Fine Structure of Prominences and Filaments

1994 ◽  
Vol 144 ◽  
pp. 289-296
Author(s):  
P. Mein

AbstractThe fine structures of prominences and filaments are involved in many phenomena such as formation and magnetostatic support, instabilities and eruptions. After a short introduction (Section 1), we concentrate on quiescent prominences, and we review some recent results about resolved structures (Section 2), statistical properties of “threads” (Section 3), and detailed analysis of average line profiles (Section 4). We mention magnetic field measurements (Section 5) and thermal problems (Section 6). New magnetostatic models (Section 7) are very promising. We discuss briefly the problem of the scale of fine structures, and we suggest some directions for further works (Section 8).

2017 ◽  
Vol 852 (1) ◽  
pp. 5 ◽  
Author(s):  
Megan Reiter ◽  
Nuria Calvet ◽  
Thanawuth Thanathibodee ◽  
Stefan Kraus ◽  
P. Wilson Cauley ◽  
...  

2014 ◽  
Vol 9 (S307) ◽  
pp. 399-400 ◽  
Author(s):  
Matt Shultz ◽  
Gregg Wade ◽  
Thomas Rivinius ◽  
Wagner Marcolino ◽  
Huib Henrichs ◽  
...  

AbstractWe present our analysis of 6 years of ESPaDOnS spectropolarimetry of the magnetic β Cep star ξ1CMa (B1 III). This high-precision magnetometry is consistent with a rotational periodProt> 40 yr. Absorption line profiles can be reproduced with a non-rotating model. We constrainR⋆,L⋆, and the stellar age via a Baade-Wesselink analysis. Spindown due to angular momentum loss via the magnetosphere predicts an extremely long rotational period if the magnetic dipoleBd> 6 kG, a strength also inferred by the best-fit sinusoids to the longitudinal magnetic field measurementsBZwhen phased with a 60-yearProt.


1963 ◽  
Vol 1 (3) ◽  
pp. 399-414 ◽  
Author(s):  
Laurence J. Cahill

1992 ◽  
Vol 177 (1-4) ◽  
pp. 516-518 ◽  
Author(s):  
H. Rakoto ◽  
T. Klein ◽  
C. Berger ◽  
G. Fourcaudot ◽  
J.C. Grieco ◽  
...  

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