秘鲁和巴西东部赤道电急流的比较

R. Rastogi, H. Chandra, R. Shah, N. Trivedi, S. L. Fontes
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引用次数: 7

摘要

本文描述了赤道电喷流的特点在Huancayo(阿华,12.1 o年代,75.3 W,倾斜1.5 o N,赤纬1.0 o E)在南美洲西部,那里的地磁场沿着地理子午线几乎是一致的,在Itinga(来4.3 o年代,47.0 o W,倾斜1.4 o N,赤纬19.3 o W)在南美东部,地磁场的对齐以西约19 o地理子午线;虽然这两个区域的磁场平均强度几乎是同一数量级。进一步比较了同一经度扇区的低纬度站Itinga和Tatuoca (TTB, 1.2°S, 48.5°W,倾角7.8°N,赤纬18.7°W)的海流。地磁场水平分量H的日变化幅度在HUA处比在ITI处高出近16%。东场的日变化,Y,表现出强烈的最低-40元还在13 - 14日人力资源LT ITI而非常低的值观察华正峰值约4元约11 - 12小时中尉垂直领域,Z,显示异常大负的-70元TTB约13小时中尉程天X中午和午夜场的波动和华之间呈正相关来高的相关系数分别为0.78和0.88。在午夜时段,Y场值与HUA和ITI也呈显著正相关(0.72),而在正午时段则无相关。HUA、ITI和TTB的X场午夜值与Dst指数呈显著相关(0.90或更大)。在ITI和TTB, Dst与正午X值的相关值约为0.7,在HUA的相关值较小(0.4)。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
A Comparison of Equatorial Electrojet in Peru and East Brazil
The paper describes the characteristics of the equatorial electrojet at Huancayo (HUA, 12.1 o S, 75.3 o W, inclination 1.5 o N, declination 1.0 o E) in western side of South America, where the geomagnetic field is aligned almost along the geographic meridian, and at Itinga (ITI, 4.3 o S, 47.0 o W, inclination 1.4 o N, declination 19.3 o W) in eastern part of South America, where the geomagnetic field is aligned about 19 o west of the geographic meridian; although the mean intensity of the magnetic field in the two regions are almost of the same order. Further comparisons are made of the current at Itinga and at Tatuoca (TTB, 1.2 o S, 48.5 o W, inclination 7.8 o N, declination 18.7 o W), a low latitude station in the same longitude sector. The daily range of horizontal component of the geomagnetic field, H, is shown to be almost 16% higher at HUA compared to that at ITI. The daily variation of the eastward field, Y, showed a strong minimum of -40 nT around 13-14 hr LT at ITI whereas very low values were observed at HUA with a positive peak of about 4 nT around 11- 12 hr LT. The vertical field, Z, showed abnormally large negative values of -70 nT at TTB around 13 hr LT. The day-to- day fluctuations of midday and midnight values of X field were positively correlated between HUA and ITI with a high correlation coefficient of 0.78 and 0.88 respectively. Values of Y field were also significantly positively correlated between HUA and ITI for midnight hours (0.72), while no correlation was observed for the midday hours. The midnight values of X field at HUA, ITI and TTB showed significant (0.90 or greater) correlation with Dst index. Correlation values of about 0.7 were observed between Dst and midday values of X at ITI and TTB and to a lesser degree (0.4) at HUA.
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