Study on technology of high-frequency pulsed magnetic field strength measurement

2012 ◽  
Author(s):  
Chen Yi-Mei ◽  
Liu Zhi-Peng ◽  
Yin Tao
Keyword(s):  
Magnetic Field ◽  
Field Strength ◽  
Magnetic Field Strength ◽  
High Frequency ◽  
Pulsed Magnetic Field ◽  
Strength Measurement

Accuracy of magnetic field strength measurement by single sheet testers

1987 ◽  
Vol 107 (1) ◽  
pp. 50-58 ◽  
Author(s):  
Takayoshi Nakata ◽  
Yoshihiro Kawase ◽  
Masanori Nakano
Keyword(s):  
Magnetic Field ◽  
Field Strength ◽  
Magnetic Field Strength ◽  
Strength Measurement ◽  
Single Sheet

Photomagnetic Medium as Weak Magnetic Field Sensor

2015 ◽  
Vol 230 ◽  
pp. 285-290
Author(s):  
Oleksandr Tychko
Keyword(s):  
Magnetic Field ◽  
External Magnetic Field ◽  
Field Strength ◽  
Magnetic Field Strength ◽  
Weak Magnetic Field ◽  
Magnetic Field Sensor ◽  
Strength Measurement ◽  
Field Sensor

Photoinduced nucleation in an external magnetic field is investigated. A possibility of a week magnetic field strength measurement is showed.

On the Configuration of the Magnetic Field of β CrB

1976 ◽  
Vol 32 ◽  
pp. 613-622
Author(s):  
I.A. Aslanov ◽  
Yu.S. Rustamov
Keyword(s):  
Magnetic Field ◽  
Field Strength ◽  
Radial Velocity ◽  
Magnetic Field Strength ◽  
Complex Shape ◽  
Rotation Period ◽  
Field Variation ◽  
Magnetic Field Variation ◽  
Secular Variations ◽  
The Magnetic Field

SummaryMeasurements of the radial velocities and magnetic field strength of β CrB were carried out. It is shown that there is a variability with the rotation period different for various elements. The curve of the magnetic field variation measured from lines of 5 different elements: FeI, CrI, CrII, TiII, ScII and CaI has a complex shape specific for each element. This may be due to the presence of magnetic spots on the stellar surface. A comparison with the radial velocity curves suggests the presence of a least 4 spots of Ti and Cr coinciding with magnetic spots. A change of the magnetic field with optical depth is shown. The curve of the Heffvariation with the rotation period is given. A possibility of secular variations of the magnetic field is shown.

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