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In the umbral atmosphere the depth dependence of the opacity due to the vibration rotation bands of various abundant molecules in the wavelength region 1 m to 10 m has been calculated. In the higher layers of the umbral atmosphere, the molecular opacity seems to dominate the opacity due to the negative hydrogen ion.  相似文献   
2.
Twenty-one CH line profiles at the centre of the solar disk were Fourier-transformed to derive the Doppler widths. The Doppler width increases linearly with the equivalent width.  相似文献   
3.
The visibility in the umbral ultraviolet spectrum of the O2 Schumann-Runge absorption band system has been explored. It is found that the band system may be visible in high dispersion sunspot spectrum.  相似文献   
4.
The calculated equivalent widths of some lines of SiO in the umbral spectrum suggest that strong lines of Si28O16, Si29O16 and Si30O16 may be present in the sunspot ultraviolet spectrum. We also find that between 37 000 and 47 000 cm–1 the quasi-continuous absorption of SiO dominates all other absorptions.  相似文献   
5.
Samanta  M.  Punetha  P.  Sarkar  S.  Dwivedi  A.  Sharma  M. 《Natural Hazards》2019,96(1):225-246
Natural Hazards - The present paper assesses the slope stability of the Tungnath Temple at Rudraprayag District, in the Indian state of Uttarakhand, and suggests the remedial measures. The...  相似文献   
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