Trends in the Airglow Temperatures in the MLT Region—Part 2: SABER Observations and Comparisons to Model Simulations

The Sounding of the Atmosphere using Broadband Emission Radiometry (SABER) temperature measurements at low latitudes from 89 km to 97 km were used to derive the F10.7 and Ap index trends, and the trends were compared to model simulations. The annual mean nonzonal (e.g., at the model simulation locat...

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Main Authors: Tai-Yin Huang, Michael Vanyo
Format: Article
Language:English
Published: MDPI AG 2021-01-01
Series:Atmosphere
Subjects:
Online Access:https://www.mdpi.com/2073-4433/12/2/167
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spelling doaj-a909b95808f44b9ca50b9caead2385c42021-01-29T00:01:22ZengMDPI AGAtmosphere2073-44332021-01-011216716710.3390/atmos12020167Trends in the Airglow Temperatures in the MLT Region—Part 2: SABER Observations and Comparisons to Model SimulationsTai-Yin Huang0Michael Vanyo1Department of Physics, Penn State Lehigh Valley, Center Valley, PA 18034, USADepartment of Physics, Penn State University Park, State College, PA 16801, USAThe Sounding of the Atmosphere using Broadband Emission Radiometry (SABER) temperature measurements at low latitudes from 89 km to 97 km were used to derive the F10.7 and Ap index trends, and the trends were compared to model simulations. The annual mean nonzonal (e.g., at the model simulation location at 18° N, 290° E) SABER temperature showed a good-to-moderate correlation with F10.7, with a trend of 4.5–5.3 K/100 SFU, and a moderate-to-weak correlation with the Ap index, with a trend of 0.1–0.3 K/nT. The annual mean zonal mean SABER temperature was found to be highly correlated with the F10.7, with a similar trend, and moderately correlated with the Ap index, with a trend in a similar range. The correlation with the Ap index was significantly improved with a slightly larger trend when the zonal mean temperature was fitted with a 1-year backward shift in the Ap index. The F10.7 (Ap index) trends in the simulated O<sub>2</sub> and the O(<sup>1</sup>S) temperature were smaller (larger) than those in the annual mean nonzonal mean SABER temperature. The trends from the simulations were better compared to those in the annual mean zonal mean temperature. The comparisons were even better when compared to the trend results obtained from fitting with a backward shift in the Ap index.https://www.mdpi.com/2073-4433/12/2/167airglow temperaturesolar cycle variationgeomagnetic activitySABER
collection DOAJ
language English
format Article
sources DOAJ
author Tai-Yin Huang
Michael Vanyo
spellingShingle Tai-Yin Huang
Michael Vanyo
Trends in the Airglow Temperatures in the MLT Region—Part 2: SABER Observations and Comparisons to Model Simulations
Atmosphere
airglow temperature
solar cycle variation
geomagnetic activity
SABER
author_facet Tai-Yin Huang
Michael Vanyo
author_sort Tai-Yin Huang
title Trends in the Airglow Temperatures in the MLT Region—Part 2: SABER Observations and Comparisons to Model Simulations
title_short Trends in the Airglow Temperatures in the MLT Region—Part 2: SABER Observations and Comparisons to Model Simulations
title_full Trends in the Airglow Temperatures in the MLT Region—Part 2: SABER Observations and Comparisons to Model Simulations
title_fullStr Trends in the Airglow Temperatures in the MLT Region—Part 2: SABER Observations and Comparisons to Model Simulations
title_full_unstemmed Trends in the Airglow Temperatures in the MLT Region—Part 2: SABER Observations and Comparisons to Model Simulations
title_sort trends in the airglow temperatures in the mlt region—part 2: saber observations and comparisons to model simulations
publisher MDPI AG
series Atmosphere
issn 2073-4433
publishDate 2021-01-01
description The Sounding of the Atmosphere using Broadband Emission Radiometry (SABER) temperature measurements at low latitudes from 89 km to 97 km were used to derive the F10.7 and Ap index trends, and the trends were compared to model simulations. The annual mean nonzonal (e.g., at the model simulation location at 18° N, 290° E) SABER temperature showed a good-to-moderate correlation with F10.7, with a trend of 4.5–5.3 K/100 SFU, and a moderate-to-weak correlation with the Ap index, with a trend of 0.1–0.3 K/nT. The annual mean zonal mean SABER temperature was found to be highly correlated with the F10.7, with a similar trend, and moderately correlated with the Ap index, with a trend in a similar range. The correlation with the Ap index was significantly improved with a slightly larger trend when the zonal mean temperature was fitted with a 1-year backward shift in the Ap index. The F10.7 (Ap index) trends in the simulated O<sub>2</sub> and the O(<sup>1</sup>S) temperature were smaller (larger) than those in the annual mean nonzonal mean SABER temperature. The trends from the simulations were better compared to those in the annual mean zonal mean temperature. The comparisons were even better when compared to the trend results obtained from fitting with a backward shift in the Ap index.
topic airglow temperature
solar cycle variation
geomagnetic activity
SABER
url https://www.mdpi.com/2073-4433/12/2/167
work_keys_str_mv AT taiyinhuang trendsintheairglowtemperaturesinthemltregionpart2saberobservationsandcomparisonstomodelsimulations
AT michaelvanyo trendsintheairglowtemperaturesinthemltregionpart2saberobservationsandcomparisonstomodelsimulations
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