Evolution of the global temperature structure of the solar corona during the minimum between solar cycles 23 and 24
The combination of differential emission measure tomography with extrapolation of the photospheric magnetic field allows determination of the electron density and electron temperature along individual magnetic field lines. This is especially useful in quiet-Sun (QS) plasmas where individual loops ca...
Guardado en:
| Autores principales: | Manchester IV, W.B., Nuevo, F.A., Huang, Z., Frazin, R., Jin, M., Vásquez, A.M. |
|---|---|
| Formato: | JOUR |
| Materias: | |
| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_0004637X_v773_n1_p_ManchesterIV |
| Aporte de: |
Ejemplares similares
-
Evolution of the global temperature structure of the solar corona during the minimum between solar cycles 23 and 24
por: Manchester IV, W.B., et al.
Publicado: (2013) -
Evolution of the global temperature structure of the solar corona during the minimum between solar cycles 23 and 24
por: Manchester IV, W.B., et al.
Publicado: (2013) -
Evolution of the global temperature structure of the solar corona during the minimum between solar cycles 23 and 24
por: Nuevo, Federico Alberto, et al.
Publicado: (2013) -
Newly discovered global temperature structures in the quiet sun at solar minimum
por: Huang, Z., et al. -
The solar minimum corona from differential emission measure tomography
por: Vásquez, A.M., et al.