𝔖 Bobbio Scriptorium
✦   LIBER   ✦

Differential rotation of short-lived solar filaments

✍ Scribed by W. M. Adams; Frances Tang


Publisher
Springer
Year
1977
Tongue
English
Weight
309 KB
Volume
55
Category
Article
ISSN
0038-0938

No coin nor oath required. For personal study only.

✦ Synopsis


We have measured the rotation rate of short-lived solar filaments as a function of their latitude. The resulting rotation curve appears to be somewhat flatter than the corresponding curve for long-lived filaments.

Solar Physics 55 (1977) 499-504. All Rights Reserved Copyright 9 1977 by D. Reidel Publishing Company, Dordrecht-Holland * This is the median time base over which we measured individual filament knots. When the finite size of the observing window (from -60 ~ to + 60 ~ from central meridian) is taken into account this implies that the true median lifetime is about four days.


πŸ“œ SIMILAR VOLUMES


Solar differential rotation determined b
✍ R. BrajΕ‘a; B. VrΕ‘nak; V. RuΕΎdjak; A. Schroll; S. Pohjolainen; S. Urpo; H. TerΓ€sr πŸ“‚ Article πŸ“… 1991 πŸ› Springer 🌐 English βš– 446 KB

The rotation rates obtained by' tracing 124 polar crown filaments are presented in comparison with previous results. Higher filament rotation rate in polar regions was detected and discussed in terms of the various phenomena such as: the projection effect due to the height of measured tracers, the c

Investigation of the solar differential
✍ D. R. Japaridze; M. Sh. Gigolashvili πŸ“‚ Article πŸ“… 1992 πŸ› Springer 🌐 English βš– 384 KB

Based on observational data on chromosphere filaments, certain characteristics of solar differential rotation during solar activity cycle No. 21 are determined at Abastumani Astrophysical Observatory. In the northern hemisphere of the Sun, propagation of a quasi-N-annual impulse of the rotation res

A model of solar differential rotation
✍ L. L. Kichatinov πŸ“‚ Article πŸ“… 1991 πŸ› Springer 🌐 English βš– 841 KB

An axisymmetric model for the Sun's differential rotation based upon a mechanism for angular momentum transport by compressible convection is developed. Convective heat transport is also considered. The model is simplified by the neglect of meridional circulation and radiative heat transport but is

Rigid and differential rotation of the s
✍ Ester Antonucci; Leif Svalgaard πŸ“‚ Article πŸ“… 1974 πŸ› Springer 🌐 English βš– 423 KB

The rotation of the solar corona has been studied using recurrence properties of the green coronal line (5303 A,) for the interval 1947-1970. Short-lived coronal activity is found to show the same differential rotation as short-lived photospheric magnetic field features. Long-lived recurrences show