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We discuss observations of the weak ?rst overtone (Δν = 2) CO absorption band near 2300 nm with the U.S. National Solar Observatory Array Camera (NAC), a modern mid‐infrared detector. This molecular band provides a thermal diagnostic that forms lower in the atmosphere than the stronger fundamental band near 4600 nm. The observed center‐to‐limb increase in CO line width qualitatively agrees with the proposed higher temperature shocks or faster plasma motions higher in the COmosphere. The spatial extent of chromospheric shock waves is currently at or below the diffraction limit of the available CO lines at existing telescopes. Five minute period oscillations in line strength and measured Doppler shifts are consistent with the p‐mode excitation of the photospheric gas. We also show recent efforts at direct imaging at 4600 nm. We stress that future large‐aperture solar telescopes must be teamed with improved, dynamic mid‐infrared instruments, like the NAC, to capitalize on the features that motivate such facilities (© 2010 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim) 相似文献
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Thomas Schad 《Solar physics》2017,292(9):132
A technique is presented that automates the direction characterization of curvilinear features in multidimensional solar imaging datasets. It is an extension of the Rolling Hough Transform (RHT) technique presented by Clark, Peek, and Putman (Astrophys. J. 789, 82, 2014), and it excels at rapid quantification of spatial and spatiotemporal feature orientation even for applications with a low signal-to-noise ratio. It operates on a pixel-by-pixel basis within a dataset and reliably quantifies orientation even for locations not centered on a feature ridge, which is used here to derive a quasi-continuous map of the chromospheric fine-structure projection angle. For time-series analysis, a procedure is developed that uses a hierarchical application of the RHT to automatically derive the apparent motion of coronal rain observed off-limb. Essential to the success of this technique is the formulation presented in this article for the RHT error analysis as it provides a means to properly filter results. 相似文献
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Measurements of maximum magnetic flux, minimum intensity, and size are presented for 12 967 sunspot umbrae detected on the
National Aeronautics and Space Administration/National Solar Observatory (NASA/NSO) spectromagnetograms between 1993 and 2004
to study umbral structure and strength during the solar cycle. The umbrae are selected using an automated thresholding technique.
Measured umbral intensities are first corrected for center-to-limb intensity dependence. Log-normal fits to the observed size
distribution confirm that the size-spectrum shape does not vary with time. The intensity – magnetic-flux relationship is found
to be steady over the solar cycle. The dependence of umbral size on the magnetic flux and minimum intensity are also independent
of the cycle phase and give linear and quadratic relations, respectively. While the large sample size does show a low-amplitude
oscillation in the mean minimum intensity and maximum magnetic flux correlated with the solar cycle, this can be explained
in terms of variations in the mean umbral size. These size variations, however, are small and do not substantiate a meaningful
change in the size spectrum of the umbrae generated by the Sun. Thus, in contrast to previous reports, the observations suggest
the equilibrium structure, as manifested by the invariant size-magnetic field relationship, as well as the mean size (i.e., strength) of sunspot umbrae do not significantly depend on the solar-cycle phase. 相似文献
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This paper examines difficulties encountered when using the Green-Nagdi rate and presents an updated configuration formulation for problems dealing with large deformations. It is shown that a natural link can be established between the updated reference configuration and linearized updated Lagrangian formulations, if Truesdell's objective stress rate is used. Owing to this connection, any limitations associated with the described formulation would be expected to also apply to an updated Lagrangian formulation and vice versa. It is pointed out that, if second-order effects are induced, the Truesdell rate appears in the rate equation for equilibrium even when strains are infinitesimal. By examining a simple-shear problem, where hypoelastic material behaviour with ‘Hooke's law’ is assumed, it is shown that the spherical state of stress is coupled with the shear stress when using the Truesdell or Green-Nagdi stress rate. It is suggested that objective stress rates, introduced in large-deformation formulations, may contribute to erroneous predictions if a constitutive law is developed independent of the adopted stress rate. 相似文献
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Why do people not learn from flood disasters? Evidence from Vietnam’s northwestern mountains 总被引：4，自引：2，他引：2
Iven Schad Petra Schmitter Camille Saint-Macary Andreas Neef Marc Lamers La Nguyen Thomas Hilger Volker Hoffmann 《Natural Hazards》2012,62(2):221-241
This article explores how the causes and impacts of a flood event as perceived by local people shape immediate responses and future mitigation efforts in mountainous northwest Vietnam. Local flood perception is contrasted with scientific perspectives to determine whether a singular flood event will trigger adjustments in mitigation strategies in an otherwise rarely flood-affected area. We present findings from interdisciplinary research drawing on both socioeconomic and biophysical data. Evidence suggests that individual farmers?? willingness to engage in flood mitigation is curbed by the common perception that flooding is caused by the interplay of a bundle of external factors, with climatic factors and water management failures being the most prominent ones. Most farmers did not link the severity of flooding to existing land use systems, thus underlining the lack of a sense of personal responsibility among farmers for flood mitigation measures. We conclude that local governments cannot depend on there being a sufficient degree of intrinsic motivation among farmers to make them implement soil conservation techniques to mitigate future flooding. Policy makers will need to design measures to raise farmers?? awareness of the complex interplay between land use and hydrology and to enhance collective action in soil conservation by providing appropriate incentives and implementing coherent long-term strategies. 相似文献
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Iven Bennett 《Theoretical and Applied Climatology》1964,13(2):216-248
Summary Daily values of global radiation from 10 stations for the period 1950–1960 are used as a base to describe the distribution of the global radiation of solar energy in the Intermontane Basin and Plateau Region of the western United States (including areas of the States from Washington and Idaho in the North to the Mexican frontier in the south). The empirical relations between radiation and more commonly available climatic and geographic variables—percent of possible sunshine, mean daily cloud cover, presence or absence of snow on the ground, optical air mass, and station elevation and latitude—are established through regression and correlation analysis for these stations and used to estimate radiation at 16 additional locations where radiation data are not collected. This provides better geographic coverage than could be obtained from use of radiation data alone. The technique also permits the filling-in of missing data in the records of the 10 stations to provide each with a complete record for the study period. Selected monthly maps of mean daily global radiation are presented for the region.
With 12 Figures 相似文献
Zusammenfassung Tagessummen der Globalstrahlung von 10 Stationen aus der Periode 1950 bis 1960 werden verwendet, um die Verteilung der Globalstrahlung von Sonne und Himmel im Westen der Vereinigten Staaten (Intermontane Basin und Plateau Region, umfassend Gebiete der Staaten von Washington und Idaho im Norden bis zur mexikanischen Grenze, jedoch unter Ausschluß der tieferen Lagen von Kalifornien) darzustellen. Die empirischen Beziehungen zwischen Strahlung und anderen, allgemeiner verfügbaren klimatischen und geographischen Variabeln — wie relative Sonnenscheindauer, Tagesmittel der Himmelsbedeckung, Vorhandensein oder Fehlen einer Schneedecke, optische Luftmasse, Meereshöhe und Breite der Station —werden durch Regressions- und Korrelationsanalyse für diese Stationen aufgestellt und dazu benützt, um für weitere 16 Orte, für welche keine Strahlungsbeobachtungen vorliegen, die Strahlungswerte abzuschätzen. Dadurch wird die geographische Verteilung besser erfaßt als lediglich durch die vorhandenen Strahlungsdaten. Das gleiche Verfahren gestattet auch, fehlende Werte in den Aufzeichnungen der Ausgangsstationen zu ergänzen und dadurch die Reihen zu vervollständigen. Eine Auswahl von Monatskarten der mittleren Tagessumen der Globalstrahlung für das Gebiet wird vorgelegt.
Résumé Pour représenter la répartition du rayonnement global du soleil et du ciel dans l'ouest des Etats-Unis, on s'est servi des sommes journalières du dit rayonnement recueillies à 10 stations pendant la période allant de 1950 à 1960. La région considérée comprend les bassins versants et les hauts plateaux s'étendant des Etats de Washington et de l'Idaho au nord jusqu'à la frontière du Méxique au sud, mais à l'exception des terres basses de la Californie. Afin d'estimer les valeurs de la radiation globale en 16 stations différentes, mais où elle n'est pas mesurée, on s'est servi de rapports empiriques entre la dite radiation et les éléments météorologiques ou géographiques généralement disponibles. Ceux-ci sont: la durée d'insolation relative, la nébulosité journalière moyenne, la présence ou l'absence d'une couche de neige, l'épaisseur optique de la masse d'air, l'altitude et la latitude du lieu. Les rapports empiriques utilisés sont calculés au moyen d'une analyse en régressions et en corrélations. On peut alors mieux se rendre compte de la répartition géographique réelle de la radiation globale qu'en se servant des seuls relevés effectués. Les mêmes procédés permettent en outre de combler les lacunes que présentent les mesures faites aux stations de base afin d'obtenir des séries complètes pour la période entière. On présente enfin un choix de cartes de la région, cartes contenant les moyennes mensuelles de la somme journalière de la radiation globale.
With 12 Figures 相似文献
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T. A. Schad 《Solar physics》2014,289(5):1477-1498
We study 7530 sunspot umbrae and pores measured by the Hinode Spectropolarimeter (SP) between November 2006 and November 2012. We primarily seek confirmation of the long term secular decrease in the mean magnetic field strength of sunspot umbrae found by Penn and Livingston (IAU Symp. 273, 126, 2011) between 1998 and 2011. The excellent SP photometric properties and full vector magnetic field determinations from full-Stokes Milne–Eddington inversions are used to address the interrelated properties of the magnetic field strength and brightness temperature for all umbral cores. We find non-linear relationships between magnetic field strength and umbral temperature (and continuum contrast), as well as between umbral radius and magnetic field strength. Using disambiguated vector data, we find that the azimuths measured in the umbral cores reflect an organization weakly influenced by Joy’s law. The large selection of umbrae displays a log-normal size spectrum similar to earlier solar cycles. Influenced by the amplitude of the solar cycle and the non-linear relationship between umbral size and core magnetic field strength, the distribution of core magnetic field strengths, fit most effectively with a skew-normal distribution, shows a weak solar cycle dependence. Yet, the mean magnetic field strength does not show a significant long term trend. 相似文献
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Hermann Schad 《国际地质力学数值与分析法杂志》1985,9(3):261-275
The application of finite element methods (FEM) is often restricted by the available computer capacity and the computing costs. The purpose of this paper, therefore, is, to present test results and to discuss possible ways of achieving a substantial reduction in computing times. Dividing the numerical analysis into the five levels–hardware, software, element-mesh and element-type, iteration technique (approximation of non-linearity) and constitutive model–one can show that the computing time can be reduced by about 20 per cent at every level. In particular, the use of the modified Newton-Raphson method for approximation of non-linearity and the constitutive model–apart from the theoretical concept (elastoplastic, hypoelastic etc.)—must be formulated in a manner which does not produce substantial changes in the coefficients of the material matrix caused by small stress changes. On the whole, computing time can be reduced to about 10 per cent of present computing costs. Thus, it would even be economically viable to solve three-dimensional non-linear problems by FEM. 相似文献
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