Physics
Scientist
Institute of Geophysics and Planetary Physics, Scripps Institution of Oceanography, La Jolla, CA 92093-0225, USA
Institute of Geophysics and Planetary Physics, Scripps Institution of Oceanography, University of California, San Diego, 9500 Gilman Drive, La Jolla, CA 92093-0225, USA of Geophysics and Planetary Physics, Scripps Institution of Oceanography, University of California, San Diego, La Jolla, CA 92093-0225, USA
Institute of Geophysics and Planetary Physics, Scripps Institution of Oceanography, University of California, La Jolla, CA 92093-0225, USA
Institute for Geophysics and Planetary Physics, Scripps Institution of Oceanography, University of California, La Jolla, CA, USA
IGPP, Scripps Institution of Oceanography, La Jolla, CA 92093, USA
Cecil H. and Ida M. Green Institute of Geophysics and Planetary Physics, Scripps Institution of Oceanography, University of California, San Diego, 9500 Gilman Drive, La Jolla, CA, 92093-0225, USA
California, University, La Jolla
Cecil H. and Ida M. Green Institute of Geophysics and Planetary Physics, Scripps Institution of Oceanography, University of California at San Diego, 9500 Gilman Drive, La Jolla, CA 92093-0225, USA
Scripps Institution of Oceanography, University of California, San Diego, 9500 Gilman Drive, La Jolla, CA 92093-0220, USA
Institute of Geophysics and Planetary Physics, Scripps Institution of Oceanography, University of California, San Diego, 9500 Gilman Drive La Jolla, CA 92093-0225, USA
Institute of Geophysics and Planetary Physics, Scripps Institution of Oceanography, 92093-0225, La Jolla, CA, USA
Institute for Geophysics and Planetary Physics, Scripps Institution of Oceanography, University of Cal
40 Ar/ 39 Ar ages and paleomagnetism of São Miguel lavas, Azores
Anisotropic paleosecular variation models: implications for geomagnetic field observables
Assessing the dipolar signal in stacked paleointensity records using a statistical error model and geodynamo simulations
Asymmetry in growth and decay of the geomagnetic dipole
Centennial to millennial geomagnetic secular variation
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