Review script for paper "2024MNRAS.527.1774V" made with predictor "DataLinkerWithSupport"

[abuonomo]

Created by Paper Data Linking Bot

Please review the download script and instrument details for the paper.

bibcode: 2024MNRAS.527.1774V predictor: DataLinkerWithSupport annotated pdf: view here (requires login)

Checklist

Download Script

• [x] Correct time ranges specified

• [x] Correct VSO instruments specified

• [x] Query returns good results or contains warning with reasoning if not

• [x] Physical observables omitted or correct

• [x] Wavelengths omitted or correct

• [x] Cadences omitted or correct

Instrument Details

• [x] Consistent with download_script.py

Metadata

• [x] Contains the bibcode for the relevant paper
• [x] VSO sources consistent with download_script.py

For more details, refer to the Contributing Guide.

[catbyrd]

Omitted GONG. Should it be included? @wafels Link: https://sdac.virtualsolar.org/cgi/show_details?source=GONG Context from paper:

In Fig. 4, ground-based GONG H α images and AIA 171 Å images are displayed at different times at the initiation of the eruption. In H α,the prominence appears brighter against the background whereasit is dark in AIA 171 Å images. Especially, the filament segment near leg L1 is set to rise from 04:20 UT, probably because the magnetic flux emergence at the foot point area. Because of projection effects, we could not produce the flux evolution results to support this inference. From the leg L1, the prominence morphology depicts a helical shape with a dip in the middle section of the corona. This helical shape in the corona implies an inverse-S shape of filament (Rust & Tumar 1994) when seen from top as evidenced on December 2 (Fig. 3). At around 04:38 UT, the kinked prominence stretched and then runs into fast rise motion