This chapter reviews the recent observations of waves and oscillations manifesting in fine-scale magnetic structures in the solar photosphere, which are often interpreted as the "building blocks' of the magnetic Sun. The authors found, through phase relationships between the various waveforms, that small-scale magnetic bright points (MBPs) in the photosphere demonstrated signatures of specific magnetoacoustic waves, in particular the sausage and kink modes. Modern magnetohydrodynamic (MHD) simulations of the lower solar atmosphere clearly show how torsional motions can easily be induced in magnetic elements in the photosphere through the processes of vortical motions and/or buffeting by neighboring granules. The authors detected significant power associated with high-frequency horizontal motions, and suggested that these cases may be especially important in the creation of a turbulent environment that efficiently promotes Alfvén wave dissipation.
|Title of host publication||Low-Frequency Waves in Space Plasmas|
|Editors||Andreas Keiling, Dong-Hun Lee, Valery Nakariakov|
|Publisher||John Wiley & Sons, Inc. |
|Number of pages||17|
|Publication status||Published - 12 Feb 2016|
|Name||Geophysical Monograph Series|