Sains Malaysiana 48(11)(2019): 2427–2435
http://dx.doi.org/10.17576/jsm-2019-4811-13
Geomagnetic Phenomena Observed by a Temporal
Station at Ulu-Slim, Malaysia during the Storm of March 27, 2017
(Fenomena Geomagnetik yang Dicerap oleh Stesen Temporal di Ulu-Slim,
Malaysia semasa Ribut
pada 27 Mac 2017)
ARAFA-HAMED,
T.1,
KHALIL,
A.2*,
NAWAWI,
M.2,
HASSAN,
H.3
& M.H. ARIFIN4
1National Research
Institute of Astronomy and Geophysics (NRIAG), Egypt
2School of Physics,
Universiti Sains
Malaysia, 11800 USM, Pulau Pinang, Malaysia
3Geology Department,
Faculty of Science, Helwan University,
Egypt
4Program Geologi, Pusat Sains Bumi dan
Alam Sekitar,
Fakulti Sains dan
Teknologi, Universiti
Kebangsaan Malaysia, 43600 UKM Bangi,
Selangor Darul Ehsan, Malaysia
Received: 7 April 2019/Accepted: 15
August 2019
ABSTRACT
A 3-axis fluxgate magnetometer
was temporally setup for continuous recording during March 2017
at 3о
54’ 6” N, 101о 29’ 41”
E, Ulu-Slim, Malaysia. On March 27th, a magnetic storm has been
triggered by energetic solar wind emitted from a coronal hole on
the sun that impacted the magnetosphere until the end of the measurement
campaign on March 29th. The values measured at a sampling rate of
600 Hz are averaged to get a 1 Hz record from March 26 16:00 LT to March 29 12:00 LT.
The 1 second data set is studied to deduce all magnetic phenomena
captured during the magnetic storm. An overview of the complete
record indicates the start of the storm and a complete absence of
the typical diurnal variation of the total-field intensity on March
28. The diurnal variations are eliminated by subtracting a moving
average of 100 samples from the recorded values. The residual shows
a clear amplification of pulsations with the start of the storm.
Pulsations enhancement are common around noon and is continuous
on March 28th due to magnetotail activities
during local night. Magnetospheric breathing as compression and expansion of the
magnetosphere at long periods of 20 to 40 min is captured twice
during the storm. An obvious occurrence of magnetotail
reconnection is deduced by a sudden, steep increase of the total
magnetic field with 50 nT at 01:30 LT on
March 28. We conclude that the continuous recording of the magnetic
field components provides very useful information about what processes
are ongoing in space and how it might affect the logistics on the
ground. The implementation of similar magnetometers as continuous
observation stations would be of crucial benefits for Malaysia in
both basic scientific and environmental aspects.
Keywords: Coronal hole; geomagnetic
storm; magnetospheric processes
ABSTRAK
Meter Magnet fluxgate 3-paksi
telah didirikan untuk rakaman berterusan
pada Mac 2017 di 3° 54’ 6” U, 101° 29’
41” T, Ulu-Slim, Malaysia. Pada 27 Mac,
ribut magnet telah
dicetuskan oleh angin suria
bertenaga yang dipancarkan
daripada lubang korona di matahari yang memberi kesan kepada
magnetosfera sehingga
berakhirnya kempen pengukuran pada 29 Mac. Nilai-nilai yang diukur pada kadar persampelan
600 Hz adalah untuk
mendapatkan rekod purata 1 Hz dari 26 Mac 16:00 waktu tempatan hingga 29 Mac 12:00 waktu tempatan. Set data 1 saat dikaji untuk menyimpulkan
semua fenomena
magnet yang direkod semasa ribut magnet. Gambaran keseluruhan rekod lengkap menandakan permulaan ribut dan ketiadaan lengkap
variasi diurnal yang tipikal
daripada keamatan
keseluruhan medan pada 28 Mac. Variasi diurnal dihapuskan dengan menolak purata bergerak 100 sampel daripada nilai yang direkodkan. Baki menunjukkan penguatan denyutan yang jelas dengan permulaan ribut. Peningkatan pulsasi adalah umum sekitar tengah
hari dan berterusan pada 28 Mac disebabkan aktiviti ekor magnet semasa malam tempatan. Pernafasan magnetosfera sebagai mampatan dan pengembangan magnetosfera pada masa yang panjang iaitu 20 hingga 40 min direkodkan dua kali semasa ribut. Satu kejadian
yang jelas mengenai
penyambungan semula ekor magnet disimpulkan oleh peningkatan mendadak daripada medan magnet keseluruhan dengan 50 nT pada
01:30 waktu tempatan
pada 28 Mac. Kami menyimpulkan bahawa rakaman berterusan komponen magnetik menyediakan maklumat yang sangat berguna tentang apa proses yang berterusan dalam ruang dan
bagaimana ia
boleh mempengaruhi logistik di lapangan. Pengukuran meter magnet yang sama
sebagai stesen
pemerhati yang berterusan akan menjadi manfaat
penting bagi
Malaysia dalam kedua-dua aspek asas saintifik
dan alam sekitar.
Kata kunci: Lubang
korona; proses magnetosfera;
ribut geomagnet
REFERENCES
Alfven, H. & Falthammar, C.G. 1963.
Cosmical Electrodynamics: Fundamental Principles.
Oxford: Clarendon Press. p. 228.
Baker, D.N., Pulkkinen, T.I., Angelopulos, V., Baumjohann, W.
& McPherron, R.L. 1996. Neutral line
model of substorms: Past results and present view. J. Geophys. Res. 101(A6): 12875- 13010.
Barnes, A. 1983. Hydromagnetic waves, turbulence,
and collisionless processes in the interplanetary
medium. In Solar- Terrestrial Physics: Principles and Theoretical
Foundations, edited by Carovillano,
R.L., Forbes, J.M. & Reidel. D. Dordrecht:
Publishing Company. pp. 155-199.
Baumjohann, W.
2002. Modes of convection in the magnetotail.
Phys. Plasmas 9: 3665-3667.
Collier, M.R. & Lepping, R.P. 1996.
Jovian magnetopause breathing. Planetary and Space Science 44(3):
187-197.
Cowley, S.W.H., Wright, D.M., Bunce, E.J., Carter, A.C., Dougherty,
M.K., Giampieri, G., Nichols, J.D. &
Robinson, T.R. 2006. Cassini observations of planetary-period magnetic
field oscillations in Saturn’s magnetosphere: Doppler shifts and
phase motion. Geophys. Res. Lett. p. 33. DOI: 10.1029/2005GL025522.
Ghamry, E.,
Lethy, A., Arafa-Hamed, T. &
Abd Elaal, E. 2016. A comprehensive
analysis of the geomagnetic storms occurred during 18 February and
2 March 2014. NRIAG Journal of Astronomy and Geophysics 5(1):
263-268.
Glassmeier, K.H.,
Soffel, H. & Negendank,
J.W. 2009. Geomagnetic Variations, Space-Time Structure, Processes,
and Effects on System Earth. Heidelberg: Springer Verlag.
Langangen, O.,
Carlsson, M. & Voort, L.R. 2007.
Velocities measured in small-scale solar magnetic elements. The
Astrophysical Journal 655: 615-623.
Lin, N.M.J.E., Anderson, B.J., McPherron,
R.L., Kivelson, M.G., Baumjohann,
W., Luehr, H., Potemera,
T.A. & Zanetti, L.J. 1991. A comparison of ULF wave fluctuations
in the solar wind, magnetosheath, and
dayside magnetosphere: 2. Field and plasma conditions in the magnetosheath.
J. Geophys. Res. 96: 3455-3464.
McPherron, R.L.
2005. Magnetic pulsations: Their sources and relation to solar wind
and geomagnetic activity. Survey of Geophysics 26: 545-592.
Nabert, C.,
Glassmeier, K.H. & Plaschke,
F. 2013. A new method for solving the MHD equations in the magnetosheath.
Ann. Geophys. 31: 419-437.
Nabert, C.,
Othmer, C. & Glassmeier, K.H.
2017. Estimating a planetary magnetic field with time-dependent
global MHD simulations using an adjoint
approach. Geophys. 35: 613-628.
Nowada, M.,
Fear, R.C., Grocott, A., Shi, Q.Q., Yang,
J. & Zong, Q.G. 2018. Subsidence of ionospheric
flows triggered by magnetotail magnetic
reconnection during transpolar arc brightening. Journal of Geophysical
Research: Space Physics 123: 3398-3420.
Paschmann, G.,
Oieroset, M. & Phan, T. 2013. In situ observations
of reconnection in space. Sci. Rev. 178: 385-417.
Potemra, T.A.
1998. The dynamic magnetosphere. In Polar Cap Boundary Phenomena.
NATO ASI Series (Series C: Mathematical and Physical Sciences),
edited by Moen, J., Egeland, A. & Lockwood, M. Dordrecht: Springer. p. 509.
Ramer, K.M., Kivelson, M.G., Sergis, N., Khurana, K.K. &
Jia, X. 2016. Spinning, breathing, and flapping: Periodicities
in Saturn’s middle magnetosphere. J. Geophys.
Res. pp. 122-126.
Schillinger,
D. & Papadopoulos, V. 2010. Accurate estimation of evolutionary
power spectra for strongly narrow-band random fields. Computer
Methods in Applied Mechanics and Engineering 199: 947-960.
Schillinger,
D., Stefanov, D. & Stavrev,
A. 2013. The method of separation for evolutionary spectral density
estimation of multi-variate and multi-dimensional non-stationary
stochastic processes. Probabilistic Engineering Mechanics 33:
58-78.
Wing,
S., Johnson, J.R., Chaston, C.C., Echim,
M., Escoubet, C.P., Lavraud,
B., Lemon, C., Nykyri, K., Otto, A., Raeder,
J. & Wang, C.P. 2014. Review of solar wind entry into and transport
within the plasma sheet. Space Sci. Rev. 184: 33-86.
*Corresponding author; email: amin_khalil@usm.my
|