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Datasets for the article "The temperature and density of a solar flare kernel measured from extreme ultraviolet lines of O IV"

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Mendeley Data2024-05-10 更新2024-06-28 收录
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https://zenodo.org/records/6726426
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This entry contains the following files: 20120309_030933_kernel_fe8_shift.save 20120309_030933_kernel_fe8_shift_fits.txt 20110814_055342_qs_offlimb_si10.save 20110814_055342_qs_offlimb_si10_fits.txt The .save files are IDL save files that can be restored into IDL using the restore command. The 20120309 save file contains: swspec - An IDL structure containing a 1D spectrum of the flare kernel for the EIS short wavelength (SW) channel. The format is that returned by eis-mask-spectrum.pro. lwspec - As above, but for the long-wavelength (LW) channel. map185 - An IDL map structure containing the Fe VIII 185.21 image that was used to select the flare kernel. mask185 - An IDL structure containing the pixel mask that is used as input to eis-mask-spectrum.pro. The Gaussian fits to the spectra (as performed with the routine spec-gauss-eis.pro) are stored in 20120309_030933_kernel_fe8shift_fits.txt. This file can be read with read_line_fits.pro in Solarsoft. The 20110814 dataset is used to obtain an off-limb coronal spectrum for calibration purposes. The save file contains: swspec - An IDL structure containing a 1D spectrum of the off-limb region for the EIS SW channel. The format is that returned by eis-mask-spectrum.pro. lwspec - As above, but for the LW channel. map - An IDL map structure containing the Si X 272 image that was used to select off-limb region. mask - An IDL structure containing the pixel mask that is used as input to eis-mask-spectrum.pro. The Gaussian fits to the spectra (as performed with the routine spec-gauss-eis.pro) are stored in 20110814_055342_qs_offlimb_si10_fits.txt. This file can be read with read_line_fits.pro in Solarsoft.
创建时间:
2023-12-16
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