scholarly journals The role of epitaxial strain on the electronic and magnetic structure of La0.7Sr0.3MnO3/LaCoO3 bilayers

AIP Advances ◽  
2021 ◽  
Vol 11 (12) ◽  
pp. 125115
Author(s):  
S. Das ◽  
S. Ghosh ◽  
R. G. Tanguturi ◽  
R. Medwal ◽  
S. Gupta ◽  
...  
Keyword(s):  
Magnetic Structure ◽  
Electronic And Magnetic Structure ◽  
Epitaxial Strain

scholarly journals Atomic, electronic and magnetic structure of graphene/iron and nickel interfaces: theory and experiment

RSC Advances ◽  
2015 ◽  
Vol 5 (12) ◽  
pp. 9173-9179 ◽  
Author(s):  
D. W. Boukhvalov ◽  
Y. N. Gornostyrev ◽  
M. A. Uimin ◽  
A. V. Korolev ◽  
A. Y. Yermakov
Keyword(s):  
Magnetic Properties ◽  
Magnetic Structure ◽  
Significant Influence ◽  
Electronic And Magnetic Structure ◽  
Theory And Experiment

Experiments and theory demonstrate the significant influence of a graphene cover to the magnetic properties of an iron substrate and the insignificant role of nickel.

Role of epitaxial strain on the magnetic structure of Fe-doped CoFe 2 O 4

2013 ◽  
Vol 345 ◽  
pp. 180-189 ◽  
Author(s):  
J.A. Moyer ◽  
D.P. Kumah ◽  
C.A.F. Vaz ◽  
D.A. Arena ◽  
V.E. Henrich
Keyword(s):  
Magnetic Structure ◽  
Epitaxial Strain

scholarly journals Concurrent effect of Alfvén waves and planar magnetic structure on geomagnetic storms

2019 ◽  
Vol 490 (3) ◽  
pp. 3440-3447 ◽  
Author(s):  
Zubair I Shaikh ◽  
Anil Raghav ◽  
Geeta Vichare ◽  
Ankush Bhaskar ◽  
Wageesh Mishra ◽  
...  
Keyword(s):  
Magnetic Structure ◽  
Geomagnetic Storms ◽  
Recovery Phase ◽  
Alfven Waves ◽  
Magnetic Clouds ◽  
Alfvén Waves ◽  
Fast Recovery ◽  
Interplanetary Coronal Mass Ejection ◽  
Mass Ejection

ABSTRACT Generally, interplanetary coronal mass ejection (ICME) triggers intense and strong geomagnetic storms. It has been established that the ICME sheath-moulded planar magnetic structure enhances the amplitude of the storms. Alfvén waves embedded in ICME magnetic clouds or high solar streams including corotating interacting regions (CIRs) in turn extend the recovery phase of the storm. Here, we investigate a geomagnetic storm with a very complex temporal profile with multiple decreasing and recovery phases. We examine the role of planar magnetic structure (PMS) and Alfvén waves in the various phases of the storm. We find that fast decrease and fast recovery phases are evident during transit of PMS regions, whereas a slight decrease or recovery is found during the transit of regions embedded with Alfvénic fluctuations.

Electronic and magnetic structure at the Fe/Fe3O4interface

2011 ◽  
Vol 84 (10) ◽  
Author(s):  
T. Kida ◽  
S. Honda ◽  
H. Itoh ◽  
J. Inoue ◽  
H. Yanagihara ◽  
...  
Keyword(s):  
Magnetic Structure ◽  
Electronic And Magnetic Structure
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