The nature of elongated granulations and stretched dark lanes in a newly emerging flux region

TL;DR

This paper investigates the characteristics of elongated granulations and stretched dark lanes in an emerging solar flux region, revealing their association with emerging magnetic flux tubes and their magnetic and dynamic properties.

Contribution

It provides detailed high-resolution observations linking elongated granules and dark lanes to emerging flux tubes with specific magnetic and flow characteristics.

Findings

Stretched dark lanes correlate strongly with blue shifts and transverse magnetic fields.

Transverse magnetic fields in dark lanes reach 300-400 G.

Features suggest an arch-shaped emerging flux tube.

Abstract

In this study, we explore the elongated granulations and stretched dark lanes within the emerging anti-Hale active region NOAA 12720. Utilizing high-resolution observations from the New Vacuum Solar Telescope, we discern a prevalence of elongated granules and stretched dark lanes associated with the emergence of new magnetic flux positioned between two primary opposing magnetic polarities. These elongated granulations and stretched dark lanes exhibit an alignment of strong transverse fields and a significant inclination angle. The endpoints of these features separate from each other, with their midpoints predominantly characterized by blue-shifted signals in the photosphere. This suggests a close association between elongated granules and stretched dark lanes with the newly emerging flux. Additionally, we find that the stretched dark lanes display a more pronounced correlation with strong blue shifts and photospheric transverse magnetic fields compared to the elongated granulations. The transverse magnetic field within these stretched dark lanes reaches magnitudes of approximately 300 to 400 G, and the inclination angle demonstrates an "arch-like" pattern along the trajectory of the stretched dark lane. Based on these observed characteristics, we infer the presence of an emerging flux tube with an "arch-like" shape situated along the stretched dark lane. Consequently, we conclude that the stretched dark lanes likely represent manifestations of the emerging flux tube, while the elongated granulations may correspond to the gaps between the emerging flux tubes.