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A Comparison of Flare Forecasting Methods. IV. Evaluating Consecutive-day Forecasting Patterns

Authors :
Peter T. Gallagher
Manolis K. Georgoulis
Yuki Kubo
Aoife E. McCloskey
Suzy Bingham
Sophie A. Murray
Sung-Hong Park
Graham Steward
Jesse Andries
Sangwoo Lee
K. D. Leka
Michael Terkildsen
Kanya Kusano
D. Shaun Bloomfield
Vasily Lobzin
Véronique Delouille
Rami Qahwaji
Kangjin Lee
Tarek A. M. Hamad Nageem
Michael Sharpe
Graham Barnes
R. A. Steenburgh
David A. Falconer
JunChul Mun
Source :
The Astrophysical Journal. 890:124
Publication Year :
2020
Publisher :
American Astronomical Society, 2020.

Abstract

A crucial challenge to successful flare prediction is forecasting periods that transition between "flare-quiet" and "flare-active". Building on earlier studies in this series (Barnes et al. 2016; Leka et al. 2019a,b) in which we describe methodology, details, and results of flare forecasting comparison efforts, we focus here on patterns of forecast outcomes (success and failure) over multi-day periods. A novel analysis is developed to evaluate forecasting success in the context of catching the first event of flare-active periods, and conversely, of correctly predicting declining flare activity. We demonstrate these evaluation methods graphically and quantitatively as they provide both quick comparative evaluations and options for detailed analysis. For the testing interval 2016-2017, we determine the relative frequency distribution of two-day dichotomous forecast outcomes for three different event histories (i.e., event/event, no-event/event and event/no-event), and use it to highlight performance differences between forecasting methods. A trend is identified across all forecasting methods that a high/low forecast probability on day-1 remains high/low on day-2 even though flaring activity is transitioning. For M-class and larger flares, we find that explicitly including persistence or prior flare history in computing forecasts helps to improve overall forecast performance. It is also found that using magnetic/modern data leads to improvement in catching the first-event/first-no-event transitions. Finally, 15% of major (i.e., M-class or above) flare days over the testing interval were effectively missed due to a lack of observations from instruments away from the Earth-Sun line.<br />Comment: 33 pages, 13 figures, accepted for publication in ApJ

Details

ISSN :
15384357
Volume :
890
Database :
OpenAIRE
Journal :
The Astrophysical Journal
Accession number :
edsair.doi.dedup.....6c2b54bf6d37632ab1fa090c17d7203b
Full Text :
https://doi.org/10.3847/1538-4357/ab65f0