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  1. Berdyugina, S. V. and S. K. Solanki (2002), The molecular Zeeman effect and diagnostics of solar and stellar magnetic fields — I. Theoretical spectral patterns in the Zeeman regimeA&A, 385, doi:10.1051/0004-6361:20020130.
  2. Berdyugina, S. V., S. K. Solanki, and C. Frutiger (2003), The molecular Zeeman effect and diagnostics of solar and stellar magnetic fields — II. Synthetic Stokes profiles in the Zeeman regimeA&A, 412, doi:10.1051/0004-6361:20031473.
  3. Berdyugina, S. V., P. A. Braun, D. M. Fluri, and S. K. Solanki (2003), The molecular Zeeman effect and diagnostics of solar and stellar magnetic fields — III. Theoretical spectral patterns in the Paschen-Back regimeA&A, 444, doi:10.1051/0004-6361:20053806.
  4. Burrus, C. A. (1958), Zeeman Effect in the 1- to 3-Millimeter Wave Region: Molecular g Factors of Several Light MoleculesJ. Chem. Phys., 30(4), 976–983, doi:10.1063/1.1730139.
  5. Christensen, H. and L. Veseth (1978), On the high-precision Zeeman effect in O2 and SOJ. Molec. Struct., 72(3), 438–444, doi:10.1016/0022-2852(78)90142-X.
  6. Croom, D. L. (1978), Millimetre Remote Sensing of the Stratosphere and Mesosphere, Appleton Laboratory.
  7. del Toro Iniesta, J. C. (2003), Introduction to Spectropolarimetry, Cambridge University Press, ISBN 0-521-81827-3.
  8. Han, Y., F. Weng, Q. Liu, and Paul van Delst (2007), A fast radiative transfer model for SSMIS upper atmosphere sounding channelsJ. Geophys. Res., 112, D11121, doi:10.1029/2006JD008208.
  9. Han, Y., P. van Delst, and F. Weng (2010), An improved fast radiative transfer model for special sensor microwave imager/sounder upper atmosphere sounding channelsJ. Geophys. Res., 115, D15109, doi:10.1029/2010JD013878.
  10. Hartmann, G. K., W. Degenhardt, M. L. Richards, H. J. Liebe, G. A. Hufford, M. G. Cotton, R. M. Belivacqua, J. J. Olivero, N. Kämpfer, and J. Langen (1996), Zeeman splitting of the 61 Gigahertz Oxygen (O2) line in the mesosphereGeophys. Res. Lett., 23(17), 2329–2332, doi:10.1029/96GL01043.
  11. Henry, A. F. (1950), The Zeeman Effect in OxygenPhys. Rev., 80(3), 396–401, doi:10.1103/PhysRev.80.396.
  12. Hill, E. L. (1929), On the Zeeman effect in doublet band spectraPhys. Rev., 34, 1507–1516, doi:10.1103/PhysRev.34.1507.
  13. Hill, R. M. and W. Gordy (1954), Zeeman Effect and Line Breadth Studies of the Microwave Lines of Oxygen, Duke University.
  14. Hufford, G. A. and H. J. Liebe (1989), Millimeter-Wave Propagation in the Mesosphere, NTIA- Report.
  15. Jefferies, J., B. W. Lites, and A. Skumanich (1989), Transfer of line radiation in a magnetic fieldAstrophys. J., 343(1), 920–935, doi:10.1086/167762.
  16. Landi Degl'Innocenti, E. (1976), MALIP - a programme to calculate the Stokes parameters profiles of magnetoactive Fraunhofer linesAstronomy & Astrophysics Suppl. S., 25, 379–390.
  17. Lenoir, W. B. (1967), Propagation of Partially Polarized Waves in a Slightly Anisotropic MediumJ. Appl. Phys., 38(13), 5283–5290.
  18. Lenoir, W. B. (1968), Microwave Spectrum of Molecular Oxygen in the MesosphereJ. Geophys. Res., 73(1), 361–376.
  19. Liebe, H. J. (1981), Modeling attenuation and phase of radio waves in the air frequencies below 1000 GHzRadio Sci., 16(6), 1183–1199.
  20. Meerts, W. L. and L. Veseth (1980), The Zeeman Spectrum of the NO MoleculeJ. Molec. Struct., 82(1), 202–213, doi:10.1016/0022-2852(80)90110-1.
  21. Mizushima, M. (1975), The Theory of Rotating Diatomic Molecules, University of Colorado.
  22. Pardo-Carrion, J. R. (1994), The effect of the Earth's magnetic field on the millimetric and submillimetric O2 lines, DEMIRM/Observatoire de Paris-Meudon, Centro Astronomico de Yebes.
  23. Pardo, J. R., L. Pagani, M. Gerin, and C. Prigent (1995), Evidence of the Zeeman Splitting in the 21→01 Rotational Transition of the Atmospheric 16O18O Molecule from Ground-based MeasurementsJ. Quant. Spectrosc. Radiat. Transfer, 54(6), 931–943.
  24. Pardo, J. R., M. Gerina, C. Prigent, J. Cernicharo, G. Rochard, and P. Brunel (1998), Remote Sensing of the Mesospheric Temperature Profile from Close-to-Nadir Observations: Discussion about the Capabilities of the 57.5–62.5 GHz Frequency Band and the 118.75 GHz Single O2 LineJ. Quant. Spectrosc. Radiat. Transfer, 60(4), 559–571.
  25. Poppe, G. P. M. and C. M J. Wijers (1990), More Efficient Computation of the Complex Error FunctionACM Trans. on Math. Softw., 16(1), 38–46, doi:10.1145/77626.77629.
  26. Rees, D. E., G. A. Murphy, and C. J. Durrant (1989), Stokes profile analysis and vector magnetic fields. II. Formal numerical solutions of the stokes transfer equationsAstrophys. J., 339, 1093-1106, doi:10.1086/167364.
  27. Rosenkranz, P. W. and D. H. Staelin (1988), Polarized thermal microwave emission from oxygen in the mesosphereRadio Sci., 23(5), 721–729.
  28. Rosenkranz, P. W. (1990), Oxygen Line Emission as a measure of Temperature in the Upper Stratosphere and Mesosphere, University of Maryland.
  29. Sampoorna, M., K. N. Nagendra, and H. Frisch (2007), Generalized Voigt functions and their derivativesJ. Quant. Spectrosc. Radiat. Transfer, 104(1), 71–85, doi:10.1016/j.jqsrt.2006.08.011.
  30. Sandor, B. J. and R. T. Clancy (1997), Mesospheric observations and modeling of the Zeeman split 233.9 GHz 18O16O lineGeophys. Res. Lett., 24(13), 1631–1634.
  31. Schadee, A. (1978), On the Zeeman effect in electronic transitions of diamotic moleculesJ. Quant. Spectrosc. Radiat. Transfer, 19, 517–531, doi:10.1016/0022-4073(78)90020-1.
  32. Schwartz, M. J., W. G. Read, and W. Van Snyder (2005), Polarized Radiative Transfer for Zeeman-Split Oxygen Lines in the EOS MLS Forward ModelIEEE T. Geosci. Remote.
  33. Schwartz, M. J., W. G. Read, and W. Van Snyder (2006), EOS MLS Forward Model Polarized Radiative Transfer for Zeeman-Split Oxygen LinesIEEE T. Geosci. Remote, 44(5), 1182–1191, doi:10.1109/TGRS.2005.862267.
  34. Stähli, O., A. Murk, N. Kämpfer, C. Mätzler, and P. Eriksson (2013), Microwave radiometer to retrieve temperature profiles from the surface to the stratopauseAtmos. Chem. Phys. Discuss., 6, 2857–2905, doi:10.5194/amtd-6-2857-2013.
  35. Tinkham, M. and M. W. P. Strandberg (1955), Theory of the fine structure of the molecular Oxygen ground state and the measurement of its paramagnetic spectrumPhys. Rev., 97(4), 937–966.
  36. Veseth, L. (1976), Theory of high-precision Zeeman effect in diatomic moleculesJ. Molec. Struct., 63(2), 180–192, doi:10.1016/0022-2852(76)90004-7.
  37. Veseth, L. (1977), Relativistic Corrections to the Zeeman Effect in Diatomic MoleculesJ. Molec. Struct., 66(2), 259–271, doi:10.1016/0022-2852(77)90216-8.
  38. Zaghloul, M. R. and A. N. Ali (2011), Algorithm 916: Computing the Faddeyeva and Voigt FunctionsACM Trans. on Math. Softw., 38(2), 15:1–15:22, doi:10.1145/2049673.2049679.
  39. Zeeman, P. (1897), On the Influence of Magnetism on the Nature of the Light Emitted by a SubstanceAstrophys. J., 5, 332–347, doi:10.1086/140355.