Variation of ionosonde foE and its comparison with IRI-2016 & a local model over Pakistan longitude sector during solar cycle 22

被引:0
|
作者
Ameen, Muhammad Ayyaz [1 ,2 ,6 ]
Muhammad, Aisha Ghulam [3 ]
Abbas, Faizan [1 ]
Tahir, Afnan [1 ,4 ]
Talha, Madeeha [1 ,5 ]
机构
[1] Pakistan Space & Upper Atmosphere Res Commiss SUPA, Karachi, Pakistan
[2] Univ Karachi, Main Univ Rd, Karachi 75270, Pakistan
[3] NED Univ Engn & Technol, Karachi, Pakistan
[4] Beihang Univ, Sch Instrumentat & Optoelect Engn, SNARS Lab, 37 Xueyuan Rd, Beijing 100191, Peoples R China
[5] Korean Astron & Space Sci Inst KASI, 776 Daedeok Daero, Daejeon, South Korea
[6] Pakistan Space & Upper Atmosphere Res Commiss SUPA, POB 8402,SUPARCO Rd, Karachi 75270, Pakistan
基金
美国海洋和大气管理局;
关键词
E-layer; foE; Pakistan; ANN; Noontime; MONOCHROMATIC RADIATION; IONOSPHERE; TIME; ATMOSPHERE; ABSORPTION; KARACHI; MINIMA; HMF2; FOF2; IRI;
D O I
10.1016/j.asr.2022.12.038
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
The study presents the variation of ionospheric critical frequency of E-layer (foE), its comparison with International Reference Iono-sphere (IRI-2016) over Pakistan and suggests an artificial neural network (ANN) based algorithm to predict noontime daily hourly val-ues. The ionosonde measurements of Karachi (Geog. Coord: 24.95 degrees N, 67.13 degrees E, dip latitude = 17.0 degrees N), Multan (30.18 degrees N, 71.48 degrees E, 21.8 degrees N) and Islamabad (33.75 degrees N, 73.13 degrees E, 25.2 degrees N) have been used for the purpose. The observed foE values have been analysed during the high, moderate and low solar activity years 1989, 1992 and 1996, respectively. Results show a strong correlation between foE and solar activity which was expected because the E-layer is essentially solar controlled. It is found that foE peaks around noon with higher values during summer. The annual relative percentage deviation between data and IRI-2016 modelled values remains less than 6% for all locations and years under study. The ANN based algorithm predicts daily noontime foE values with a goodness of fit of 78%, compared to the IRI-2016 prediction, which has a goodness of fit of 71%. It is noted that the performance of IRI-2016 in predicting monthly hourly median values of foE improves with decreasing solar activity. The study confirms the data authenticity of foE over Pakistan and suggests an ANN based algorithm in predicting noontime values with no immediate updates to IRI-2016 for this Asian longitude sector.(c) 2022 COSPAR. Published by Elsevier B.V. All rights reserved.
引用
收藏
页码:4340 / 4350
页数:11
相关论文
共 32 条
  • [21] Statistics of GPS TEC at the northern EIA crest region of the Indian subcontinent during the solar cycle 24 (2013-2018): comparison with IRI-2016 and IRI-2012 models
    Arup Patari
    Bapan Paul
    Anirban Guha
    Astrophysics and Space Science, 2021, 366
  • [22] Variation of hmF2 and NmF2 deduced from DPS-4 over Multan (Pakistan) and their comparisons with IRI-2012 & IRI-2016 during the deep solar minimum between cycles 23 & 24
    Ameen, Muhammad Ayyaz
    Khursheed, Haqqa
    Jabbar, Mehak Abdul
    Ali, Muneeza Salman
    Chishtie, Farrukh
    ADVANCES IN SPACE RESEARCH, 2018, 61 (07) : 1726 - 1735
  • [23] Solar cycle variation of ionospheric parameters over the low latitude station Hainan, China, during 2002-2012 and its comparison with IRI-2012 model
    Wang, G. J.
    Shi, J. K.
    Wang, Z.
    Wang, X.
    Romanova, E.
    Ratovsky, K.
    Polekh, N. M.
    ADVANCES IN SPACE RESEARCH, 2017, 60 (02) : 381 - 395
  • [24] foF2 variability at a southern low-latitude station and the performance of IRI-2016 model during ascending phase of solar cycle-24
    Rao, S. S.
    Chakraborty, Monti
    Pandey, R.
    Singh, A. K.
    ADVANCES IN SPACE RESEARCH, 2019, 64 (11) : 2269 - 2279
  • [25] Variation of bottom-side profile parameters (B0, B1) over Multan and their comparisons with IRI-2016 during deep solar minimum of solar cycles 23/24
    Ameen, Muhammad Ayyaz
    Khursheed, Haqqa
    Jabbar, Mehak Abdul
    Ali, Muneeza Salman
    Murtaza, Ghulam
    Atiq, Muhammad
    Bouya, Zahra
    Yu, Xiao
    ADVANCES IN SPACE RESEARCH, 2021, 68 (05) : 2059 - 2068
  • [26] Comparison of maximum usable frequency (MUF) variability over Peninsular Malaysia with IRI model during the rise of solar cycle 24
    Malik, R. A.
    Abdullah, M.
    Abdullah, S.
    Homam, M. J.
    JOURNAL OF ATMOSPHERIC AND SOLAR-TERRESTRIAL PHYSICS, 2016, 138 : 87 - 92
  • [27] Comparison of Performance of the IRI 2016, IRI-Plas 2017, and NeQuick 2 Models During Different Solar Activity (2013-2018) Years Over South American Sector
    Tariku, Yekoye Asmare
    RADIO SCIENCE, 2020, 55 (08)
  • [28] Comparison of observed equatorial spread-F statistics between two longitudinally separated magnetic equatorial stations and the IRI-2016 model during low and high solar activities
    Thammavongsy, P.
    Supnithi, P.
    Myint, L. M. M.
    Sripathi, S.
    Hozumi, K.
    Lakanchanh, D.
    ADVANCES IN SPACE RESEARCH, 2022, 69 (06) : 2501 - 2511
  • [29] foF2 variability over New Delhi during different solar cycle conditions and comparison with IRI-2001 model
    Sethi, N. K.
    Dabas, R. S.
    Ninawe, Yogesh
    ADVANCES IN SPACE RESEARCH, 2007, 40 (06) : 855 - 860
  • [30] Assessment of IRI-2012 profile parameters by comparison with the ones inferred using NeQuick2, ionosonde and FORMOSAT-1 data during the high solar activity over Brazilian equatorial and low latitude sector
    Venkatesh, K.
    Fagundes, P. R.
    de Jesus, R.
    de Abreu, A. J.
    Pillat, V. G.
    Sumod, S. G.
    JOURNAL OF ATMOSPHERIC AND SOLAR-TERRESTRIAL PHYSICS, 2014, 121 : 10 - 23