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The formation of Mg I 4571 Å in the solar atmosphere

III: The Holweger solar model

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References

  • Altrock, R. C. and Cannon, C. J.: 1972, Solar Phys. 26, 21.

    Google Scholar 

  • Athay, R. G. and Canfield, R. C.: 1969, Astrophys. J. 156, 695.

    Google Scholar 

  • Gingerich, O. and de Jager, C.: 1968, Solar Phys. 3, 5.

    Google Scholar 

  • Gingerich, O., Noyes, R. W., Kalkofen, W., and Cuny, Y.: 1971, Solar Phys. 18, 347.

    Google Scholar 

  • Holweger, H.: 1967, Z. Astrophys. 65, 365.

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  • White, O. R., Altrock, R. C., Brault, J. W., and Slaughter, C. D.: 1972, Solar Phys. 23, 18.

    Google Scholar 

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Altrock, R.C., Cannon, C.J. The formation of Mg I 4571 Å in the solar atmosphere. Sol Phys 30, 31–33 (1973). https://doi.org/10.1007/BF00156169

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