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pro vyhledávání: '"Merkuryev, S. A."'
A new approach to estimating the velocity of the pole moving is considered. The method uses the model-calculated spatial distribution of the (vector) horizontal component \textbf{H} for a given year and its change relative to the closest epochs. The
Externí odkaz:
http://arxiv.org/abs/2212.12820
Based on satellite data, both large and small-scale flows were identified on the core surface .At the same time, the observed rapid decrease in the dipole component of the main geomagnetic field does not find a satisfactory explanation. In the previo
Externí odkaz:
http://arxiv.org/abs/2010.09062
Autor:
Ivanov, S. A., Merkuryev, S. A.
Marine magnetic anomalies of the tiny wiggles (TW) type can be used to solve geohistorical and paleomagnetic problems. The model fields corresponding to Paleocene-Eocene anomalies in the northwestern Indian Ocean, which were formed during the fasts p
Externí odkaz:
http://arxiv.org/abs/1612.06001
Autor:
Ivanov, S. A., Merkuryev, S. A.
We use the Cramer-Rao bound to show which short magnetic reversals can be recovered successfully from a magnetic anomaly profile. Using a simple variant of the Vine-Matthews model, we show, in particular, that errors in determining the duration of a
Externí odkaz:
http://arxiv.org/abs/1302.0486
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