Titlebook: Sunspots: Theory and Observations; John H. Thomas,Nigel O. Weiss Book 1992 Kluwer Academic Publishers 1992 Oscillation.Sunspot.cluster.con

deciduous

憤怒事實(shí)

雪崩

文件夾

悲觀

Observations of the Mesoscale Magnetic Structure of Sunspotssual and infrared lines are reviewed and partly considered from the point of view of self-similarity. The Evershed flow is briefly examined with regard to the non-uniqueness of the inferred intrinsic flow field and its relation to the inclination of the penumbral magnetic field.

屈尊

放逐

The Fate of the Heat Flux Blocked by Sunspotsre involved, and the adjustments are different on the two time scaes. On time scales longer than the thermal time scale τ. of the convection zone (10. yr), a significant fraction of the heat flux blocked by spots can reappear elsewhere at the surface. The average spot coverage over this time scale l

Vulvodynia

集聚成團(tuán)

High Resolution Observations of the Magnetic and Velocity Field of Simple Sunspotstograms, Dopplergrams, and continuum images nearly simultaneously. In addition the spectral resolution of the filter (88,000) allows the construction of “spectra” for all points in the field of view. The changing patterns of the line of sight magnetic and flow fields with position around the spots a

焦慮