Auroral-zone electron precipitation accompanying a sudden impulse in the geomagnetic field.
Auroral zone electron precipitation occurring in strong transient magnetic disturbances observed by bremsstrahlung
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Auroral zone electron precipitation occurring in strong transient magnetic disturbances observed by bremsstrahlung
IMP-II and OGO-I measurements on plasma characteristics in transition region between solar wind and geomagnetic field
VLF measurements of Poynting flux along geomagnetic field with Injun 5 satellite
Spherical harmonic expansion for volumes of tubes of unit flux in geomagnetic field for use in magnetospheric dynamics
Polar aurorae brightness related to geomagnetic field variation and short periodic pulsations of earth currents
IMP-II and OGO-I measurements on plasma characteristics in transition region between solar wind and geomagnetic field
Described here are the various types of historical data (by which we mean actual measurements of the field taken in the past) which are available for geomagnetic field modelling, concentrating exclusively on observations made prior to the 20th century. These data take quite diverse forms, being derived from voyages of discovery or scientific expeditions, from surveys on land, or from observatories after the formation of the Gottingen Magnetic Union. Toward the latter part of the 19th Century, declination was measured quite regularly by various naval vessels for the purpose of constructing charts. Prior to the invention of a method for measuring field intensities by Gauss in 1832, all measurements were of declination or inclination. During the 19th Century over 40,000 observations are available in one year (the first International Polar Year 1882-83). Prior to 1800 there are only of the order of 12,000 measurements. We discuss measurement methods and the types of instruments used, and focus on specific problems which have been noted, such as those associated with the measurement of intensity on iron ships in the late 19th Century.
Certain species of living creatures are known to orientate themselves in the geomagnetic field. Given the small magnitude of approximately 48 μT, the underlying quantum mechanical phenomena are expected to exhibit coherence times in the microsecond regime. In this contribution, we show the sensitivity of organic light-emitting diodes (OLEDs) to magnetic fields far below Earth’s magnetic field, suggesting that coherence times of the spins of charge-carrier pairs in these devices can be similarly long. By electron paramagnetic resonance (EPR) experiments, a lower bound for the coherence time can be assessed directly. Moreover, this technique offers the possibility to determine the distribution of hyperfine fields within the organic semiconductor layer. We extend this technique to a material system exhibiting both fluorescence and phosphorescence, demonstrating stable anticorrelation between optically detected magnetic resonance (ODMR) spectra in the singlet (fluorescence) and triplet (phosphorescence) channels. The experiments demonstrate the extreme sensitivity of OLEDs to both static as well as dynamic magnetic fields and suggest that coherent spin precession processes of coulombically bound electron-spin pairs may play a crucial role in the magnetoreceptive ability of living creatures.
Particle fluxes in outer radiation belt and unstable radiation zone of outer geomagnetic field, discussing electron diffusion into magnetosphere and magnetic disturbances
Very low frequency electromagnetic hiss propagation along geomagnetic field in earth magnetosphere
Cyclonic convective cell fluctuation and nonuniform core rotation effects on reversal of geomagnetic field, investigating fossil magnetism
Geomagnetic field inclination determination by incoherently scattered signal Faraday rotation calibration and simultaneous ionosonde measurements of ionospheric electron density
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Magnetic field variations at high latitudes and geomagnetic structure of magnetosphere in terms of equatorial boundaries of oval auroral zones and of westerly current vortex
Asymptotic acceptance cone variation of cosmic ray neutron monitors in geomagnetic field distorted by solar wind, noting particle trajectories
Relation of westward drift of geomagnetic field to rotation of earth core
With the use of a prediction technique it is shown that the polarity (toward or away from the sun) of the interplanetary magnetic field can be reliably inferred from observations of the polar geomagnetic field.
The effects of temperature changes at the earth's core-mantle boundary on the velocity field of the core are analyzed. It is assumed that the geomagnetic field is maintained by thermal convection in the outer core. A model for the thermal interaction of the core and the mantle is presented which is consistent with current views on the presence of heat sources in the core and the properties of the lower mantle. Significant long-term variations in the frequency of geomagnetic reversals may be the result of fluctuating temperatures at the core-mantle boundary, caused by intermittent convection in the lower mantle. The thermal structure of the lower mantle region D double prime, extending from 2700 to 2900 km in depth, constitutes an important test of this hypothesis and offers a means of deciding whether the geomagnetic dynamo is thermally driven.