The 3410 A band of the PH molecule in the solar photospheric spectrum

Details The 3410 A band of the PH molecule in the solar photospheric spectrum The 3410 A band of the PH molecule in the solar photospheric spectrum

Feb 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984soph...90..259d&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 90, Feb. 1984, p. 259-268. Research supported by the Fundacao de Amparo aPesquisa do Estado

Physics

6

Molecular Spectra, Phosphorus Compounds, Photosphere, Solar Spectra, Ultraviolet Spectra, Hydrogen Compounds, Line Spectra, Molecular Rotation, Oscillator Strengths

Scientific paper

Some weak unidentified solar photospheric lines in the wavelength range: (3400 - 3465) Å may be due to PH lines of the (0, 0) band of the PH(A3Πi - X3Σ-) system. These faint PH molecular lines have resulted an excitation temperature of the order of 4500K. Using experimental lifetime data for PH in the A3Πi state, an absorption oscillator strength f00 = 0.0075 is derived for the 3410 Å band of the PH (A3Πi - X3Σ-) system. Accurate line positions, oscillator strength and transition probability for the 4.4 μ fundamental rotation-vibration band of the PH molecule are obtained. A comparison of positions of some lines of the 4.4 μ band with those obtained on new tracings of high resolution solar spectra shows many coincidences with weak solar lines.

Affiliated with

Also associated with

No associations

Rating

The 3410 A band of the PH molecule in the solar photospheric spectrum does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The 3410 A band of the PH molecule in the solar photospheric spectrum, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The 3410 A band of the PH molecule in the solar photospheric spectrum will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1859413