整个太阳活动周期内低纬度下电离层对太阳耀斑事件的响应

IF 1.4 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS
Gaurish Tripathi, Ashutosh K. Singh, Prashant Singh, Abhay Kumar Singh
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引用次数: 0

摘要

地球较低的电离层受到太阳耀斑的极大影响。在太阳耀斑事件期间,x射线通量的突然增强导致额外的电离,这增加了电离层下部的电子密度。在本文中,我们首先利用甚低频(VLF)波和GOES 0.1-0.8 nm x射线通量的振幅测量,研究了2011 - 2018年完整太阳周期24期间太阳耀斑事件(SFE)期间电离层下部的时间行为。在我们的低纬度站点瓦拉纳西(geom)观测到从澳大利亚nwc发射机发射的固定频率(19.8 kHz) VLF波。纬度。14 - 55/ N,地球。长。1540年,印度。与太阳耀斑相关的振幅增强由两个传统的Wait参数表征,即虚拟反射高度(H/ in km)和锐度因子(β in km−1),即电子密度梯度。利用这些经验确定的H/和β值在长波传播能力(LWPC)中预测太阳耀斑在比观测到的更宽频率范围内引起的VLF振幅扰动。结果表明,随着耀斑强度的增加,锐度因子增大,而虚反射高度减小。这些观测表明,H/从78 km减少到62 km, β从0.34 km−1增加到0.51 km−1的“饱和”水平。在太阳活动周期的不同阶段对这些参数的比较研究表明,在太阳活动周期的上升阶段,β较低。相反,在下降阶段,其值较高。H/在循环的下降阶段比上升阶段降低得更多。在太阳活动周期的高峰期,H/和β值介于上升相值和下降相值之间,但较为分散。这表明电离层下部在太阳活动周期的不同阶段表现不同。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Response of low-latitude lower ionosphere during solar flare events over the complete solar cycle 24

The lower ionosphere of Earth is greatly impacted by solar flares. During a solar flare event, a sudden enhancement in X-ray flux leads to additional ionization, which increases electron density in the lower ionosphere. In this paper, we first investigated time the behaviour of lower ionosphere during solar flare events (SFE) over the complete solar cycle 24 during the years 2011 to 2018 by using amplitude measurement of very low frequency (VLF) waves and GOES 0.1–0.8 nm X-ray flux. The fixed frequency (19.8 kHz) VLF wave transmitted from the NWC-transmitter, Australia is observed at our low-latitude station Varanasi (geom. lat. 14o 55/ N, geom. long. 154o E), India. The amplitude enhancements associated with solar flares are characterised by the two traditional Wait parameters, virtual reflection height (H/ in km) and the sharpness factor (β in km− 1) i.e. electron density gradient. These empirically determined values of H/ and β were employed in Long Wave Propagation Capability (LWPC) to predict VLF amplitude perturbations induced by the solar flare throughout a wider frequency range than was observable. It is found that the sharpness factor increases with the increasing strength of solar flares, but the virtual reflection height decreases. These observations show a decrease in H/ from 78 km to 62 km and an increase in β from 0.34 km− 1 up to a ‘saturation’ level of 0.51 km− 1. A comparative study of these parameters during different phases of the solar cycle shows that during the rising phase of the solar cycle, β is found to be lower. In contrast, during the declining phase, its value is higher. Also, H/ decreases more during the decreasing phase of the cycle than during the rising phase. During the peak of the solar cycle, H/ and β values are found to lie between rising and decreasing phase values, although more dispersed. This indicates that the lower ionosphere behaves differently during different phases of the solar cycle.

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来源期刊
Acta Geodaetica et Geophysica
Acta Geodaetica et Geophysica GEOCHEMISTRY & GEOPHYSICS-
CiteScore
3.10
自引率
7.10%
发文量
26
期刊介绍: The journal publishes original research papers in the field of geodesy and geophysics under headings: aeronomy and space physics, electromagnetic studies, geodesy and gravimetry, geodynamics, geomathematics, rock physics, seismology, solid earth physics, history. Papers dealing with problems of the Carpathian region and its surroundings are preferred. Similarly, papers on topics traditionally covered by Hungarian geodesists and geophysicists (e.g. robust estimations, geoid, EM properties of the Earth’s crust, geomagnetic pulsations and seismological risk) are especially welcome.
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