1963
DOI: 10.1016/0021-9169(63)90116-8
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Observation of movement of perturbations in the F-region

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Cited by 49 publications
(16 citation statements)
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“…Distorted traces similar to those recorded for medium-scale travelling ionospheric disturbances (see e.g. Heisler, 1963, and references therein) are present on the daytime ionograms. The foF2 fluctuations, which also occur over periods of 30min or more, constitute large-scale structures (LSSs) and can be positive or negative as is shown by Fig.…”
Section: The Generation Of Ls-tids and Their Initial Equatorial Movemsupporting
confidence: 65%
“…Distorted traces similar to those recorded for medium-scale travelling ionospheric disturbances (see e.g. Heisler, 1963, and references therein) are present on the daytime ionograms. The foF2 fluctuations, which also occur over periods of 30min or more, constitute large-scale structures (LSSs) and can be positive or negative as is shown by Fig.…”
Section: The Generation Of Ls-tids and Their Initial Equatorial Movemsupporting
confidence: 65%
“…8 of Moore and Boulton (1987) shows. The UA-NPD maximum occurs in the middle of the day and is probably responsible for the absence of range-spread ionogram traces at these times, although distorted daytime ionogram traces exist due to the passage of AGWs which were detected earlier by Munro (1958) and Heisler (1963). Fig.…”
Section: Discussionmentioning
confidence: 95%
“…It seems likely that any ionospheric disturbance condition associated with the passage of an AGW may involve this inverse association. Some time ago Munro (1958) and Heisler (1963) detected AGWs which were responsible for daytime disturbances which generally involved distorted F layer ionogram traces. Bowman (1992b) has investigated these traces and found that also the annual and sunspot-cycle variations are similar to those found for nighttime spread-F.…”
Section: Article In Pressmentioning
confidence: 99%
“…The most significant outcome of this study is the detection of examples of the wavy structure of the electron density which has a wavelength around 500km and an amplitude from about 20 to 30% with respect to the background density. This may be understood as a manifestation of TID (Travelling Ionospheric Disturbance) phenomena that were reported previously by MUNRO (1956), HFisLER (1963) and BOWMEN (1965) based on the observations from the bottom-side of the ionosphere using ionospheric sounders. The in-situ observation by satellite TAIYO can, for the first time, provide all-over views of the cross sections of the electron density distribution affected by this TID phenomena in a form of wavy patterns.…”
Section: Introductionmentioning
confidence: 99%