Sains Malaysiana 52(8)(2023): 2309-2322
http://doi.org/10.17576/jsm-2023-5208-11
Examining
Solar Flare Effects on Earth's Ionosphere using Ground-Based Measurements
(Pengkajian Kesan Nyalaan Suria terhadap Ionosfera Bumi menggunakan Pengukuran Dasar)
NURUL SHAZANA ABDUL HAMID1,2,*, RAJA ADIBAH
RAJA HALIM1, IDAHWATI SARUDIN3, AKIMASA
YOSHIKAWA4,5 & AKIKO FUJIMOTO6
1Department of Applied Physics, Faculty of Science and
Technology, Universiti Kebangsaan Malaysia, 43600 UKM Bangi, Selangor, Malaysia
2Space Science Centre (ANGKASA), Institute of Climate
Change, Universiti Kebangsaan Malaysia, 43600 UKM, Bangi, Selangor, Malaysia
3School of Physics, Universiti Sains Malaysia, 11800 USM, Penang, Malaysia
4Department of Earth and Planetary Sciences, Faculty of
Sciences, 33 Kyushu University, 6-10-1 Hakozaki,
Higashi-ku, Fukuoka 812-8581, Japan
5International Research Center for Space and Planetary
Environmental Science (i-SPES), Kyushu University,
819-0395 Fukuoka, Japan
6Department of Artificial Intelligence, Faculty of
Computer Science and Systems Engineering, Kyushu Institute of Technology,
680-4, Kawazu, Iizuka,
Fukuoka 820-8502, Japan
Diserahkan: 28 Januari 2023/Diterima: 2 Ogos 2023
Abstract
This study investigated the simultaneous effects of solar flares
(SFs) on both the D and E layers of Earth's ionosphere. The analysis
focused on the M and X-class SFs that occurred during the 24th solar cycle as
these two classes of SFs are known to produce significant effects on Earth’s
environment, particularly during the daytime period. The data utilized to
detect the SF events in this study were ground-based magnetometer data from the
equatorial regions. Effects of the selected SF events on the E layer were
investigated based on the EUEL index constructed using the geomagnetic data.
Meanwhile, the changes in the strength of radio VLF signals in the D ionospheric layer during the selected SF events were
monitored using Sudden Ionospheric Disturbance (SID)
data. Two case studies were performed which consisted of four SF events from a
total of 23 events that were detected by geomagnetic data during the period of
study. Further analysis on the selected SF events showed the common effects of
SFs on the D layer, which is the increment on the VLF signal measured from the
SID stations although a different response was detected in the EUEL index
variations. This indicates that the VLF signal always shows an increment even
though a decrement in the ionization of the E layer occurs as a result of the
SF events. The difference in responses could be attributed to the distinct
changes in electron density of both layers during the SF occurrence. Further
studies are needed to elucidate the underlying mechanism responsible for this
unique response, utilizing appropriate parameters such as total electron
content, as well as the electron density data to thoroughly analyze the ionospheric response during SF events.
Keywords:
EEJ current; geomagnetic field; SID; solar flare; VLF signal
Abstrak
Penyelidikan ini mengkaji kesan nyalaan suria (SF)
secara serentak pada kedua-dua lapisan D dan E ionosfera Bumi. Analisis
memfokuskan kepada SF kelas M dan X yang berlaku semasa kitaran suria ke-24
kerana kedua-dua kelas SF ini menghasilkan kesan yang ketara ke atas
persekitaran Bumi, terutamanya pada waktu siang. Data yang digunakan untuk
mengesan kejadian SF dalam kajian ini ialah data magnetometer cerapan dasar
dari rantau-rantau khatulistiwa. Kesan kejadian SF yang dipilih pada lapisan E
telah dikaji berdasarkan indeks EUEL yang dibina menggunakan data medan
geomagnet tersebut. Sementara itu, data Gangguan Ionosfera Mendadak (SID)
digunakan untuk memantau perubahan kekuatan isyarat radio VLF pada
lapisan D ionosfera untuk kejadian SF yang terpilih. Dua kajian kes telah
dilakukan yang terdiri daripada empat kejadian SF daripada 23 peristiwa yang
dikesan oleh data geomagnet sepanjang tempoh kajian. Analisis lanjut mengenai
kejadian SF terpilih telah memerhatikan kesan umum SF pada lapisan D iaitu kenaikan
pada isyarat VLF yang diukur dari stesen SID walaupun tindak balas berbeza
dikesan dalam variasi indeks EUEL. Ini menunjukkan bahawa isyarat VLF sentiasa
menunjukkan kenaikan walaupun pengurangan dalam pengionan lapisan E terjadi
kesan daripada kejadian SF. Perbezaan dalam tindak balas ini boleh disebabkan
oleh perubahan yang berbeza dalam ketumpatan elektron pada kedua-dua lapisan
semasa berlakunya kejadian SF. Kajian lanjut diperlukan untuk menerangkan
mekanisme tindak balas unik ini dengan menggunakan parameter yang sesuai
seperti jumlah kandungan elektron serta data ketumpatan elektron untuk
menganalisis secara menyeluruh akan tindak balas ionosfera semasa kejadian SF.
Kata kunci: Arus EEJ; isyarat VLF; medan geomagnet; nyalaan suria; SID
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*Pengarang untuk surat-menyurat; email:
shazana.ukm@gmail.com
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