The absorption spectrum of monodeuterated methane /CH3D/ in the 6000-12000 A spectral region

1977 ◽  
Vol 213 ◽  
pp. L139 ◽  
Author(s):  
R. G. Danehy ◽  
B. L. Lutz ◽  
T. Owen ◽  
T. W. Scattergood ◽  
W. Goetz
2010 ◽  
Vol 111 (15) ◽  
pp. 2197-2210 ◽  
Author(s):  
A.D. Bykov ◽  
O.V. Naumenko ◽  
E.R. Polovtseva ◽  
S.-M. Hu ◽  
A.-W. Liu

1946 ◽  
Vol 24f (2) ◽  
pp. 123-129 ◽  
Author(s):  
W. A. Bryce

Exposure of milk powders to sunlight resulted in a much greater destruction of riboflavin than did exposure to ultra-violet light in the range 3200 to 4200 Å. The rate of photolysis was greater for skim-milk powders than for whole milk powders. Increased intensities of visible light accelerated riboflavin destruction. In the spectral region of 4200 to 5600 Å the wave band causing the greatest destruction in liquid skim-milk had a principal wave-length of 4450 Å, which corresponded to a maximum in the absorption spectrum of riboflavin. The rate of photolysis of riboflavin was a function of both wave-length and intensity of the impinging energy.


2000 ◽  
Vol 201 (2) ◽  
pp. 297-309 ◽  
Author(s):  
Olga Naumenko ◽  
Elena Bertseva ◽  
Alain Campargue ◽  
David W. Schwenke

2004 ◽  
Author(s):  
L. R. Brown ◽  
O. V. Naumenko ◽  
E. R. Polovtseva ◽  
Leonid N. Sinitsa

1980 ◽  
Vol 58 (6) ◽  
pp. 788-802 ◽  
Author(s):  
M. Q. Syed ◽  
A. W. Harrison

Ground based measurements of stratospheric NO2, using four different established methods based on twilight sky observations in the spectral region 437.0–451.0 nm have been made at two locations: Primrose Lake (54.78°N, 110.05°W) and at Priddis (50.86°N, 114.29°W), Alberta, Canada, during March and April 1979. The four methods differ from one another on the basis of: (a) whether or not stratospheric ozone is taken into account, (b) whether a continuous NO2 absorption spectrum or just the absorption at a few discrete wavelengths is used for analysis, and (c) the assumed altitude distribution of NO2 concentration. Two different independently developed altitude distribution models are employed in obtaining the NO2 vertical column abundance and its effective altitude from a set of slant column abundances, measured in the twilight sky at different solar zenith angles in the range 85–96°. A comparison shows that the use of one or the other of these two models alone could introduce a difference of as much as 30% in the derived vertical column abundance.


Sign in / Sign up

Export Citation Format

Share Document