@Article{Kane:2003:DiEvSo,
author = "Kane, Rajaram Purushottam",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)}",
title = "Dissimilarity in the evolution of solar EUV and solar radio
emission (2800 MHz) during 1999–2002",
journal = "Journal of Geophysical Research",
year = "2003",
volume = "108",
number = "A12",
pages = "4pp",
keywords = "solar indices, dissimilarities.",
abstract = "For solar UV and EUV the F10 (2800 MHZ solar radio emission),
Lyman alpha, and Mg II are used as proxies. During 19992002, many
solar indices showed two maxima, one near July 2000 and another
near January 2002. For F10 and Lyman alpha, the second maximum was
higher than the first maximum by 10%, but for Rz, the second
maximum was lower than the first maximum by 4%. The observed EUV
(2634 nm from SEM-SOHO) had the second maximum higher than the
first maximum, but only by 3.5%. The model values given in
SOLAR2000 [Tobiska et al., 2000] show patterns of 2634 nm
qualitatively similar to F10, with second maximum larger than the
first maximum, but the magnitude is much larger, 20%. Thus there
is a discrepancy of 15% between observed EUV and SOLAR2000 model
EUV during 20012002. The model values are overestimates and do not
seem to have taken into account the observed EUV values.",
doi = "10.1029/2003JA009869",
url = "http://dx.doi.org/10.1029/2003JA009869",
issn = "0148-0227 and 2156-2202",
language = "en",
targetfile = "jgra16970.pdf",
urlaccessdate = "03 maio 2024"
}