Sentence examples for magnetic fields based from inspiring English sources

We present a technique for generating discretely consistent magnetic fields based on classical one-dimensional fittings.

This relationship suggests the possibility of predicting the variations in interplanetary magnetic fields based on solar observations at the time of launch of coronal mass ejections.

In particular, the possibilities for tracing back minimally scattered SEP (>10 MeV) ions to their sources has greatly improved as a result of computational models of the coronal and interplanetary magnetic fields based on solar magnetograms.

It describes seasonal and solar cycle variations, separates primary and induced magnetic fields based upon advanced 3D-models of the mantle electrical conductivity, and relies on core, lithospheric and magnetospheric field models derived from other SCARF algorithms for removing non-ionospheric fields from the data.

Another limitation of the study is the use of calculated magnetic fields based on power lines configuration and not on direct measurements of exposure.

To assess exposure of study subjects through the period 1986-2007 in this investigation, we defined exposure corridors through calculation of magnetic fields based on average currents run in the year 2001, the earliest available, which were nearly 13% higher than the average current in the whole study period, thus raising the risk of some misclassification of exposure.

The data were corrected for secular variation by subtracting a regional magnetic field based on IGRF (International Geomagnetic Reference Field) 2005.

In the end, the team found quality dates for 44 zircons with an ancient field; the oldest is 4.2 billion years old 750 million years older than the oldest previous estimate of the Earth's magnetic field based on zircons.

In this paper we present an analytical solution for a three-dimensional triplet(s) fit in a homogeneous magnetic field based on a multiple scattering model.

This paper numerically discussed the dynamical behavior of fluxoids under the alternative magnetic field based on the analysis of time-dependent Ginzburg Landau equation.

We propose a new method for determination of the neutron-star magnetic field based on observation of the fundamental and first cyclotron-annihilation resonances due to pair creation in the ground and first excited states (Landau levels).