scholarly journals Effect of crustal magnetic fields on the near terminator ionosphere at Mars: Comparison of in situ magnetic field measurements with the data of radio science experiments on board Mars Global Surveyor

2003 ◽  
Vol 108 (A12) ◽  
Author(s):  
A. M. Krymskii
Keyword(s):  
Magnetic Field ◽  
Magnetic Fields ◽  
Field Measurements ◽  
Mars Global Surveyor ◽  
Radio Science ◽  
Magnetic Field Measurements

scholarly journals Magnetic Field Measurements for Fast-Changing Magnetic Fields

2005 ◽  
Author(s):  
Animesh Jain ◽  
John Escallier ◽  
George Ganetis ◽  
Wing Louie ◽  
Andrew Marone ◽  
...  
Keyword(s):  
Magnetic Field ◽  
Magnetic Fields ◽  
Field Measurements ◽  
Magnetic Field Measurements

In situ magnetic field measurements during AMPTE solar wind Li+releases

1986 ◽  
Vol 91 (A2) ◽  
pp. 1261 ◽  
Author(s):  
H. Lühr ◽  
D. J. Southwood ◽  
N. Klöcker ◽  
M. Acuña ◽  
B. Häusler ◽  
...  
Keyword(s):  
Magnetic Field ◽  
Solar Wind ◽  
Field Measurements ◽  
Magnetic Field Measurements

scholarly journals Identification of auroral oval boundaries from in situ magnetic field measurements

1998 ◽  
Vol 103 (A3) ◽  
pp. 4187-4197 ◽  
Author(s):  
J. B. Gary ◽  
L. J. Zanetti ◽  
B. J. Anderson ◽  
T. A. Potemra ◽  
J. H. Clemmons ◽  
...  
Keyword(s):  
Magnetic Field ◽  
Field Measurements ◽  
Auroral Oval ◽  
Magnetic Field Measurements

Statistics of magnetic field measurements in OBA stars and the evolution of their magnetic fields

2017 ◽  
Vol 338 (8) ◽  
pp. 910-918 ◽  
Author(s):  
A. S. Medvedev ◽  
A. F. Kholtygin ◽  
S. Hubrig ◽  
M. Schöller ◽  
S. Fabrika ◽  
...  
Keyword(s):  
Magnetic Field ◽  
Magnetic Fields ◽  
Field Measurements ◽  
Magnetic Field Measurements

scholarly journals Magnetic fields and internal mixing of main sequence B stars

2014 ◽  
Vol 9 (S307) ◽  
pp. 401-403 ◽  
Author(s):  
G. A. Wade ◽  
C. P. Folsom ◽  
J. Grunhut ◽  
J. D. Landstreet ◽  
V. Petit
Keyword(s):  
Magnetic Field ◽  
Magnetic Fields ◽  
Main Sequence ◽  
Field Measurements ◽  
High Quality ◽  
B Stars ◽  
Surface Rotation ◽  
Internal Mixing ◽  
Magnetic Field Measurements

AbstractWe have obtained high-quality magnetic field measurements of 19 sharp-lined B-type stars with precisely-measured N/C abundance ratios (Nieva & Przybilla 2012). Our primary goal is to test the idea (Meynetet al. 2011) that a magnetic field may explain extra drag (through the wind) on the surface rotation, thus producing more internal shear and mixing, and thus could provide an explanation for the appearance of slowly rotating N-rich main sequence B stars.

Static magnetic field measurements in residences in relation to resonance hypotheses of interactions between power-frequency magnetic fields and humans

2001 ◽  
Vol 22 (5) ◽  
pp. 294-305 ◽  
Author(s):  
W. T. Kaune ◽  
R. S. Banks ◽  
M. S. Linet ◽  
E. E. Hatch ◽  
R. A. Kleinerman ◽  
...  
Keyword(s):  
Magnetic Field ◽  
Magnetic Fields ◽  
Static Magnetic Field ◽  
Field Measurements ◽  
Magnetic Field Measurements ◽  
Power Frequency

scholarly journals New magnetic field measurements of β Cephei stars and slowly pulsating B stars

2008 ◽  
Vol 4 (S259) ◽  
pp. 389-390
Author(s):  
Swetlana Hubrig ◽  
M. Briquet ◽  
P. De Cat ◽  
M. Schöller ◽  
T. Morel ◽  
...  
Keyword(s):  
Magnetic Field ◽  
Magnetic Fields ◽  
Main Sequence ◽  
Field Measurements ◽  
Clear Picture ◽  
Magnetic Survey ◽  
B Stars ◽  
Pulsating Stars ◽  
Magnetic Field Measurements ◽  
The Magnetic Field

AbstractWe present the results of the continuation of our magnetic survey with FORS 1 at the VLT of a sample of B-type stars consisting of confirmed or candidate β Cephei stars and Slowly Pulsating B stars. Roughly one third of the studied β Cephei stars have detected magnetic fields. The fraction of magnetic Slowly Pulsating B and candidate Slowly Pulsating B stars is found to be higher, up to 50%. We find that the domains of magnetic and non-magnetic pulsating stars in the H-R diagram largely overlap, and no clear picture emerges as to the possible evolution of the magnetic field across the main sequence.

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