کد مقاله کد نشریه سال انتشار مقاله انگلیسی نسخه تمام متن
8965510 1646723 2018 50 صفحه PDF دانلود رایگان
عنوان انگلیسی مقاله ISI
Vertical diffusion transport of atomic oxygen in the mesopause region consistent with chemical losses and continuity: Global mean and inter-annual variability
ترجمه فارسی عنوان
حمل و نقل عمودی انتقال اکسیژن اتمی در ناحیه ماوزوپوز مطابق با تلفات شیمیایی و تداوم: میانگین جهانی و تغییرات بین سالیانه
موضوعات مرتبط
مهندسی و علوم پایه علوم زمین و سیارات فیزیک زمین (ژئو فیزیک)
چکیده انگلیسی
This study describes the vertical diffusion velocity and eddy transport coefficient means derived from the climatological measurements of mesospheric [O] by SABER. Fifty years ago, Colegrove et al. (1967) described a process to transition between the two regions of the atmosphere using transport and continuity equations along with a 1-D composition profile. The two parts of this study are calculations of the downward O diffusion velocities and eddy diffusion coefficients using O densities derived from SABER for: 1) the global mean (±55°) and 2) the inter-annual variation of global and equatorial annual mean O densities. The derived transport diffusion velocities range from ∼1 to 4 cm s−1 at 95-83 km, and kzz varies between ∼9.0-5.0 × 105 cm2 s−1 over the same altitude range. The values of kzz derived here in the 80-100 km region are larger at 98 km than those calculated by Salinas et al. (2016) using SABER CO2 measurements and ∼0.5 times less than Qian et al. (2009, 2013 and TIEGCM model) which were derived from studies of thermospheric O/N2 measurements. Consideration of the kzz altitude profiles in the mesosphere, the mean values for both Salinas et al. (2016) and this study is ∼7. E+05 cm2s-1. The standard deviation of the inter-annual variability in kzz (and downward transport velocities) from globally averaged O profiles is <5%. The deviation is slightly larger (7.4%) at the equator, where a QBO trend is noted at 88 km, although not sufficiently large to be detected in the time history of the mesospheric O column density. The global average column density of O in the mesosphere (80-100 km) had a 0.30% change per sunspot. We suggest that model studies may need to consider higher turbulence (and kzz) in the 100-110 km region in order to satisfy both mesospheric and thermospheric composition.
ناشر
Database: Elsevier - ScienceDirect (ساینس دایرکت)
Journal: Journal of Atmospheric and Solar-Terrestrial Physics - Volume 178, October 2018, Pages 47-57
نویسندگان
, , , ,