates outward, along a plane specified by a position angle (e.g., the ecliptic), with constant angular half-width (λ). This is an extension to earlier, more simple models: fixed-Φ fitting (λ=0°) and harmonic mean fitting (λ=90°). In contrast to previous models, this approach has the advantage of allowing one to assess clearly if a particular location in the heliosphere, such as a planet or spacecraft, might be expected to be hit by the ICME front. Our correction formulas are especially significant for glancing hits, where small differences in the direction greatly influence the expected speeds (up to 100?–?200 km?s?1) and arrival times (up to two days later than the apex). For very wide ICMEs (2λ>120°), the geometric correction becomes very similar to the one derived by Möstl et al. (Astrophys. J. 741, 34, 2011) for the harmonic mean model. These analytic expressions can also be used for empirical or analytical models to predict the 1 AU arrival time of an ICME by correcting for effects of hits by the flank rather than the apex, if the width and direction of the ICME in a plane are known and a circular geometry of the ICME front is assumed. 相似文献
904.
905.
Trace metals were analysed in sea spiders collected on two Polarstern cruises in the Weddell Sea. We found a substantial interspecific heterogeneity of Cd, Cu, Ni, and Zn, indicating varying accumulation strategies and metabolic demands for essential elements. Means and 95%-confidence intervals for all 44 samples analysed are 26+/-7 mg Cd kg(-1), 38+/-22 mg Cu kg(-1), 62+/-13 mg Ni kg(-1) and 990+/-130 mg Zn kg(-1) DW. Only for Pb do we find values less than 1.0 mg kg(-1) for most collectives analysed, in good agreement with other Antarctic arthropods such as crustaceans. Our study provides further evidence for the frequently reported "Cd anomaly" in many polar arthropods. While Cu concentrations in pantopods are within the reported range for Antarctic amphipods and decapods, Ni concentrations are exceptionally high and might be part of predation defence mechanisms. These possibilities should be investigated in more detail in future studies. 相似文献
906.
During geothermal power production using a borehole doublet consisting of a production and injection well, the reservoir conditions such as permeability k, porosity φ and Skempton coefficient B at the geothermal research site Gross Schoenebeck/Germany will change. Besides a temperature decrease at the injection well and a change of the chemical equilibrium, also the pore pressure p p will vary in a range of approximately 44 MPa ± 10 MPa in our reservoir at ?3850 to ?4258 m depth. This leads to a poroelastic response of the reservoir rocks depending on effective pressure p eff (difference between mean stress and pore pressure), resulting in a change in permeability k, porosity φ and the poroelastic parameter Skempton coefficient B. Hence, we investigated the effective pressure dependency of Flechtinger sandstone, an outcropping equivalent of the reservoir rock via laboratory experiments. The permeability decreased by 21% at an effective pressure range from 3 to 30 MPa, the porosity decreased by 11% (p eff = 6 to 65 MPa) and the Skempton coefficient decreased by 24% (p eff = 4 to 25 MPa). We will show which mechanisms lead to the change of the mentioned hydraulic and poroelastic parameters and the influence of these changes on the productivity of the reservoir. The most significant changes occur at low effective pressures until 15 to 20 MPa. For our in situ reservoir conditions p eff = 43 MPa a change of 10 MPa effective pressure will result in a change in matrix permeability of less than 4% and in matrix porosity of less than 2%. Besides natural fracture systems, fault zones and induced hydraulic fractures, the rock matrix its only one part of geothermal systems. All components can be influenced by pressure, temperature and chemical reactions. Therefore, the determined small poroelastic response of rock matrix does not significantly influence the sustainability of the geothermal reservoir. 相似文献
907.
T. Neubert M. Rycroft T. Farges E. Blanc O. Chanrion E. Arnone A. Odzimek N. Arnold C.-F. Enell E. Turunen T. Bösinger Á. Mika C. Haldoupis R. J. Steiner O. van der Velde S. Soula P. Berg F. Boberg P. Thejll B. Christiansen M. Ignaccolo M. Füllekrug P. T. Verronen J. Montanya N. Crosby 《Surveys in Geophysics》2008,29(2):71-137
The paper reviews recent advances in studies of electric discharges in the stratosphere and mesosphere above thunderstorms,
and their effects on the atmosphere. The primary focus is on the sprite discharge occurring in the mesosphere, which is the
most commonly observed high altitude discharge by imaging cameras from the ground, but effects on the upper atmosphere by
electromagnetic radiation from lightning are also considered. During the past few years, co-ordinated observations over Southern
Europe have been made of a wide range of parameters related to sprites and their causative thunderstorms. Observations have
been complemented by the modelling of processes ranging from the electric discharge to perturbations of trace gas concentrations
in the upper atmosphere. Observations point to significant energy deposition by sprites in the neutral atmosphere as observed
by infrasound waves detected at up to 1000 km distance, whereas elves and lightning have been shown significantly to affect
ionization and heating of the lower ionosphere/mesosphere. Studies of the thunderstorm systems powering high altitude discharges
show the important role of intracloud (IC) lightning in sprite generation as seen by the first simultaneous observations of
IC activity, sprite activity and broadband, electromagnetic radiation in the VLF range. Simulations of sprite ignition suggest
that, under certain conditions, energetic electrons in the runaway regime are generated in streamer discharges. Such electrons
may be the source of X- and Gamma-rays observed in lightning, thunderstorms and the so-called Terrestrial Gamma-ray Flashes
(TGFs) observed from space over thunderstorm regions. Model estimates of sprite perturbations to the global atmospheric electric
circuit, trace gas concentrations and atmospheric dynamics suggest significant local perturbations, and possibly significant
meso-scale effects, but negligible global effects. 相似文献
908.
909.
910.
A reliable geochemical paleo-indicator for phosphorus remains elusive, despite the importance of understanding historical
changes in the nutrient status of aquatic ecosystems. We assessed the potential of phytate (salts of myo-inositol hexakisphosphate) as a novel phosphorus-specific paleo-indicator by measuring its concentrations in dated sediments
from an embayment in Helsinki, Finland, with a known 200-year history of trophic changes. Phytate was extracted in a solution
containing sodium hydroxide and EDTA and detected by solution 31P NMR spectroscopy with spectral deconvolution. Concentrations varied markedly with sediment depth and paralleled previously
determined changes in diatom assemblages and geochemical indicators linked to trophic status. In contrast, total sediment
phosphorus did not reflect phosphorus inputs to the embayment, presumably due to the mobilization of inorganic phosphate under
anoxic conditions during periods of high pollutant loading. Importantly, phytate appeared to be stable in these brackish sediments,
in contrast to other organic and inorganic phosphates which declined abruptly with depth. We therefore conclude that phytate
represents a potentially important indicator of historical changes in phosphorus inputs to water bodies, although additional
studies are required to confirm its stability under conditions likely to be encountered in lakes and coastal ecosystems. 相似文献