Line-by-line photoabsorption cross-sections of the NO δ(1,0) band were measured with the VUV Fourier transform spectrometer from Imperial College, London, using synchrotron radiation at Photon Factory, KEK, Japan, as a continuum light source. The analysis of the NO δ(1,0) band provides accurate rotational line positions and term values as well as the photoabsorption cross-sections. The molecular constants of the C(1)2 II level are found to be T0 = 54 690.155±0.03 cm–1, Bv = 1.944 06±0.000 62 cm–1, Dv = (5.91±0.42)×10–5 cm–1, AD = –0.0187±0.0050 cm–1, p = –0.0189±0.0037 cm–1, and q = –0.015 21±0.000 20 cm–1. The sum of the line strengths for all rotational transitions of the NO δ(1,0) band is determined as 4.80×10–15 cm2 cm–1, corresponding ...
An account is given of progress during the period 8/l/96-7/31/97 on work on (a) cross section measur...
Author Institution: Harvard-Smithsonian Center for Astrophysics; Blackett Laboratory, Imperial Colle...
Oscillator strengths for 48 rotational lines in the 0-0 band of the c1Σ ← X1Σ transition of 14N2, a ...
State-of-the-art models of the vacuum ultraviolet (VUV) absorbing properties of the atmosphere call ...
The β(6,0) and the γ(3,0) bands of NO near 198 nm were analyzed using the VUV FT spectrometer with s...
The analysis of the ε(0,0) band around 187.6 nm was reported using the VUV FTS with synchrotron radi...
Author Institution: Harvard Smithsonian Center for Astrophysics; University of Hong Kong; Imperial C...
Author Institution: Harvard Smithsonian Center for Astrophysics; University of Hong Kong; Imperial C...
Author Institution: University of Hong Kong; Harvard Smithsonian Center for Astrophysics, Cambridge;...
Current research on the Earth's upper atmosphere requires molecular parameters of unprecedented deta...
Author Institution: Harvard Smithsonian Center for Astrophysics; Imperial College of Science, Techno...
Fourier transform spectrometers (FTS) are usually based upon amplitude division interferometers thro...
Author Institution: Harvard-Smithsonian Center for Astrophysics, 60 Garden St.; Imperial College of ...
The photoabsorption spectrum of the O2 Schumann-Runge bands was measured with resolution comparable ...
Fourier transform spectrometers (FTS) are usually based upon amplitude division interferometers thro...
An account is given of progress during the period 8/l/96-7/31/97 on work on (a) cross section measur...
Author Institution: Harvard-Smithsonian Center for Astrophysics; Blackett Laboratory, Imperial Colle...
Oscillator strengths for 48 rotational lines in the 0-0 band of the c1Σ ← X1Σ transition of 14N2, a ...
State-of-the-art models of the vacuum ultraviolet (VUV) absorbing properties of the atmosphere call ...
The β(6,0) and the γ(3,0) bands of NO near 198 nm were analyzed using the VUV FT spectrometer with s...
The analysis of the ε(0,0) band around 187.6 nm was reported using the VUV FTS with synchrotron radi...
Author Institution: Harvard Smithsonian Center for Astrophysics; University of Hong Kong; Imperial C...
Author Institution: Harvard Smithsonian Center for Astrophysics; University of Hong Kong; Imperial C...
Author Institution: University of Hong Kong; Harvard Smithsonian Center for Astrophysics, Cambridge;...
Current research on the Earth's upper atmosphere requires molecular parameters of unprecedented deta...
Author Institution: Harvard Smithsonian Center for Astrophysics; Imperial College of Science, Techno...
Fourier transform spectrometers (FTS) are usually based upon amplitude division interferometers thro...
Author Institution: Harvard-Smithsonian Center for Astrophysics, 60 Garden St.; Imperial College of ...
The photoabsorption spectrum of the O2 Schumann-Runge bands was measured with resolution comparable ...
Fourier transform spectrometers (FTS) are usually based upon amplitude division interferometers thro...
An account is given of progress during the period 8/l/96-7/31/97 on work on (a) cross section measur...
Author Institution: Harvard-Smithsonian Center for Astrophysics; Blackett Laboratory, Imperial Colle...
Oscillator strengths for 48 rotational lines in the 0-0 band of the c1Σ ← X1Σ transition of 14N2, a ...