Open AccessDay‐to‐day variability of the E layer
Author(s) -
Moore Luke,
Mendillo Michael,
Martinis Carlos,
Bailey Scott
Publication year - 2006
Publication title -
journal of geophysical research: space physics
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.67
H-Index - 298
eISSN - 2156-2202
pISSN - 0148-0227
DOI - 10.1029/2005ja011448
Subject(s) - middle latitudes , ionosonde , latitude , atmospheric sciences , atmosphere (unit) , ionosphere , environmental science , climatology , geology , meteorology , electron density , geodesy , physics , geophysics , electron , quantum mechanics
Noontime day‐to‐day variability of ionosonde and incoherent scatter radar (ISR) measurements of the E layer are analyzed for two time periods: 9–27 March 1999 and 4 October–4 November 2002. E layer variability is found to be between 5 and 7% at midlatitudes for these periods. Polar latitudes demonstrate variability ranging from ∼7 to 50%, resulting primarily from a combination of photochemical and auroral processes. In order to understand the relative importance of the various sources that drive the variability in the E layer, a one‐dimensional time‐dependent photochemical model of the Earth's upper atmosphere is developed. The model is able to reproduce E layer electron density and variability for both time periods at a number of mid‐ and low‐latitude stations. It is shown that E layer variability is dominated by variations in the incident solar flux for mid‐ and low‐latitude stations, while auroral ionization processes are estimated to contribute roughly 30% of the total variability observed at polar stations. Changes in the solar declination over the time periods studied are responsible for a secondary source of E layer variability at midlatitudes and for a primary source at high latitudes. Day‐to‐day changes in neutral atmosphere species (including observed NO densities) contribute the least to overall E layer variations, except at low latitudes, where their contribution to variability is comparable to variability induced by changes in solar declination.