High resolution reconstruction of solar prominence images observed by the New Vacuum Solar Telescope

•We proposed a modified cross correlation method to align prominence data.•We compared the alignment accuracy of the conventional method and the modified method.•We successfully reconstructed the prominences and other off-limb objects observed by NVST.•The results demonstrate that the high resolutio...

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Published inNew astronomy Vol. 49; pp. 8 - 12
Main Authors Xiang, Yong-yuan, Liu, Zhong, Jin, Zhen-yu
Format Journal Article
LanguageEnglish
Published Elsevier B.V 01.11.2016
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ISSN1384-1076
1384-1092
DOI10.1016/j.newast.2016.05.002

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Abstract •We proposed a modified cross correlation method to align prominence data.•We compared the alignment accuracy of the conventional method and the modified method.•We successfully reconstructed the prominences and other off-limb objects observed by NVST.•The results demonstrate that the high resolution observation of solar prominence by a ground-based solar telescope is feasible. A high resolution image showing fine structures is crucial for understanding the nature of solar prominence. In this paper, high resolution imaging of solar prominence on the New Vacuum Solar Telescope (NVST) is introduced, using speckle masking. Each step of the data reduction especially the image alignment is discussed. Accurate alignment of all frames and the non-isoplanatic calibration of each image are the keys for a successful reconstruction. Reconstructed high resolution images from NVST also indicate that under normal seeing condition, it is feasible to carry out high resolution observations of solar prominence by a ground-based solar telescope, even in the absence of adaptive optics.
AbstractList A high resolution image showing fine structures is crucial for understanding the nature of solar prominence. In this paper, high resolution imaging of solar prominence on the New Vacuum Solar Telescope (NVST) is introduced, using speckle masking. Each step of the data reduction especially the image alignment is discussed. Accurate alignment of all frames and the non-isoplanatic calibration of each image are the keys for a successful reconstruction. Reconstructed high resolution images from NVST also indicate that under normal seeing condition, it is feasible to carry out high resolution observations of solar prominence by a ground-based solar telescope, even in the absence of adaptive optics.
•We proposed a modified cross correlation method to align prominence data.•We compared the alignment accuracy of the conventional method and the modified method.•We successfully reconstructed the prominences and other off-limb objects observed by NVST.•The results demonstrate that the high resolution observation of solar prominence by a ground-based solar telescope is feasible. A high resolution image showing fine structures is crucial for understanding the nature of solar prominence. In this paper, high resolution imaging of solar prominence on the New Vacuum Solar Telescope (NVST) is introduced, using speckle masking. Each step of the data reduction especially the image alignment is discussed. Accurate alignment of all frames and the non-isoplanatic calibration of each image are the keys for a successful reconstruction. Reconstructed high resolution images from NVST also indicate that under normal seeing condition, it is feasible to carry out high resolution observations of solar prominence by a ground-based solar telescope, even in the absence of adaptive optics.
Author Liu, Zhong
Jin, Zhen-yu
Xiang, Yong-yuan
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  surname: Jin
  fullname: Jin, Zhen-yu
  organization: Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China
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Keywords Techniques: speckle imaging
Methods: solar image reconstruction
Sun: prominences
Language English
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SSID ssj0007198
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Snippet •We proposed a modified cross correlation method to align prominence data.•We compared the alignment accuracy of the conventional method and the modified...
A high resolution image showing fine structures is crucial for understanding the nature of solar prominence. In this paper, high resolution imaging of solar...
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SubjectTerms Alignment
Calibration
High resolution
Image reconstruction
Methods: solar image reconstruction
Reconstruction
Solar prominences
Space telescopes
Sun: prominences
Techniques: speckle imaging
Title High resolution reconstruction of solar prominence images observed by the New Vacuum Solar Telescope
URI https://dx.doi.org/10.1016/j.newast.2016.05.002
https://www.proquest.com/docview/1811881134
https://www.proquest.com/docview/1835579738
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