Results 21 to 30 of about 10,311,463 (236)
Improvement of measuring accuracy of magnetic field strength in single sheet testers by using two H coils [PDF]
The accuracy of the measured magnetic field strength of single sheet testers using an H coil[1-4] is examined by finite element analysis. An improved measuring method which uses two H coils is proposed from this investigation.
Nakano, Masanori +2 more
core +1 more source
The effect of the strength of the self-induced magnetic field around a current carrying wire on thermomagnetic convection cooling in ferrofluid is experimentally and numerically investigated.
Van Dau +7 more
core +1 more source
The dependence of the magnetic field strength of a sunspot umbra on its intensity and brightness temperature [PDF]
A partial decrease of the convective energy by the magnetic field of a sunspot causes the temperature of the magnetized plasma to decrease and this leads to a magneto-hydrostatic equilibrium.
Hashem Hamedivafa
doaj +1 more source
Oscillating magnetic field disrupts magnetic orientation in Zebra finches, Taeniopygia guttata [PDF]
Background Zebra finches can be trained to use the geomagnetic field as a directional cue for short distance orientation. The physical mechanisms underlying the primary processes of magnetoreception are, however, largely unknown.
Wiltschko, Wolfgang +20 more
core +1 more source
The magnetic-field strengths of accreting millisecond pulsars [PDF]
Accepted for publication in ...
Mukherjee, Dipanjan +3 more
openaire +4 more sources
Baryon-Dark matter interaction in presence of magnetic fields in light of EDGES signal
We have shown that in presence of a cosmic magnetic field the bounds on baryon dark matter cross-section ($${\hat{\sigma }}$$ σ^ ), dark-matter mass ($$m_d$$ md ) and values of the magnetic field ($$B_0$$ B0 ) can strongly influence each other.
Jitesh R. Bhatt +3 more
doaj +1 more source
Estimating the Magnetic Field Strength in Hot Jupiters [PDF]
Abstract A large fraction of known Jupiter-like exoplanets are inflated as compared to Jupiter. These “hot” Jupiters orbit close to their parent star and are bombarded with intense starlight. Many theories have been proposed to explain their radius inflation and several suggest that a small fraction of the incident starlight is ...
Rakesh K. Yadav, Daniel P. Thorngren
openaire +2 more sources
The Magnetic Field Strength in the Large Magellanic Cloud [PDF]
We have measured a value of 4±5m--2rad for the rotation measure of the radio pulsar PSR0529-66 in the LMC and, after allowing for the dispersion and rotation measures of our Galaxy on the pulsar's line of sight, we deduce that the magnetic field strength in the LMC is in the range 0 to 5μGauss oriented away from the Sun.
M.E. Costa +2 more
openaire +1 more source
The article discusses the principle of operation and the main components of jet-drop optical measuring systems (JDOMS) based on the pendant drop method for monitoring electric field strength (EFS), magnetic field (MFS) and gravitational field (GFS).To ...
E. V. Leun
doaj +1 more source
Skyrme model study of proton and neutron properties in a strong magnetic field
The proton and neutron properties in a uniform magnetic field are investigated. The Gell–Mann–Nishijima formula is shown to be satisfied for baryon states. It is found that with increasing magnetic field strength, the proton mass first decreases and then
Bing-Ran He
doaj +1 more source

