F-layer peak height variation near the equatorial anomaly crest during moderate solar activity

The variations of F-layer peak density height or hmax for March, June, September and December during moderate solar activity period (2006 - 2007) have been analyzed to describe the short term variability of this parameter near the southern crest of equatorial anomaly. The parameters were derived fro...

Full description

Saved in:
Bibliographic Details
Main Authors: Rhazali Z.A., Zain A.F.M.
Other Authors: 16022936300
Format: Conference paper
Published: 2023
Subjects:
Tags: Add Tag
No Tags, Be the first to tag this record!
id my.uniten.dspace-29997
record_format dspace
spelling my.uniten.dspace-299972023-12-29T15:43:55Z F-layer peak height variation near the equatorial anomaly crest during moderate solar activity Rhazali Z.A. Zain A.F.M. 16022936300 23494494500 equatorial ionosphere F-layer peak density height h<sub>max</sub> hmF2 Ionosphere Solar radiation Equatorial anomaly Equatorial ionosphere hmF2 Magnetic dip Peak density Seasonal peaks Solar activity Solar energy The variations of F-layer peak density height or hmax for March, June, September and December during moderate solar activity period (2006 - 2007) have been analyzed to describe the short term variability of this parameter near the southern crest of equatorial anomaly. The parameters were derived from ionograms obtained from the Parit Raja (Lat. 1�52'N, Long. 103�48'E, magnetic dip 14.3�) ionosonde station. The results show that hmax is greater during midday around 1200 to 1400 LT and slowly decreases in the evening until the lowest level at midnight. The seasonal peak ranges from 400 to 600 km with the highest level observed in December solstice (550 km) and the minimum in June solstice (430 km). The equinoxes months peak values are between 500 and 550 km. hmax is lowest during midnight (2400 LT) with values range from 230 to 300 km. Highest variability is obtained in March equinox while June solstice shows very minimal variability in h max. � 2013 IEEE. Final 2023-12-29T07:43:55Z 2023-12-29T07:43:55Z 2013 Conference paper 10.1109/IconSpace.2013.6599509 2-s2.0-84889061435 https://www.scopus.com/inward/record.uri?eid=2-s2.0-84889061435&doi=10.1109%2fIconSpace.2013.6599509&partnerID=40&md5=b9a07987a6700ef66e8371e3ca2b10b9 https://irepository.uniten.edu.my/handle/123456789/29997 6599509 424 428 Scopus
institution Universiti Tenaga Nasional
building UNITEN Library
collection Institutional Repository
continent Asia
country Malaysia
content_provider Universiti Tenaga Nasional
content_source UNITEN Institutional Repository
url_provider http://dspace.uniten.edu.my/
topic equatorial ionosphere
F-layer peak density height
h<sub>max</sub>
hmF2
Ionosphere
Solar radiation
Equatorial anomaly
Equatorial ionosphere
hmF2
Magnetic dip
Peak density
Seasonal peaks
Solar activity
Solar energy
spellingShingle equatorial ionosphere
F-layer peak density height
h<sub>max</sub>
hmF2
Ionosphere
Solar radiation
Equatorial anomaly
Equatorial ionosphere
hmF2
Magnetic dip
Peak density
Seasonal peaks
Solar activity
Solar energy
Rhazali Z.A.
Zain A.F.M.
F-layer peak height variation near the equatorial anomaly crest during moderate solar activity
description The variations of F-layer peak density height or hmax for March, June, September and December during moderate solar activity period (2006 - 2007) have been analyzed to describe the short term variability of this parameter near the southern crest of equatorial anomaly. The parameters were derived from ionograms obtained from the Parit Raja (Lat. 1�52'N, Long. 103�48'E, magnetic dip 14.3�) ionosonde station. The results show that hmax is greater during midday around 1200 to 1400 LT and slowly decreases in the evening until the lowest level at midnight. The seasonal peak ranges from 400 to 600 km with the highest level observed in December solstice (550 km) and the minimum in June solstice (430 km). The equinoxes months peak values are between 500 and 550 km. hmax is lowest during midnight (2400 LT) with values range from 230 to 300 km. Highest variability is obtained in March equinox while June solstice shows very minimal variability in h max. � 2013 IEEE.
author2 16022936300
author_facet 16022936300
Rhazali Z.A.
Zain A.F.M.
format Conference paper
author Rhazali Z.A.
Zain A.F.M.
author_sort Rhazali Z.A.
title F-layer peak height variation near the equatorial anomaly crest during moderate solar activity
title_short F-layer peak height variation near the equatorial anomaly crest during moderate solar activity
title_full F-layer peak height variation near the equatorial anomaly crest during moderate solar activity
title_fullStr F-layer peak height variation near the equatorial anomaly crest during moderate solar activity
title_full_unstemmed F-layer peak height variation near the equatorial anomaly crest during moderate solar activity
title_sort f-layer peak height variation near the equatorial anomaly crest during moderate solar activity
publishDate 2023
_version_ 1806425806063271936
score 13.214268