How do core surface flow models vary when inverted from IGRF-14 candidate field models? [PDF]
Rogers HF, Mandea M.
europepmc +2 more sources
Gravitational dynamos and the low-frequency geomagnetic secular variation. [PDF]
Olson P.
europepmc +1 more source
Waves in planetary dynamos. [PDF]
Hori K, Nilsson A, Tobias SM.
europepmc +1 more source
Forecasting secular variation using physics-informed neural networks for IGRF-14. [PDF]
Shakespeare-Rees N +6 more
europepmc +1 more source
Core Surface Flow Changes Associated With the 2017 Pacific Geomagnetic Jerk. [PDF]
Whaler KA +3 more
europepmc +1 more source
Detecting dipolarity of the geomagnetic field in the paleomagnetic record. [PDF]
Lhuillier F, Shcherbakov VP, Sycheva NK.
europepmc +1 more source
Extraordinarily long duration of Eocene geomagnetic polarity reversals. [PDF]
Yamamoto Y +3 more
europepmc +1 more source
A database of geomagnetic observatory monthly means: from historic to the satellite era. [PDF]
Brown W, Macmillan S, Maume E, Eaton E.
europepmc +1 more source
Lack of evidence for a fine-scale magnetic map sense for fall migratory Eastern North American monarch butterflies (Danaus plexippus). [PDF]
Guerra PA, Parlin AF, Matter SF.
europepmc +1 more source
A secular variation candidate for IGRF-14 based on core-flow inversion via an ensemble Kalman smoother. [PDF]
Gwirtz K, Sabaka T, Kuang W.
europepmc +1 more source

