High-resolution microwave spectra of solar bursts

Solar Physics ◽  
1989 ◽  
Vol 120 (2) ◽  
pp. 351-368 ◽  
Author(s):  
M. St�hli ◽  
D. E. Gary ◽  
G. J. Hurford
Solar Physics ◽  
1986 ◽  
Vol 104 (1) ◽  
pp. 227-233 ◽  
Author(s):  
Kenneth R. Lang

2019 ◽  
Vol 364 (6) ◽  
Author(s):  
Qing-Fu Du ◽  
Chang-Shuo Chen ◽  
Qiao-Man Zhang ◽  
Xin Li ◽  
Yong Song

Nature ◽  
1964 ◽  
Vol 202 (4931) ◽  
pp. 475-476 ◽  
Author(s):  
A. H. BARRETT ◽  
M. L. MEEKS ◽  
S. WEINREB

1989 ◽  
Vol 44 (12) ◽  
pp. 1196-1200 ◽  
Author(s):  
N. Heineking ◽  
H. Dreizler ◽  
K. Endo ◽  
Y. Kamura

Abstract The rotational spectra of pyridine-N-oxide and x-picoline-N-oxide ( = 2-methvlpyridine-N-oxide) have been observed by means of pulsed microwave spectroscopy. For both molecules, the 14N quadrupole coupling constants have been obtained. For α-picoline-N-oxide. in addition the parameters of the internal rotation motion and the centrifugal distortion constants have been determined.


2018 ◽  
Vol 10 (6) ◽  
pp. 77
Author(s):  
Ch. O. Qajar ◽  
S. B. Kazymova ◽  
M. R. Menzeleyev ◽  
A. S. Gasanova

The modeling of low-resolution (LR) microwave spectra of phenol C6H5OH molecule has been provided in the frequency regions of 0-700 GHz basing on high-resolution (HR) microwave spectral data. The frequency ranges of most intensive absorption level of low-resolution microwave spectra determined. The most intensive spectral lines forming spectra extremums are developed. The recommendations related to perspectives of practical use of achieved results are given.


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