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Cited article:

Physical Characteristics of Umbral Dots Derived from a High-Resolution Observations

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Linear Acoustic Waves in a Nonisothermal Atmosphere. II. Photospheric Resonator Model of Three-minute Umbral Oscillations

Jongchul Chae, Juhyung Kang and Yuri E. Litvinenko
The Astrophysical Journal 883 (1) 72 (2019)
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PROPERTIES OF UMBRAL DOTS AS MEASURED FROM THE NEW SOLAR TELESCOPE DATA AND MHD SIMULATIONS

A. Kilcik, V. B. Yurchyshyn, M. Rempel, et al.
The Astrophysical Journal 745 (2) 163 (2012)
https://doi.org/10.1088/0004-637X/745/2/163

TEMPORAL EVOLUTION OF VELOCITY AND MAGNETIC FIELD IN AND AROUND UMBRAL DOTS

Hiroko Watanabe, Luis R. Bellot Rubio, Jaime de la Cruz Rodríguez and Luc Rouppe van der Voort
The Astrophysical Journal 757 (1) 49 (2012)
https://doi.org/10.1088/0004-637X/757/1/49

Solar Surface Magnetism and Irradiance on Time Scales from Days to the 11-Year Cycle

V. Domingo, I. Ermolli, P. Fox, et al.
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Application of an Improved Method of Image Segmentation and Some Considerations on Identification and Tracking of Umbral Dots

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On the fine structure of the quiet solar Ca II K atmosphere

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Solar Image Restoration By Use Of Multi-frame Blind De-convolution With Multiple Objects And Phase Diversity

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Penumbral structure at 0$\farcs$1 resolution

L. H. M. Rouppe van der Voort, M. G. Löfdahl, D. Kiselman and G. B. Scharmer
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Astrophysics in 2002

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