Figure 7 from A Statistical Inference Method for Interpreting the CLASP Observations

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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 7.

Histogram of the cosines of the normal vectors, ﹩{\mu }_{{\boldsymbol{n}}}﹩, in the 3D MHD model of Carlsson et al. (2016) and its best least-squares fit with the distribution of Equation (18) with a ≈ 5.

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