Acta Optica Sinica, Volume. 45, Issue 18, 1828015(2025)
Wavefront Detection Methods for Solar Prominence Based on Real Collected Images (Invited)
Fig. 1. Physical image and optical path diagram of NVST. (a) Physical image; (b) optical path diagram
Fig. 4. Acquired images in fact. (a) Prominence image; (b) dark-field image; (c) flat-field image
Fig. 5. Three-dimensional graphs for the correlation of the single sub-aperture. (a) CC algorithm; (b) AD algorithm
Fig. 7. Time series of slope signal for the first sub-aperture. (a) Horizontal direction; (b) vertical direction
Fig. 8. Time series of slope signals for all sub-apertures. (a) Horizontal direction; (b) vertical direction
Fig. 9. Time series for all tilt signals. (a) Horizontal direction; (b) vertical direction
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Chan Wang, Lanqiang Zhang, Xian Ran, Dingkang Tong, Changhui Rao. Wavefront Detection Methods for Solar Prominence Based on Real Collected Images (Invited)[J]. Acta Optica Sinica, 2025, 45(18): 1828015
Category: Remote Sensing and Sensors
Received: May. 30, 2025
Accepted: Jul. 31, 2025
Published Online: Sep. 19, 2025
The Author Email: Changhui Rao (chrao@ioe.ac.cn)
CSTR:32393.14.AOS251189