The study brought together data from several spacecraft, as well as supporting observations from solar wind probes and ground -
based geomagnetic observatories, to develop a model that describes the Earth's magnetic field and its interaction with the solar wind not just theoretically as had been the case previously, but based on actual measurements.
Not exact matches
«This discrepancy between 1D - and 3D -
based calculations of the 1989 storm demonstrates the importance of realistic data, rather than relying on previous 1D models, to determine the impact that a
geomagnetic storm has on power grids,» Lucas said.
But there is another magnetically
based north pole: the north
geomagnetic pole.
The research entitled «Network analysis of
geomagnetic substorms using the SuperMAG database of ground -
based magnetometer stations» has just been published in the Journal of Geophysical Research: Space Physics by a team of researchers from the Centre for Fusion, Space and Astrophysics in the Department of Physics at the University of Warwick; The Department of Physics and Technology, University of Bergen, Bergen, Norway; and The Johns Hopkins University Applied Physics Laboratory, Laurel, Maryland, USA.
The team investigated patterns of magnetic reversals — another method to determine age
based on knowledge about an era's magnetic orientation — and calibrated the sediments containing the fossils using
Geomagnetic Polarity Time Scale (GPTS).
Based on the theoretical
geomagnetic field computer models (Which are all incorrect as the
geomagnetic field is not generated in the core.
Re «I believe, sudden, rapid, and sever global cooling is possible and likely
based on the paleoclimatic and paleo -
geomagnetic records.»
I believe, sudden, rapid, and sever global cooling is possible and likely
based on the paleoclimatic and paleo -
geomagnetic records.
The SWPC is
based in Boulder, Colo., and observes the Sun in real time from both ground -
based observatories and satellites in order to predict
geomagnetic storms.
The JPL - Oxford University paper is
based on the
geomagnetic measurements http://trs-new.jpl.nasa.gov/dspace/bitstream/2014/13763/1/00-0133.pdf
«The solar and volcanic forcings we use are derived from reconstructions
based on proxy data and are therefore also subject to considerable uncertainties, although recent explosive volcanic eruptions are likely to have cooled climate, and independent records of solar activity levels inferred from the cosmogenic isotope 10Be (43) and
geomagnetic records (44) provide support to reconstructions (22, 45) that show generally increasing solar activity during the 20th century (12).»
The BHMF trend thus obtained is then compared with the most recent reconstructions of the near - Earth HMF strength
based on
geomagnetic, sunspot number, and cosmogenic isotope data.
Typical reconstructions of historic heliospheric magnetic field (HMF) BHMF are
based on the analysis of the sunspot activity,
geomagnetic data or on measurement of cosmogenic isotopes stored in terrestrial reservoirs like trees (14C) and ice cores (10Be).
The modeling approach is
based on presenting the ionospheric parameter (most frequently the F - layer critical frequency foF2) by analytical expressions as a function of one or more
geomagnetic or solar indices, called drivers.
http://www.agci.org/docs/lean.pdf «Global (and regional) surface temperature fluctuations in the past 120 years reflect, as in the space era, a combination of solar, volcanic, ENSO, and anthropogenic influences, with relative contributions shown in Figure 6.22 The adopted solar brightness changes in this scenario are
based on a solar surface flux transport model; although long - term changes are «50 % larger than the 11 - year irradiance cycle, they are significantly smaller than the original estimates
based on variations in Sun - like stars and
geomagnetic activity.
A number of new millennial - scale
geomagnetic field reconstructions have been published over the last years,
based on improved global archeo - and paleomagnetic data compilations.
The somewhat contradictory results for the similarity of radionuclide -
based dipole reconstructions and
geomagnetic field models on these time scales point out that
geomagnetic field models have to be improved further before they can provide a truly robust means to eliminate the influence of
geomagnetic variability in cosmogenic radionuclide production studies.
Here we review several spherical harmonic models and compare their dipole field predictions to reconstructions
based on virtual axial dipole moments and virtual
geomagnetic poles.
Nilsson et al. (2011) computed a synthetic tilt modulated VADM record for a location in western Eurasia
based on dipole strength estimates obtained from 10Be flux and taking into account the dipole tilt
based on the reconstruction of the northern
geomagnetic pole position from VGP of globally distributed sediment records.
Similarities in these variations to the reconstructions
based on
geomagnetic data hardly seem to exist.
For comparison purposes, we
base our calculations on the assumption that the variations seen in 14C and 10Be records after applying different low - pass filters originate only from
geomagnetic dipole variations.
Dipole moment reconstructions from
geomagnetic models CALS3k.3 (light blue) and CALS3k.4 (dark blue) and
based on 14C (brown) and 10Be (green) records.
The 14C production record and the 10Be flux records have been converted into
geomagnetic field intensity estimates
based on the results of Masarik & Beer (1999) after the low - pass filtering.