2002年印度上空地磁场水平分量的分析

R. Jayapal, C. Anilkumar, K. Unnikrishnan, C. Venugopal
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引用次数: 1

摘要

波尔兹曼-吉布斯(B-G)熵是一种广泛用于量化开放系统中不确定性的熵测度。然而,它不能描述具有大变异性和多重分形的非平衡系统。B - G熵的一种推广是Tsallis熵。利用2002年在印度各站点观测到的地球磁场水平分量值。在2000 - 2002年间,太阳活动周期23达到最大值。数据来自Ettaiyapuram (ETT,纬度90 10′N,经度780 01′E,地磁纬度0.130 N)、Visakhapatnam (VIS, 170 41′N, 830 19′E, 8.170 N)、HYD, 170 25′N, 780 33′E, 8.170 N)、Alibag (ABG, 180 37′N, 720 52′E, 10.020 N)和Tirunelveli (TVI, 80 42′N, 770 48′E, 0.320 S)。使用这些值作为输入,我们证明了Tsallis熵可以用来检测不同台站之间观测到的地磁场水平分量的微小差异。该方法是一种非常简单和优雅的方法,可以检测到相似信号对之间的微小变化。
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Tsallis’ Analysis of the Horizontal Component of the Earth’s Magnetic Field over India during 2002
A widely used measure of entropy to quantify uncertainity in an open system is the Boltzmann-Gibbs (B-G) entropy. It, however, cannot describe non-equilibrium systems with large variability and multi-fractality. A generalisation of the B - G entropy is the Tsallis’ entropy. The values of the horizontal components of the Earth’s magnetic field, observed at various stations in India in 2002 were used. During the years 2000 – 2002, solar cycle 23 reached its maximum. Data from Ettaiyapuram (ETT, latitude = 90 10’ N, longitude =  780 01’ E, geomagnetic latitude = 0.130 N), Visakhapatnam (VIS, 170 41’ N,  830 19’ E, 8.170 N), Hyderabad (HYD, 170 25’ N,  780 33’ E,  8.170  N), Alibag (ABG, 180 37’ N,  720 52’ E, 10.020 N) and Tirunelveli (TVI, 80 42’ N, 770 48’ E, 0.320 S) were used. Using these values as inputs, we demonstrate that Tsallis’ entropy can be used to detect minor differences in the horizontal components of the geomagnetic field observed between different pairs of stations. The method is a very simple and elegant one to detect minor variations between pairs of similar signals.
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