z-logo
open-access-imgOpen Access
Statistical study of nighttime medium‐scale traveling ionospheric disturbances using midlatitude airglow images
Author(s) -
Shiokawa K.,
Ihara C.,
Otsuka Y.,
Ogawa T.
Publication year - 2003
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 - 10.1029/2002ja009491
Subject(s) - airglow , ionosphere , ionosonde , middle latitudes , thermosphere , f region , amplitude , geology , latitude , atmospheric sciences , solar maximum , geodesy , local time , physics , solar cycle , geophysics , electron density , solar wind , mathematics , optics , plasma , statistics , quantum mechanics
We have investigated statistical characteristics of the nighttime medium‐scale traveling ionospheric disturbances (MSTIDs) observed in 630‐nm airglow images at two stations, Rikubetsu (43.5°N, 34.8°MLAT) and Shigaraki (34.9°N, 25.4°MLAT), in Japan for 1998–2000 near the solar maximum period. Most of the observed MSTIDs propagate southwestward in the images. The typical wavelength, velocity, period, and amplitude are 100–300 km, 50–100 m/s, 0.5–1.5 h, and 5–15%, respectively. Seasonal variations in these parameters are not clear. The occurrence rate has a major peak (50–60%) in summer that appears ∼2 months earlier at lower latitudes and a minor peak in winter. Similar occurrence characteristics are obtained from midlatitude spread‐ F signatures using multipoint ionosonde data in Japan, though the coincidence of the spread‐ F and the MSTIDs in airglow images is only 10–15%.

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here
Accelerating Research

Address

John Eccles House
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom