Observations of a round, unipolar sunspot in the Zeeman triplet Fe I A6302.5 with the High Altitude Observatory Stokes Polarimeter are used to derive the vector magnetic field in the spot. The behavior of the magnitude, inclination, and azimuth of the field vector B across the spot is discussed. A l
β¦ LIBER β¦
Sunspots with the Strongest Magnetic Fields
β Scribed by W. Livingston; J. W. Harvey; O. V. Malanushenko; L. Webster
- Publisher
- Springer
- Year
- 2006
- Tongue
- English
- Weight
- 1023 KB
- Volume
- 239
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
π SIMILAR VOLUMES
Vector magnetic fields in sunspots
β
Joseph B. Gurman; Lewis L. House
π
Article
π
1981
π
Springer
π
English
β 910 KB
Sunspot models with twisted magnetic fie
β
Vladimir Osherovich; T. Flaa
π
Article
π
1983
π
Springer
π
English
β 275 KB
The return-flux sunspot model is generalized by including azimuthal magnetic field B e . The basic equation is obtained and numerical solutions are compared with the analogous solutions for the Schl~iter-Temesvary sunspot theory for two cases: B e ~ B r and B e ~ rB r. The solutions demonstrate that
Magnetic fields in small and young sunsp
β
V. Bumba
π
Article
π
1967
π
Springer
π
English
β 831 KB
Magnetic field oscillations of sunspots?
β
J. Staude
π
Article
π
2002
π
John Wiley and Sons
π
English
β 536 KB
Small-scale solar magnetic fields and βi
β
Cornelis Zwaan
π
Article
π
1967
π
Springer
π
English
β 183 KB
The spiral configuration of sunspot magn
β
M. J. Hagyard; E. A. West; N. P. Cumings
π
Article
π
1977
π
Springer
π
English
β 515 KB