CASHEW, A RESPONSE TO THE COCOA CRISIS IN DIMBOKRO IN THE N'ZI REGION? (IVORY COAST)

Susmita Hazra, Jonathan Risner
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Abstract

As the Sun progresses through its solar cycle and its activity increases, a greater number of sunspots occur, and solar fluxes become more intense. The change in solar activity is related to the change in electron and ion density of the ionosphere. Studying this relation is very important in terms of space plasma studies and space weather predictions, which play a significant role in radio and satellite communication as well as GPS navigation. In this paper, we are presenting the sunspot and solar flux data for solar cycle 24 (year 2008-2020). We are using C/NOFS satellite data to understand the variationof ion densities of the upper atmosphere with solar cycle 24. Our analysis shows decrease of H+ density by a factor of 10 and increase of O+ density by a factor of 10 during solar maxima. This data set can be used as a framework for future advancement in empirical modelling of regional and global ion density of the ionosphere.
腰果,应对恩济地区 DEMBOKRO 的可可危机?(象牙海岸)
随着太阳活动周期的延长,太阳黑子的数量会增加,太阳通量也会变得更强。太阳活动的变化与电离层电子和离子密度的变化有关。研究这种关系对空间等离子体研究和空间天气预报非常重要,而空间等离子体研究和空间天气预报在无线电和卫星通信以及全球定位系统导航中发挥着重要作用。本文将介绍太阳周期 24(2008-2020 年)的太阳黑子和太阳通量数据。我们利用 C/NOFS 卫星数据来了解太阳周期 24 上层大气离子密度的变化。我们的分析表明,在太阳最大值期间,H+密度下降了 10 倍,O+密度上升了 10 倍。这组数据可作为未来推进区域和全球电离层离子密度经验建模的框架。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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