Could the Mw = 9.3 Sumatra Earthquake Trigger a Geomagnetic Jerk?
Author(s)
Language
English
Obiettivo Specifico
3.3. Geodinamica e struttura dell'interno della Terra
3.4. Geomagnetismo
Status
Published
JCR Journal
N/A or not JCR
Peer review journal
Yes
Journal
Issue/vol(year)
12 / 86 (2005)
Publisher
AGU
Pages (printed)
123
Date Issued
March 22, 2005
Abstract
The magnetic field observed at the Earth’s
surface is not a stationary feature. It is characterized by time variations ranging from
milliseconds (micropulsations) to millions of
years (the time interval between field reversals). Time variations with periods of a year or longer are related to Earth’s outer core sources, whereas for shorter timescales an external origin is invoked (i.e., solar activity). One of the most interesting time variations of the geomagnetic field is represented by the “geomagnetic jerk.” It is idealized as a rapid change in the slope of the secular variation, defined as the first derivative of the geomagnetic field. This means that the secular variation roughly appears as a series of straightline
segments separated by geomagnetic jerks.
surface is not a stationary feature. It is characterized by time variations ranging from
milliseconds (micropulsations) to millions of
years (the time interval between field reversals). Time variations with periods of a year or longer are related to Earth’s outer core sources, whereas for shorter timescales an external origin is invoked (i.e., solar activity). One of the most interesting time variations of the geomagnetic field is represented by the “geomagnetic jerk.” It is idealized as a rapid change in the slope of the secular variation, defined as the first derivative of the geomagnetic field. This means that the secular variation roughly appears as a series of straightline
segments separated by geomagnetic jerks.
References
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jerks, J.Geophys.Res.,101,21,975–21,994.
Alfonsi, L.,A. Piersanti, and G. Spada (1997), Did the
1977 Sumba earthquake excite the Chandler wobble?,
Earth Planet. Sci. Lett.,153, 287–292.
Bellanger, E., J.-L. Le Mouël, M.Mandea,and
S. Labrosse (2001), Chandler wobble and geomagnetic
jerks,Phys. Earth Planet. Inter.,124, 95–103.
Bloxam, J., S.Zatman, and M.Dumberry (2002),The
origin of geomagnetic jerks, Nature,420, 65–68.
Chao,B. F. (2005), Did the 26 December 2004 Sumatra,
Indonesia, earthquake disrupt the Earth’s rotation
as the mass media have said?, Eos Trans.AGU,
86(1), 1–2.
Gibert,D.,M.Holschneider, and J.-L. Le Mouël (1998),
Wavelet analysis of the Chandler wobble,
J.Geophys. Res.,103, 27,069–27,089.
Gross, R. S. (2000),The excitation of the Chandler
wobble,Geophys. Res. Lett.,27, 2329–2332.
Gross, R. S., and B. F.Chao, (1985), Excitation study of
the LAGEOS-derived Chandler wobble, J.Geophys.
Res.,90, 9369–9380.
Malin, S. R. C., and B. M.Hodder (1982),Was the 1970
geomagnetic jerk of internal or external origin?,
Nature,296, 726–728.
Mandea,M., E. Bellanger, and J.-L. Le Mouël (2000),
A geomagnetic jerk for the end of the 20th century?,
Earth Planet. Sci. Lett.,183, 369–373.
Sabadini, R.,A. Piersanti, and G. Spada (1995),
Toroidal/poloidal partitioning of global postseismic
deformation,Geophys. Res. Lett.,22, 985–988.
Waddington, R.,D.Gubbins, and N.Baber (1995),
Geomagnetic field analysis: 5. Determining steady
core-surface flows directly from geomagnetic
observations,Geophys. J. Int.,122, 326–350.
G.Saracco (1996),Worldwide wavelet analysis of geomagnetic
jerks, J.Geophys.Res.,101,21,975–21,994.
Alfonsi, L.,A. Piersanti, and G. Spada (1997), Did the
1977 Sumba earthquake excite the Chandler wobble?,
Earth Planet. Sci. Lett.,153, 287–292.
Bellanger, E., J.-L. Le Mouël, M.Mandea,and
S. Labrosse (2001), Chandler wobble and geomagnetic
jerks,Phys. Earth Planet. Inter.,124, 95–103.
Bloxam, J., S.Zatman, and M.Dumberry (2002),The
origin of geomagnetic jerks, Nature,420, 65–68.
Chao,B. F. (2005), Did the 26 December 2004 Sumatra,
Indonesia, earthquake disrupt the Earth’s rotation
as the mass media have said?, Eos Trans.AGU,
86(1), 1–2.
Gibert,D.,M.Holschneider, and J.-L. Le Mouël (1998),
Wavelet analysis of the Chandler wobble,
J.Geophys. Res.,103, 27,069–27,089.
Gross, R. S. (2000),The excitation of the Chandler
wobble,Geophys. Res. Lett.,27, 2329–2332.
Gross, R. S., and B. F.Chao, (1985), Excitation study of
the LAGEOS-derived Chandler wobble, J.Geophys.
Res.,90, 9369–9380.
Malin, S. R. C., and B. M.Hodder (1982),Was the 1970
geomagnetic jerk of internal or external origin?,
Nature,296, 726–728.
Mandea,M., E. Bellanger, and J.-L. Le Mouël (2000),
A geomagnetic jerk for the end of the 20th century?,
Earth Planet. Sci. Lett.,183, 369–373.
Sabadini, R.,A. Piersanti, and G. Spada (1995),
Toroidal/poloidal partitioning of global postseismic
deformation,Geophys. Res. Lett.,22, 985–988.
Waddington, R.,D.Gubbins, and N.Baber (1995),
Geomagnetic field analysis: 5. Determining steady
core-surface flows directly from geomagnetic
observations,Geophys. J. Int.,122, 326–350.
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