Climatology of ionospheric slab thickness

The ionospheric slab thickness &#x03C4; defined as a ratio of the total electron content (TEC) to the F-region peak electron density (<i>Nm</i>F2) has been analysed during the solar maximum (1981) and minimum (1985) phases of an intense, the 21st, solar cycle. Hourly values of TEC...

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Bibliographic Details
Main Authors: B. Jayachandran, T. N. Krishnankutty, T. L. Gulyaeva
Format: Article
Language:English
Published: Copernicus Publications 2004-01-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/22/25/2004/angeo-22-25-2004.pdf
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Summary:The ionospheric slab thickness &#x03C4; defined as a ratio of the total electron content (TEC) to the F-region peak electron density (<i>Nm</i>F2) has been analysed during the solar maximum (1981) and minimum (1985) phases of an intense, the 21st, solar cycle. Hourly values of TEC and <i>Nm</i>F2 collected at Hawaii (low-latitude), Boulder (mid-latitude) and Goosebay (high-latitude) are used in the study. Climatology of the slab thickness is described by the diurnal, seasonal, solar and magnetic activity variations of &#x03C4; for the different latitude zones. It is found that, for magnetically quiet days of solar maximum, increased ionization of <i>Nm</i>F2 and TEC during the daytime is accompanied by an increased thickness of the ionosphere compared to the night-time for non-auroral latitudes. However, the reverse is found to be true during the solar minimum compensating TEC against a weak night-time ionization of <i>Nm</i>F2. For the high-latitude the night-time slab thickness is higher compared to the daytime for both the solar phases. Ratios of daily peak to minimum values of slab thickness vary from 1.3 to 3.75 with the peaks of &#x03C4; often observed at pre-sunrise and post-sunset hours. The average night-to-day ratios of &#x03C4; vary from 0.68 to 2.23. The day-to-day variability of &#x03C4;, expressed in percentage standard deviation, varies from 10% by day (equinox, high-latitude) to 67% by night (summer, mid-latitude) during solar minimum and from 10% by day (winter and equinox, mid-latitude) to 56% by night (equinox, high-latitude) during solar maximum. A comprehensive review of slab thickness related literature is given in the paper. <br><br><b>Key words.</b> Ionospheric physics
ISSN:0992-7689
1432-0576