Image Details

Choose export citation format:

A Statistical Inference Method for Interpreting the CLASP Observations

  • Authors: J. Štěpán, J. Trujillo Bueno, L. Belluzzi, A. Asensio Ramos, R. Manso Sainz, T. del Pino Alemán, R. Casini, R. Kano, A. Winebarger, F. Auchère, R. Ishikawa, N. Narukage, K. Kobayashi, T. Bando, Y. Katsukawa, M. Kubo, S. Ishikawa, G. Giono, H. Hara, Y. Suematsu, T. Shimizu, T. Sakao, S. Tsuneta, K. Ichimoto, J. Cirtain, P. Champey, B. De Pontieu, and M. Carlsson

2018 The Astrophysical Journal 865 48.

  • Provider: AAS Journals

Caption: Figure 3.

PDFs ﹩{p}^{\mu }(q| {\boldsymbol{\theta }})﹩ (top panels) and ﹩{p}^{\mu }(u| {\boldsymbol{\theta }})﹩ (bottom panels) for various CTR model parameters ﹩{\boldsymbol{\theta }}=\{a,\bar{B}\}﹩ (indicated at the top of each panel). For the sake of simplicity, we assume that the joint PDF can be factorized as ﹩{p}^{\mu }({\boldsymbol{S}}| {\boldsymbol{\theta }})={p}^{\mu }(q| {\boldsymbol{\theta }}){p}^{\mu }(u| {\boldsymbol{\theta }})﹩. For each value of μ (horizontal axis), the darker shades of gray indicate larger PDF values. The dashed red curves in the top panels show the CLV of the q signals after averaging the q values at each μ (cf. Figure 2). The PDFs are normalized to unity at each μ value. See the text for more details. The gray-scale color table differs from panel to panel in order to improve the contrast of the individual plots. The normalization is such that ﹩\int {p}^{\mu }(q| {\boldsymbol{\theta }})\ {dq}=\int {p}^{\mu }(u| {\boldsymbol{\theta }})\ {du}=1﹩ for every μ.

Other Images in This Article
Copyright and Terms & Conditions