PMSE long term observations using SuperDARN SANAE HF radar measurements

It is known that the presence of nanometre-scale ice particles and neutral air turbulence in the Polar summer mesosphere modify the D-region plasma, resulting in strong backscatter. These strong backscatters are referred to as Polar Mesosphere Summer Echoes (PMSE). Although studies on PMSE have been...

Full description

Bibliographic Details
Main Authors: Olakunle Ogunjobi, Venkataraman Sivakumar, Judy Ann Elizabeth Stephenson, Zolile Mtumela
Format: Article
Language:English
Published: Chinese Geoscience Union 2017-01-01
Series:Terrestrial, Atmospheric and Oceanic Sciences
Online Access: http://tao.cgu.org.tw/media/k2/attachments/v283p371.pdf
id doaj-5d184dfa974f4114b2f1e15f9d813b32
record_format Article
spelling doaj-5d184dfa974f4114b2f1e15f9d813b322020-11-24T22:15:56ZengChinese Geoscience UnionTerrestrial, Atmospheric and Oceanic Sciences1017-08392311-76802017-01-0128337110.3319/TAO.2016.09.19.01PMSE long term observations using SuperDARN SANAE HF radar measurementsOlakunle OgunjobiVenkataraman SivakumarJudy Ann Elizabeth StephensonZolile MtumelaIt is known that the presence of nanometre-scale ice particles and neutral air turbulence in the Polar summer mesosphere modify the D-region plasma, resulting in strong backscatter. These strong backscatters are referred to as Polar Mesosphere Summer Echoes (PMSE). Although studies on PMSE have been ongoing for over three decades, aspects revealed by various instruments are still the subject of discussion. As a sequel to the paper by Ogunjobi et al. (2015), we report on the long term trends and variations in PMSE occurrence probability from Super Dual Auroral Radar Network (SuperDARN) high frequency (HF) radar measurements over the South African National Antarctic Expedition IV (SANAE IV). In this current paper, a simple multiple-filter technique is employed to obtain the occurrence probability rate for SuperDARN-PMSE during the summer periods for the years 1998 - 2007. The SuperDARN-PMSE occurrence probability rate in relation to geomagnetic activity is examined. The mesospheric neutral winds and temperature trends during these periods, are further studied and presented in this paper. Both the monthly and diurnal variations in occurrence are consistent with previous reports, confirming the presence of PMSE from SuperDARN SANAE IV radar measurements and the influence of pole to pole mesospheric transport circulation. The special mesospheric mean flow observed prior to the year 2002 is ascribed to the influence of solar activity. The SuperDARN-PMSE occurrence probability peaks with lowered geomagnetic activity. These present results support the hypothesis that the particle precipitation also plays an important role in SuperDARN-PMSE occurrence. http://tao.cgu.org.tw/media/k2/attachments/v283p371.pdf
collection DOAJ
language English
format Article
sources DOAJ
author Olakunle Ogunjobi
Venkataraman Sivakumar
Judy Ann Elizabeth Stephenson
Zolile Mtumela
spellingShingle Olakunle Ogunjobi
Venkataraman Sivakumar
Judy Ann Elizabeth Stephenson
Zolile Mtumela
PMSE long term observations using SuperDARN SANAE HF radar measurements
Terrestrial, Atmospheric and Oceanic Sciences
author_facet Olakunle Ogunjobi
Venkataraman Sivakumar
Judy Ann Elizabeth Stephenson
Zolile Mtumela
author_sort Olakunle Ogunjobi
title PMSE long term observations using SuperDARN SANAE HF radar measurements
title_short PMSE long term observations using SuperDARN SANAE HF radar measurements
title_full PMSE long term observations using SuperDARN SANAE HF radar measurements
title_fullStr PMSE long term observations using SuperDARN SANAE HF radar measurements
title_full_unstemmed PMSE long term observations using SuperDARN SANAE HF radar measurements
title_sort pmse long term observations using superdarn sanae hf radar measurements
publisher Chinese Geoscience Union
series Terrestrial, Atmospheric and Oceanic Sciences
issn 1017-0839
2311-7680
publishDate 2017-01-01
description It is known that the presence of nanometre-scale ice particles and neutral air turbulence in the Polar summer mesosphere modify the D-region plasma, resulting in strong backscatter. These strong backscatters are referred to as Polar Mesosphere Summer Echoes (PMSE). Although studies on PMSE have been ongoing for over three decades, aspects revealed by various instruments are still the subject of discussion. As a sequel to the paper by Ogunjobi et al. (2015), we report on the long term trends and variations in PMSE occurrence probability from Super Dual Auroral Radar Network (SuperDARN) high frequency (HF) radar measurements over the South African National Antarctic Expedition IV (SANAE IV). In this current paper, a simple multiple-filter technique is employed to obtain the occurrence probability rate for SuperDARN-PMSE during the summer periods for the years 1998 - 2007. The SuperDARN-PMSE occurrence probability rate in relation to geomagnetic activity is examined. The mesospheric neutral winds and temperature trends during these periods, are further studied and presented in this paper. Both the monthly and diurnal variations in occurrence are consistent with previous reports, confirming the presence of PMSE from SuperDARN SANAE IV radar measurements and the influence of pole to pole mesospheric transport circulation. The special mesospheric mean flow observed prior to the year 2002 is ascribed to the influence of solar activity. The SuperDARN-PMSE occurrence probability peaks with lowered geomagnetic activity. These present results support the hypothesis that the particle precipitation also plays an important role in SuperDARN-PMSE occurrence.
url http://tao.cgu.org.tw/media/k2/attachments/v283p371.pdf
work_keys_str_mv AT olakunleogunjobi pmselongtermobservationsusingsuperdarnsanaehfradarmeasurements
AT venkataramansivakumar pmselongtermobservationsusingsuperdarnsanaehfradarmeasurements
AT judyannelizabethstephenson pmselongtermobservationsusingsuperdarnsanaehfradarmeasurements
AT zolilemtumela pmselongtermobservationsusingsuperdarnsanaehfradarmeasurements
_version_ 1725792143303245824