Alfven waves in graphite and a new interpretation of galvanomagnetic properties of graphite in high magnetic fields

1984 ◽  
Vol 52 (11) ◽  
pp. 913-916
Author(s):  
G.A. Kapustin ◽  
V.S. Babichenko ◽  
E.Z. Meilikhov
Keyword(s):  
Magnetic Fields ◽  
Alfven Waves ◽  
Alfvén Waves ◽  
High Magnetic Fields ◽  
Galvanomagnetic Properties ◽  
New Interpretation

Anomalies in the Galvanomagnetic Properties of Fe1.9V1.1Al Pseudogap Semiconductors at High Magnetic Fields

2010 ◽  
Vol 159 (1-2) ◽  
pp. 208-211 ◽  
Author(s):  
V. V. Marchenkov ◽  
V. I. Okulov ◽  
K. A. Okulova ◽  
H. W. Weber
Keyword(s):  
Magnetic Fields ◽  
High Magnetic Fields ◽  
Galvanomagnetic Properties

Alfven Waves in a Cold Plasma with Curved Magnetic Fields

1988 ◽  
Author(s):  
Philip M. Carrion ◽  
Akira Hasegawa ◽  
Waldo Patton ◽  
Manju Prakash
Keyword(s):  
Magnetic Fields ◽  
Cold Plasma ◽  
Alfven Waves ◽  
Alfvén Waves

scholarly journals Bipolar Outflow and Turbulence in Molecular Clouds Due to Protostellar Alfvén Waves

1992 ◽  
Vol 150 ◽  
pp. 407-408
Author(s):  
V. Jatenco-Pereira ◽  
R. Opher
Keyword(s):  
Magnetic Fields ◽  
Molecular Clouds ◽  
Alfven Waves ◽  
Gravitational Energy ◽  
Alfven Wave ◽  
Alfvén Waves ◽  
Physical Parameters ◽  
Low Velocity ◽  
Bipolar Outflows ◽  
Oriented Parallel

There is strong evidence for magnetic fields in molecular clouds to be oriented parallel to the direction of bipolar outflows. We have evidence for Alfvén waves in molecular clouds from the facts that: (i) the velocity width of CO lines, ΔV, is approximately twice the gravitational energy, and (ii) polarization maps indicate well-defined magnetic fields. These facts indicate that ΔV is wave-like and not eddy-like. We study the Alfvén wave protostellar model of Jatenco-Pereira and Opher (1989) to explain the observed bipolar outflows and turbulence in molecular clouds. We assume that the Alfvén waves are primarily dissipated by non-linear damping and examine the physical parameters necessary to produce the observed massive low-velocity bipolar outflows (u∞ ∿ 10 − 50 km s−1 and Ṁ ∿ 10−3 M⊙ yr−1) and turbulence in molecular clouds.

scholarly journals On Stochastic Dynamics of Protons in Solar Magnetic Loops

1990 ◽  
Vol 142 ◽  
pp. 448-449
Author(s):  
V.N. Senatorov ◽  
V.M. Tomozov
Keyword(s):  
Magnetic Fields ◽  
Stochastic Dynamics ◽  
Alfven Waves ◽  
Alfvén Waves ◽  
Solar Magnetic Fields

It is shown that stochastization of particles due to Alfven waves is accompanied by their effective acceleration in loop structures of solar magnetic fields.

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