1965
DOI: 10.1175/1520-0469(1965)022<0262:dtcita>2.0.co;2
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Diurnal Temperature Change in the Atmosphere between 30 and 60 km Over White Sands Missile Range

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Cited by 27 publications
(11 citation statements)
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“…Observations of diurnal temperature change in the stratosphere were done by Beyers and Miers (1965) over White Sands Missile Range (32 °N). According to their results the diurnal temperature range is less than 5°C below 40 km and about 10°C near the stratopause, though these values are somewhat larger than Leovy's theoretical results.…”
Section: Vertical Time-sections Of Temperaturementioning
confidence: 98%
“…Observations of diurnal temperature change in the stratosphere were done by Beyers and Miers (1965) over White Sands Missile Range (32 °N). According to their results the diurnal temperature range is less than 5°C below 40 km and about 10°C near the stratopause, though these values are somewhat larger than Leovy's theoretical results.…”
Section: Vertical Time-sections Of Temperaturementioning
confidence: 98%
“…It is suggested that this might be another manifestation of a diurnal variation in the mesopause barrier penetration which complements the morning to afternoon difference noted in Section 4. BEYERS and MIERS (1965) found a difference in temperature of 20K between early morning and afternoon at 55 km. This is already half of the largest seasonal variation used by GELLER (1970) to explain the seasonal variation in lunar tide.…”
Section: Lems Of Identifying Lunar Geomagnetic Effects At Huancayo)mentioning
confidence: 99%
“…This Meteorological Rocket Network (MRN) has expanded the atmospheric volume which is currently subject to meteorological scrutiny from limitations of the order of 30 km peak altitude to a current synoptic data ceiling of the order of 80 km. A number of very important findings have resulted from MRN synoptic exploration of the upper atmosphere, the most notable of which (for our current purposes) is the discovery of large diurnal variations of the temperature (Beyers and Miers, 1965), wind (Miers, 1965) and ozone ) fields of the stratopause region. Solar ultraviolet heating of the ozonosphere is indicated by the data to be concentrated in middle and low latitudes in a relatively thin layer in the 45 to 50 km altitude region and the transport of this diurnal heat pulse downward and upward from the stratopause level is then accomplished by secondary physical processes.…”
Section: Introductionmentioning
confidence: 94%
“…Diurnal variations in the temperature (Beyers and Miers, 1965) and wind (Miers, 1965) fields of the stratospheric circulation of the order of 150 and 30 mps respectively were discovered through application of the sensitive measuring systems of the Meteorological Rocket Network. The diurnal variation of the wind field has been shown to be a general characteristic of MRN data .…”
Section: Diurnal Circulationsmentioning
confidence: 99%