deletions | additions       diff --git a/WH_YIS_THIS_PARA_WIDER__.tex b/WH_YIS_THIS_PARA_WIDER__.tex  index e212d4d..aa38dd6 100644  --- a/WH_YIS_THIS_PARA_WIDER__.tex  +++ b/WH_YIS_THIS_PARA_WIDER__.tex 
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From this diagram we conclude that magnetic fields above 10 kG  are not present at the hydrogen-burning shell for stars below 1.1\msol when  they are near the red giant luminosity bump (\numax\ $\sim50$\muhz). By  assuming magnetic  flux conservation this corresponds to 1 kG near the hydrogen-burning cores of Sun like stars.   %For stars with suppressed modes we derive the lower limit of how  %strong the field in the core [at least] needs to be for suppression to