Abundance determination in solar active region
Abundance determination in solar active region
- New search for: Monsignori Fossi, B. C.
- New search for: Landini, M.
- New search for: Thomas, R. J.
- New search for: Neupert, W. M.
- New search for: Monsignori Fossi, B. C.
- New search for: Landini, M.
- New search for: Thomas, R. J.
- New search for: Neupert, W. M.
An improved method has been developed to evaluate element abundances from emission line intensities of thin plasmas, depending on the differential emission measure (DEM) of the source. Observations made by the Solar EUV Rocket Telescope and Spectrograph (SERTS) Rocket EUV Spectrograph are used to perform a detailed analysis of the DEM distribution for temperatures larger than 10(exp 5) K in a solar active region. Comparison of the DEM distributions obtained by means of lines from different elements allows the verification of relative abundances for the most common elements of the solar corona, and gives an abundance estimates for the minor components, such as Na, Al, Ar, Cr, Mn and Zn.
Document information
Abundance determination in solar active region
Advances in Space Research ; 14 , 4
1994-04-01
Miscellaneous
No indication
English
Similar titles
Abundance Determination in Solar Active Region
| British Library Conference Proceedings | 1994
Abundance Determination in Solar Active Region
| Online Contents | 1994
Abundance determination in solar active region
| Elsevier | 1993
Abundance variations in solar active regions
| Elsevier | 1991
Abundance variations in solar active regions
| NTRS | 1991