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dc.contributor.authorNicolet, M.
dc.coverage.temporal20th century
dc.date1963
dc.date.accessioned2016-03-07T17:14:06Z
dc.date.accessioned2021-12-09T09:52:44Z
dc.date.available2016-03-07T17:14:06Z
dc.date.available2021-12-09T09:52:44Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/8409
dc.descriptionA general analysis of solar radio fluxes between 1000 and 10.000 Mc/s has been made for an entire solar cycle. It is shown that a correlation between a solar radio-flux index and the temperature of thermo-pause can be found in the range of 8-10 cm if its basic component is associated with a 27-day mean value. A linear correlation is found between the 27-day mean of the 8-cm radio flux and the thermo-pause temperature. However, there is a departure from linearity at 10.7 cm for fluxes of less than 150 units. The oscillation during a so-called 27-day period has a value that is about 50 per cent that of basic component. It is shown that no corpuscular effect is needed in addition to the normal heating of the thermosphere by ultraviolet radiation. A table is given to deduce the relationships between radio fluxes at 8 and 10 cm and average nighttime and daytime temperatures. Finally, the maximum, mean, and minimum temperatures have been deducted for nighttime and daytime conditions between 1952 and 1962.
dc.languageeng
dc.publisherIRM
dc.publisherKMI
dc.publisherRMI
dc.relation.ispartofseriesContributions, n° - Bijdragen, nr.
dc.titleSolar Radio Flux and temperature of the Upper atmosphere
dc.typeBook
dc.subject.frascatiEarth and related Environmental sciences
dc.audienceGeneral Public
dc.audienceScientific
dc.subject.freesolar radiation
dc.subject.freeatmospheric Temperature
dc.subject.freeultraviolet radiation
dc.subject.freesunspot
dc.subject.freeheating
dc.subject.freeair
dc.subject.freesolar flares
dc.subject.freesolar spectrum
dc.subject.freeupper atùosphere
dc.subject.freedensity
dc.subject.freeoscommation
dc.subject.freecooling
dc.subject.freeatmospheres
dc.source.volume87
dc.source.page26
Orfeo.peerreviewedYes


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