Influence of film width and magnetic field orientation on AC loss in YBCO thin film

2004 ◽  
Vol 17 (3) ◽  
pp. 485-492 ◽  
Author(s):  
Naoyuki Amemiya ◽  
Takamasa Nishioka ◽  
Zhenan Jiang ◽  
Kenji Yasuda
Keyword(s):  
Magnetic Field ◽  
Thin Film ◽  
Ac Loss ◽  
Ybco Thin Film ◽  
Field Orientation ◽  
Magnetic Field Orientation

Quantification of cardiac magnetic field orientation during ventricular de- and repolarization

2008 ◽  
Vol 53 (9) ◽  
pp. 2291-2301 ◽  
Author(s):  
Peter Van Leeuwen ◽  
Birgit Hailer ◽  
Silke Lange ◽  
Anita Klein ◽  
Daniel Geue ◽  
...  
Keyword(s):  
Magnetic Field ◽  
Field Orientation ◽  
Magnetic Field Orientation

Chiral nematic suspensions of cellulose crystallites; phase separation and magnetic field orientation

1994 ◽  
Vol 16 (1) ◽  
pp. 127-134 ◽  
Author(s):  
Jean-François Revol ◽  
Louis Godbout ◽  
Xue-Min Dong ◽  
Derek G. Gray ◽  
Henri Chanzy ◽  
...  
Keyword(s):  
Magnetic Field ◽  
Phase Separation ◽  
Field Orientation ◽  
Magnetic Field Orientation ◽  
Chiral Nematic

Magnetic Flux Generation in YBCO Thin Film Loops by Optical Excitation Under Magnetic Field

1999 ◽  
pp. 199-202
Author(s):  
Hitoshi Saijo ◽  
Masathugu Yamashita ◽  
Toshihiko Kiwa ◽  
Takashi Kondo ◽  
Osamu Morikawa ◽  
...  
Keyword(s):  
Magnetic Field ◽  
Thin Film ◽  
Magnetic Flux ◽  
Optical Excitation ◽  
Ybco Thin Film

scholarly journals Localized TEC enhancements in the Southern Hemisphere

2019 ◽  
Author(s):  
Ilya K. Edemskiy
Keyword(s):  
Magnetic Field ◽  
Solar Activity ◽  
Southern Hemisphere ◽  
Occurrence Rate ◽  
Continuous Series ◽  
Electron Content ◽  
Field Orientation ◽  
Total Electron ◽  
Magnetic Field Orientation ◽  
Global Ionospheric Maps

Abstract. The paper is dedicated to investigation of localized TEC (total electron content) enhancements (LTEs), particularly of LTE series, detected in the Southern Hemisphere using global ionospheric maps for different solar activity years (2014, 2015, 2018). It is shown that LTE intensity varies in dependence on solar flux and does not directly depend on interplanetary magnetic field orientation. The enhancements occur in a subsolar region and could be observed during a continuous series of days. The highest LTE occurrence rate is observed during period of local winter (April-September) for all analyzed years. The longest observed LTE series was detected during 2014 and lasted 80 days or 120 days if we exclude 2 daily gaps.

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