Open AccessEl Niño–Southern Oscillation: Magnitudes and asymmetry
Author(s) -
Douglass David H.
Publication year - 2010
Publication title -
journal of geophysical research: atmospheres
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.67
H-Index - 298
eISSN - 2156-2202
pISSN - 0148-0227
DOI - 10.1029/2009jd013508
Subject(s) - el niño southern oscillation , magnitude (astronomy) , asymmetry , oscillation (cell signaling) , gaussian , climatology , southern oscillation , physics , perturbation (astronomy) , geology , chemistry , astrophysics , biochemistry , quantum mechanics
The alternating warm/cold phenomena in the Pacific, known as El Niño–Southern Oscillation (ENSO), is characterized by large perturbations to the worldwide climate. Indices have been defined to characterize this phenomenon. However, the commonly used indices contain an unwanted effect from the annual cycle that can be reduced by digital filtering. Using a filtered ENSO index N L on data from 1856 to the present allows more accurate calculations of various quantities to be made. New results are (1) the distribution of positive values of N L is Gaussian. Thus, large‐magnitude El Niño events come from the tail of this distribution and not from some rare external perturbation. (2) The probability of occurrence of an El Niño of any magnitude can be calculated. A 1997–1998 El Niño will occur once in approximately 70 ± 20 years, while an El Niño 25% larger will occur once in approximately 700 ± 200 years. (3) The distribution of negative values of N L deviates from Gaussian because of a deficiency of large La Niña events. (4) Examination of the 20 largest El Niño events since 1856 shows that there is no increase in the frequency of such events with time.