GCM evaluation of a mechanism for El Niño triggering by the El Chichón ash cloud

1995 ◽  
Vol 22 (17) ◽  
pp. 2369-2372 ◽  
Author(s):  
Alan Robock ◽  
Karl E. Taylor ◽  
Georgiy L. Stenchikov ◽  
Yuhe Liu
Keyword(s):  
El Niño ◽  
El Nino ◽  
2006 ◽  
Vol 19 (12) ◽  
pp. 2984-2994 ◽  
Author(s):  
James K. Angell

Abstract The mean monthly polar stereographic map analyses of the Free University of Berlin terminated at the end of 2001. This paper summarizes the changes in size of the 300-mb north circumpolar vortex, and quadrants, for the full period of record, 1963–2001, where the size has been defined by planimetering the area poleward of contours in the jet stream core. A contracted vortex has tended to be a deep vortex in winter but a shallow vortex in summer. During 1963–2001 there was a statistically significant decrease in vortex size of 1.5% per decade, the decrease in size of Western Hemisphere quadrants being twice that of Eastern Hemisphere quadrants. A significant increase in Arctic Oscillation (AO) index accompanies the significant decrease in vortex size, but since the vortex contracts appreciably in all four seasons, whereas the positive trend in the AO index is mainly in winter, the vortex cannot serve as a proxy for the AO index. The evidence for vortex contraction at the time of the 1976–77 regime shift is not conclusive, but there is good evidence for a 6% increase in vortex size due to the 1991 Pinatubo eruption. There is little change in vortex size following the 1982 El Chichon eruption, however. Because on average there is a significant 4% contraction of the vortex following an El Niño, it is proposed that the vortex expansion to be expected following the 1982 El Chichon eruption has been contravened by the contraction following the strong 1982–83 El Niño. There is little relation between vortex size and phase of the quasi-biennial oscillation (QBO), and the evidence for a contracted vortex near 11-yr sunspot maxima is tenuous because the vortex record extends through only three full sunspot cycles. There is a highly significant tendency for opposite vortex quadrants 0°–90°E and 90°W–180° to vary in size together, indicating either a pulsating polar vortex or the propagation of planetary wavenumber 2.


2016 ◽  
Vol 29 (4) ◽  
pp. 1325-1338 ◽  
Author(s):  
A. Meyer ◽  
D. Folini ◽  
U. Lohmann ◽  
T. Peter

Abstract Tropical land mean surface air temperature and precipitation responses to the eruptions of El Chichón in 1982 and Pinatubo in 1991, as simulated by the atmosphere-only GCMs (AMIP) in phase 5 of the Coupled Model Intercomparison Project (CMIP5), are examined and compared to three observational datasets. The El Niño–Southern Oscillation (ENSO) signal was statistically separated from the volcanic signal in all time series. Focusing on the ENSO signal, it was found that the 17 investigated AMIP models successfully simulate the observed 4-month delay in the temperature responses to the ENSO phase but simulate somewhat too-fast precipitation responses during the El Niño onset stage. The observed correlation between temperature and ENSO phase (correlation coefficient of 0.75) is generally captured well by the models (simulated correlation of 0.71 and ensemble means of 0.61–0.83). For precipitation, mean correlations with the ENSO phase are −0.59 for observations and −0.53 for the models, with individual ensemble members having correlations as low as −0.26. Observed, ENSO-removed tropical land temperature and precipitation decrease by about 0.35 K and 0.25 mm day−1 after the Pinatubo eruption, while no significant decrease in either variable was observed after El Chichón. The AMIP models generally capture this behavior despite a tendency to overestimate the precipitation response to El Chichón. Scatter is substantial, both across models and across ensemble members of individual models. Natural variability thus may still play a prominent role despite the strong volcanic forcing.


Irriga ◽  
2015 ◽  
Vol 20 (2) ◽  
pp. 371-387 ◽  
Author(s):  
Givanildo De Gois ◽  
Rafael Coll Delgado ◽  
José Francisco De Oliveira Júnior

Foi avaliado o desempenho dos modelos esférico, exponencial e gaussiano na interpolação espacial do índice SPI em episódios de El Niño forte no Tocantins (TO), Brasil. O método utilizado foi a Krigagem Ordinária (KO). Os eventos foram 1982-83, 1990-93 e 1997-98. O Estado do TO foi dividido em duas regiões: ocidental e oriental. Foi aplicada à estatística descritiva baseado em índices existentes na literatura. Os modelos esférico e exponencial são similares quanto à magnitude dos erros estatísticos e com desempenho considerado ótimo para os ciclos iniciais de 1982-83 e 1990-93, a exceção foi o ciclo 1997-98, seguido do modelo gaussiano com desempenho abaixo em comparação aos demais. Ambos os modelos esférico e exponencial identificam espacialmente os eventos de seca em ambas as regiões no TO e, principalmente nos anos iniciais dos ciclos dos El Niños forte. Isso se deve aos efeitos de grande escala associado ao aumento dos aerossóis devido às erupções do El Chichón (1982) e Pinatubo (1991), seguido dos padrões de precipitação para os El Niños os quais o gradiente interbacias do Pacífico e Atlântico se forma em sua fase inicial, apresentam anomalias mais acentuadas, do que os El Niños com o gradiente interbacias na sua fase de decaimento.


2020 ◽  
Vol 55 (4) ◽  
pp. 1-14
Author(s):  
K. Legal ◽  
P. Plantin
Keyword(s):  
El Niño ◽  

2020 ◽  
Vol 54 (3) ◽  
pp. 1-15
Author(s):  
K. Legal ◽  
P. Plantin
Keyword(s):  
El Niño ◽  

Author(s):  
C. Thévenin-Lemoine ◽  
F. Accadbled ◽  
J. Sales de Gauzy
Keyword(s):  
El Niño ◽  

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