On the seasonal effect of orbital variations on the climates of the next 4000 years
A northern hemisphere thermodynamic climate model is used to compute the effect of the insolation anomalies due to orbital variations in the climates for the next 4000 years. Berger's mean monthly anomalies of insolation are used in the computations, which are carried out for 1000, 2000, 30...
Main Author: | |
---|---|
Format: | Article |
Language: | English |
Published: |
Copernicus Publications
1996-11-01
|
Series: | Annales Geophysicae |
Online Access: | https://www.ann-geophys.net/14/1198/1996/angeo-14-1198-1996.pdf |
Summary: | A northern hemisphere thermodynamic climate
model is used to compute the effect of the insolation anomalies due to orbital
variations in the climates for the next 4000 years. Berger's mean monthly
anomalies of insolation are used in the computations, which are carried out for
1000, 2000, 3000 and 4000 years after present (kyears AP). The numerical
simulations show that in the climates of the next 4000 years, due to the effect
of the orbital variations, springs and summers will be increasingly dryer and
falls and winters wetter than the present climate. |
---|---|
ISSN: | 0992-7689 1432-0576 |