Diurnal variation of ozone depletion during the October-November 2003 solar proton events

Journal of Geophysical Research: Space Physics

Volumn 110, Issue A9, 2005, Pages

  Verronen, Pekka T ^a   Seppälä, Annika ^a   Clilverd, Mark A ^b   Rodger, Craig J ^c   Kyrölä, Erkki ^a   Enell, Carl Fredrik ^d   Ulich, Thomas ^d   Turunen, Esa ^d  

^a FINNISH METEOROLOGICAL INSTITUTE   (Finland)

^b BRITISH ANTARCTIC SURVEY   (United Kingdom)

^c UNIVERSITY OF OTAGO   (New Zealand)

^d UNIVERSITY OF OULU   (Finland)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 33646827602     PISSN: None     EISSN: 21699402     Source Type: Journal    
DOI: 10.1029/2004JA010932     Document Type: Article

References (65)

1. 3 by different ionmolecule reaction mechanisms, J. Geophys. Res., 102, 12,921-12,926.
2. Aikin, A, C., and H. J. P. Smith (1999), Mesospheric constituent variations during electron precipitation events, J. Geophys. Res., 104, 26,457-26,472.
3. Banks, P. M., and G. Kockarts (1973), Acronomy, vol. B, chap. 15, Elsevier, New York.
4. Barr, R., D. L. Jones, and C. J. Rodger (2000), ELF and VLF radio waves, J. Atmos. Ten. Phys., 62, 1689-1718.
5. Bates, D. R. (1988), Recombination in the normal E and F layers of the ionosphere, Planet. Space Sci., 36, 55-63.
6. Bertaux, J. L., G. Megie, T. Widcmann, E. Chasscficre, R. Pellinen, E. Kyrölä, S. Korpela, and P. Simon (1991), Monitoring of ozone trend by stellar occultations: The GOMOS instrument, Adv. Space Res., 11(3), 237-242.
7. Bertaux, J. L., et al. (2004), First results on GOMOS/Envisat, Adv. Space Res., 33, 1029-1035.
8. Bethe, A. H., and J. Ashkin (1953), Passage of radiations through matter, in Experimetal Nuclear Physics, vol. 1, edited by E. Segre, pp. 166-251, John Wiley, Hoboken, N. J.
9. Brasseur, G., and S. Solomon (1986), Agronomy of the Middle Atmosphere, 2nd ed., Springer, New York.
10. Burns, C. J., E. Turunen, H. Matveinen, H. Ranta, and J. K. Hargreayes (1991), Chemical modeling of the quiet summer D- and E-regions using EISCAT electron density profiles, J. Atmos. Terr. Phys., 53, 115-134.
11. 2 distribution and the temperature in the mesosphere, Geophys. Res. Lett., 29(15), 1729, doi: 10.1029/2002GL015309.
12. Clilverd, M. A., C. Rodger, T. Ulich, A. Seppälä, E. Turunen, A. Botman, and N. Thomson (2005), Modelling a large solar proton event in the southern polar cap, J. Geophys. Res., doi: 10.1029/2004JA010922, in press.
13. Crutzen, P. J., I. S. A. Isakscn, and G. C. Reid (1975), Solar proton events: Stratospheric sources of nitric oxide, Science, 189, 457-458.
14. Cummer, S. A., T. F. Bell, U. S. Inan, and D. L. Chenette (1997), VLF remote sensing of high energy auroral particle precipitation, J. Geophys. Res., 102(11), 7477-7484.
15. Fell, C., J. I. Steinfeld, and S. Miller (1990), Quenching of N(2D) by O(3P), J. Chem. Phys., 92, 4768-4777.
16. Ferguson, J. A., and F. P. Snyder (1990), Computer programs for assessment of long wavelength radio communications, Tech. Doc. 1773, Natl. Ocean Syst. Cent., Alexandria, Va.
17. Freier, P. S., and W. R. Webber (1963), Exponential rigidity spectrums for solar-flare cosmic rays, J. Geophys. Res., 68, 1605-1629.
18. Fuller-Rowell, T. J. (1993), Modeling the solar cycle change in nitric oxide in the thermosphere and upper mesosphere, J. Geophys. Res., 98, 1559-1570.
19. Hargreaves, J. K. (1992), The Solar-Terrestrial Environment, Cambridge Atmos. and Space Sci. Ser., Cambridge Univ. Press, New York.
20. Hedin, A. E. (1991), Extension of the MSIS thcrmospheric model into the middle and lower atmosphere, J. Geophys. Res., 96, 1159-1172.
21. Jackman, C. H., and R. D. McPeters (1985), The responce of ozone to solar proton events during solar cycle 21: A theoretical interpretation, J. Geophys. Res., 90(D5), 7955-7966.
22. Jackman, C. H., M. C. Cemiglia, J. E. Nielscn, D. J. Allen, J. M. Zawodny, R. D. McPeters, A. R. Douglass, J. E. Rosenfield, and R. B. Hood (1995), Two-dimensional and three-dimensional model simulations, measurements, and interpretation of the October 1989 solar proton events on the middle atmosphere, J. Geophys. Res., 100, 11,641-11,660.
23. Jackman, C. H., E. L. Fleming, and F. M. Vitt (2000), Influence of extremely large solar proton events in a changing stratosphere, J. Geophys. Res., 105, 11,659-11,670.
24. Jackman, C. H., R. D. McPeters, G. J. Labow, E. L. Fleming, C. J. Praderas, and J. M. Russel (2001), Northern hemisphere atmospheric effects due to the July 2000 solar proton events, Geophys. Res. Lett., 28, 2883-2886.
25. Jones, A. V. (1974), Aurora, Springer, New York.
26. Kazil, J., E. Kopp, S. Chabrillat, and J. Bishop (2003), The University of Bern Atmospheric Ion Model: Time-dependent modeling of the ions in the mesosphere and lower thermosphere, J. Geophys. Res., 108(D14), 4432, doi:10.1029/2002JD003024.
27. Koppers, G. A. A., and D. P. Murtagh (1996), Model studies of the influence of 02 photodissociation parameterizations in the Schumann-Runge bands on ozone related photolysis in the upper atmosphere, Ann. Geophys., 14, 68-79.
28. Kyrölä, E., E. Sihvola, Y. Kotivuori, M. Tikka, T. Tuomi, and H. Haario (1993), Inverse theory for occultation measurements: 1. Spectral inversion, J. Geophys. Res., 98, 7367-7381.
29. Kyrölä, E., et al. (2004), GOMOS on Envisat: An overview, Adv. Space Res., 33, 1020-1028.
30. McEwan, M. J., and L. F. Phillips (1975), Chemistry of the Atmosphere, 309 pp., Halsted Press, New York.
31. + + O reaction, J. Geophys. Res., 79, 2925.
32. McPeters, R. D., and C. H. Jackman (1985), The response of ozone to solar proton events during solar cycle 21: The observations, J. Geophys. Res., 90, 7945-7954.
33. Meijer, Y. J., et al. (2004), Pole-to-pole, validation of ENVISAT/GOMOS ozone profiles using data from ground-based and balloon-sonde measurements, J. Geophys. Res., 109, D23305, doi:10.1029/2004JD004834.
34. Minschwaner, K., and D. E. Siskind (1993), A new calculation of nitric oxide photolysis in the stratosphere, mesosphere, and lower thermosphere, J. Geophys. Res., 98, 20,401 -20,412.
35. Mul, P. M., and J. W. McGowan (1979), Merged electron-ion beam experiments. III - Temperature dependence of dissociative recombination for atmospheric ions NO/+/, O2/+/, and N2/+/. J. Phys. B, 12, 1591-1601.
36. Ohshio, M., R. Maeda, and H. Sakagami (1966), Height distribution of local photoionization efficiency, J. Radio Res. Lab., 13, 245.
37. Patterson, J. D., T. P. Armstrong, C. M. Laird, D. L.Detriek, and A. T. Weatherwax (2001), Correlation of solar energetic protons and polar cap absorption, J. Geophys. Res., 106, 149-163.
38. Porter, H. S., C. H. Jackman, and A. E. S. Green (1976), Efficiencies for production of atomic nitrogen and oxygen by rclativistic proton impact in air, J. Chem. Phys., 65, 154-167.
39. Press, W. H., S. A. Teukolsky, W. T. Vetterling, and B. P. Flannery (1992), Numerical Recipes in FORTRAN, The Art of Scientific Computing, Clarendon, Oxford, U.K.
40. Randall, C. E., D. E. Siskind, and R. M. Bevilacqua (2001), Stratospheric NO, enhancements in the southern hemisphere vortex in winter/spring of 2000, Geophys. Res. Lett., 28, 2385-2388.
41. Reames, D. V. (1999), Particle acceleration at the Sun and in the heliosphere, Space Sci. Rev., 90, 413-491.
42. Rees, M. H. (1982), On the interaction of auroral protons with the Earth's atmosphere, Planet. Space Sci., 30, 463-472.
43. Rees, M. H. (1989), Physics and Chemistry of the Upper Atmosphere, Cambridge Atmos. and Space Sci. Ser., Cambridge Univ. Press, New York.
44. Reid, G. C. (1961), A study of the enhanced ionization produced by solar protons during a polar cap absorbtion event, J. Geophys. Res., 66,4071 - 4085.
45. Reid, G. C., S. Solomon, and R. R. Garcia (1991), Response of the middle atmosphere to the solar proton events of August-December, 1989, Geophys. Res. Lett., 18, 1019-1022.
46. Rietveld, M. T., E. Turunen, H. Matveincn, N. P. Goncharpv, and P. Pollari (1996), Artificial periodic irregularities in the auroral ionosphere, Ann. Geophys., 14, 1437-1453.
47. Rusch, D. W., J.-C. Gérard, S. Solomon, P. J. Crutzen, and G. C. Reid (1981), The effect of particle precipitation events on the neutral and ion chemistry of the middle atmosphere - I. Odd nitrogen, Planet. Space Sci., 29, 767-774.
48. Sander, S. P., et al. (2003), Chemical kinetics and photochemical data for use in stratospheric modeling: Evaluation 14, JPL Publ. 02-25, Jet Propul. Lab., Calif. Inst. of Technol., Pasadena, Calif.
49. Seppälä, A., P. T. Verronen, E. Kyrölä, S. Hassinen, L. Backman, A. Hauchecome, J. L. Bertaux, and D. Fussen (2004), Solar proton events of October-November 2003: Ozone depletion in the northern hemisphere polar winter as seen by GOMOS/Envisat, Geophys. Res. Lett., 31 L19107, doi:10.1029/2004GL021042.
50. Shimazaki, T. (1984), Minor Constituents in the Middle Atmosphere, Dev. in Earth and Planet. Phys., vol. 6, Springer, New York.
51. Siskind, D. E., D. J. Strickland, R. R. Meier, T. Majeed, and F. G. Eparvier (1995), On the relationship between the solar soft X ray flux and thermospheric nitric oxide: An update with an improved photoelectron model J. Geophys. Res., 100, 19,687-19,694.
52. Solomon, S., D. W. Rusch, J.-C. Gérard, G. C. Reid, and P. J. Crutzen (1981), The effect of particle precipitation events on the neutral and ion chemistry of the middle atmosphere: II. Odd hydrogen, Planet. Space Sci., 8, 885-893.
53. Solomon, S., G. C. Reid, D. W. Rusch, and R. J. Thomas (1983), Mesospheric ozone depletion during the solar proton event of July 13, 1982:2. Comparions between theory and measurements, Geophys. Res. Lett., 10, 257-260.
54. Thomas, L., and M. R. Bowman (1986), A study of pro-sunrise changes in negative ions and electrons in the D-region, J. Atmos. Terr. Phys., 4, 219.
55. Thomas, R. J., C. A. Barth, G. J. Rottman, D. W. Rusch, G. H. Mount, G. M. Lawrence, R. W. Sanders, G. E. Thomas, and L. E. Clemens (1983), Mesosphcric ozone depletion during the solar proton event of July 13, 1982: 1. Measurement, Geophys. Res. Lett., 10, 253-255.
56. Thomson, N. R., C. J. Rodger, and R. L. Dowden (2004), Ionosphere gives size of greatest solar flare, Geophys. Res. Lett., 31, L06803, doi:I0.1029/2003GL019345.
57. Tobiska, W. K., T. Woods, F. Eparvier, R. Viereck, L. D. B. Floyd, G. Rottman, and O. R. White (2000), The SOLAR2000 empirical solar irradiance model and forecast tool, J. Atmos. Terr. Phys., 62, 1233-1250.
58. Torr, M. A., D. G. Torr, and R. A. Ong (1979), Ionization frequencies for major thermospheric constituents as a function of solar cycle 21, Geophys. Res. Lett., 6, 771-774.
59. Turunen, E. (1993), EISCAT incoherent scatter radar observations and model studies of day to twilight variations in the D region during the PCA event of August 1989, J. Atmos. Terr. Phys., 55, 767-781.
60. Turunen, E., H. Matyeinen, J. Tolvanen, and H. Ranta (1996), D-region ion chemistry model, in STEP Handbook of Ionospheric Models, edited by R. W. Schunk, pp. 1-25, SCOSTEP Secretariat, Boulder, Colo.
61. Ulich, T., E. Turunen, and T. Nygrén (2000), Effective recombination coefficient in the lower ionosphere during bursts of auroral electrons, Adv. Space Res., 25, 47-50.
62. +, Phys. Rev. A, 57, 3627-3634.
63. Verronen, P. T., E. Turunen, T. Ulich, and E. Kyrölä (2002), Modelling the effects of the October 1989 solar proton event on mesospheric odd nitrogen using a detailed ion and neutral chemistry model, Ann. Gcophys., 20, 1967-1976.
64. World Meteorological Organization (1985), Global ozone research and monitoring project, in Atmospheric Ozone 1985, Rep. 16, Geneva.
65. 2P) atoms in auroras, J. Geophys. Res., 85, 687-694.