Digital Archive (ERDA)
Development and Maintenance by the Database Team

Detailed File Information
Global geomagnetic Laschamp excursion characteristics - LSMOD and GGF100k
File Name
Data Type animation
Computer Program Not specified
File Size 100.97 MB - 1 file
Expert Level Science Overview (Specialist)
Contributor Monika Korte
Source Korte et al., 2019 doi: 10.3389/feart.2019.00086
Resource Matrix The Earth's Magnetic Field
These animations illustrate global geomagnetic field characteristics from 50 to 30~ka BP from several different spherical harmonic field models as compared in the related publication. LSMOD.2 is our preferred model, giving the currently best representation of the geomagnetic field evolution over the Laschamp (~41 ka) and Mono Lake (~36 to 31 ka) excursions. Model GGF100k is from S. Panosvska, C. G. Constable and M. Korte (2018), Extending global continuous geomagnetic field reconstructions on timescales beyond human civilization, Geochem. Geophys. Geosyst., 19, doi:10.1029/2018GC007966.

The panels from left to right are, in row 1: Maps of field intensity at Earth's surface (F surf.), paleo-secular variation index Pi, radial field component (Br at the core-mantle boundary (CMB, with continents for reference purpose); row 2: maps of virtual dipole moment (VDM) at Earth's surface and virtual geomagnetic pole (VGP) latitude, the geomagnetic power spectrum at the CMB (red dots) compared to the present-day (IGRF 12th generation) spectrum (grey dots), and two polar views of Br at the CMB with the inner core tangent cylinder outlined in black; row 3: time series of dipole latitude (Dip. Lat., blue, right ordinate) and dipole moment (DM, black, left ordinate) in top and of the three dipole spherical harmonic coefficients (g10, g11, h11) in the bottom panel, time series of globally averaged Pi with value given below, and time series of dipole (D) and non-dipole (ND) power at the CMB in the top and quadrupole (Q) and octupole (O) power in the bottom panel. The age is given in the top right and indicated by red vertical bars on the time series in row 3.

Related contribution "Global geomagnetic Laschamp excursion characteristics - further models" contains results from models derived to investigate the robustness of features and a previously published model.
Click to return to previous page