  We construct static, nonextremal black hole solutions of the Einstein-Maxwell
equations in $d=6,7$ spacetime dimensions, with an event horizon of $S^2\times
S^{d-4}$ topology. These configurations are asymptotically flat, the U(1) field
being purely magnetic, with a spherical distribution of monopole charges but no
net charge measured at infinity. They can be viewed as generalizations of the
$d=5$ static dipole black ring, sharing its basic properties, in particular the
presence of a conical singularity. The magnetized version of these solutions is
constructed by applying a Harrison transformation, which puts them into an
external magnetic field. For $d=5,6,7$, balanced configurations approaching
asymptotically a Melvin universe background are found for a critical value of
the background magnetic field.
