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Spectroscopic diagnosis of a B-class flare and an associated filament eruption
DOI: 10.1007/s10509-025-04404-z Bibcode: 2025Ap&SS.370...13B

Kayshap, Pradeep; Babu, B. Suresh; Tripathi, Sharad C.

The flare ribbon and an associated filament eruption are diagnosed using O IV 1401.16 Å, Si IV 1402.77 Å, and Mg II k 2796.35 Å spectral lines provided by Interface Region Imaging Spectrograph (IRIS). The flare ribbons have downflow (redshifts) in all these lines, and this redshift decreases from the transition region to the chromosphere. While th…

2025 Astrophysics and Space Science
IRIS 0
Self-absorption in solar surge as observed by IRIS
DOI: 10.1007/s10509-024-04323-5 Bibcode: 2024Ap&SS.369...61B

Kayshap, Pradeep; Babu, B. Suresh; Tripathi, Sharad C.

Solar surges are collimated flows of plasma that occur in the periphery of active regions (ARs). The kinematics, physical properties, and triggering mechanisms of a solar surge were studied through imaging and spectroscopic diagnosis. The surge has a typical inverted Y-shape, and it moves with a speed of more than 200 km/s in the transition-region…

2024 Astrophysics and Space Science
IRIS 1
The bi-directional moving structures in a coronal bright point
DOI: 10.1007/s10509-016-2893-y Bibcode: 2016Ap&SS.361..301L

Li, Dong; Ning, Zongjun; Su, Yingna

We report the bi-directional moving structures in a coronal bright point (CBP) on 2015 July 14. It is observed by the Atmospheric Imaging Assembly (AIA) onboard Solar Dynamics Observatory (SDO). This CBP has a lifetime of ∼10 minutes, and a curved shape. The observations show that many bright structures are moving intermittently outward from the C…

2016 Astrophysics and Space Science
IRIS 19