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dc.date.accessioned 2023-07-06T12:53:29Z
dc.date.available 2023-07-06T12:53:29Z
dc.date.issued 1994
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/155128
dc.description.abstract The impulsive phase of a solar flare hard X-rays emission is a rich source of information to understand the physics processes acting during the flare phenomenon. Particularly, in some cases, it shows the superposition of many intensity variations with time scales of tens to tenths of seconds. Looking for an objective method to separate and characterize these possible time scale fluctuations we tried the novel method of the Discrete Wavelet Transform (DWT), applying it to some hard X-rays flares observed with good time resolution (64 ms) by the Large Area Detector (LAD) of BATSE, an instrument on board the CGRO satellite. en
dc.language es es
dc.subject Galaxia es
dc.title Critical analysis of solar hard X-ray observations en
dc.type Articulo es
sedici.identifier.issn 1669-9521 es
sedici.creator.person Ghielmetti, H. es
sedici.creator.person Rovira, M. es
sedici.subject.materias Astronomía es
sedici.description.fulltext true es
mods.originInfo.place Asociación Argentina de Astronomía es
sedici.subtype Comunicacion es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.relation.journalTitle Boletín de la Asociación Argentina de Astronomía es
sedici.relation.journalVolumeAndIssue no. 39 es


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Except where otherwise noted, this item's license is described as Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)