RESPONSE OF F2- REGION MAXIMUM ELECTRON DENSITY (NmF2/foF2) TO SOLAR ACTIVITY USING PEARSON PRODUCT MOMENT CORRELATION

E. Onori
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Abstract

Introduction: The ionosphere owes its origin primarily to ultraviolet radiation from the Sun. The ionosphere is an essential part of the Earth’s upper atmosphere. It is ionized by solar radiation and influences transionospheric radio wave propagation. Maximum electron density of the F2- layer (NmF2) is an important parameter for studying the ionosphere. The ionospheric F2-region maximum electron density (NmF2) depends strongly on solar activity, it also suffers temporal and spatial variations. Aim: The aim of this paper is to investigate the response of NmF2 to solar activity during high solar activity (HSA), moderate solar activity (MSA) and low solar activity (LSA) years using correlation analysis. Materials and Methods: The data used in this work are the hourly NmF2 values derived from foF2 data observed at Jicamarca (Lat.11.9 oS, Long.76.8 oW) and Puerto Rico (Lat.18.5 oN, Long.67.2 oW) during high solar activity HSA (2002), moderate solar activity MSA (2011) and low solar activity LSA (2006) years. The NmF2 data were evaluated using the relation in equation 1 NmF2 = 1.24 x 1010 (foF2)2 (1) Where NmF2 is in el/m3 and foF2 is in MHz. Pearson Product Moment Correlation (PPMC) was used to further analyse the NmF2 data. Results: Our results revealed two unequal NmF2 peaks. The NmF2 peaks values at Jicamarca (60 - 240; 63– 204) x 1010 el/m3 are observed to be higher in values than those at Puerto Rico (63 – 187; 57 – 164) x 1010 el/m3. The highest NmF2 peak values of 240 and 187x 1010 el/m3 occurred during March equinox at 09:00 and 14:00 hours at Jicamarca and Puerto Rico respectively during HSA year. Conclusion: Correlation analysis for the three epochs of solar activity revealed that NmF2 showed positive correlation with sunspot number with highest correlation values of 0.904 and 0.976 at Jicamarca and Puerto Rico stations respectively during MSA year.
利用PEARSON积矩相关分析F2-区最大电子密度(NmF2/foF2)对太阳活动的响应
电离层的起源主要是由于太阳的紫外线辐射。电离层是地球上层大气的重要组成部分。它被太阳辐射电离并影响跨层无线电波的传播。F2层的最大电子密度(NmF2)是研究电离层的一个重要参数。电离层f2区最大电子密度(NmF2)受太阳活动的影响较大,且存在时空变化。目的:利用相关分析研究NmF2在太阳活动高(HSA)年、太阳活动中(MSA)年和太阳活动低(LSA)年对太阳活动的响应。材料和方法:本研究使用的数据是在Jicamarca (Lat.11.9 oS, Long.76.8 oW)和Puerto Rico (Lat.18.5 oN, Long.67.2 oW)太阳活动高HSA年(2002)、太阳活动中MSA年(2011)和太阳活动低LSA年(2006)期间观测到的foF2每小时NmF2值。NmF2数据使用公式1中的关系进行评估NmF2 = 1.24 x 1010 (foF2)2(1)其中NmF2单位为el/m3, foF2单位为MHz。使用Pearson积矩相关(PPMC)进一步分析NmF2数据。结果:我们的结果显示两个不等的NmF2峰。NmF2峰值在Jicamarca (60 ~ 240);63 - 204) × 1010 el/m3的数值高于波多黎各(63 - 187;57 - 164) × 1010 el/m3。在HSA年,Jicamarca和Puerto Rico的NmF2峰值分别出现在3月春分的09:00和14:00,分别为240和187x 1010 el/m3。结论:NmF2与太阳黑子数呈显著正相关,MSA年Jicamarca站和Puerto Rico站的相关值最高,分别为0.904和0.976。
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