Asymmetric behaviour and geomagnetic dependencies of zonal winds in the middle latitude upper thermosphere

التفاصيل البيبلوغرافية
العنوان: Asymmetric behaviour and geomagnetic dependencies of zonal winds in the middle latitude upper thermosphere
المؤلفون: O. Ogunjobi, Z. Mtumela, W.T. Sivla
المساهمون: 27840220 - Ogunjobi, Olankunle
المصدر: Advances in Space Research. 66:2141-2150
بيانات النشر: Elsevier BV, 2020.
سنة النشر: 2020
مصطلحات موضوعية: Geomagnetic activity, Atmospheric Science, 010504 meteorology & atmospheric sciences, Aerospace Engineering, Equinox, Atmospheric sciences, 01 natural sciences, Wind speed, Physics::Geophysics, Latitude, Altitude, 0103 physical sciences, Astrophysics::Solar and Stellar Astrophysics, Solstice, Interhemispheric asymmetry, 010303 astronomy & astrophysics, Upper thermosphere, Physics::Atmospheric and Oceanic Physics, 0105 earth and related environmental sciences, Astronomy and Astrophysics, Zonal winds, Geophysics, Earth's magnetic field, Space and Planetary Science, Middle latitudes, Physics::Space Physics, General Earth and Planetary Sciences, Astrophysics::Earth and Planetary Astrophysics, Thermosphere, Geology
الوصف: In this study we use the CHAMP wind observations from 2002 to 2004 to investigate features of mid-latitude thermospheric winds at low and high geomagnetic activity levels. The winds are observed between the geomagnetic latitudes 40–50° north or south within an altitude range of 370–450 Km and averaged longitudinally. The low geomagnetic activity level wind generally leads eastward in both hemispheres for all the seasons. Maximum westward speeds going above 100 m/s are observed at all levels of geomagnetic activity. Most investigations on F-region parameters assume the equinoxes are fundamentally the same. A first time separation of Equinox season using CHAMP winds reveals equinoctial asymmetric behavior of the wind speed at the two levels considered. Interhemispheric asymmetry in neutral wind behaviour is clearly evident in the solstice seasons with local winds considered in each of the hemispheres. This is consistent with asymmetry in the amount of solar illumination received in each of the hemispheres and differences in the magnetic field strength at magnetically conjugate regions.
تدمد: 0273-1177
URL الوصول: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d04eedda4f2f1af88374d8b28625ea7e
https://doi.org/10.1016/j.asr.2020.07.020
حقوق: OPEN
رقم الأكسشن: edsair.doi.dedup.....d04eedda4f2f1af88374d8b28625ea7e
قاعدة البيانات: OpenAIRE