摘要: The coordinates of the cooling cycle described in Paper I are re-defined order to provide an account which part played by sunspot is separated from role supergranule cells transporting energy away it.
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Frank N. Edmonds, Carol J. Webb, Spectral analyses of solar photospheric fluctuations Solar Physics. ,vol. 25, pp. 44- 70 ,(1972) , 10.1007/BF00155743
J. M. Beckers, E. H. Schr�ter, The intensity, velocity and magnetic structure of a sunspot region Solar Physics. ,vol. 4, pp. 142- 164 ,(1968) , 10.1007/BF00148076
N. O. Weiss, Magnetic Flux Tubes and Convection in the Sun Monthly Notices of the Royal Astronomical Society. ,vol. 128, pp. 225- 235 ,(1964) , 10.1093/MNRAS/128.3.225
Henry Norris Russell, Note on Cooling by Expansion in Sun-Spots The Astrophysical Journal. ,vol. 54, pp. 293- ,(1921) , 10.1086/142645
C. J. Cannon, The effect of two-dimensional macroscopic velocity fields on models of the lower solar chromosphere Solar Physics. ,vol. 21, pp. 82- 92 ,(1971) , 10.1007/BF00155776
Willi Deinzer, On the Magneto-Hydrostatic Theory of Sunspots. The Astrophysical Journal. ,vol. 141, pp. 548- ,(1965) , 10.1086/148144
P. R. Wilson, Facular models and the sunspot energy deficit Solar Physics. ,vol. 21, pp. 101- 112 ,(1971) , 10.1007/BF00155779
K. Harvey, J. Harvey, Observations of moving magnetic features near sunspots Solar Physics. ,vol. 28, pp. 61- 71 ,(1973) , 10.1007/BF00152912
P. R. Wilson, The Structure of a Sunspot. I: The Birth and Development of a Sunspot Solar Physics. ,vol. 3, pp. 243- 257 ,(1968) , 10.1007/BF00155160
MartinD. Altschuler, Yoshinari Nakagawa, CarlG. Lilliequist, Concerning the origin of evershed motion in sunspots Solar Physics. ,vol. 3, pp. 466- 481 ,(1968) , 10.1007/BF00171620