Uncertainties in estimates of the occurrence rate of rare space weather events

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Uncertainties in estimates of the occurrence rate of rare space weather events Jeffrey J. Love Geomagnetism Program USGS Natural Hazards Mission jlove@usgs.gov Love, J. J., 2012. Credible occurrence probabilities for extreme geophysical events: Earthquakes, volcanic eruptions, magnetic storms, Geophys. Res. Lett., 39, L10301, doi:10.1029/2012gl051431.

Rare-event analysis is important for lots of geophysical hazards

Magnetic observatory data Magnetic storms were discovered in the 19 th century through groundbased measurement of geomagnetic activity. The only complete record of the 1859 Carrington event was collected through visual measurement at the Colaba magnetic observatory in India. Standard measures of magnetic storm intensity (Dst, AE, Kp, aa, etc.) are all derived from modern magnetic observatory data. In this study, we will count magnetic storm events defined by a maximum Dst that exceeds a chosen threshold. Colaba observatory in Bombay India USGS San Juan Puerto Rico observatory

Frequentist and Bayesian Statistical Analyses Frequentist analysis (Classical): Model parameters are deterministic, Ronald Fisher (1890-- proposed on the basis of independent theories, parameter values are 1962) subjected to tests of statistical significance by comparing model predictions against a null hypothesis of randomness. Bayesian analysis: Model parameters are treated as an idealized statistical realization of probability, inference of parameter values is made on the basis of data and prior beliefs. The Jeffreys prior preserves posterior probability under reparameterization. Thomas Bayes (1701-1761) Pierre-Simon Laplace (1749-1827) Harold Jeffreys (1891-- 1989)

Frequentist and Bayesian Statistical Analyses Frequentist analysis (Classical): Model parameters are deterministic, Ronald Fisher (1890-- proposed on the basis of independent theories, parameter values are 1962) subjected to tests of statistical significance by comparing model predictions against a null hypothesis of randomness. Maximum Likelihood: Model parameters are deterministic, but they are estimated from a data set. Bayesian analysis: Model parameters are treated as an idealized statistical realization of probability, inference of parameter values is made on the basis of data and prior beliefs. The Jeffreys prior preserves posterior probability under reparameterization. Thomas Bayes (1701-1761) Pierre-Simon Laplace (1749-1827) Harold Jeffreys (1891-- 1989)

Frequentist Bayesian with Jeffreys Prior

Three magnetic storm events with Dst 589 nt since 1859 Average occurrence rate: 1.961 /century 95% credibility interval: [0.350, 4.878]/century Most likely 10-yr occurrence probability (N 1): 0.178 95% credibility interval: [0.034, 0.386] One magnetic storm event with Dst 1760 nt since 1859 (Carrington) Average occurrence rate: 0.654 /century 95% credibility interval: [0.163, 1.471]/century Most likely 10-yr occurrence probability (N 1): 0.063 95% credibility interval: [<0.001, 0.230] Riley: 10-yr occurrence probability for Carrington event: 0.120

How might statistical estimations be improved? Old magnetic observatory data sets might reveal other extreme events measured in terms of Dst or related absolute measures of disturbance. Satellite (SOHO, STEREO, etc.) monitoring and counting of extreme coronal mass ejections that haven t arrived at Earth: Baker, D. N. et al., A major solar eruptive event in July 2012: Defining extreme space weather scenarios, Space Weather, 2013. Ngwira, C., et al. Simulation of the 23 July 2012 extreme space weather event: What if this extremely rare CME was Earth directed?, Space Weather, 2013. Statistical models need to be improved, perhaps by combining the Bayesian Poisson models (presented here) with the power-law models: Love, J. J., Credible occurrence probabilities for extreme geophysical events: Earthquakes, volcanic eruptions, magnetic storms, Geophys. Res. Lett., 2012. Riley, P., On the probability of occurrence of extreme space weather events, Space Weather, 2012. Ice core records of transient enhancements in nitrate, proposed to be related to proton events (not magnetic storms), now appear to be unreliable: Wolff, E. W. et al., The Carrington event not observed in most ice core nitrate records, Geophys. Res. Lett., 2012.

It is the mark of an educated mind to rest satisfied with the degree of precision which the nature of the subject admits and not to seek exactness where only an approximation is possible. Aristotle (384-322 BC)