EGU22-7290
https://doi.org/10.5194/egusphere-egu22-7290
EGU General Assembly 2022
© Author(s) 2022. This work is distributed under
the Creative Commons Attribution 4.0 License.

The Kalmag and ArchKalmag14K geomagnetic field models: their derivation principle, properties and availability

Julien Baerenzung, Maximilian Arthus Schanner, Monika Korte, Jan Saynisch, and Matthias Holschneider
Julien Baerenzung et al.
  • University of Potsdam, Institute for mathematics, Berlin, Germany (baerenzung@gmx.de)

The recent Kalmag and archaeomagnetic ArchKalmag14K models together represent the global geomagnetic field model evolution over the past 14000 years and resolve temporal scales of the order of a month over the last 122 years. They are obtained through the sequential assimilation of archeomagnetic and volcanic data, and survey, observatory and satellite data, respectively. Both these models provide full posterior information about the core field, and in the case of Kalmag also about other magnetic sources such as the lithospheric or some tidal fields. These models are made accessible online through different physical and statistical quantities associated with them. In this presentation, we will detail our modeling strategy, the type of results we are getting with it, and how the community can access and use our models by an online interface at https://ionocovar.agnld.uni-potsdam.de/Kalmag/ and https://ionocovar.agnld.uni-potsdam.de/Kalmag/Archeo/.

How to cite: Baerenzung, J., Schanner, M. A., Korte, M., Saynisch, J., and Holschneider, M.: The Kalmag and ArchKalmag14K geomagnetic field models: their derivation principle, properties and availability, EGU General Assembly 2022, Vienna, Austria, 23–27 May 2022, EGU22-7290, https://doi.org/10.5194/egusphere-egu22-7290, 2022.