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University of Illinois at Urbana-Champaign

The energy cycle of ENSO

Abstract

dc:description

The spatial pattern of warming in sea surface temperatures (SSTs) can have major impacts on Earth’s top-of-atmosphere (TOA) energy budget, a phenomenon known in recent research as the “pattern effect”. Much of this pattern effect has been attributed to variability in low cloud radiative effect (CRE), and previous studies have shown that ENSO variability in CRE could inform long-term cloud radiative feedbacks. While ENSO teleconnections and predictability have been extensively researched for decades, ENSO-induced variability in atmospheric radiation has not been fully characterized. Here I use ENSO as an emergent constraint on the pattern effect. We find strong linear relationships between modeled ENSO feedbacks and their respective pattern effects, especially for net CRE. Observed ENSO feedbacks lie within the middle of the model ensemble and suggest a pattern effect magnitude of 1.00 ± 0.35 W /m2/K when calculated relative to preindustrial conditions. Model-simulated pattern effects also exhibit similar spatial distributions as the pattern diversity of ENSO, hinting at similar physics governing the two phenomena. Additionally, I add to previous studies of the ENSO-radiation relationship by exploring the impact of the ENSO cycle and pattern diversity on observed top-of-atmosphere (TOA) radiation. I find that both eastern Pacific (EP) and central Pacific (CP) ENSO SST patterns have associated all-sky radiation patterns that are dominated by low-cloud radiative effect (CRE) anomalies that are primarily driven by EIS CRE, with regional contributions by SST CRE, EIS CRE, and Tadv CRE. Clear-sky radiation anomalies do not contribute as significantly to the net radiative response patterns because they are driven by a negative Planck+lapse-rate feedback that is partially compensated by a positive longwave water vapor feedback. This competition between clear-sky feedbacks results in little contribution to the total radiative response patterns. These findings suggest that ENSO provides a potential emergent constraint on model pattern effect uncertainty, demonstrates the influence of ENSO pattern diversity on the drivers of the ENSO SST-radiation relationship, and depicts the first-order importance of ENSO pattern diversity in setting TOA radiation anomalies.

Degree

thesis:*
Name thesis:degree_name
M.S.
Level thesis:degree_level
Thesis
Discipline thesis:degree_discipline
Atmospheric Sciences
Grantor
University of Illinois at Urbana-Champaign
Year dc:date
2024

Author and committee

dc:creator, dc:contributor.*
Author dc:creator
  • Hanke, Tyler J
Contributors dc:contributor
  • Proistosescu, Cristian
  • Raghuraman, Shiv P
  • Wang, Zhuo

Subjects

dc:subject × 5

Rights

dc:rights
Statement dc:rights
  • Copyright 2024 Tyler Hanke
Language dc:language
en, eng

Identifiers

dc:identifier.*
Handle dc:identifier
https://hdl.handle.net/2142/127279

Chain of custody

source
Harvested from
University of Illinois - Urbana-Champaign
Base URL
www.ideals.illinois.edu/oai-pmh
Last updated
2026-07-22
Source record
OAI-PMH GetRecord
citation

Hanke, Tyler J. The energy cycle of ENSO. Thesis thesis, University of Illinois at Urbana-Champaign, 2024. https://hdl.handle.net/2142/127279