Context. Bright heads of penumbral filaments, penumbral grains (PGs), show
apparent horizontal motions inwards, towards the umbra, or outwards, away from
the umbra.
Aims. We aim to prove statistically whether the direction of PGs' apparent
motion is related to the inclination of the surrounding magnetic field.
Methods. We use spectropolarimetric observations of five sunspot penumbrae to
compare magnetic inclinations inside PGs with those in their surroundings. The
data are taken by three observatories: Hinode satellite, Swedish Solar
Telescope, and GREGOR solar telescope. The direction of PGs' motion is
determined by feature tracking. The atmospheric conditions in PGs and their
surroundings, including the magnetic field information, are retrieved by means
of height-stratified spectropolarimetric inversions.
Results. On a sample of 444 inward- and 269 outward-moving PGs we show that
43% of the inward-moving PGs have magnetic inclination larger by 8∘±4∘ than the inclination in their surroundings and 51% of the
outward-moving PGs have the inclination smaller by 13∘±7∘ than
the surrounding one. The opposite relation of inclinations is observed at only
one-fifth of the inward- and outward-moving PGs.
Conclusions. Rising hot plasma in PGs surrounded by a less inclined magnetic
field may adapt its trajectory to be more vertical, causing an inward apparent
motion of PGs. Oppositely, it may be dragged by a more horizontal surrounding
magnetic field such that an outward apparent motion is observed.Comment: 7 pages, 4 figures, 2 table