STScI Logo
STScI Logo
HST
Banner
FAQ
STScI

Part II: ACS Data Handbook

TOC PREV NEXT INDEX PDF

2.3 Data Storage Requirements


Users are reminded to consider the large size of WFC exposures when allocating disk space for storing and reprocessing ACS data. Raw images serve as input to the calibration pipeline and have the file sizes (in MB) given in Table 2.4. The WFC image includes two SCI arrays, while the HRC and SBC detectors have a single array. The raw image sizes presume that both the SCI and DQ arrays are populated with short integer values, but that the ERR arrays are NULL (all pixels have a value of zero).

During CALACS processing, the SCI arrays are converted from integer to floating point values. The null ERR array is populated with floating point values, and the null DQ array is populated with integer values. As a result, the size of calibrated images (in MB) is much larger. The image size in pixels is given in Table 2.5. Calibrated images taken with the WFC and HRC detectors are smaller than raw images because the overscan regions have been trimmed during processing.

After calibration, MultiDrizzle combines the science, data quality, and error arrays for each detector into a single science, weight, and context extension. Once the distortion is corrected, the size of the drizzled images will be larger (in pixels and also in MB) than the calibrated images due to the fact that their projection on the sky is rhombus-shaped, rather than square. The specific dimensions of the drizzled image depend on the image orientation and on which distortion model is currently in use in the pipeline and will vary slightly (~1-2 pixels) due to the effects of velocity aberration.

Table 2.4: Size (in MB) of raw, calibrated, and drizzled ACS images for each detector. The drizzled image sizes are distortion-corrected only and assume no additional rotation, dither offset or scale change.
Detector Size of FITS file (Sraw) Size of FITS file (Scal) Size of FITS file (Sdrz)
WFC (2 Chips)
68.7 MB
168 MB
215 MB
HRC (1 Chip)
4.4 MB
10.5 MB
16 MB
SBC (1 Chip)
4.2 MB
10.5 MB
16 MB

 
Table 2.5: Size (in pixels) for raw, calibrated, and drizzled ACS images for each detector. The drizzled image sizes are distortion-corrected only and assume no additional rotation, dither offset or scale change. The size of drizzled images will vary slightly due to velocity aberration effects.
Detector Xraw Yraw Xcal Ycal Xdrz Ydrz
WFC (2 Chips)
4144
2068
4096
2048
4213
4240
HRC (1 Chip)
1062
1044
1024
1024
1164
1138
SBC (1 Chip)
1024
1024
1024
1024
1397
1341

 

While the size of calibrated, drizzled HRC and SBC images is comparable to that of STIS or WFPC2, the ACS WFC images are over 16 times as large. The following equation can be used to estimate the minimum amount of free storage required for processing associated ACS data:

where:

  • Dmin is the minimum free disk space required for processing,
  • n is the number of exposures in each CR-SPLIT set or REPEAT-OBS set,
  • Sraw is the size of the raw exposure (from Table 2.4),
  • Scal is the size of the calibrated exposure (from Table 2.4),
  • Sdrz is the size of the distortion-corrected exposure (from Table 2.4),
  • p is the percentage shift (in pixels) across all dither positions

TOC PREV NEXT INDEX PDF
Space Telescope Science Institute
http://www.stsci.edu
Voice: (410) 338-1082
help@stsci.edu

Copyright  | Help  | Printable Page