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http://hdl.handle.net/2248/4620
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DC Field | Value | Language |
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dc.contributor.author | Viswanathan, B | - |
dc.contributor.author | Shanmugavel, R | - |
dc.contributor.author | Bagare, S. P | - |
dc.contributor.author | Rajamanickam, N | - |
dc.contributor.author | Sriramachandran, P | - |
dc.date.accessioned | 2009-07-03T14:04:10Z | - |
dc.date.available | 2009-07-03T14:04:10Z | - |
dc.date.issued | 2009-07 | - |
dc.identifier.citation | Solar Physics, Vol. 257, No. 2, pp. 261 - 269 | en |
dc.identifier.issn | 0038-0938 | - |
dc.identifier.uri | http://hdl.handle.net/2248/4620 | - |
dc.description | Restricted Access | en |
dc.description | The original publication is available at springerlink.com | - |
dc.description.abstract | High-resolution Fourier transform spectrometer sunspot umbral spectra obtained at the National Solar Observatory/Kitt Peak were used to identify molecular rotational lines arising from the infrared band systems of CrH and CrD molecules. Measurement of the equivalent width used the Gaussian-profile approximation method, which is suitable especially for faint lines. Equivalent widths are measured for an adequate number of best lines of the A – X (0,0) band of CrH and the A – X (0,0;1,0) bands of CrD and, thereby, the effective rotational temperatures are estimated. | en |
dc.language.iso | en | en |
dc.publisher | Springer | en |
dc.relation.uri | http://dx.doi.org/10.1007/s11207-009-9374-1 | en |
dc.relation.uri | http://adsabs.harvard.edu/abs/2009SoPh..257..261V | en |
dc.rights | © Springer | en |
dc.subject | Sunspots | en |
dc.subject | Effective rotational temperature | en |
dc.subject | CrH and CrD molecular lines | en |
dc.title | Identification of CrH and CrD molecular lines in the sunspot umbral spectrum | en |
dc.type | Article | en |
Appears in Collections: | IIAP Publications |
Files in This Item:
File | Description | Size | Format | |
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Identification of CrH and CrD molecular Restricted Access | Restricted Access | 250.75 kB | Adobe PDF | View/Open Request a copy |
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