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scostep 2010 (stp12) - Leibniz-Institut für Atmosphärenphysik an der ...

scostep 2010 (stp12) - Leibniz-Institut für Atmosphärenphysik an der ...

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STP12 Abstracts<br />

Berlin, 12 - 16 July <strong>2010</strong><br />

SCOSTEP Symposium <strong>2010</strong><br />

Influence of solar variability on rotation <strong>an</strong>d climate of the Earth<br />

Kuznetsova Tamara<br />

IZMIRAN, Russi<strong>an</strong> Academy of Sciences, 142190 Moscow region, Troitsk, Russia<br />

The paper presents results of our study of connection between ch<strong>an</strong>ges of solar activity<br />

(sunspot numbers W), rotation rate (w) <strong>an</strong>d global temperature (Tgl) to un<strong>der</strong>st<strong>an</strong>d their<br />

connection on different time scales in the past, present <strong>an</strong>d close future. We use W for the<br />

period 1700-2005, proxy data of north hemisphere temperature Tnh <strong>an</strong>d global temperature<br />

Tgl for the last 1000 yrs <strong>an</strong>d also w for the last 335 yrs. We apply MGM method of spectral<br />

<strong>an</strong>alysis elaborated by us that c<strong>an</strong> qu<strong>an</strong>titatively describe both trends <strong>an</strong>d non-stationary<br />

oscillations to evaluate their input in data. Trend in Tnh shows rise since Maun<strong>der</strong> minimum<br />

with present rate ~0.5 deg.C/100yr correlated with trend in W. High-amplitude 200-yr cycles<br />

in W <strong>an</strong>d in Tgl have passed their maxima <strong>an</strong>d show decrease of their parameters<br />

accomp<strong>an</strong>ied by acceleration of Earth for now. The 200-yr cycle variation extracted from data<br />

of interpl<strong>an</strong>etary magnetic field (IMF) measured at the Earth’s orbit also shows the IMF<br />

decline. Moreover, the 200-yr solar cycle contributed to the Tgl rise since ~1890. We suggest<br />

a possible expl<strong>an</strong>ation of observed unexplained increasing in the Tnh for the interval 1905-<br />

1940 <strong>an</strong>d its subsequent decrease for 1940-1976 with rate 0.75 deg.C/100yr by variation in w<br />

with period of ~72 yr. Characteristics of the other cycles in Tgl, w <strong>an</strong>d W with the same<br />

periods are also discussed. Based on our results we suggest a possible mech<strong>an</strong>ism for the 22yr<br />

variation in W, Tgl <strong>an</strong>d w <strong>der</strong>ived in our study to be explained. Basic idea of the<br />

mech<strong>an</strong>ism is electromagnetic interaction of the solar wind with magnetosphere <strong>an</strong>d<br />

subsequent entry of the solar wind electro-magnetic flux into polar caps. We used<br />

measurements of the IMF <strong>an</strong>d the solar wind velocity for 1964-2005 to calculate value <strong>an</strong>d<br />

direction of necessary electromagnetic parameters. The flux coming to polar cap leads in the<br />

end to heating of polar ionosphere <strong>an</strong>d atmosphere, temperature contrast between two caps,<br />

intensification of the inter-hemisphere heat machine in the upper atmosphere, ch<strong>an</strong>ge of<br />

<strong>an</strong>gular moment of atmospheric zonal winds (<strong>an</strong>d consequently <strong>an</strong>gular velocity of the Earth<br />

w). The mech<strong>an</strong>ism successfully reproduces the 22-yr variations in W, Tgl <strong>an</strong>d w.

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