Frequency modulation reveals the phasing of orbital eccentricity during Cretaceous Oceanic Anoxic Event II and the Eocene hyperthermals
Identifikátory výsledku
Kód výsledku v IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985530%3A_____%2F16%3A00458676" target="_blank" >RIV/67985530:_____/16:00458676 - isvavai.cz</a>
Výsledek na webu
<a href="http://dx.doi.org/10.1016/j.epsl.2016.02.047" target="_blank" >http://dx.doi.org/10.1016/j.epsl.2016.02.047</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1016/j.epsl.2016.02.047" target="_blank" >10.1016/j.epsl.2016.02.047</a>
Alternativní jazyky
Jazyk výsledku
angličtina
Název v původním jazyce
Frequency modulation reveals the phasing of orbital eccentricity during Cretaceous Oceanic Anoxic Event II and the Eocene hyperthermals
Popis výsledku v původním jazyce
Major advances in our understanding of paleoclimate change derive from a precise reconstruction of the periods, amplitudes and phases of the Milankovitch cycles’ of precession, obliquity and eccentricity. While numerous quantitativeapproaches exist for the identification of these astronomical cycles in stratigraphic data, limitations in radioisotopic dating, and instability of the theoretical astronomical solutions beyond ∼50 Myr ago, can challenge identification of the phase relationships needed to constrain climate response and anchor floating astrochronologies. Here we demonstrate that interference patterns accompanying frequency modulation (FM) of short eccentricity provide a robust basis for identifying the phase of long eccentricity forcing in stratigraphic data. One-and two-dimensional models of sedimentary distortion of the astronomical signal are used to evaluate the veracity of the FM method, and indicate that pristine eccentricity FM can be readily distinguishedin paleo-records. Apart from paleoclimatic implications, the FM approach provides a quantitative technique for testing and calibrating theoretical astronomical solutions, and for refining chronologies for the deep past.n
Název v anglickém jazyce
Frequency modulation reveals the phasing of orbital eccentricity during Cretaceous Oceanic Anoxic Event II and the Eocene hyperthermals
Popis výsledku anglicky
Major advances in our understanding of paleoclimate change derive from a precise reconstruction of the periods, amplitudes and phases of the Milankovitch cycles’ of precession, obliquity and eccentricity. While numerous quantitativeapproaches exist for the identification of these astronomical cycles in stratigraphic data, limitations in radioisotopic dating, and instability of the theoretical astronomical solutions beyond ∼50 Myr ago, can challenge identification of the phase relationships needed to constrain climate response and anchor floating astrochronologies. Here we demonstrate that interference patterns accompanying frequency modulation (FM) of short eccentricity provide a robust basis for identifying the phase of long eccentricity forcing in stratigraphic data. One-and two-dimensional models of sedimentary distortion of the astronomical signal are used to evaluate the veracity of the FM method, and indicate that pristine eccentricity FM can be readily distinguishedin paleo-records. Apart from paleoclimatic implications, the FM approach provides a quantitative technique for testing and calibrating theoretical astronomical solutions, and for refining chronologies for the deep past.n
Klasifikace
Druh
J<sub>x</sub> - Nezařazeno - Článek v odborném periodiku (Jimp, Jsc a Jost)
CEP obor
DB - Geologie a mineralogie
OECD FORD obor
—
Návaznosti výsledku
Projekt
<a href="/cs/project/LH12041" target="_blank" >LH12041: Oscilace mořské hladiny a změny atmosférických koncentrací CO2 během vrcholného skleníkového klimatu (cenoman-turon, pánev Western Interior)</a><br>
Návaznosti
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Ostatní
Rok uplatnění
2016
Kód důvěrnosti údajů
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Údaje specifické pro druh výsledku
Název periodika
Earth and Planetary Science Letters
ISSN
0012-821X
e-ISSN
—
Svazek periodika
442
Číslo periodika v rámci svazku
15 May
Stát vydavatele periodika
NL - Nizozemsko
Počet stran výsledku
14
Strana od-do
143-156
Kód UT WoS článku
000375348700014
EID výsledku v databázi Scopus
2-s2.0-84960968488