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91.
Thomas R. Metcalf Marc L. DeRosa Carolus J. Schrijver Graham Barnes Adriaan A. van Ballegooijen Thomas Wiegelmann Michael S. Wheatland Gherardo Valori James M. McTtiernan 《Solar physics》2008,247(2):269-299
We compare a variety of nonlinear force-free field (NLFFF) extrapolation algorithms, including optimization, magneto-frictional,
and Grad – Rubin-like codes, applied to a solar-like reference model. The model used to test the algorithms includes realistic
photospheric Lorentz forces and a complex field including a weakly twisted, right helical flux bundle. The codes were applied
to both forced “photospheric” and more force-free “chromospheric” vector magnetic field boundary data derived from the model.
When applied to the chromospheric boundary data, the codes are able to recover the presence of the flux bundle and the field’s
free energy, though some details of the field connectivity are lost. When the codes are applied to the forced photospheric
boundary data, the reference model field is not well recovered, indicating that the combination of Lorentz forces and small
spatial scale structure at the photosphere severely impact the extrapolation of the field. Preprocessing of the forced photospheric
boundary does improve the extrapolations considerably for the layers above the chromosphere, but the extrapolations are sensitive
to the details of the numerical codes and neither the field connectivity nor the free magnetic energy in the full volume are
well recovered. The magnetic virial theorem gives a rapid measure of the total magnetic energy without extrapolation though,
like the NLFFF codes, it is sensitive to the Lorentz forces in the coronal volume. Both the magnetic virial theorem and the
Wiegelmann extrapolation, when applied to the preprocessed photospheric boundary, give a magnetic energy which is nearly equivalent
to the value derived from the chromospheric boundary, but both underestimate the free energy above the photosphere by at least
a factor of two. We discuss the interpretation of the preprocessed field in this context. When applying the NLFFF codes to
solar data, the problems associated with Lorentz forces present in the low solar atmosphere must be recognized: the various
codes will not necessarily converge to the correct, or even the same, solution.
On 07/07/2007, the NLFFF team was saddened by the news that Tom Metcalf had died as the result of an accident. We remain grateful
for having had the opportunity to benefit from his unwavering dedication to the problems encountered in attempting to understand
the Sun’s magnetic field; Tom had completed this paper several months before his death, leading the team through the many
steps described above. 相似文献
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岩浆岩体严重影响井田的煤质、储量等,对采区工作面布置、巷道掘进及回采工作造成严重的影响,因而探测岩浆岩侵入煤层的范围对煤矿安全高效生产具有重大意义。在总结岩浆岩侵入体的地质特征基础上,建立岩浆侵入煤层地震地质模型,通过正演,对多种属性进行交互分析,发现主频能量属性与振幅类属性对岩浆岩反应较为敏感,并且随着岩浆岩厚度的逐渐增加能量类与振幅类属性逐渐降低。通过对QN煤矿103工作面高密度三维地震资料连井剖面10煤进行属性分析,发现频带宽度、中心频率、主振幅属性可以较好地识别岩浆侵入区。通过对勘探区10煤层进行频带宽度、中心频率和主振幅属性分析识别岩浆侵入区,其识别结果与钻孔实际揭露吻合较好,证明采用地震属性识别技术可以识别煤层岩浆岩侵入区范围。 相似文献
94.
着重介绍了目前变质作用P-T─t轨迹研究在变质作用温压确定、变质作用不同阶段时间标定、变质作用动态演化过程的组构标志、变质作用演化热模拟以及变质作用P─T─t轨迹与大地构造环境之间关系等方面所存在的若干问题。 相似文献
95.
Exurbia from the bottom-up: Confronting empirical challenges to characterizing a complex system 总被引:2,自引:0,他引:2
Daniel G. Brown Derek T. Robinson Li An Moira Zellner William Rand Rick Riolo Bobbi Low 《Geoforum》2008,39(2):805-818
We describe empirical results from a multi-disciplinary project that support modeling complex processes of land-use and land-cover change in exurban parts of Southeastern Michigan. Based on two different conceptual models, one describing the evolution of urban form as a consequence of residential preferences and the other describing land-cover changes in an exurban township as a consequence of residential preferences, local policies, and a diversity of development types, we describe a variety of empirical data collected to support the mechanisms that we encoded in computational agent-based models. We used multiple methods, including social surveys, remote sensing, and statistical analysis of spatial data, to collect data that could be used to validate the structure of our models, calibrate their specific parameters, and evaluate their output. The data were used to investigate this system in the context of several themes from complexity science, including have (a) macro-level patterns; (b) autonomous decision making entities (i.e., agents); (c) heterogeneity among those entities; (d) social and spatial interactions that operate across multiple scales and (e) nonlinear feedback mechanisms. The results point to the importance of collecting data on agents and their interactions when producing agent-based models, the general validity of our conceptual models, and some changes that we needed to make to these models following data analysis. The calibrated models have been and are being used to evaluate landscape dynamics and the effects of various policy interventions on urban land-cover patterns. 相似文献
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通过三维激光扫描仪可以获取到表示空间对象的点云数据。通过设置仪器的采样间隔可以获取到表示对象不同精密程度的点集。但是由于离散点之间缺乏相应的拓扑关系,限制了以点为基本图元的模型的应用。以空间离散特征点集为研究对象,研究了一种三维建模算法。算法基于距离较近的点之间比距离较远的点之间存在拓扑连接的可能性更大的前提,对点集进行预处理,然后在此基础上进行快速建模,最终获取到以三角形为基本面片的格网模型。所建立的模型易于进行各项空间分析和操作。该算法也能够有效地应用于更为复杂的建模任务中,以达到一体化建模的目的。 相似文献
100.
在测量工作中,由于气候环境、观测方法、观测仪器以及观测人员自身因素等多方面的原因,可能造成观测数据的丢失或者不完全。文中针对这类数据的处理,采用加权平均法和三次样条插值法对缺失数据进行修复,建立GM (1,1)模型,并与非等间隔预测模型进行对比。通过两组仿真数据和两组实测数据验证发现:对于呈指数增长的序列和高增长序列修复之后建模预测精度更高;三次样条插值法数据修复后GM (1,1)建模预测精度较加权平均法预测精度更高;对于低增长序列,直接采用非等间隔建模预测精度更高。 相似文献