Laser‐induced emission in the 1.9 μm region from excited state–excited state transitions in PuF6

1985 ◽  
Vol 83 (12) ◽  
pp. 6128-6129 ◽  
Author(s):  
W. W. Rice ◽  
J. E. Barefield
2012 ◽  
Vol 86 (6) ◽  
Author(s):  
S. MacMullin ◽  
M. Boswell ◽  
M. Devlin ◽  
S. R. Elliott ◽  
N. Fotiades ◽  
...  

1960 ◽  
Vol 13 (2) ◽  
pp. 99 ◽  
Author(s):  
JA McDonell ◽  
DG Sargood ◽  
JR Moroney ◽  
JR Prescott

The energies of some neutron groups leading to low excited states of "C in the reaction lOB(d,ny)"C have been measured. These lead to values of 4�3�0�3 MeV and 6�53 � O' 02 MeV for the energies of the second and fourth excited states respectively. y-Ray spectra have also been studied in coincidence with different neutron groups. Ground state transitions were observed from the second, third, and fourth excited states, together with cascade decays of the fourth excited state through each of the second and third. Deductions from these y-ray spectra considerably reduce the number of spin possibilities which have been found for these levels by other workers.


2010 ◽  
Vol 18 (12) ◽  
pp. 12832 ◽  
Author(s):  
Maria Ana Cataluna ◽  
Daniil I. Nikitichev ◽  
Spiros Mikroulis ◽  
Hercules Simos ◽  
Christos Simos ◽  
...  

2007 ◽  
Vol 3 (S242) ◽  
pp. 162-163
Author(s):  
B. Hutawarakorn Kramer ◽  
J. L. Caswell ◽  
A. Sukom ◽  
J. E. Reynolds

AbstractOH masers are sensitive probes of the kinematics, physical conditions, and magnetic fields in star-forming regions. The maser site OH 330.953-0.182 has been studied using the Long Baseline Array of the Australia Telescope National Facility. Simultaneous observations of the 1665- and 1667-MHz hydroxyl ground-state transitions yield a series of maps at velocity spacing 0.09kms−1, in both right- and left-hand circular polarization, with tenth-arcsec spatial resolution. Several clusters of maser spots have been detected within a five-arcsec region. Eight Zeeman pairs were found, and in one case, at 1665 MHz, there is a nearby 1667-MHz pair indicating a similar value of magnetic field and velocity. Over the whole site, all magnetic field estimates are toward us (negative), and range from -3.7 to -5.8 mG. We also compared the morphology and kinematics of the 1665- and 1667-MHz maser spots with those from the excited state of OH at 6035 MHz and from methanol at 6668 MHz.


1977 ◽  
Vol 67 (7) ◽  
pp. 947 ◽  
Author(s):  
M. S. Skolnick ◽  
A. C. Carter ◽  
Y. Couder ◽  
R. A. Stradling

2000 ◽  
Author(s):  
Levon V. Asryan ◽  
Marius Grundmann ◽  
Nikolai N. Ledentsov ◽  
Oliver Stier ◽  
Robert A. Suris ◽  
...  

2011 ◽  
Vol 59 (6) ◽  
pp. 3391-3395 ◽  
Author(s):  
Kwanjae Lee ◽  
Byounggu Jo ◽  
Cheul-Ro Lee ◽  
Jin Soo Kim ◽  
Jong Su Kim ◽  
...  

Author(s):  
C. G. Leburn ◽  
N. K. Metzger ◽  
A. A. Lagatsky ◽  
C. T. A. Brown ◽  
W. Sibbett ◽  
...  

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