@Article{Kane:2006:ArDoSo,
author = "Kane, Rajaram Purushottam",
affiliation = "Instituto Nacional de Pesquisas Espaciais, Divis{\~a}o de
Geof{\'{\i}}sica Espacial (INPE.DGE)",
title = "Are the double-peaks in solar indices during solar maxima of cycle
23 reflected in ionospheric foF2?",
journal = "Journal of Atmospheric and Solar-Terrestrial Physics",
year = "2006",
volume = "68",
number = "8",
pages = "877--880",
month = "May",
keywords = "solar indices, Euv, ionospheric foF2 , EUV, DENSITY, MODEL.",
abstract = "The 12-month running means of solar indices indicated that during
2000-2002, all solar indices (including EUV) had two maxima. one
near July 2000 and another near end of 2001. but the magnitudes of
the second maximum relative to the first maximum were different
for different solar indices. For EUV 26-34 nm relevant for
ionospheric (foF2)(2), the second maximum was similar to 3% higher
than the first maximum. The 12-month running means of (foF2)(2) at
some mid-latitude locations in both hemispheres showed similar two
maxima, but the magnitudes of the second maximum relative to the
first maximum were not similar to those of observed solar EUV
(similar to 3%) and were very different at different locations
(-3% to + 18%). Even on the solar cycle time scale (solar minimum
to solar maximum), changes of (foF2)(2) at different locations
were not alike (factors of 3.1-4.5).",
copyholder = "SID/SCD",
issn = "1364-6826",
language = "en",
targetfile = "Are the double peaks in solar indices.pdf",
urlaccessdate = "13 maio 2024"
}