Collisional and Radiative Relaxation of Selected States in Neon I and Argon II

1971 ◽  
Vol 4 (3) ◽  
pp. 815-821 ◽  
Author(s):  
R. Arrathoon ◽  
D. A. Sealer
Keyword(s):  
Radiative Relaxation

A Photoluminescent Au(I)/Ag(I)/PNN coordination complex for Relatively Rapid and Reversible Alcohol Sensing

2021 ◽  
Author(s):  
Yanhui Tao ◽  
Yuwei Wang ◽  
Shengnan Hu ◽  
David James Young ◽  
Chengrong Lu ◽  
...  
Keyword(s):  
Molecular Weight ◽  
Coordination Complex ◽  
Trinuclear Complex ◽  
Low Molecular Weight ◽  
Radiative Relaxation ◽  
Π Interactions

Trinuclear complex [Au2Ag(dppmaphen)2(CN)2]PF6 photoluminesces on exposure to low molecular weight alcohols. This emission is likely due to C-H···π interactions between the analyte and –PPh2 group, that inhibits non-radiative relaxation of...

scholarly journals The Stability of Mars’s Annular Polar Vortex

2017 ◽  
Vol 74 (5) ◽  
pp. 1533-1547 ◽  
Author(s):  
William J. M. Seviour ◽  
Darryn W. Waugh ◽  
Richard K. Scott
Keyword(s):  
Relaxation Time ◽  
Time Scales ◽  
Time Scale ◽  
Thermal Relaxation ◽  
Polar Vortex ◽  
Radiative Relaxation ◽  
Equilibrium Profile ◽  
Rotating Shallow Water ◽  
The Stability ◽  
Topographic Forcing

Abstract The Martian polar atmosphere is known to have a persistent local minimum in potential vorticity (PV) near the winter pole, with a region of high PV encircling it. This finding is surprising, since an isolated band of PV is barotropically unstable, a result going back to Rayleigh. Here the stability of a Mars-like annular vortex is investigated using numerical integrations of the rotating shallow-water equations. The mode of instability and its growth rate is shown to depend upon the latitude and width of the annulus. By introducing thermal relaxation toward an annular equilibrium profile with a time scale similar to that of the instability, a persistent annular vortex with similar characteristics as that observed in the Martian atmosphere can be simulated. This time scale, typically 0.5–2 sols, is similar to radiative relaxation time scales for Mars’s polar atmosphere. The persistence of an annular vortex is also shown to be robust to topographic forcing, as long as it is below a certain amplitude. It is therefore proposed that the persistence of this barotropically unstable annular vortex is permitted owing to the combination of short radiative relaxation time scales and relatively weak topographic forcing in the Martian polar atmosphere.

scholarly journals Non-radiative relaxation of the Eu3+5D1 level in NaGdTiO4

1984 ◽  
Vol 107 (3) ◽  
pp. 351-354 ◽  
Author(s):  
P.A.M. Berdowski ◽  
G. Blasse
Keyword(s):  
Radiative Relaxation
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