Magnetic-Field-Induced Localization of Electrons in Fluctuation Potential Wells of Impurities

1990 ◽  
Vol 157 (1) ◽  
pp. 17-59 ◽  
Author(s):  
B. A. Aronzon ◽  
I. M. Tsidilkovskii
2003 ◽  
Vol 83 (13) ◽  
pp. 2590-2592 ◽  
Author(s):  
B. Arnaudov ◽  
T. Paskova ◽  
O. Valassiades ◽  
P. P. Paskov ◽  
S. Evtimova ◽  
...  

1968 ◽  
Vol 40 (4) ◽  
pp. 812-815 ◽  
Author(s):  
J. DURKAN ◽  
R. J. ELLIOTT ◽  
N. H. MARCH

2005 ◽  
Vol 04 (04) ◽  
pp. 489-499 ◽  
Author(s):  
QASEM RAMADAN ◽  
VICTOR SAMPER ◽  
DANIEL POENAR ◽  
CHEN YU

In this study we present a set of guidelines for the design of current carrying micro-conductors/micro-coils (MCs) for magnetic nanoparticles manipulation in biomedical applications. Precise spatial manipulation requires steep magnetic field gradients and due to the consequences of scaling laws, these gradients should be maximized as the size of the particle reduces. Conventional planar coils have many construction and functional limitations, such as generating only small magnetic field gradients, Joule heating, and limited ability to move particles with high spatial resolution. On the other hand, micro-coils can provide a satisfactory solution to all these problems. The geometrical and structural parameters play significant roles in determining the ability to move guide and transport nanoparticles. Design guidelines were generated from a detailed theoretical treatment and finite element analysis (FEA). The spatial distributions of magnetic fields, field gradients and magnetic forces on particles were simulated using FEA for different geometrical/structural parameters and wire arrangements. An array of wires create a chain of magnetic potential wells that are controllable in terms of magnitude and direction and therefore can be used to control the motion and position of magnetic nano-particles by tuning the current through the array.


1967 ◽  
Vol 31 ◽  
pp. 381-383
Author(s):  
J. M. Greenberg

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.


1967 ◽  
Vol 31 ◽  
pp. 375-380
Author(s):  
H. C. van de Hulst

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.


1967 ◽  
Vol 31 ◽  
pp. 355-356
Author(s):  
R. D. Davies

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.


1994 ◽  
Vol 144 ◽  
pp. 559-564
Author(s):  
P. Ambrož ◽  
J. Sýkora

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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