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Ground-based Ku-band microwave observations of ozone in the polar middle atmosphere.

Authors :
Newnham, David A.
Clilverd, Mark A.
Clark, William D. J.
Kosch, Michael
Verronen, Pekka T.
Rogers, Alan E. E.
Source :
Atmospheric Measurement Techniques Discussions; 11/17/2021, p1-24, 24p
Publication Year :
2021

Abstract

Ground-based observations of 11.072 GHz atmospheric ozone (O<subscript>3</subscript>) emission have been made using the Ny-Ã…lesund Ozone in the Mesosphere Instrument (NAOMI) at the UK Arctic Research Station (latitude 78°55’0” N, longitude 11°55’59” E), Spitsbergen. Seasonally-averaged O<subscript>3</subscript> vertical profiles in the Arctic polar mesosphere-lower thermosphere region for night-time and twilight conditions in the period 15 August 2017 to 15 March 2020 have been retrieved over the altitude range 62– 98 km. NAOMI measurements are compared with corresponding, overlapping observations by the Sounding of the Atmosphere using Broadband Emission Radiometry (SABER) satellite instrument. The NAOMI and SABER data are binned according to the SABER instrument 60-day yaw cycles into 3-month ‘winter’ (15 December–15 March), ‘autumn’ (15 August– 15 November), and ‘summer’ (15 April–15 July) periods. The NAOMI observations show the same year-to-year and seasonal variabilities as the SABER 9.6 μm O<subscript>3</subscript> data. The winter night-time (solar zenith angle, SZA = 110°) and twilight (75° = SZA = 110°) NAOMI and SABER 9.6 &#956m O<subscript>3</subscript> volume mixing ratio (VMR) profiles agree to within the measurement uncertainties. However, for autumn twilight conditions the SABER 9.6 µm O<subscript>3</subscript> secondary maximum VMR values are higher than NAOMI over altitudes 88–97 km by 47% and 59% respectively in 2017 and 2018. Comparing the two SABER channels which measure O<subscript>3</subscript> at different wavelengths and use different processing schemes, the 9.6 &#956m O<subscript>3</subscript> autumn twilight VMR data for the three years 2017–19 are higher than the corresponding 1.27 µm measurements with the largest difference (58%) in the 65–95 km altitude range similar to the NAOMI observation. The SABER 9.6 &#956m O<subscript>3</subscript> summer daytime (SZA < 75°) mesospheric O<subscript>3</subscript> VMR is also consistently higher than the 1.27 µm measurement, confirming previously reported differences between the SABER 9.6 µm channel and measurements of mesospheric O<subscript>3</subscript> by other satellite instruments. [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
18678610
Database :
Complementary Index
Journal :
Atmospheric Measurement Techniques Discussions
Publication Type :
Academic Journal
Accession number :
153742760
Full Text :
https://doi.org/10.5194/amt-2021-339