The Problem of Meridional Heat Transport in the Astronomical Climate Theory
The reduction of solar radiation arriving in the summer half of the years by 65° N has been found to be a consequence of decreased inclination of the rotation axis and increased meridional contrast in insolation, rather than a result of climate cooling. Thus, the astronomical climate theory involves...
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| Veröffentlicht in: | Izvestiya. Atmospheric and oceanic physics 2019-12, Vol.55 (10), p.1572-1583 |
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| container_title | Izvestiya. Atmospheric and oceanic physics |
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| creator | Fedorov, V. M. |
| description | The reduction of solar radiation arriving in the summer half of the years by 65° N has been found to be a consequence of decreased inclination of the rotation axis and increased meridional contrast in insolation, rather than a result of climate cooling. Thus, the astronomical climate theory involves a paradox related to the fact that the change in the meridional heat transfer due to a change in the inclination of the rotation axis is disregarded. In this context, the mechanism of the astronomical chronology of climatic events in the Pleistocene needs to be revised. |
| doi_str_mv | 10.1134/S0001433819100025 |
| format | Article |
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| source | Springer Online Journals Complete |
| subjects | Celestial bodies Climate Climatology Earth and Environmental Science Earth Sciences Geophysics/Geodesy Heat transfer Heat transport Inclination Meridional heat transport Pleistocene Rotation Solar radiation |
| title | The Problem of Meridional Heat Transport in the Astronomical Climate Theory |
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