On the Distribution of Intensity in the Continuous Spectra of the Sun And the Fi
On the Distribution of Intensity in the Continuous Spectra of the Sun And the Fi
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5^; if we determine the effective temperature from the distribution of intensity in this region, we find a far too low value. At least to some extent this may be due to the correction which ought to be applied to »Sghuster's approximation*. On the other hand, for the wave-lengths 0. 52 — 0. 65 ^ the strong inclinations of the two curves are almost exactly the same. It is interesting to compare this fact with the run of the residuals in the vertical columns of large q in table 4. There is a mark...ed minimum of the residuals 54 Bertil Lindblad, for A 0. 534 fi and X 0. 604 fi; perhaps the coincidence of these two facts for this part of the spectrum is not a mere chance. Beyond X 2. 00 jti the energy-curve observed dech'nes rapidly, but the accuracy of the curve beyond this wave-length is rendered uncertain by the effect of terrestrial water vapor.
Previously we have seen that the introduction of the variable factor K has diminished the change of the product aZ with the wave-length as well as the magnitude of the residuals i table 4.
What to read after On the Distribution of Intensity in the Continuous Spectra of the Sun And the Fi?
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To quickly assess the difficulty of the text, read a short excerpt:
5^; if we determine the effective temperature from the distribution of intensity in this region, we find a far too low value. At least to some extent this may be due to the correction which ought to be applied to »Sghuster's approximation*. On the other hand, for the wave-lengths 0. 52 — 0. 65 ^ the strong inclinations of the two curves are almost exactly the same. It is interesting to compare this fact with the run of the residuals in the vertical columns of large q in table 4. There is a mark...ed minimum of the residuals 54 Bertil Lindblad, for A 0. 534 fi and X 0. 604 fi; perhaps the coincidence of these two facts for this part of the spectrum is not a mere chance. Beyond X 2. 00 jti the energy-curve observed dech'nes rapidly, but the accuracy of the curve beyond this wave-length is rendered uncertain by the effect of terrestrial water vapor.
Previously we have seen that the introduction of the variable factor K has diminished the change of the product aZ with the wave-length as well as the magnitude of the residuals i table 4.
What to read after On the Distribution of Intensity in the Continuous Spectra of the Sun And the Fi?
You can find similar books in the "Read Also" column, or choose other free books by Bertil Lindblad to read onlineMoreLess
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