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Astron. Astrophys. 319, 1036-1036 (1997)

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Response functions for the inversion of data from unresolved solar magnetic elements

L.R. Bellot Rubio , B. Ruiz Cobo and M. Collados

Instituto de Astrofísica de Canarias, E-38200 La Laguna (Tenerife), Spain

Astron. Astrophys. 306, 960-972 (1996)

Fig. 2 of this paper was not printed. Figure and caption are as follows:

[FIGURE] Fig. 2. Analytical (solid line) and numerical (dashed line) RF to the magnetic temperature for the continuum of Stokes I computed at
[FORMULA] = 6302.25 Å and multiplied by the internal temperature. They have been normalized to the HSRA continuum and to the area of the resolution element

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© European Southern Observatory (ESO) 1997

Online publication: July 3, 1998