Statistical prediction models

2022 ◽  
pp. 15-34
Author(s):  
Stephen Niksa
2011 ◽  
Vol 24 (4) ◽  
pp. 567-573 ◽  
Author(s):  
Sung-Min Myoung ◽  
Doo-Jin Lee ◽  
Hwa-Soo Kim ◽  
Jin-Nam Jo

2020 ◽  
Vol 51 ◽  
pp. 11-19
Author(s):  
Karol Semrád ◽  
Katarína Draganová ◽  
Peter Koščák ◽  
Jozef Čerňan

2020 ◽  
Author(s):  
Jun Meng ◽  
Jingfang Fan ◽  
Josef Ludescher ◽  
Ankit Agarwala ◽  
Xiaosong Chen ◽  
...  

<p>The El Niño Southern Oscillation (ENSO) is one of the most prominent interannual climate phenomena. An early and reliable ENSO forecasting remains a crucial goal, due to its serious implications for economy, society, and ecosystem. Despite the development of various dynamical and statistical prediction models in the recent decades, the “spring predictability barrier” (SPB) remains a great challenge for long (over 6-month) lead-time forecasting. To overcome this barrier, here we develop an analysis tool, the System Sample Entropy (SysSampEn), to measure the complexity (disorder) of the system composed of temperature anomaly time series in the Niño 3.4 region. When applying this tool to several near surface air temperature and sea surface temperature datasets, we find that in all datasets a strong positive correlation exists between the magnitude of El Niño and the previous calendar year’s SysSampEn (complexity). We show that this correlation allows to forecast the magnitude of an El Niño with a prediction horizon of 1 year and high accuracy (i.e., Root Mean Square Error = 0.23°C for the average of the individual datasets forecasts). For the 2018 El Niño event, our method forecasts a weak El Niño with a magnitude of 1.11±0.23°C.  Our framework presented here not only facilitates a long–term forecasting of the El Niño magnitude but can potentially also be used as a measure for the complexity of other natural or engineering complex systems.</p>


2017 ◽  
Vol 53 (2) ◽  
pp. 207-216 ◽  
Author(s):  
Jin-Yong Kim ◽  
Kyong-Hwan Seo ◽  
Jun-Hyeok Son ◽  
Kyung-Ja Ha

2020 ◽  
Author(s):  
samuel Ismael BILLONG IV ◽  
Georges Edouard Kouamou ◽  
Thomas Bouetou

Abstract Modeling has become a tool capable of guiding public policies, especially in the area of health. Specifically, modeling in epidemiology makes it possible to follow the evolution of infections and to understand the behavior of viruses. Unfortunately, the traditional SIR models and the statistical prediction models commonly used suffer from the lack of accurate information and the unavailability of a large amount of data, also they do not take into account the interactions within the population. This paper proposes a hybrid SIR model which takes into consideration the spatio-temporal dynamics of individuals. The model is based on the discrete stochastic diffusion equations. To build the equation system, the 2D diffusion equations are coupled to the human displacement probability law pattern through a discretization made by the finite volume method for complex geometries. Beyond the health consequences it causes, COVID-19 (coronavirus) is a test case used to validate the proposed model. We used the case of a developed country before confinement to fit to the chosen displacement pattern, and to analyze the sensitivity of the parameters of the model taking into account the accuracy of the statistics provided.


2020 ◽  
Author(s):  
Jens Hüsers ◽  
Guido Hafer ◽  
Jan Heggemann ◽  
Stefan Wiemeyer ◽  
Swen Malte John ◽  
...  

Abstract Background: Diabetes mellitus is a major global health issue with a growing prevalence. In this context, the number of diabetic complications is also on the rise, such as diabetic foot ulcers (DFU), which are closely linked to the risk of lower extremity amputation (LEA). Statistical prediction tools may support clinicians to initiate early tertiary LEA prevention for DFU patients. Thus, we designed Bayesian prediction models, as they produce transparent decision rules, quantify uncertainty intuitively and acknowledge prior available scientific knowledge.Method: A logistic regression using observational collected according to the standardised PEDIS classification was utilised to compute the six-month amputation risk of DFU patients for two types of LEA: 1.) any-amputation and 2.) major-amputation. Being able to incorporate information which is available before the analysis, the Bayesian models were fitted following a twofold strategy. First, the designed prediction models waive the available information and, second, we incorporated the a priori available scientific knowledge into our models. Then, we evaluated each model with respect to the effect of the predictors and validity of the models. Next, we compared the performance of both models with respect to the incorporation of prior knowledge.Results: This study included 237 patients. The mean age was 65.9 (SD 12.3), and 83.5 per cent were male. Concerning the outcome, 31.6% underwent any- and 12.2% underwent a major-amputation procedure. The risk factors of perfusion, ulcer extent and depth revealed an impact on the outcomes, whereas the infection status and sensation did not. The major-amputation model using prior information outperformed the uninformed counterpart (AUC 0.765 vs AUC 0.790, Cohen’s d 2.21). In contrast, the models predicting any-amputation performed similarly (0.793 vs 0.790, Cohen’s d 0.22).Conclusions: Both of the Bayesian amputation risk models showed acceptable prognostic values, and the major-amputation model benefitted from incorporating a priori information from a previous study. Thus, PEDIS serves as a valid foundation for a clinical decision support tool for the prediction of the amputation risk in DFU patients. Furthermore, we demonstrated the use of the available prior scientific information within a Bayesian framework to establish chains of knowledge.


CHEST Journal ◽  
2020 ◽  
Vol 158 (1) ◽  
pp. S29-S38 ◽  
Author(s):  
Michael W. Kattan ◽  
Thomas A. Gerds

2021 ◽  
Vol 257 (2) ◽  
pp. 50
Author(s):  
Rongxin Tang ◽  
Wenti Liao ◽  
Zhou Chen ◽  
Xunwen Zeng ◽  
Jing-song Wang ◽  
...  

Abstract Solar flare formation mechanisms and their corresponding predictions have commonly been difficult topics in solar physics for decades. The traditional forecasting method manually constructs a statistical relationship between the measured values of solar active regions and solar flares that cannot fully utilize the information related to solar flares contained in observational data. In this article, we first used neural-network methods driven by the measured magnetogram and magnetic characteristic parameters of the sunspot group to learn the prediction model and predict solar flares. The prediction fusion model is based on a deep neural network, convolutional neural network, and bidirectional long short-term memory neural network and can predict whether a sunspot group will have a flare event above class M or class C in the next 24 or 48 hr. The real skill statistics (TSS) and F1 scores were used to evaluate the performances of our fusion model. The test results clearly show that this fusion model can make full use of the information related to solar flares and combine the advantages of each independent model to capture the evolution characteristics of solar flares, which is a much better performance than traditional statistical prediction models or any single machine-learning method. We also proposed two frameworks, namely F1_FFM and TSS_FFM, which optimize the F1 score and TSS score, respectively. The cross validation results show that they have their respective advantages in the F1 score and TSS score.


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