The dynamics of rapid redshifted and blueshifted excursions to the solar Hα LINE

Kuridze, David, Henriques, Vasco, Mathioudakis, Mihalis, Erdélyi, Robert, Zaqarashvili, Teimuraz, Shelyag, Sergiy, Keys, Peter and Keenan, Francis (2015) The dynamics of rapid redshifted and blueshifted excursions to the solar Hα LINE. The Astrophysical Journal, 802 (1). p. 26. ISSN 1538-4357

[img]
Preview
Text
1501.06205v1.pdf - Accepted Version

Download (1MB) | Preview
Official URL: http://dx.doi.org/10.1088/0004-637X/802/1/26

Abstract

We analyze high temporal and spatial resolution time series of spectral scans of the Hα line obtained with the CRisp Imaging SpectroPolarimeter instrument mounted on the Swedish Solar Telescope. The data reveal highly dynamic, dark, short-lived structures known as Rapid Redshifted and Blueshifted Excursions (RREs, RBEs) that are on-disk absorption features observed in the red and blue wings of spectral lines formed in the chromosphere. We study the dynamics of RREs and RBEs by tracking their evolution in space and time, measuring the speed of the apparent motion, line of sight (LOS) Doppler velocity, and transverse velocity of individual structures. A statistical study of their measured properties shows that RREs and RBEs have similar occurrence rates, lifetimes, lengths, and widths. They also display non-periodic, nonlinear transverse motions perpendicular to their axes at speeds of 4–31 km s−1. Furthermore, both types of structures either appear as high speed jets and blobs that are directed outwardly from a magnetic bright point with speeds of 50–150 km s−1, or emerge within a few seconds. A study of the different velocity components suggests that the transverse motions along the LOS of the chromospheric flux tubes are responsible for the formation and appearance of these redshifted/blueshifted structures. The short lifetime and fast disappearance of the RREs/RBEs suggests that, similar to type II spicules, they are rapidly heated to transition region or even coronal temperatures. We speculate that the Kelvin Helmholtz instability triggered by observed transverse motions of these structures may be a viable mechanism for their heating.

Item Type: Article
Subjects: F300 Physics
F500 Astronomy
G100 Mathematics
Department: Faculties > Engineering and Environment > Mathematics and Information Sciences
Depositing User: Sergiy Shelyag
Date Deposited: 23 May 2016 15:19
Last Modified: 13 May 2017 15:26
URI: http://nrl.northumbria.ac.uk/id/eprint/26890

Actions (login required)

View Item View Item

Downloads

Downloads per month over past year

View more statistics


Policies: NRL Policies | NRL University Deposit Policy | NRL Deposit Licence