English
 
Privacy Policy Disclaimer
  Advanced SearchBrowse

Item

ITEM ACTIONSEXPORT

Released

Journal Article

Variabilität des Erdmagnetfelds im Holozän

Authors
/persons/resource/monika

Korte,  Monike
System Erde : GFZ Journal Vol. 2, Issue 1 (2012), System Erde : GFZ Journal 2012, Deutsches GeoForschungsZentrum;
2.3 Earth's Magnetic Field, 2.0 Physics of the Earth, Departments, GFZ Publication Database, Deutsches GeoForschungsZentrum;

/persons/resource/ufrank

Frank,  Ute
System Erde : GFZ Journal Vol. 2, Issue 1 (2012), System Erde : GFZ Journal 2012, Deutsches GeoForschungsZentrum;
5.2 Climate Dynamics and Landscape Evolution, 5.0 Earth Surface Processes, Departments, GFZ Publication Database, Deutsches GeoForschungsZentrum;

External Ressource
Fulltext (public)

GFZ_syserde.02.01.8.pdf
(Publisher version), 416KB

Supplementary Material (public)
There is no public supplementary material available
Citation

Korte, M., Frank, U. (2012): Variabilität des Erdmagnetfelds im Holozän. - System Erde, 2, 1, 42-45.
https://doi.org/10.2312/GFZ.syserde.02.01.8


Cite as: https://gfzpublic.gfz-potsdam.de/pubman/item/item_65128
Abstract
The geomagnetic field shields our habitat against solar wind and galactic cosmic rays. Since the magnetic shielding influences cosmic ray induced ionization of the atmosphere on centennial time-scales, it might have effects on cloud formation and consequently climate. In order to identify possible links between geomagnetic variations and climate change, which are controversially discussed, good global geomagnetic field reconstructions on multi-centennial to millennial time-scales are a prerequisite to interpret records of climate change. Scientists from GFZ together with collaborators from the US, Switzerland and Great Britain have worked on millennial scale magnetic field models for nearly 10 years. A first model spanning the past 10 kyrs, the Holocene, was published last year. The resolution and accuracy of the model is still limited due to data distribution and quality, but higher resolution models for the past 3 kyrs are feasible and have been published previously. These models provide continuous descriptions of dipole moment and tilt variations through the Holocene and of the global field intensity distribution, which all are relevant to estimate the magnetic shielding effect.