Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

Analysis of Aditya-L1/VELC [Fe XIV] 5303 Å Spectroscopic Observations of the Solar Corona: Development of a Data-processing Pipeline

  • Authors: V. Muthu Priyal, Jagdev Singh, R. Ramesh, P. Savarimuthu, S. Nagashree, E. Yuvashree, K. Sasikumar Raja

V. Muthu Priyal et al 2026 The Astrophysical Journal Supplement Series 287 .

  • Provider: AAS Journals

Caption: Figure 8.

Panels (a) and (b) show the pixel position of the 5302.3 Å absorption-line minimum for slit 1, as a function of time, before and after spectral drift correction, respectively. Each data point is an average of ≈800 pixels along the spatial direction of the slit. The location of the absorption line in the slit can be seen in Figure 4.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article

Show More

Copyright and Terms & Conditions

Additional terms of reuse