Statistical response of middle atmosphere composition to solar proton events in WACCM-D simulations: importance of lower ionospheric chemistry
- Standort
-
Deutsche Nationalbibliothek Frankfurt am Main
- Umfang
-
Online-Ressource
- Sprache
-
Englisch
- Erschienen in
-
Statistical response of middle atmosphere composition to solar proton events in WACCM-D simulations: importance of lower ionospheric chemistry ; year:2020 ; pages:1-24
Atmospheric chemistry and physics / Discussions. Discussions ; (2020), 1-24
- Urheber
-
Kalakoski, Niilo
Verronen, Pekka T.
Seppälä, Annika
Szeląg, Monika E.
Kero, Antti
Marsh, Daniel R.
- DOI
-
10.5194/acp-2019-1133
- URN
-
urn:nbn:de:101:1-2020012304090176928440
- Rechteinformation
-
Open Access; Der Zugriff auf das Objekt ist unbeschränkt möglich.
- Letzte Aktualisierung
-
14.08.2025, 10:50 MESZ
Datenpartner
Dieses Objekt wird bereitgestellt von:
Deutsche Nationalbibliothek. Bei Fragen zum Objekt wenden Sie sich bitte an den Datenpartner.
Deutsche Nationalbibliothek. Bei Fragen zum Objekt wenden Sie sich bitte an den Datenpartner.
Beteiligte
- Kalakoski, Niilo
- Verronen, Pekka T.
- Seppälä, Annika
- Szeląg, Monika E.
- Kero, Antti
- Marsh, Daniel R.
Ähnliche Objekte (12)
Statistical response of middle atmosphere composition to solar proton events in WACCM-D simulations: the importance of lower ionospheric chemistry
On the importance of middle-atmosphere observations on ionospheric dynamics using WACCM-X and SAMI3
Hybrid simulations of proton precipitation patterns onto the upper atmosphere of Mars
Observations and simulations of ionospheric storms
Millicharged particles from proton bremsstrahlung in the atmosphere
Radiation hydrodynamics in simulations of the solar atmosphere
foF2 seismo-ionospheric effect analysis: actual data and numerical simulations
Accelerating HEP simulations with Neural Importance Sampling
Proton conduction via large-scale atomistic simulations
Proton conduction via large-scale atomistic simulations
Analysis of ionospheric structure influences on residual ionospheric errors in GNSS radio occultation bending angles based on ray tracing simulations
Analysis of ionospheric structure influences on residual ionospheric errors in GNSS radio occultation bending angles based on ray tracing simulations
Statistical response of middle atmosphere composition to solar proton events in WACCM-D simulations: the importance of lower ionospheric chemistry
On the importance of middle-atmosphere observations on ionospheric dynamics using WACCM-X and SAMI3
Hybrid simulations of proton precipitation patterns onto the upper atmosphere of Mars
Observations and simulations of ionospheric storms
Millicharged particles from proton bremsstrahlung in the atmosphere
Radiation hydrodynamics in simulations of the solar atmosphere
foF2 seismo-ionospheric effect analysis: actual data and numerical simulations
Accelerating HEP simulations with Neural Importance Sampling
Proton conduction via large-scale atomistic simulations
Proton conduction via large-scale atomistic simulations
Analysis of ionospheric structure influences on residual ionospheric errors in GNSS radio occultation bending angles based on ray tracing simulations
Analysis of ionospheric structure influences on residual ionospheric errors in GNSS radio occultation bending angles based on ray tracing simulations
Statistical response of middle atmosphere composition to solar proton events in WACCM-D simulations: the importance of lower ionospheric chemistry
On the importance of middle-atmosphere observations on ionospheric dynamics using WACCM-X and SAMI3
Hybrid simulations of proton precipitation patterns onto the upper atmosphere of Mars
Observations and simulations of ionospheric storms
Millicharged particles from proton bremsstrahlung in the atmosphere
Radiation hydrodynamics in simulations of the solar atmosphere
foF2 seismo-ionospheric effect analysis: actual data and numerical simulations
Accelerating HEP simulations with Neural Importance Sampling
Proton conduction via large-scale atomistic simulations
Proton conduction via large-scale atomistic simulations
Analysis of ionospheric structure influences on residual ionospheric errors in GNSS radio occultation bending angles based on ray tracing simulations