Atmospheric ionization events can modify the concentration of neutral species in the stratosphere and mesosphere. In particular, ozone is destroyed because of the production of significant quantities of odd nitrogen and hydrogen compounds which react photochemically to destroy ozone. Direct evidence of ozone depletion comes from data taken during and following two solar flares generating large fluxes of 10-100 Mev protons, which bombarded the polar stratosphere and mesosphere. Observations of ozone taken during X-ray emission by solar flares and energetic electron precipitation during aurorae indicates ozone destruction above 50 km by ionization produced odd hydrogen. Lightning is apparently a large contributor to the tropospheric odd nitro...
We have modeled atmospheric effects, especially ozone depletion, due to a solar proton event which p...
© Author(s) 2018. This work is distributed under the Creative Commons Attribution 3.0 LicenseWe anal...
International audience[1] Geomagnetic storms triggered by coronal mass ejections and high‐speed sola...
Solar proton events (SPEs) can cause changes in constituents in the Earth's middle atmosphere. ...
International audienceSolar proton events and electron precipitation affect the concentrations of mi...
Ozone depletion in the stratosphere associated with the solar proton event of August 4, 1972, was ob...
Geomagnetic storms triggered by coronal mass ejections and high-speed solar wind streams can lead to...
Solar proton fluxes have been measured by satellites for over forty years (1963-present). Several sa...
Ozonesonde data from four sites are analyzed in relation to 191 solar protons events (SPEs) from 198...
Intense solar activity during 1989 prompted six major particle events. Four of these occurred betwee...
Ozonesonde data from four sites are analyzed in relation to 191 solar protons events (SPEs) from 198...
We analyze the impact of energetic particle precipitation on the stratospheric nitrogen budget, ozon...
Energetic electron precipitation (EEP) from the Earth’s outer radiation belt continuously affects th...
Solar particle events (SPEs) have been investigated since the late 1960's for possible effects on th...
Solar proton events and electron precipitation affect the concentrations of middle atmospheric c...
We have modeled atmospheric effects, especially ozone depletion, due to a solar proton event which p...
© Author(s) 2018. This work is distributed under the Creative Commons Attribution 3.0 LicenseWe anal...
International audience[1] Geomagnetic storms triggered by coronal mass ejections and high‐speed sola...
Solar proton events (SPEs) can cause changes in constituents in the Earth's middle atmosphere. ...
International audienceSolar proton events and electron precipitation affect the concentrations of mi...
Ozone depletion in the stratosphere associated with the solar proton event of August 4, 1972, was ob...
Geomagnetic storms triggered by coronal mass ejections and high-speed solar wind streams can lead to...
Solar proton fluxes have been measured by satellites for over forty years (1963-present). Several sa...
Ozonesonde data from four sites are analyzed in relation to 191 solar protons events (SPEs) from 198...
Intense solar activity during 1989 prompted six major particle events. Four of these occurred betwee...
Ozonesonde data from four sites are analyzed in relation to 191 solar protons events (SPEs) from 198...
We analyze the impact of energetic particle precipitation on the stratospheric nitrogen budget, ozon...
Energetic electron precipitation (EEP) from the Earth’s outer radiation belt continuously affects th...
Solar particle events (SPEs) have been investigated since the late 1960's for possible effects on th...
Solar proton events and electron precipitation affect the concentrations of middle atmospheric c...
We have modeled atmospheric effects, especially ozone depletion, due to a solar proton event which p...
© Author(s) 2018. This work is distributed under the Creative Commons Attribution 3.0 LicenseWe anal...
International audience[1] Geomagnetic storms triggered by coronal mass ejections and high‐speed sola...