HR: 14:00h
AN: U42A-02 [PDF]
TI: Trends of the Geomagnetic Dipole from Observations Over the Last Three Centuries
AU: Mozzoni, D T
EM: cyric@geomag.gfdi.fsu.edu
AF: GFDI and CSIT
Florida State University, 18 Keene Bldg, Tallahassee, FL 32306-4360 United States
AU: * Cain, J C
EM: cain@geomag.gfdi.fsu.edu
AF: GFDI and CSIT
Florida State University, 18 Keene Bldg, Tallahassee, FL 32306-4360 United States
AB:
A review is made of published geomagnetic models
utilizing data from the 18th century when absolute measurements
were first introduced and those created with angular data back to
the 15th century, through those using spacecraft surveys such as
POGO, Magsat, \O rsted and CHAMP. The more detailed variations
since 1900 of the strength of the centered dipole are viewed to
evaluate whether the apparent $\sim 60$ year periodicity in the
average 5% decay per century is a valid feature of the observed
poloidal field or a result of the irregular distribution of data
used prior to full global coverage by spacecraft.
Simulated data using distributions for past epochs computed with
recent global models were analyzed. The results indicate that
whereas the higher components are suspect for early and mid 20th
century, the variations seen in the dipole itself are likely
valid. No acceleration of dipole decay over the average
century--long rate is indicated from these studies provided this
periodicity is taken into account.
The energy being lost by the dipole continues to be fed into that
of the $n=2$ and $n=3$ terms as originally noted by Verosub and
Cox, though there is excess loss presumably being converted to
heat. The direction of the dipole axis has continued to slowly
drift on a clockwise path (westward) as represented by $G-H(1,1)$
dialgrams since 1690, with the absolute value of that non--axial
contribution decreasing at least since the middle of the 19th
century.
DE: 1532 Reference fields (regional, global)
DE: 1545 Spatial variations (all harmonics and anomalies)
DE: 1560 Time variations--secular and long term
SC: U
MN: 2003 Fall Meeting