The following HTML text is provided to enhance online
readability. Many aspects of typography translate only awkwardly to HTML.
Please use the page image
as the authoritative form to ensure accuracy.
Page 36
For the purposes of the U.S. Global Change Research Program,
discussed below are three times scales associated with different
mechanisms for solar variability: the relatively recent climate (a
hundred to a few thousand years), the weather (tens of years), and
orbital variations (many thousands of years).
Solar Irradiance Changes and the
Relatively Recent Climate
There has been much speculation that climate changes over the
past few thousand years have been the product of variations in the
Sun's radiative output. Eddy (1976) pointed out the coincidence in
time between the Maunder Minimum of solar activity and the lowest
temperatures of the Little Ice Age in Europe and North America (see
Figure 1.3). He also presented qualitative evidence that other
century-scale variations in climate over the past millennium
coincided roughly with variations in solar activity deduced from
anomalies in the 14C cosmogenic
isotope record. Whereas the long term trend in records of
cosmogenic isotopes such as 14C
and 10Be reflects, primarily,
changes in the Earth's magnetic field that affect the interaction
of cosmic rays with the Earth's atmosphere, the wiggles
superimposed on the smooth long term trend are believed to occur
because of the modulation of the local cosmic ray intensity by
magnetic fields embedded in the solar wind, which varies in
response to solar activity (Damon and Sonett, 1991; Beer et al.,
1991; Stuiver and Braziunas, 1993). Thus, enhanced solar activity
corresponds to 14C minima, and the
mechanism proposed by Eddy for the apparent relationship between
climate and the 14C wiggles
involved changes in the total solar irradiance linked to the long
term envelope of the 11-year sunspot cycle and reflected in the
14C record.
The extent to which cosmogenic isotope variations really
indicate terrestrially relevant variations in solar energy outputs,
either radiative or particle, and the scaling of the relationship
over long times, is poorly known; the paleoclimate record is
similarly somewhat uncertain (Bradley and Jones, 1993). Although
results are mixed (Wigley and Kelly, 1990; Crowley and Howard,
1990; Damon and Jirikowic, 1994), there is some suggestion of a
relationship; during the past 10,000 years, six of the seven
strongest maxima in the 14C
wiggles correspond closely to climate minima,