Cosmic energies and mankind: graphs for reflection - страница 3

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См.: JereH. Jenkins, EphraimFischbach, JohnB. Buncher, JohnT. Gruenwald, DennisE. KrauseandJoshuaJ. Mattes, «EvidenceforCorrelationsBetweenNuclearDecayRatesandEarth-SunDistance» (arXiv:0808.3283v1 [astro-ph]).

These cosmic energies are so great that they affect the temperature changes on Earth.



Synchronous changes of the Earth's rotational velocity (v×10^10) in relative units (slid blue line), accumulated anomalies of the annual number of days with processes of the circulation form -C (red) and moving averages of the air temperature global anomalies for five years after the trend exclusion according to the HadCRUT3data (black).

Ref.: N. S. Sidorenkov. "Impact of the annual and monthly Earth’s rotation on cycling of the atmospheric processes, weather and climate changes", Hydro-meteorological Centre of Russia.

Solar activity is a concrete manifestation of cosmic energies. There are profound works in this field.



Time evolution

(a) the variations of magnetic flux at the bottom (tachocline zone) of the Sun convective zone (see Dikpati, G. de Toma, and P. A. Gilman, 2008);

(b) fractional change in female breast cancer mortality (see: Juckett David A., 2009);

(c) fractional change in female breast cancer mortality for birth cohort in UK (see: Juckett David A., 2009);

(d) geomagnetic field secular variations (Y-component, nT/year) as observed at the Eskdalemuir observatory (England) (see: http://www.geomag.bgs.ac.uk./gifs/ annual_means.shtml), where the variations (gY/gt) are directly proportional to the westward drift of magnetic features;

(e) Malignant brain tumor (brain stem) (see: Legler Julie M., 1999) ;

(f) the number of deaths from ICD9 item n 191 Malignant neoplasm of brain (see: Pechholdova M., 2008);

(g) Brain lymphoma incidences in US;

(h) the mortality rates from infectious diseases (incl. Tuberculosis) at ages 15 – 34 in France (see: Mesle F., 2006);

The curves (a) and (b) are smoothed by the sliding intervals of 5 and 11 years.



Time evolution of (a) the variations of the magnetic flux at the bottom (the tachocline zone) of the Sun convective zone (see: M. T. Santini, G. Rainaldi, and P. Indovina., 2009), (b) the geomagnetic feld secular variations (the Y-component, nT / year) measured at the Eskdalemuir observatory (England), (see: A. R. Liboff, 2009 ). Curves are smoothed by the sliding intervals in 5 and 11 years.