scholarly journals High-resolution calorimetry in pulsed magnetic fields

2021 ◽  
Vol 92 (4) ◽  
pp. 043901
Author(s):  
Shusaku Imajo ◽  
Chao Dong ◽  
Akira Matsuo ◽  
Koichi Kindo ◽  
Yoshimitsu Kohama
Keyword(s):  
High Resolution ◽  
Magnetic Fields ◽  
Pulsed Magnetic Fields

scholarly journals High resolution magnetostriction measurements in pulsed magnetic fields using fiber Bragg gratings

2010 ◽  
Vol 81 (3) ◽  
pp. 033909 ◽  
Author(s):  
Ramzy Daou ◽  
Franziska Weickert ◽  
Michael Nicklas ◽  
Frank Steglich ◽  
Ariane Haase ◽  
...  
Keyword(s):  
High Resolution ◽  
Magnetic Fields ◽  
Fiber Bragg Gratings ◽  
Bragg Gratings ◽  
Pulsed Magnetic Fields

Practical High Resolution Microscopy

1968 ◽  
Vol 26 ◽  
pp. 302-303
Author(s):  
P. A. Marsh ◽  
T. Mullens ◽  
D. Price
Keyword(s):  
High Resolution ◽  
Magnetic Fields ◽  
Low Frequency ◽  
Resolving Power ◽  
Careful Attention ◽  
Electron Microscopes ◽  
The Relationship ◽  
High Resolution Microscopy ◽  
New Facilities

It is possible to exceed the guaranteed resolution on most electron microscopes by careful attention to microscope parameters essential for high resolution work. While our experience is related to a Philips EM-200, we hope that some of these comments will apply to all electron microscopes.The first considerations are vibration and magnetic fields. These are usually measured at the pre-installation survey and must be within specifications. It has been our experience, however, that these factors can be greatly influenced by the new facilities and therefore must be rechecked after the installation is completed. The relationship between the resolving power of an EM-200 and the maximum tolerable low frequency interference fields in milli-Oerstedt is 10 Å - 1.9, 8 Å - 1.4, 6 Å - 0.8.

scholarly journals Magnetic Fields in the Lower Corona Associated with the Expanding Limb Burst On March 30th 1969 Inferred from the Microwave High-Resolution Observations

1971 ◽  
Vol 43 ◽  
pp. 413-416 ◽  
Author(s):  
Shinzo Énomé ◽  
Haruo Tanaka
Keyword(s):  
Magnetic Field ◽  
High Resolution ◽  
Magnetic Fields ◽  
The West ◽  
Lower Corona ◽  
Energetic Electrons ◽  
West Limb ◽  
Flare Region ◽  
Solar Microwave ◽  
Solar Microwave Burst

An expansion of the source of a great solar microwave burst was observed a little beyond the west limb on March 30, 1969. This expansion is interpreted in terms of diffusion of energetic electrons in a turbulent magnetic field in the flare region. The height of the source is estimated to have been 104 km.

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