Pliocene equatorial temperature: Lessons from atmospheric superrotation

نویسندگان

  • Eli Tziperman
  • Brian Farrell
چکیده

[1] There is proxy evidence that the pronounced east-west temperature difference observed today across the equatorial Pacific Ocean may not have existed in the early Pliocene (4–5 Ma BP) and that the east Pacific cold tongue developed gradually toward the end of the Pliocene (2 Ma BP). The east Pacific temperature influences weather and climate worldwide, and the Pliocene climate may be an instructive analogue to a future warm climate arising from anthropogenic elevation of CO2, making understanding the Pliocene equatorial SST gradient especially relevant. A mechanism for maintaining a weaker Pliocene equatorial temperature gradient is proposed that borrows from theories of atmospheric superrotation. The mechanism is based on enhanced or rearranged tropical convective activity during the warmer Pliocene climate exciting atmospheric Rossby waves that propagated poleward from the equator. These waves produced an equatorward flux of westerly momentum that weakened the surface easterlies and therefore the east-west thermocline slope and SST gradient.

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Superrotation in Terrestrial Atmospheres

Atmospheric superrotation with prograde equatorial winds and an equatorial angular momentum maximum is ubiquitous in planetary atmospheres. It is clear that eddy fluxes of angular momentum toward the equator are necessary to generate it. But under what conditions superrotation arises has remained unclear. This paper presents simulations and a scaling theory that establish conditions under which...

متن کامل

Abrupt Transition to Strong Superrotation Driven by Equatorial Wave Resonance in an Idealized GCM

Persistent superrotation is seen in the atmospheres of other terrestrial bodies (Venus, Titan) but not in that of present Earth, which is distinguished by equatorial easterlies. Nevertheless, superrotation has appeared in numerical simulations of Earth’s atmosphere, from two-layer models to multilevel comprehensive GCMs. Simulations of warm climates that generate enhanced tropical convective va...

متن کامل

Equatorial Superrotation and Barotropic Instability: Static Stability Variants

Altering the tropospheric static stability changes the nature of the equatorial superrotation associated with unstable, low-latitude, westerly jets, according to calculations with a dry, global, multilevel, spectral, primitive equation model subject to a simple Newtonian heating function. For a low static stability, the superrotation fluxes with the simplest structure occur when the stratospher...

متن کامل

Convective Generation of Equatorial Superrotation in Planetary Atmospheres

In rapidly rotating planetary atmospheres that are heated from below, equatorial superrotation can occur through convective generation of equatorial Rossby waves. If the heating from below is sufficiently strong that convection penetrates into the upper troposphere, then the convection generates equatorial Rossby waves, which can induce the equatorward angular momentum transport necessary for s...

متن کامل

Spontaneous transition to superrotation in warm climates simulated by CAM3

Spontaneous transition to superrotation in warm climates simulated by CAM3" (2010). [1] Recent paleoclimate proxy reconstructions show that tropical surface temperatures may have been as high as 35°–40°C in the Early Cenozoic. Here, we study the tropical atmospheric circulation's response to temperatures in this range using a full‐complexity atmospheric general circulation model (AGCM). We find...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2009