HR: 1340h
AN: GP33A-0925 [Abstracts]
TI: Constraint on the heterogeneity of mantle conductivity structure obtained from the geomagnetic jerks
AU: * Nagao, H
EM: nagao@jamstec.go.jp
AF: Japan Agency for Marine-Earth Science and Technology, 3173-25 Showa-machi,
Kanazawa-ku, Yokohama, 236-0001, Japan
AU: Shimizu, H
EM: shimizu@eri.u-tokyo.ac.jp
AF: The University of Tokyo, 1-1-1 Yayoi, Bunkyo-ku, Tokyo, 113-0032, Japan
AU: Utada, H
EM: utada@eri.u-tokyo.ac.jp
AF: The University of Tokyo, 1-1-1 Yayoi, Bunkyo-ku, Tokyo, 113-0032, Japan
AB:
It is well-known that the occurrence time of each geomagnetic jerk in the southern hemisphere delays a few years
comparing with the northern hemisphere (e.g., Alexandrescu et al [1996], Nagao et al. [2002, 2003]). Two
physical mechanisms are possible for this interesting phenomenon; the distribution of the magnetic field at the
core-mantle boundary (CMB) and/or the effect of the mantle conductivity on the magnetic field diffusion. Although
which mechanism is significant is still controversial, it is valuable to obtain a constraint on the mantle conductivity
that can explain this occurrence time lag.
Backus [1983] derived theoretically, in the case of 1-D mantle, several characteristic time constants of a jerk
related to the mantle conductivity, in which significant ones are delay time and smoothing time. We have been
developing a tool using the Kalman filter, which enables us to determine automatically the amplitude, occurrence
time, smoothing time of a jerk, and estimation error in each determined parameter. We apply this tool to the
eastward component of geomagnetic monthly means obtained at worldwide geomagnetic observatories, and find
that the distribution of amplitude has a spherical harmonic component of S22 and that the occurrence time in
the African region delays a few years comparing with the other regions. When a jerk is assumed to occur
simultaneously at the whole CMB, the mantle conductance is required to be an order of 109S in order to explain
this time lag. This conductance is much larger than the upper constraint estimated from several decades
variation in the length-of-day (LOD) on the basis of the electromagnetic core-mantle coupling theory. Therefore, a
lateral heterogeneity is to be taken into account in order to satisfy both the jerk occurrence time lag and the LOD
variation.
We carry out a numerical experiment in the wave number and frequency domains using the MIDM (Koyama et al.
[2002]) of how a magnetic field (especially in the case of S22) input from the CMB diffuses in the 3-D mantle,
and obtain a transfer function between an input at the CMB and the corresponding output at the Earthfs surface.
We can construct a synthetic but realistic time-variant magnetic field model utilizing this transfer function, and
obtain the time constants of a jerk. We will discuss in the presentation a constraint on the heterogeneity of the
mantle conductivity structure by comparing the time constants of the jerks estimated from the data analysis with
those obtained from the numerical experiment.
DE: 1515 Geomagnetic induction
DE: 1555 Time variations: diurnal to decadal
DE: 1560 Time variations: secular and longer
SC: Geomagnetism and Paleomagnetism [GP]
MN: 2007 Fall Meeting