Podrobnosti záznamu

    Responses of the basic cycles of 178.7 and 2402 yr in solar-terrestrial phenomena during the Holocene
    Charvátová, Ivanka
    Hejda, Pavel
Typ dokumentu
    článek v odborném periodiku
Zdrojový dokument - seriál
    Pattern Recognition in Physics
    Roč. 2, January
    s. 21-26
    doplnit KW + UT ISI?
    Projekt: OC09070, GA MŠk3cav_un_auth*0252836
    Rozsah: 6 s. : E
Klíčové slovo
Abstrakt (anglicky)
   Reconstructions of solar-terrestrial (ST) phenomena, in sufficient quality, several thousands of years backward by means of radiocarbon (14C), 10Be or 18O isotopes have been employed for study of possible responses of the ordered (trefoil) and disordered intervals (types) of the solar inertial motion (SIM) as well as of the 370 yr exceptional segments occurring in steps of 2402 yr in these phenomena. The trefoil intervals are about 50 yr long, and the Sun returns to the trefoil intervals always after 178.7 yr, on average. During intermediate intervals the Sun moves along chaotic (disordered) lines. It was also found that very long (nearly 370 yr) intervals of the solely trefoil orbit of the SIM occurred in steps of 2402 yr. Such exceptional intervals occurred in the years 159 BC-208 AD, 2561-2193 BC, 4964-4598 BC, etc. A stable behaviour of ST phenomena during these long segments is documented.
    AV ČR Brno, Geofyzikální ústav
Kód přispěvatele
    AV ČR, GFÚ
Zdrojový formát
Datum importu
    23. 10. 2014