12-14 September, 2011, Lucknow - Earth Science India
12-14 September, 2011, Lucknow - Earth Science India
12-14 September, 2011, Lucknow - Earth Science India
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National Conference on <strong>Science</strong> of Climate Change and <strong>Earth</strong>’s Sustainability: Issues and Challenges ‘A Scientist-People Partnership’<br />
<strong>12</strong>-<strong>14</strong> <strong>September</strong>, <strong>2011</strong>, <strong>Lucknow</strong><br />
the 10,000-17,000 years BP period in the Southern Ocean and attributed to enhanced<br />
wind-driven upwelling [Anderson et al., 2009].<br />
WAS MID-BRUNHES CLIMATE SHIFT (MBCS) A<br />
RESPONSE TO ECCENTRICITY MINIMUM REPEATED<br />
AT EVERY 400-KA IN THE LAST ~3 MILLION YEARS?<br />
S.M. Gupta, B. Nagender Nath and M.B.L. Mascarenhas-Pereira<br />
National Institute of Oceanography, (CSIR), Dona Paula, Goa, 403 004<br />
email: smgupta@nio.org , nagender@nio.org, mariab@nio.org<br />
Mid-Brunhes Climate Shift (MBCS) at ~300 ka (kilo-years) was first recorded as<br />
a conspicuous change in the variation of eolian grain size data from northwest Pacific in<br />
the early eighties. Since then, it is recorded in several climate proxies, i.e., planktonic<br />
foraminifers, radiolarians, magnetic susceptibility and the calcium carbonate content in<br />
the world oceans. Recently, the MBCS are reported from the radiolarians/g data, and<br />
subsequently in planktonic foraminiferal variation from equatorial <strong>India</strong>n Ocean. Here,<br />
we analyze radiolarians/g dry sediment, organic carbon, particle mean size data from a<br />
sediment record in the central <strong>India</strong>n Ocean, and the differential summer solar<br />
insolation at 30 o N-30 o S, precession, and <strong>Earth</strong>’s orbital eccentricity by continuous<br />
wavelet (Morlet) transform (CWT) spectrum to study the variation in the strength of<br />
power through the time, which are associated with orbital forcing responsible for<br />
MBCS event. Results suggest that strength of the spectral power associated with<br />
insolation cycles due to its precession (23-ka) and eccentricity (<strong>12</strong>6-ka) components<br />
weakened during the MBCE. Thus, the weakening of insolation might have resulted in<br />
climatic events similar to MBCS in the geological past. Analyses of our data, published<br />
data, orbital eccentricity and the solar insolation suggest that possibly, there were<br />
possibly seven climate shifts (S1-S7) similar to MBCS, at almost regular interval of<br />
~400-ka cycles in the last 3 million years (Ma).<br />
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