Quiet-time variations of F2-layer parameters at Jicamarca and comparison with IRI-2001 during solar minimum

dc.creatorLee, C. C.
dc.creatorReinisch, B. W.
dc.creatorSu, S. Y.
dc.creatorChen, W. S.
dc.date.accessioned2018-11-05T12:07:47Z
dc.date.accessioned2023-05-24T14:22:35Z
dc.date.available2018-11-05T12:07:47Z
dc.date.available2023-05-24T14:22:35Z
dc.date.created2018-11-05T12:07:47Z
dc.date.issued2008
dc.identifierLee, C. C., Reinisch, B. W., Su, S. Y., & Chen, W. S. (2008). Quiet-time variations of F2-layer parameters at Jicamarca and comparison with IRI-2001 during solar minimum.==$Journal of Atmospheric and Solar-Terrestrial Physics, 70$==(1), 184-192. https://doi.org/10.1016/j.jastp.2007.10.008
dc.identifierhttp://hdl.handle.net/20.500.12816/3276
dc.identifierJournal of Atmospheric and Solar-Terrestrial Physics
dc.identifierhttps://doi.org/10.1016/j.jastp.2007.10.008
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/6428970
dc.description.abstractWe analyze Jicamarca ionograms to study the quiet-condition variations in the peak electron density (NmF2), its height (hmF2), and F2-layer thickness parameter (B0) of the equatorial F2 layer during solar minimum. The sunrise peak is found in hmF2 and B0 for all months. During daytime and nighttime, the variation in the hmF2 value is mainly responsible for that in NmF2 and B0. The sunset peaks of hmF2 and B0 exist in the equinoctial months, but not in the winter months. Moreover, the observed values of hmF2, NmF2, and B0 are generally similar to the modeled values of IRI-2001.
dc.languageeng
dc.publisherElsevier
dc.relationurn:issn:1364-6826
dc.rightsinfo:eu-repo/semantics/restrictedAccess
dc.subjectIonosphere
dc.subjectEquatorial ionosphere
dc.subjectIonospheric dynamics
dc.subjectModeling and forecasting
dc.titleQuiet-time variations of F2-layer parameters at Jicamarca and comparison with IRI-2001 during solar minimum
dc.typeinfo:eu-repo/semantics/article


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