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Third generation of the Potsdam Magnetic Model of the Earth (POMME)

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TLDR
The Potsdam Magnetic Model of Earth (POMME) as discussed by the authors is a geomagnetic field model providing an estimate of the Earth's core, crustal, magnetospheric, and induced magnetic fields.
Abstract
The Potsdam Magnetic Model of the Earth (POMME) is a geomagnetic field model providing an estimate of the Earth's core, crustal, magnetospheric, and induced magnetic fields. The internal field is represented to spherical harmonic (SH) degree 90, while the secular variation and acceleration are given to SH degree 16. Static and time-varying magnetospheric fields are parameterized in Geocentric Solar-Magnetospheric (GSM) and Solar-Magnetic (SM) coordinates and include Disturbance Storm-Time (Dst index) and Interplanetary Magnetic Field (IMF-By) dependent contributions. The model was estimated from five years of CHAMP satellite magnetic data. All measurements were corrected for ocean tidal induction and night-side ionospheric F-region currents. The model is validated using an independent model from a combined data set of Orsted and SAC-C satellite measurements. For the core field to SH degree 13, the root mean square (RMS) vector difference between the two models at the center of the model period is smaller than 4 nT at the Earth's surface. The RMS uncertainty increases to about 100 nT for the predicted field in 2010, as inferred from the difference between the two models.

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Journal ArticleDOI

Dynamo Scaling Laws and Applications to the Planets

TL;DR: The scaling laws for planetary dynamos relate the characteristic magnetic field strength, characteristic flow velocity and other properties to primary quantities such as core size, rotation rate, electrical conductivity and heat flux as discussed by the authors.
Journal ArticleDOI

Longitudinal variation of the E-region electric fields caused by atmospheric tides

TL;DR: In this article, the post-sunset EIA made by the IMAGE and TIMED satellites are compared with CHAMP, Orsted and SAC-C observations of the noontime equatorial electrojet (EEJ).
Book ChapterDOI

Numerical Dynamo Simulations

TL;DR: In this article, numerical simulations of the geodynamo that solve the fundamental equations of convection-driven flow and magnetic induction in a rotating spherical shell successfully reproduce many observed features of geomagnetic field.
Journal ArticleDOI

Conditions for Earth-like geodynamo models

TL;DR: In this article, the authors define quantitative criteria for the degree of semblance of a model field with the geomagnetic field, based on the field morphology at the core-mantle boundary.
Journal ArticleDOI

Quasi-geostrophic flows responsible for the secular variation of the Earth's magnetic field

TL;DR: In this paper, a large jet encircling the inner core and carrying a significant part of the core angular momentum and axial vortices of ∼700 km diameter mainly clustering around the cylinder tangent to the solid inner core, are inferred from geomagnetic SV.
References
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Journal ArticleDOI

International Reference Ionosphere 2000

Dieter Bilitza
- 01 Mar 2001 - 
TL;DR: The International Reference Ionosphere (IRI) is the international standard for the specification of ionospheric densities and temperatures as mentioned in this paper, which was developed and is being improved-updated by a joint working group of the International Union of Radio Science (URSI) and the Committee on Space Research (COSPAR).
Book

Foundations of geomagnetism

TL;DR: In this article, the Mie representation of the main field has been studied in the context of classical electrodynamics and spherical harmonics, as well as Gauss' theory of main field and hydromagnetics.
Journal ArticleDOI

CHAOS—a model of the Earth's magnetic field derived from CHAMP, Ørsted, and SAC‐C magnetic satellite data

TL;DR: In this paper, the authors derived a model of the near-Earth magnetic field (up to spherical harmonic degree n = 50 for the static field, and up to n = 18 for the first time derivative) using more than 6.5 yr of high-precision geomagnetic measurements from the three satellites Orsted, CHAMP and SAC-C taken between 1999 March and 2005 December.
Journal ArticleDOI

Magnetic signatures of equatorial spread F as observed by the CHAMP satellite

TL;DR: In this paper, the authors derived the global distribution of magnetic signatures of postsunset equatorial spread F (ESF) events from a continuous database covering the years 2001-2004.
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