Local isometries of $\mathcal {L}(X,C(K))$

Rao, T. S. S. R. K.

doi:10.1090/s0002-9939-05-07832-9

Cited by 4 publications

(1 citation statement)

References 12 publications

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“…The NVST is a ground-based solar telescope, and the adaptive optics (AO) system (Rao et al 2016) is not yet widely used in daily observations. In order to overcome the influence of seeing, the speckle masking technique (Liu et al 1998;Xiang et al 2016) is used to obtain the high resolution monochromatic images of each off-band.…”

Section: Instrumentations and Observationsmentioning

confidence: 99%

The Co-alignment of Winged Hα Data Observed by the New Vacuum Solar Telescope*

Cai¹,

Yang²,

Xiang³

et al. 2022

Res. Astron. Astrophys.

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The New Vacuum Solar Telescope (NVST) has been publishing its novel winged Ha data (WHD) since April 2021, namely the Ha imaging spectroscopic data. Compared with the prior released version, the new data has been further co-aligned among the off-band images and packaged into a standard solar physics community format. In this study, we apply the optical flow method to co-align spectroscopic data, and assess the alignment accuracy of algorithm under the different similarities between the images of off-band and line center. As a result, the alignment accuracy can reach up to 0.004 ′′ and 0.095 ′′ in the near wing from line center of 0.2 Å and 0.4 Å, which corresponding to the similarity of about 0.8 and 0.4, respectively. Our algorithm can meet the alignment accuracy requirement of within 0.1 arc sec under the similarity ≥0.3, corresponding to the maximum offset wavelength of 0.5 – 0.6 Å. Otherwise, it is necessary to increase more intermediate off-band images for transition alignment. In addition, the article illustrates the final product of the WHD in detail, which will provide convenience for the solar physicists to use high resolution Ha imaging spectroscopic data of NVST.

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Section: Instrumentations and Observationsmentioning

confidence: 99%