Oscillatory behavior in the quiet Sun observed with the New Solar Telescope

Abstract

Surface photometry of the quiet Sun has achieved an angular resolution of $0".1$ with the New Solar Telescope at Big Bear Solar Observatory revealing that a disproportionate fraction of the oscillatory events appear above observed bright point-like structures. During the tracking of these structures, we noted that the more powerful oscillatory events are cospatial with them, indicating that observed flux tubes may be the source of many observed oscillatory events.

arXiv comment5 pages 4 figures

References in corpus (6)

• Emergence of Small-Scale Magnetic Loops in the Quiet Sun Internetwork
• Non-linear numerical simulations of magneto-acoustic wave propagation in small-scale flux tubes
• Solar Oscillations and Convection: I. Formalism for Radial Oscillations
• Imaging Spectropolarimetry with IBIS: Evolution of Bright Points in the Quiet Sun
• The Influence of Magnetic Field on Oscillations in the Solar Chromosphere
• The Position of High Frequency Waves with Respect to the Granulation Pattern

Cited by in corpus (5)

• Photospheric Signatures of Granular-scale Flux Emergence and Cancellation at the Penumbral Boundary
• Response of Granulation to Small Scale Bright Features in the Quiet Sun
• Umbral Dynamics in the Near Infrared Continuum
• Signature of Collision of Magnetic Flux Tubes in the Quiet Solar Photosphere
• Substructure of Quiet Sun Bright Points