𝔖 Bobbio Scriptorium
✦   LIBER   ✦

The Evershed motion in sunspots

✍ Scribed by S. M. Chitre


Publisher
Springer
Year
1968
Tongue
English
Weight
373 KB
Volume
4
Category
Article
ISSN
0038-0938

No coin nor oath required. For personal study only.

✦ Synopsis


The Evershed motion is postulated as a steady, laminar flow of material along a limiting field line which separates the umbral magnetic field from the penumbral. Assuming that the Evershed flow starts from the spot-base with a velocity which is adequate to carry the convective flux at that level, the velocity at the surface comes out to be of the order of 1 km/sec, in good agreement with the observed Evershed velocity.


πŸ“œ SIMILAR VOLUMES


Fine structure and evershed motions in t
✍ D. J. Galloway πŸ“‚ Article πŸ“… 1975 πŸ› Springer 🌐 English βš– 348 KB

The observed inhomogeneity of the intensity and Evershed motions means any model of the penumbra must be essentially inhomogeneous. A simple model is put forward in which the interaction of convection rolls with an initially homogeneous magnetohydrostatic sunspot field causes a concentration of flux

Oscillatory motions in sunspots
✍ J. M. Beckers; R. B. Schultz πŸ“‚ Article πŸ“… 1972 πŸ› Springer 🌐 English βš– 601 KB

We observe vertical velocity oscillations in some sunspot umbrae with periods of about 180 s and peak to peak amplitudes up to 1 km s -1. These oscillations are not visible in either the line depth, line width or the continuum intensity. No correlation seems to exist between the occurence of these o

Motions and lifetimes of the penumbral b
✍ Klara TΓΆnjes; Hubertus WΓΆhl πŸ“‚ Article πŸ“… 1982 πŸ› Springer 🌐 English βš– 561 KB

It is confirmed that the penumbral bright grains are moving towards the sunspots umbra. We find different prope r motions of 0.08 to 0.33 km s -1 for different penumbrae and different reduction methods. The lifetimes of these bright grains are about 1.5 to 3 hr depending on the position in the penum