000006790 001__ 6790
000006790 005__ 20240208145006.0
000006790 0247_ $$2DOI$$a10.24414/nc7j-b391
000006790 037__ $$aDATASET-2024-0024
000006790 100__ $$aBechet, Sabrina
000006790 245__ $$aUSET whole-disk images - L1 centered
000006790 260__ $$c2024
000006790 520__ $$aThe USET station hosts since 2002 three modern telescopes equipped with digital cameras recording full-disk images of the Sun in three different parts of the visible-light spectrum: broad-band white-light to observer the photosphere, and two telescopes with narrow-band filters (H-alpha line at 656.3 nm and Ca II K line at 393.37 nm) to monitor the chromosphere, where solar eruptive phenomena can be detected. The images have been recentered (less than 1 pixel precision), information about coordinate system was added in the header, so that data can be further processed with existing solar libraries and softwares. The image file format is FITS. The FITS header has been made homogeneous throughout the dataset and complies with the SOLARNET recommendations.
000006790 594__ $$aSTCE
000006790 6531_ $$aUSET
000006790 6531_ $$aSunspot
000006790 6531_ $$aPhotosphere
000006790 6531_ $$aChromosphere
000006790 700__ $$aClette, Frédéric
000006790 8560_ $$fsabrina.bechet@ksb-orb.be
000006790 85642 $$ahttps://www.sidc.be/uset/data/cameras/output_img/FTS/L0/
000006790 980__ $$aDATASET