Solar proton activity during cycle 23 and changes in the ozonosphere: Numerical simulation and analysis of observational data

Krivolutsky, A. A.; Kuminov, A. A.; Kukoleva, A. A.; Repnev, A. I.; Pereyaslova, N. K.

doi:10.1134/s0016793208040038

Cited by 11 publications

(13 citation statements)

References 15 publications

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“…Below, we present the modeling results of a numerical scenario for the effect of solar protons dur ing the SPE of July 14, 2000 (one of the strongest SPRs in the 23rd cycle of solar activity). The results of simulations of the effect of this event, performed with the help of one dimensional (Krivolutsky et al, 2005(Krivolutsky et al, , 2006(Krivolutsky et al, , 2008 and two dimensional (Jackman et al, 2001) models, showed sufficiently good agreement with measurement data obtained by the HALOE (UARS) instrument over the northern polar region during the SPE. The present paper describes the results of three dimensional modeling.…”

Section: Response To Corpuscular Flowssupporting

confidence: 65%

“…Furthermore, different research groups conducted a number of stud ies on the photochemical modeling of the ozone response to solar proton events (SPEs) of different capacity (Jackman et al, 1990(Jackman et al, , 2001Krivolutsky et al, 2005Krivolutsky et al, , 2008Funke et al, 2011). We also note the results of the ship missile experiment at high latitudes of the Southern Hemisphere in October 1989 during strong geomagnetic disturbances and particle precipi tation (Zadorozhny et al, 1994).…”

Section: Response To Corpuscular Flowsmentioning

confidence: 96%

“…24 (taken from Krivolutsky et al, 2008). These results were obtained from the processing of measurement data on the composition obtained from the UARS sat ellite (HALOE instrument).…”

Section: Response To Corpuscular Flowsmentioning

confidence: 99%

“…The measurement data were obtained from the UARS satellite (HALOE instrument)(Krivolutsky et al, 2008).…”

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confidence: 99%

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The three-dimensional photochemical model CHARM. Incorporation of solar activity

et al. 2015

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We describe the numerical global photochemical model CHARM (CHemical Atmospheric Research Model) and the results of a numerical simulation of climatological distributions of ozone and other atmospheric trace gases in a height range of up to 90 km. We also present the results of numerical scenarios of an impact induced by a change in UV radiation fluxes in the solar activity cycle and conditioned by ozone depletion in polar regions by high energy particles of cosmic origin. The spatial transport of chemically active species is described in the model (the Prather scheme) on the basis of global fields of wind components and temperature calculated by the ARM (Atmospheric Research Model) general circulation model.

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Section: Response To Corpuscular Flowssupporting

confidence: 65%

Section: Response To Corpuscular Flowsmentioning

confidence: 96%

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The three-dimensional photochemical model CHARM. Incorporation of solar activity

et al. 2015

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“…The results of processing of the rocket-borne TO measurements reported in (Callis et al, 1979) are indicative of the correlation between the ozone concentrations at altitudes above 26 km and the solar activity. Solar proton flares can also cause the ozone depletion in the Earth's atmosphere (Stephenson et al, 1992;Shumilov et al, 1996;Kasatkina et al, 1998;Tassev et al, 1999;Krivolutsky et al, 2001;Kuznetsov, 2002). Volcanic eruptions are another natural factor affecting the TO.…”

Section: The Effect Of Major Meteor Streams On the Total Ozone In Thementioning

confidence: 99%

The Effect of Major Meteor Streams on the Total Ozone in the Earth’s Atmosphere

Gorbanev

Stogneeva

Shestopalov

et al. 2017

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Energetic Particle Influence on the Earth’s Atmosphere

et al. 2015

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This manuscript gives an up-to-date and comprehensive overview of the effects of energetic particle precipitation (EPP) onto the whole atmosphere, from the lower thermosphere/mesosphere through the stratosphere and troposphere, to the surface. The paper summarizes the different sources and energies of particles, principally galactic cosmic rays (GCRs), solar energetic particles (SEPs) and energetic electron precipitation (EEP). All the proposed mechanisms by which EPP can affect the atmosphere are discussed, including chemical changes in the upper atmosphere and lower thermosphere, chemistry-dynamics feedbacks, the global electric circuit and cloud formation. The role of energetic particles in Earth's atmosphere is a multi-disciplinary problem that requires expertise from a range of scientific backgrounds. To assist with this synergy, summary tables are provided, which are intended to evaluate the level of current knowledge of the effects of energetic particles on processes in the entire atmosphere.

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Solar proton activity during cycle 23 and changes in the ozonosphere: Numerical simulation and analysis of observational data

Cited by 11 publications

References 15 publications

The three-dimensional photochemical model CHARM. Incorporation of solar activity

The three-dimensional photochemical model CHARM. Incorporation of solar activity

The Effect of Major Meteor Streams on the Total Ozone in the Earth’s Atmosphere

Energetic Particle Influence on the Earth’s Atmosphere

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