Podrobnosti záznamu

Název
    Responses of the basic cycles of 178.7 and 2402 yr in solar-terrestrial phenomena during the Holocene
Autor
    Charvátová, Ivanka
    Hejda, Pavel
Jazyk
    anglicky
Typ dokumentu
    článek v odborném periodiku
Zdrojový dokument - seriál
    Pattern Recognition in Physics
Svazek/č.
    Roč. 2, January
Strany
    s. 21-26
Rok
    2014
Poznámky
    doplnit KW + UT ISI?
    Projekt: OC09070, GA MŠk3cav_un_auth*0252836
    Rozsah: 6 s. : E
Klíčové slovo
    178.7
    2402
    Basic
    Cycles
    During
    Holocene
    Phenomena
    Responses
    Solar-terrestrial
    Yr
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.
Přispěvatel
    AV ČR Brno, Geofyzikální ústav
Kód přispěvatele
    AV ČR, GFÚ
Zdrojový formát
    U
Datum importu
    23. 10. 2014