Multivariable statistical analysis between geomagnetic field, climate, and orbital periodicities over the last 500 KYR, and their relationships during the last interglacial
Autores:
Luiggina Cappellotto, María Julia Orgeira, Víctor Manuel Velasco Herrera, Rodolfo Gustavo Cionco
Año de la publicación:
2 022
Revista:
Global and Planetary Change 213 (2022)
Abstract:
Relationships between geomagnetic field (GF) variations, paleoclimates, and Milankovitch cycles have increasingly
attracted the attention of researchers mainly because of the assumption that GF may have acted as a climate
forcing, suggesting that GF variations and orbital forcing may be linked in a complex synergistic way, especially,
during interglacials and interstadials. We first performed an exhaustive analysis of the relationship between GF, a
paleotemperature proxy, astroclimatic parameters, and the summer solstice mean daily insolation at 65 N over
the last 500 kyr. We evaluated the relationship between the variables at the orbital scale, using wavelets, cross
wavelets, and multiple cross wavelets. Our novel approach to the subject is the use of a new multiple cross
wavelet algorithm, which allowed us to simultaneously analyze several data series and determine the relative
phases between the signals. We confirm that the eccentricity modulates the GF behavior, and that the precession
could have been related to some short-term GF variations. Both orbital parameters seem to be precursors of GF
changes. Also, it is especially interesting to investigate the role of the GF reversion events because they could
have acted as an indirect climate forcing, and we focused on the relationship among forcings during Marine
Isotope Stage (MIS) 5. During this period, two GF reversions (Blake and post-Blake) could have been associated
with relative climate cooling. The consequent lack or weakening of shielding associated with GF events and
downward insolation, both influenced by orbital forcing, could finally have promoted a relative global climate
cooling during MIS 5.
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