Results 81 to 90 of about 733 (165)
Prandtl-number dependence of convection-driven dynamos in rotating spherical fluid shells [PDF]
The value of the Prandtl number P exerts a strong influence on convection-driven dynamos in rotating spherical shells filled with electrically conducting fluids.
Busse, F.H., Simitev, R.
core +3 more sources
Revisiting the Excitation of Free Core Nutation
Abstract Earth possesses a Poincaré mode called Free Core Nutation (FCN) due to the misalignment of the rotation axes of the mantle and fluid outer core. FCN is the primary signal in the observations of Celestial Pole Offsets (CPO) and maintained by geophysical mechanisms that are yet to be understood. Earlier studies suggested an origin in Atmospheric
Mostafa Kiani Shahvandi +4 more
wiley +1 more source
Magnetic observatory data and metadata : types and availability [PDF]
The availability of magnetic observatory data has evolved rapidly with the transition of observatories from analogue photographic magnetograms to digital electronic recordings, and the advent of the internet for instant global access to information ...
Alex, Sobhana +6 more
core +1 more source
Abstract The aurora and associated high energy particles and currents pose a space weather hazard to communication networks and ground‐based infrastructure. Forecasting the location of the auroral oval forms an integral component of daily space weather operations.
M. K. Mooney +20 more
wiley +1 more source
Dynamic evolution of amplitude and position of geomagnetic secular acceleration pulses since 2000
Recent studies on the behavior of geomagnetic secular acceleration (SA) pulses have provided a basis for understanding the dynamic processes in the Earth’s core.
Chunhua Bai +3 more
doaj +1 more source
The Swarm Initial Field Model for the 2014 geomagnetic field [PDF]
Data from the first year of ESA's Swarm constellation mission are used to derive the Swarm Initial Field Model (SIFM), a new model of the Earth's magnetic field and its time variation.
Arnaud Chulliat +35 more
core +3 more sources
Time Sequence of Magnetospheric Responses to a Southward IMF Turning
Abstract We use MHD simulations to study the time sequence of magnetospheric responses to a synthetic event with a southward interplanetary magnetic field (IMF) turning. The onset of dayside magnetopause reconnection launches a weak rarefaction wave and sunward flow in the equatorial magnetosphere simultaneously with a tailward flow through the polar ...
Andrey Samsonov +6 more
wiley +1 more source
Forecasting geomagnetic time series for global field modelling [PDF]
The secular variation (SV) of the geomagnetic field is difficult to accurately predict with our current incomplete knowledge of its governing physics. Many academic and applied studies rely on the extrapolation of global field models beyond their most ...
Brown, William +2 more
core
The radiation environment in a Low Earth Orbit: the case of BeppoSAX
Low-inclination, low altitude Earth orbits (LEO) are of increasing importance for astrophysical satellites, due to their low background environment. Here, the South Atlantic Anomaly (SAA) is the region with the highest amount of radiation.
Campana, R. +4 more
core +1 more source
Evidence for a new geomagnetic jerk in 2014
AbstractThe production of quasi‐definitive data at Ebre observatory has enabled us to detect a new geomagnetic jerk in early 2014. This has been confirmed by analyzing data at several observatories in the European‐African and Western Pacific‐Australian sectors in the classical fashion of looking for the characteristic V shape of the geomagnetic secular
J. Miquel Torta +3 more
openaire +1 more source

