All Tables
- Table 1:
Observing log.
- Table 2:
Abundance ratios with respect to Fe for various phases (A-E) of the large flare (values rounded to multiples
of 0.1), and
for the low-level pre-flare section (Q). All values are normalized with the
solar ratios. The basic solar abundances of Anders & Grevesse (1989) have been used, except
for Fe for which the value given in Grevesse & Sauval (1999) has been adopted. Errors are
based on 1
errors of the individual abundances (see text for details). "Fe/Fe''
is unity by definition, but the error bars indicate the fractional uncertainty of
the Fe abundance.
The last line gives the Fe abundance relative to solar photospheric values.