| (56) HR 6819 is a binary system with no black hole. Revisiting the source with infrared interferometry and optical integral field spectroscopy
- Frost, A. J. et al
- published in Astronomy & Astrophysics, 659 issue L3, pp. 12 (2022)
- SCART-2023-0074
|
| (51) Coronal Microjets in Quiet-Sun Regions Observed with the Extreme Ultraviolet Imager on Board the Solar Orbiter
- Hou, Zhenyong et al
- published in The Astrophysical Journal Letters, 918 issue 1, id.L20 (2021)
- SCART-2022-0036
|
| (51) Investigating coronal loop morphology and dynamics from two vantage points
- Mandal, Sudip et al
- published in Astronomy & Astrophysics, 682, pp. id.L9 (2024)
- SCART-2024-0145
|
| (50) Statistical study of fine scale Extreme-UV quiet Sun brightenings: Closest Perihelion observations of the quiet solar corona with SolO/EUI
- Narang, Nancy et al
- Poster presented at EclipseSA: Joint SolO, PSP & DKIST Meeting , San Antonio, Texas, US on 2024-04-08
- POSTER-2024-0067
|
| (50) Automated Detection of Accelerating Solar Eruptions using Parabolic Hough Transform
- Patel, Ritesh et al
- published in Solar Physics (2020)
- SCART-2021-0041
| |
guest ::
