Sensitive detection of magnetic fields including their orientation with a magnetometer based on atomic phase coherence

1998 ◽  
Vol 58 (3) ◽  
pp. 2587-2595 ◽  
Author(s):  
Hwang Lee ◽  
Michael Fleischhauer ◽  
Marlan O. Scully
Keyword(s):  
Magnetic Fields ◽  
Phase Coherence ◽  
Sensitive Detection ◽  
Atomic Phase

From Lamb shift to light shifts: Vacuum and subphoton cavity fields measured by atomic phase sensitive detection

1994 ◽  
Vol 72 (21) ◽  
pp. 3339-3342 ◽  
Author(s):  
M. Brune ◽  
P. Nussenzveig ◽  
F. Schmidt-Kaler ◽  
F. Bernardot ◽  
A. Maali ◽  
...  
Keyword(s):  
Lamb Shift ◽  
Sensitive Detection ◽  
Phase Sensitive ◽  
Phase Sensitive Detection ◽  
Light Shifts ◽  
Atomic Phase

Quantum sensitivity limits of an optical magnetometer based on atomic phase coherence

1994 ◽  
Vol 49 (3) ◽  
pp. 1973-1986 ◽  
Author(s):  
Michael Fleischhauer ◽  
Marlan O. Scully
Keyword(s):  
Phase Coherence ◽  
Atomic Phase

scholarly journals Return to the Origin as a Probe of Atomic Phase Coherence

2017 ◽  
Vol 118 (18) ◽  
Author(s):  
Clément Hainaut ◽  
Isam Manai ◽  
Radu Chicireanu ◽  
Jean-François Clément ◽  
Samir Zemmouri ◽  
...  
Keyword(s):  
Phase Coherence ◽  
Atomic Phase

scholarly journals White-light cavities, atomic phase coherence, and gravitational wave detectors

1997 ◽  
Vol 134 (1-6) ◽  
pp. 431-439 ◽  
Author(s):  
A Wicht ◽  
K Danzmann ◽  
M Fleischhauer ◽  
M Scully ◽  
G Müller ◽  
...  
Keyword(s):  
Gravitational Wave ◽  
White Light ◽  
Phase Coherence ◽  
Gravitational Wave Detectors ◽  
Atomic Phase

Calculated Coronal Magnetic Fields and Their Comparison with the Coronal Structures as Observed during Five Solar Eclipses

1994 ◽  
Vol 144 ◽  
pp. 559-564
Author(s):  
P. Ambrož ◽  
J. Sýkora
Keyword(s):  
Magnetic Field ◽  
Solar Cycle ◽  
Magnetic Fields ◽  
Solar Corona ◽  
Coronal Magnetic Field ◽  
Coronal Magnetic Fields ◽  
Solar Eclipses ◽  
Coronal Structures

AbstractWe were successful in observing the solar corona during five solar eclipses (1973-1991). For the eclipse days the coronal magnetic field was calculated by extrapolation from the photosphere. Comparison of the observed and calculated coronal structures is carried out and some peculiarities of this comparison, related to the different phases of the solar cycle, are presented.

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