Please use this identifier to cite or link to this item: http://nopr.niscpr.res.in/handle/123456789/37944
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dc.contributor.authorJoseph, Julius-
dc.date.accessioned2016-12-01T05:06:35Z-
dc.date.available2016-12-01T05:06:35Z-
dc.date.issued1973-03-
dc.identifier.issn0975-105X (Online); 0367-8393 (Print)-
dc.identifier.urihttp://nopr.niscair.res.in/handle/123456789/37944-
dc.description42-46en_US
dc.description.abstractA theoretical approach is adopted to find out the energy increase in ionizing radiation during a flare from the available ionospheric data. The total ion production rate is equated with individual ion production rates due to four prominent spectral bands in the extreme ultraviolet and X-ray regions. Such equations, containing four unknowns corresponding to the photon fluxes, are formed for 17 heights in the range 150 to 230 km. The equations are solved for photon flux value for normal days and at the time of flare.en_US
dc.language.isoen_USen_US
dc.publisherNISCAIR-CSIR, Indiaen_US
dc.rights CC Attribution-Noncommercial-No Derivative Works 2.5 Indiaen_US
dc.sourceIJRSP Vol.02(1) [March 1973]en_US
dc.titleEnhancement of Ionizing Radiation during a Solar Flare from Ionospheric Dataen_US
dc.typeArticleen_US
Appears in Collections:IJRSP Vol.02(1) [March 1973]

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