Abstract
During the Neoproterozoic period, most landmasses were assembled into the super-continent, Rodinia, and parts experienced glaciation in low paleolatitudes. We examine possible causes of glaciation by increasing rotation rate, reducing the solar constant and carbon dioxide concentrations for an idealized super-continent that is centered in the Northern Hemispehre tropics-subtropics. Further, we introduce a 2 km north-south mountain chain in the western regions of this super-continent. A mixed layer ocean or prescribed time varying sea surface temperatures are used in these simulations. Our results show that neither an individual factor or a combination of these factors can cool temperatures enough to bring about glaciation on the tropical super-continent. We conclude that other factors would be needed to initiate glaciation.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 3525-3528 |
| Number of pages | 4 |
| Journal | Geophysical Research Letters |
| Volume | 25 |
| Issue number | 18 |
| DOIs | |
| State | Published - Sep 15 1998 |
All Science Journal Classification (ASJC) codes
- Geophysics
- General Earth and Planetary Sciences
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