@Article{Kane:2009:FlSoAc,
author = "Kane, Rajaram Purushottam",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)}",
title = "Fluctuations of Solar Activity during the Declining Phase of the
11-Year Sunspot Cycle",
journal = "Solar Physics",
year = "2009",
volume = "255",
number = "1",
pages = "163--168",
note = "0038-0938",
abstract = "The number of coronal mass ejections (CMEs) erupting from the Sun
follows a trend similar to that of sunspot numbers during the
rising and maximum phase of the solar cycle. In the declining
phase, the CME number has large fluctuations, dissimilar to those
of sunspot numbers. In several studies of solar -aEuro parts per
thousand interplanetary and solar -aEuro parts per thousand
terrestrial relationships, the sunspot numbers and the 2800-MHz
flux (F10) are used as representative of solar activity. In the
rising phase, this may be adequate, but in the declining phase,
solar parameters such as CMEs may have a different behaviour.
Cosmic-ray Forbush decreases may occur even when sunspot activity
is low. Therefore, when studying the solar influence on the Earth,
one has to consider that although geomagnetic conditions at solar
maximum will be disturbed, conditions at solar minimum may not be
necessarily quiet.",
doi = "10.1007/s11207-008-9303-8",
url = "http://dx.doi.org/10.1007/s11207-008-9303-8",
issn = "0038-0938 and 1573-093X",
language = "en",
targetfile = "kane fluctuation.pdf",
urlaccessdate = "30 abr. 2024"
}