The magnetic dipole $(M1)$ operator consists not only of the usually dominant isovector (IV) spin $(\ensuremath{\sigma}\ensuremath{\tau})$ term, but also of IV orbital $(l\ensuremath{\tau}),$ isoscalar (IS) spin $(\ensuremath{\sigma}),$ and IS orbital (l) terms. On the other hand, the Gamow-Teller (GT) operator contains only the $\ensuremath{\sigma}\ensuremath{\tau}$ term. Under the assumption that isospin is a good quantum number, isobaric analog structure is expected in a pair of $T=1/2$ mirror nuclei, and thus analogous transitions are found. For the $M1$ transitions in the $T=1/2$ mirror nuclei pair ${}^{23}\mathrm{Na}{\ensuremath{-}}^{23}\mathrm{Mg},$ the contributions of these various terms have been studied by comparing the strengths of the analogous $M1$ $\ensuremath{\gamma}$ transitions and the GT transitions deduced from high-resolution ${}^{23}\mathrm{Na}{(}^{3}\mathrm{He}{,t)}^{23}\mathrm{Mg}$ charge-exchange measurements. In some $M1$ transitions, unusually large orbital contributions were observed even for strong transitions, while in some others, almost no orbital contribution was found. It is known that ${}^{23}\mathrm{Na}$ and ${}^{23}\mathrm{Mg}$ are deformed. The large difference of the orbital contributions is explained based on the different selection rules for l and $\ensuremath{\sigma}$ operators in transitions connecting different deformed bands. Precise excitation energies are determined for the states above the proton separation energy in ${}^{23}\mathrm{Mg}.$ These states are of astrophysical interest because of their important role played in the ${}^{22}\mathrm{Na}(p,\ensuremath{\gamma}{)}^{23}\mathrm{Mg}$ reaction of the Ne-Na cycle in nucleosynthesis.
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