Solar proton events of October–November 2003: Ozone depletion in the Northern Hemisphere polar winter as seen by GOMOS/Envisat

By A. Seppälä, P. Verronen, E. Kyrölä, S. Hassinen, L. Backman, Alain Hauchecorne, Jean-Loup Bertaux, D. Fussen. 2004

150 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atmospheric Science

View Paper: https://www.semanticscholar.org/paper/c6b30470e24fc2c43cb210a498f8e52215845d58

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In Astronomy and Astrophysics

1. M. Lockwood
2. J. Russell
3. J. Fennell
4. Eugene V. Rozanov
5. D. Marsh
6. A. Jaynes
7. T. Egorova
8. J. Foster

In Atmospheric Science

1. M. Lockwood
2. J. Russell
3. C. Randall
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6. M. Clilverd
7. D. Marsh
8. C. Sioris

Citations in the corpus

• Composition changes after the "Halloween" solar proton event: the High Energy Particle Precipitation in the Atmosphere (HEPPA) model versus MIPAS data intercomparison study (2011, methodology): “The Bremen two-dimensional model is based on the twodimensional transport, chemistry and radiation model formerly described in Sinnhuber et al. (2009) and Chipperfield a d Feng (2003).”
• Energetic particle precipitation effects on the Southern Hemisphere stratosphere in 1992–2005 (2007, background): “…to increases in odd nitrogen and odd hydrogen from the thermosphere to the upper stratosphere [Degenstein et al., 2005; Jackman et al., 2005a; López-Puertas et al., 2005a, 2005b; Orsolini et al., 2005; Rohen et al., 2005; Seppälä et al., 2004; Verronen et al., 2005; von Clarmann et al., 2005].”
• Recent oppositely directed trends in solar climate forcings and the global mean surface air temperature (2007, background): “Lastly, we note that transient bursts of solar energetic particles, often associated with very large solar flares, have been observed to have effects on the Earth’s middle and lower atmosphere, including the large-scale destruction of polar stratospheric and tropospheric ozone (Jackman et al. 1993, ”
• Energy transport in the thermosphere during the solar storms of April 2002 (2005, unknown): “: ENERGY TRANSPORT IN THE THERMOSPHERE A12S25 evidenced by the observed destruction of mesospheric ozone [Seppälä et al., 2004].”
• Observation of NO(x) Enhancement and Ozone Depletion in the Northern and Southern hemispheres after the October-November 2003 Solar Proton Events (2005, background): “On the other hand, NOx enhancements as well as O3 depletions are well confirmed in a large number of observations [Weeks et al., 1972; Crutzen et al., 1975; Heath et al., 1977; McPeters et al., 1981; Thomas et al., 1983; Solomon et al., 1981, 1983; McPeters and Jackman, 1985; McPeters, 1986; Reid e”
• Stratospheric effects of energetic particle precipitation in 2003–2004 (2005, methodology): “…NO2 were measured by the MIPAS (Michelson Interferometer for Passive Atmospheric Sounding) instrument [Orsolini et al., 2005] (hereinafter referred to as O05), and enhancements in NO2 were measured by the GOMOS (Global Ozone Monitoring by Occultation of Stars) instrument [Seppälä et al., 2004].”
• Space Weather Effects in the Earth’s Radiation Belts (2018, background): “Both short-term (days) and longer-term (weeks) ozone depletion has been observed after strong precipitation events, e.g. SPEs (Reid et al. 1991; Jackman et al. 2001; Seppälä et al. 2004).”
• Geomagnetic activity and polar surface air temperature variability (2009, methodology): “…for the time taken for the EPP-NOx, originally produced in the mesosphere or thermosphere, to descend to the stratosphere, we average the Ap values over a 4-month period starting two months prior to the surface air temperature examination months [e.g., Siskind et al., 2000; Seppälä et al., 2007].”