Work

Sensitivity of the Fe IX λ171 Line Profile to Slow Magneto-Acoustic Waves Propagating in a Solar Coronal Loop

Year: 2024

Type: article

Source: Kinematics and Physics of Celestial Bodies

DOI: 10.3103/s0884591324060059

Authors: S. G. Mamedov, Z. F. Aliyeva, Z. A. Samedov

Institutions: Shamakhy Astrophysical Observatory named after Nasraddin Tusi, Baku State University

Language: English

Topic: Solar and Space Plasma Dynamics

Subfield: Astronomy and Astrophysics

Field: Physics and Astronomy

Domain: Physical Sciences

Open Access status: closed

OpenAlex ID: W4405006494

FWCI:

Cites: 30

Cited by:

Related to: 10