Thermal Conductance between 3He Solid Film and Graphite Substrate in Magnetic Field

2006 ◽  
Author(s):  
Masashi Morishita
Keyword(s):  
Magnetic Field ◽  
Thermal Conductance ◽  
Graphite Substrate ◽  
Solid Film

Magnetic field dependent thermal conductance in La0.67Ca0.33MnO3

2015 ◽  
Vol 381 ◽  
pp. 188-193 ◽  
Author(s):  
C. Euler ◽  
P. Hołuj ◽  
A. Talkenberger ◽  
G. Jakob
Keyword(s):  
Magnetic Field ◽  
Thermal Conductance ◽  
Field Dependent

Experimental Investigation of Magnetically-Induced Thermal Conductance Variations in a Ferromagnetic Nanofluid

2011 ◽  
Author(s):  
Alexander M. Gardner ◽  
Indira Seshadri ◽  
Ganpati Ramanath ◽  
Theodorian Borca-Tasciuc
Keyword(s):  
Magnetic Field ◽  
Thermal Conductivity ◽  
Experimental Investigation ◽  
Magnetic Fields ◽  
Thermal Resistance ◽  
Applied Magnetic Field ◽  
Thermal Conductance ◽  
Flow Characteristics ◽  
Test Apparatus ◽  
The Subject

Ferrofluids have been the subject of great interest in engineering because of their unique flow characteristics under magnetic fields (Rosensweig, 1987). However, there are limited experiments which show the potential of ferrofluids to undergo controlled changes in thermal conductivity (Philip et al., 2008) under magnetic fields. The purpose of this experiment is to investigate thermal transport in ferrofluids. A test apparatus was designed and the thermal resistance of a commercially available ferromagnetic fluid within a test cell was measured as a function of the applied magnetic field.

Transient Thermal Analysis of Epoxy-Impregnated Superconducting Windings in Linearly Ramped Fields

1978 ◽  
Vol 100 (4) ◽  
pp. 702-707 ◽  
Author(s):  
T. E. Laskaris
Keyword(s):  
Magnetic Field ◽  
Experimental Data ◽  
Thermal Analysis ◽  
Temperature Distribution ◽  
Thermal Conductance ◽  
Eddy Current Losses ◽  
Transient Thermal Analysis ◽  
Transient Thermal ◽  
Current Carrying Capability ◽  
The Magnetic Field

Heat is generated in superconducting windings whenever the magnetic field changes. During these transient periods, the current carrying capability of the superconductor is limited by the temperature distribution inside the winding, especially in epoxy-impregnated winding composites that have limited thermal conductance. A finite-difference transient thermal analysis of a superconducting winding composite is presented. The analysis is employed to predict the critical current of a cylindrical coil and a modular racetrack winding under linear ramping of the magnetic field, when eddy current losses and hysteresis losses prevail. The dependence of these losses on the magnetic field and temperature is properly accounted for. The analytical predictions are compared to experimental data and the agreement is excellent.

Magnetic-field strengths from optical polarization data

1967 ◽  
Vol 31 ◽  
pp. 381-383
Author(s):  
J. M. Greenberg
Keyword(s):  
Magnetic Field ◽  
Optical Polarization ◽  
Polarization Data ◽  
Term Model ◽  
Source Of Information ◽  
Field Strengths

Van de Hulst (Paper 64, Table 1) has marked optical polarization as a questionable or marginal source of information concerning magnetic field strengths. Rather than arguing about this–I should rate this method asq+-, or quarrelling about the term ‘model-sensitive results’, I wish to stress the historical point that as recently as two years ago there were still some who questioned that optical polarization was definitely due to magnetically-oriented interstellar particles.

Observing the galactic magnetic field

1967 ◽  
Vol 31 ◽  
pp. 375-380
Author(s):  
H. C. van de Hulst
Keyword(s):  
Magnetic Field ◽  
Fair Agreement ◽  
Solar Neighbourhood ◽  
Galactic Magnetic Field ◽  
The Magnetic Field

Various methods of observing the galactic magnetic field are reviewed, and their results summarized. There is fair agreement about the direction of the magnetic field in the solar neighbourhood:l= 50° to 80°; the strength of the field in the disk is of the order of 10-5gauss.

Structure in the radiation of the galactic disk

1967 ◽  
Vol 31 ◽  
pp. 355-356
Author(s):  
R. D. Davies
Keyword(s):  
Magnetic Field ◽  
Galactic Disk ◽  
Galactic Magnetic Field ◽  
Measured Polarization

Observations at various frequencies between 136 and 1400 MHz indicate a considerable amount of structure in the galactic disk. This result appears consistent both with measured polarization percentages and with considerations of the strength of the galactic magnetic field.

Calculated Coronal Magnetic Fields and Their Comparison with the Coronal Structures as Observed during Five Solar Eclipses

1994 ◽  
Vol 144 ◽  
pp. 559-564
Author(s):  
P. Ambrož ◽  
J. Sýkora
Keyword(s):  
Magnetic Field ◽  
Solar Cycle ◽  
Magnetic Fields ◽  
Solar Corona ◽  
Coronal Magnetic Field ◽  
Coronal Magnetic Fields ◽  
Solar Eclipses ◽  
Coronal Structures

AbstractWe were successful in observing the solar corona during five solar eclipses (1973-1991). For the eclipse days the coronal magnetic field was calculated by extrapolation from the photosphere. Comparison of the observed and calculated coronal structures is carried out and some peculiarities of this comparison, related to the different phases of the solar cycle, are presented.

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