Data Access
The "AIA Active Region Patches" comprise an unbiased multi-wavelength set of FITS files of data extracted from SDO/AIA full-disk data. The spatial extractions are based on SDO/HMI "Active Region Patch" (HARP) definitions, and match the HARP numbering. However, the AARPs have extended bounding-boxes to cover the larger visible extent of coronal loops. There is no spatial binning and no additional geometric or regridding performed. The spectral down-sampling comprises the omission of 1700 images; all other filters are included (94, 131, 171, 193, 211, 304, 335, 1600). The temporal sampling consists of 11 images at 72s cadence (13 min) for each wavelength, centered at 15:48, 16:48, 17:48, 18:48, 19:48, 20:48 and 21:48, daily. No AEC-invoked (shorter exposure) data were included; exposure times were consistent but not multiplied through (data are presented in DN). The SSW aia_prep and corrections for time-dependent sensitivity degradation were applied.
Version:2.5.0
The "AIA Active Region Patches" comprise an unbiased multi-wavelength set of FITS files of data extracted from SDO/AIA full-disk data. The spatial extractions are based on SDO/HMI "Active Region Patch" (HARP) definitions, and match the HARP numbering. However, the AARPs have extended bounding-boxes to cover the larger visible extent of coronal loops. There is no spatial binning and no additional geometric or regridding performed. The spectral down-sampling comprises the omission of 1700 images; all other filters are included (94, 131, 171, 193, 211, 304, 335, 1600). The temporal sampling consists of 11 images at 72s cadence (13 min) for each wavelength, centered at 15:48, 16:48, 17:48, 18:48, 19:48, 20:48 and 21:48, daily. No AEC-invoked (shorter exposure) data were included; exposure times were consistent but not multiplied through (data are presented in DN). The SSW aia_prep and corrections for time-dependent sensitivity degradation were applied.
| Role | Person | StartDate | StopDate | Note | |
|---|---|---|---|---|---|
| 1. | Author | spase://SMWG/Person/Karin.Dissauer | |||
| 2. | Author | spase://SMWG/Person/K.D.Leka | Corresponding Author | ||
| 3. | Author | spase://SMWG/Person/Eric.L.Wagner |
EUV Intensity at the 94 Angstrom wavelength emitted by Iron-18 (Fe XVIII) at temperatures of 6 million Kelvin
EUV Intensity at the 131 Angstrom wavelength emitted by Iron-20 (Fe XX) and Iron-23 (Fe XXIII) at temperatures greater than 10 million Kelvin
EUV Intensity at the 171 Angstrom wavelength emitted by Iron-9 (Fe IX) at temperatures of 600,000 Kelvin
EUV Intensity at the 193 Angstrom wavelength emitted by Iron-12 (Fe XII; 1.3 MK) and Iron-24 (Fe XXIV; 20MK)
EUV Intensity at the 211 Angstrom wavelength emitted by Iron-14 (Fe XII) at temperature of 2 million Kelvin
EUV Intensity at the 304 Angstrom wavelength emitted by Helium-2 (He II) at temperature of 50,000 Kelvin
EUV Intensity at the 335 Angstrom wavelength emitted by Iron-16 (Fe XVI) at temperature of 2.5 million Kelvin
Far UV Intensity at the 1600 Angstrom wavelength emitted by Carbon-4 (C IV) at temperature of 100,000 million Kelvin