论文标题

太阳电晕中电子密度和温度描述的热力学解释

Thermodynamics Interpretation of Electron Density and Temperature Description in the Solar Corona

论文作者

Berdichevsky, Daniel B., Gómez, Jenny M. Rodríguez, Vieira, Luis E., Lago, Allison Dal

论文摘要

我们达到了CODET模型的热力学解释及其对电子密度和温度的预测,该密度和温度基于全球平衡的水力磁性物理学。在理想的磁性水力动力学(MHD)的背景下,热力学解释与模型与模型的一致性。进一步注意到,Codet预测了太阳电晕电子气体的多面性异常指数。结果表明,这种不寻常的特征与假设低静态太阳电晕是一种磁磁性状态,该状态具有较早描述的基础结构,该结构早先被描述为通过在给定温度和压力下的气体固体表面来解释2-D吸附过程。在我们的情况下,假定我们存在3-D相似的聚结过程,即热力学平衡中的Langmuir无定形晶格。通过这种方式,培养基磁渗透性,非分散性声速,1.1至1.3 $ r _ {\ odot} $的预期平衡时间和能量密度的预期平衡时间和能量密度是在大多数近似太阳中的大多数最小值确定了几个月,从2008年到2008年,可定量确定。

We reach a thermodynamic interpretation of CODET model and its prediction to electrons density and temperature grounded on the physics of hydro magnetism in global equilibrium. The thermodynamic interpretation finds consistency with the model with a magneto-matter medium that is diamagnetic, in the context of ideal magnetohydrodynamics (MHD). It is further noticed that the CODET predicts a polytropic anomalous index for the electron gas of the Sun's corona. It is shown that this unusual characteristic is consistent with assuming that the low quiescent solar corona is a magneto-matter state which possesses an underlying structure that was earlier described to explain the 2-D adsorption process by a surface of a solid of molecules of a gas at a given temperature and pressure by Langmuir. In our case, it is assumed that we are in the presence of a 3-D similar coalescence process, i.e. a Langmuir amorphous lattice in thermodynamic equilibrium. In this way, constitutive properties of the medium magnetic permeability, the non-dispersive acoustic speed, the expected equilibration time for the 1.1 to 1.3$R_{\odot}$, and energy density are determined quantitatively for most of the quiescent corona in a near solar minimum that extends for several months from 2008 to 2009.

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