Abstract
AbstractThe magnetic field vectors derived from the Hanle effect measured in prominences during the ascending phase and maximum of Cycle 21 have been plotted on the corresponding synoptic maps of Meudon Observatory (e.g., Figure 2). Most of these measurements have been performed in a single line, He I D3. Our previous analysis of 2-line measurements have already proven that prominence magnetic fields have Inverse polarity (Bommier et al. 1994) and remain close to the horizontal plane (Bommier et al. 1986, 1994). We also found earlier that the field component along the filament axis shows a remarkable large scale pattern, especially at high latitudes (Leroy et al. 1983). Given the geometry of horizontal Inverse field, we reinvestigate this large scale organization through our complete set of observations (296 prominences). These new maps fully confirm and extend to medium latitudes the law of reversal of the axial field from one prominence band to the adjacent ones (see Figure 2). This behavior, together with the Inverse polarity pattern, gives a picture consistent with a North-South global field distorted by the differential rotation (see Figure 3).
Publisher
Cambridge University Press (CUP)
Cited by
8 articles.
订阅此论文施引文献
订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献
1. Chirality of Solar Filaments and the Supporting Magnetic Field;Helicities in Geophysics, Astrophysics, and Beyond;2023-12-15
2. Prominence oscillations;Living Reviews in Solar Physics;2018-04-23
3. The magnetic Rayleigh–Taylor instability in solar prominences;Reviews of Modern Plasma Physics;2017-12-15
4. The inference of the magnetic field vector in prominences;Proceedings of the International Astronomical Union;2013-06
5. Magnetohydrodynamic Waves in Partially Ionized Prominence Plasmas;Multi-scale Dynamical Processes in Space and Astrophysical Plasmas;2012