@Article{Kane:2003:Fl~27,
author = "Kane, Rajaram Purushotam",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)}",
title = "Fluctuations in the ~ 27-day sequences in the solar index F10
during solar cycles 22-23",
journal = "Journal of Atmospheric and Solar-Terrestrial Physics",
year = "2003",
volume = "65",
number = "10",
pages = "1169--1174",
month = "July",
keywords = "solar radio emission, 2800 MHz solar flux, 27-day periodicity,
solar cycle 22, solar cycle 23, time-series, radio emissions,
periodicities, rotation, irradiance, flux, uv.",
abstract = "A study of the daily values of the 10.7 cm (2800 MHz, F 10) solar
radio flux revealed fluctuations with peak spacings in a very wide
range (~ 13-40 days). There can be multiple reasons for such a
wide range. Amongst these, there is a possibility that the
dominant radiance within an active region may move rapidly forward
or backward with respect to the solar surface, to give spacings
different from ~ 27 days (solar rotation period). This needs to be
checked with an actual image analysis. An earlier conclusion by
Pap et al. (Solar Phys. (1990) 165) that 27-day solar rotation is
more pronounced in the declining phase of a solar cycle, seems to
be true for cycles 22-23 also. However, during any year, the
magnitudes of the 27-day oscillation can vary by more than a
factor of two from one oscillation to another.",
copyholder = "SID/SCD",
doi = "10.1016/S1364-6826(03)00167-6",
url = "http://dx.doi.org/10.1016/S1364-6826(03)00167-6",
issn = "1364-6826",
language = "en",
targetfile = "1-s2.0-S1364682603001676-main.pdf",
urlaccessdate = "09 maio 2024"
}