Atmospheric Sciences Seminar

September 29, 3:30pm - 5:00pm
Mānoa Campus, Virtual Meeting

The Unbearable Nonrandomness of Convection

Brian Mapes
Professor, Department of Atmospheric Sciences
Director, Meteorology and Physical Oceanography Program
RSMAS, University of Miami

You are invited to our weekly online Atmospheric Sciences Fall 2021 seminars via Zoom meeting.
When: September 29, 2021 at 3:30PM HST
Meeting admission: 3:15PM HST

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As a security precaution, unmuting microphones, starting video, screen share, and using the 'chat' feature will be disabled for those attending the seminar, except for ATMO faculty. If you would like to say something, please use the 'raise hand' feature. The host or a co-host can then enable you to unmute your microphone.

Air is transparent to visible light, but the layer up to about 14km high cools by emitting infrared radiation. Gravity therefore creates mechanical energy to drive air motions (convection), in order to carry energy up there from the sun-warmed surface. But this purpose (telos, in Greek) doesn’t totally determine the form and scales and timing of convection. These are left to chance, further subject to the twitchy amplifying effect of water vapor condensation. The equator to pole sunlight gradient gives teleological purpose to some planet-spanning large scales (slant-wise convection in mid latitudes), so those are part of the mix. Surface features like continents and beautiful island chains imprint themselves in the sky. But many other kinds of motions have no apparent purpose — except perhaps to thwart our hopes of prediction, by scrambling each other! Sometimes, when telos is absent, nature maximizes randomness as a principle (or at least a useful assumption, turning our ignorance into a principle). But even that fails us in the atmosphere, because those twitchy amplifying feedbacks have subtly systematic aspects that introduce long threads of memory and history and coherent structures in space. Turbulence is a discouraging subject!

To focus discussion, I will emphasize precipitating deep tropical convection within the almost-uniformly warm tropics, or (for more rigor) in strictly uniform idealized "tropics-world" simulations. After a spectral kinetic energy equation is implanted in listener minds, this talk surveys some of the many conditional biases in the probability of development of convection’s unit structure (“cells”), and what those imply about the many scales of motion driven by convection's gravitational work. Of course, all the field’s familiar named phenomena will be mentioned among those flywheels and splashes, but I hope these are illuminated a bit differently by this context, for experts to ponder once again and students to approach freshly.

Event Sponsor
SOEST Atmospheric Sciences, Mānoa Campus

More Information
808-956-8775, SEE FLYER (PDF)

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