MIPS IOC Data Volume Estimate | Last modified: | 18-Sep-99 | ||||||||||||||
Total | Data | Compressed | Uncompressed | Uncompressed | Data Rate | Uncompressed | Uncompressed | |||||||||
IOC-MIPS_ | Name | Tot Time | Tot Time | DCEs | Groups | EXP | Mode | DATA (bits) | DATA (bits) | DATA (Mbytes) | Volume/time | Max data (bits) | Max data (Mbytes) | Notes | ||
(sec) | (hrs) | (est) | (est) | (sec) | (est) | (est) | (est) | (kbs -- est) | (upper limit) | (upper limit) | ||||||
1 | 100a | First light | 1200 | 0.33 | 120 | 3 | 40 | 10 | SUR | 3.7916E+07 | 7.5640E+07 | 9.46 | 63.03 | 7.9450E+08 | 99.31 | |
2 | 110a | Confirmation of on-board data processing | 3600 | 1.00 | 288 | 1 | 96 | all | both | 2.9710E+08 | 5.9374E+08 | 74.22 | 164.93 | 2.3835E+09 | 297.94 | |
algorithms | ||||||||||||||||
3 | 105a | On-board S/W: Command | 900 | 0.25 | 72 | 3 | 24 | 10 | both | 5.1061E+07 | 1.0201E+08 | 12.75 | 113.34 | 5.9587E+08 | 74.48 | |
expansion and data manipulation | ||||||||||||||||
4 | 355a | Cluster option validation | 2700 | 0.75 | 300 | 1 | 100 | 10 | SUR | 9.4790E+07 | 1.8910E+08 | 23.64 | 70.04 | 1.7876E+09 | 223.45 | |
5 | 345a | Opt temp for 24 um array | 5400 | 1.50 | 990 | 1 | 330 | 10,30 | RAW | 2.1812E+09 | 4.3608E+09 | 545.09 | 807.55 | 3.5752E+09 | 446.90 | RAW mode requires Observatory waits not counted here. |
6 | 115a | Detector response to Stims -- 24 um | 1200 | 0.33 | 60 | 1 | 20 | 10 | SUR | 1.8958E+07 | 3.7820E+07 | 4.73 | 31.52 | 7.9450E+08 | 99.31 | |
7 | 247a | Detector response to Stims -- 70 and 160 um | 2400 | 0.67 | 120 | 2 | 40 | 10 | SUR | 3.7916E+07 | 7.5640E+07 | 9.46 | 31.52 | 1.5890E+09 | 198.62 | |
8 | 120a | Calibration of Stims against celestial standards 24 um | 1800 | 0.50 | 285 | 1 | 95 | 3 | SUR | 4.4767E+07 | 8.9078E+07 | 11.13 | 49.49 | 1.1917E+09 | 148.97 | |
9 | 350a | Calib of Stims against celestial standards 70 & 160 um | 5400 | 1.50 | 2580 | 2 | 860 | 3 | SUR | 4.0526E+08 | 7.9814E+08 | 99.77 | 147.80 | 3.5752E+09 | 446.90 | |
10 | 125a | Transfer function test | 10800 | 3.00 | 450 | 1 | 150 | 30,10 | SUR | 2.1028E+08 | 4.1984E+08 | 52.48 | 38.87 | 7.1505E+09 | 893.81 | |
11 | 130a | 24 um and 70 um array | 5400 | 1.50 | 1080 | 1 | 360 | 10 | SUR | 3.4125E+08 | 6.8076E+08 | 85.10 | 126.07 | 3.5752E+09 | 446.90 | |
geometries and scan mirror vectors | ||||||||||||||||
12 | 135a | SED of CSE | 1200 | 0.33 | 288 | 1 | 96 | 10 | SUR | 9.0999E+07 | 1.8154E+08 | 22.69 | 151.28 | 7.9450E+08 | 99.31 | |
13 | 140a | SED slit profile | 2400 | 0.67 | 540 | 1 | 180 | 10 | SUR | 1.7062E+08 | 3.4038E+08 | 42.55 | 141.83 | 1.5890E+09 | 198.62 | |
14 | 145a | SED wavelength cal | 900 | 0.25 | 108 | 1 | 36 | 10 | SUR | 3.4125E+07 | 6.8076E+07 | 8.51 | 75.64 | 5.9587E+08 | 74.48 | |
15 | 160a | Anneal frequency | 11880 | 3.30 | 3000 | 1 | 1000 | 10 | SUR | 9.4790E+08 | 1.8910E+09 | 236.38 | 159.18 | 7.8655E+09 | 983.19 | Might be able to piggy back on other tests |
16 | 150a | Determination of radiometric throughput 24 um | 3600 | 1.00 | 702 | 1 | 234 | 10 | SUR | 2.2181E+08 | 4.4250E+08 | 55.31 | 122.92 | 2.3835E+09 | 297.94 | |
17 | 205a | Determination of radiometric throughput 70 & 160 um | 7200 | 2.00 | 1500 | 1 | 500 | 10 | SUR | 4.7395E+08 | 9.4550E+08 | 118.19 | 131.32 | 4.7670E+09 | 595.87 | |
18 | 010a | Detector aliveness check | 3600 | 1.00 | 90 | 3 | 30 | 3 | RAW | 2.9866E+07 | 5.9587E+07 | 7.45 | 16.55 | 2.3835E+09 | 297.94 | |
19 | 155a | Latent images and saturation behavior 24 um | 1200 | 0.33 | 144 | 1 | 48 | 10 | SUR | 4.5499E+07 | 9.0768E+07 | 11.35 | 75.64 | 7.9450E+08 | 99.31 | |
20 | 210a | Latent images and saturation behavior | 2400 | 0.67 | 192 | 1 | 64 | 10 | SUR | 6.0666E+07 | 1.2102E+08 | 15.13 | 50.43 | 1.5890E+09 | 198.62 | |
21 | 220a | Slew state validation | 1800 | 0.50 | 324 | 3 | 108 | 10 | SUR | 1.0237E+08 | 2.0423E+08 | 25.53 | 113.46 | 1.1917E+09 | 148.97 | |
22 | 225a | Instrument stability | 11880 | 3.30 | 3000 | 3 | 1000 | 10 | SUR | 9.4790E+08 | 1.8910E+09 | 236.38 | 159.18 | 7.8655E+09 | 983.19 | |
23 | 230a | Effect of bias and integration times on sensitivity | 5100 | 1.42 | 96 | 1 | 32 | 10 | SUR | 3.0333E+07 | 6.0512E+07 | 7.56 | 11.87 | 3.3766E+09 | 422.08 | |
24 | 235a | 160 um array geometry | 600 | 0.17 | 144 | 1 | 48 | 10 | SUR | 4.5499E+07 | 9.0768E+07 | 11.35 | 151.28 | 3.9725E+08 | 49.66 | |
25 | 240a | Spectral leak checks | 4080 | 1.13 | 720 | 1 | 240 | 10 | SUR | 2.2750E+08 | 4.5384E+08 | 56.73 | 111.24 | 2.7013E+09 | 337.66 | |
26 | 245a | Optimum bias setting | 10800 | 3.00 | 1695 | 1 | 565 | 30,10 | SUR | 5.6961E+08 | 1.1365E+09 | 142.06 | 105.23 | 7.1505E+09 | 893.81 | |
27 | 250a | Cosmic ray limits on integration times | 1320 | 0.37 | 144 | 1 | 48 | 10 | SUR | 4.5499E+07 | 9.0768E+07 | 11.35 | 68.76 | 8.7395E+08 | 109.24 | |
28 | 255a | Radiometry tests | 43200 | 12.00 | 9720 | 3 | 3240 | all | SUR | 3.0712E+09 | 6.1269E+09 | 765.86 | 141.83 | 2.8602E+10 | 3575.23 | 6 x 2hr sessions |
29 | 260a | Read noise and dark current and stability #1 | 32400 | 9.00 | 11700 | 1 | 3900 | all | both | 3.9759E+09 | 7.9331E+09 | 991.64 | 244.85 | 2.1451E+10 | 2681.42 | |
30 | 261a | Read noise and dark current and stability #2 | 32400 | 9.00 | 11700 | 1 | 3900 | all | both | 3.9759E+09 | 7.9331E+09 | 991.64 | 244.85 | 2.1451E+10 | 2681.42 | |
31 | 262a | Read noise and dark current and stability #3 | 32400 | 9.00 | 11700 | 1 | 3900 | all | both | 3.9759E+09 | 7.9331E+09 | 991.64 | 244.85 | 2.1451E+10 | 2681.42 | |
32 | 265a | Scan to determine confusion limits | 7200 | 2.00 | 1680 | 3 | 560 | 10 | SUR | 5.3083E+08 | 1.0590E+09 | 132.37 | 147.08 | 4.7670E+09 | 595.87 | |
33 | 270a | Total power at Ecliptic Pole | 2400 | 0.67 | 180 | 1 | 60 | 10 | RAW | 1.9843E+08 | 3.9658E+08 | 49.57 | 165.24 | 1.5890E+09 | 198.62 | |
34 | 275a | Photometry of a CSE | 2700 | 0.75 | 288 | 1 | 96 | 10,30 | SUR | 1.1279E+08 | 2.2512E+08 | 28.14 | 83.38 | 1.7876E+09 | 223.45 | Can be an ERO |
35 | 280a | Super Res of SVS-13 | 3600 | 1.00 | 2160 | 1 | 720 | 3 | SUR | 3.3929E+08 | 6.7512E+08 | 84.39 | 187.53 | 2.3835E+09 | 297.94 | Can be an ERO |
36 | 285a | Scan map of a PN or SNR | 9000 | 2.50 | 2520 | 3 | 840 | 10 | SUR | 7.9624E+08 | 1.5884E+09 | 198.56 | 176.49 | 5.9587E+09 | 744.84 | Can be an ERO |
37 | 290a | Scan map of HH 7-11 region | 10800 | 3.00 | 8640 | 3 | 2880 | 3 | SUR | 1.3571E+09 | 2.7005E+09 | 337.56 | 250.04 | 7.1505E+09 | 893.81 | Can be an ERO |
38 | 295a | Scan map of M31 or M33 | 30600 | 8.50 | 20634 | 3 | 6878 | 4 | SUR | 3.7095E+09 | 7.3860E+09 | 923.25 | 241.37 | 2.0260E+10 | 2532.46 | Can be an ERO |
39 | 300a | SED AOT validation | 5400 | 1.50 | 765 | 1 | 255 | all | SUR | 2.4172E+08 | 4.8221E+08 | 60.28 | 89.30 | 3.5752E+09 | 446.90 | |
40 | 305a | Pipeline quality flatfields | 12600 | 3.50 | 3792 | 3 | 1264 | 10 | SUR | 1.1982E+09 | 2.3902E+09 | 298.78 | 189.70 | 8.3422E+09 | 1042.78 | |
41 | 310a | Off-axis glints | 54000 | 15.00 | 16680 | 1 | 5560 | 4 | SUR | 2.9987E+09 | 5.9706E+09 | 746.33 | 110.57 | 3.5752E+10 | 4469.04 | |
42 | 315a | Behavior as a function of sky background | 10800 | 3.00 | 1566 | 3 | 522 | 10 | SUR | 4.9481E+08 | 9.8711E+08 | 123.39 | 91.40 | 7.1505E+09 | 893.81 | |
43 | 320a | Phot/SR AOT validation | 7200 | 2.00 | 1620 | 1 | 540 | all | SUR | 5.1187E+08 | 1.0211E+09 | 127.64 | 141.83 | 4.7670E+09 | 595.87 | |
44 | 325a | Scan AOT validation | 34200 | 9.50 | 7776 | 3 | 2592 | all | SUR | 2.4570E+09 | 4.9015E+09 | 612.69 | 143.32 | 2.2643E+10 | 2830.39 | |
45 | 330a | Total power AOT validation | 2520 | 0.70 | 1050 | 1 | 350 | all | RAW | 4.2029E+08 | 8.3890E+08 | 104.86 | 332.90 | 1.6684E+09 | 208.56 | |
46 | 335a | Point spread functions | 12600 | 3.50 | 3672 | 1 | 1224 | 10 | SUR | 1.1602E+09 | 2.3146E+09 | 289.32 | 183.70 | 8.3422E+09 | 1042.78 | |
47 | 340a | Ultimate scattered light levels | 36000 | 10.00 | 7380 | 1 | 2460 | 10,30 | SUR | 2.6996E+09 | 5.3873E+09 | 673.41 | 149.65 | 2.3835E+10 | 2979.36 | |
48 | 045a | Bias level commanding | --- | --- | 0 | --- | --- | --- | 0.0000E+00 | 0.0000E+00 | 0.00 | Can be done with sensitivity task | ||||
49 | 015a | CE state validation | 3600 | 1.00 | 0 | --- | --- | none | RT telemetry | 0.00 | 0.00 | 2.3835E+09 | 297.94 | |||
50 | 020a | Command and data paths | 3600 | 1.00 | 0 | --- | --- | none | RT telemetry | 0.00 | 0.00 | 2.3835E+09 | 297.94 | |||
51 | 005a | Electronics live tests | 3600 | 1.00 | 0 | --- | --- | none | RT telemetry | 0.00 | 0.00 | 2.3835E+09 | 297.94 | |||
52 | 035a | CE EEPROM test | 900 | 0.25 | 0 | --- | --- | none | RT telemetry | 0.00 | 0.00 | 5.9587E+08 | 74.48 | |||
53 | 025a | Scan mirror operational test | 60 | 0.02 | 0 | --- | --- | none | RT telemetry | 0.00 | 0.00 | 3.9725E+07 | 4.97 | |||
54 | 030a | Heaters, temp sensors | 300 | 0.08 | 0 | --- | --- | none | RT telemetry | 0.00 | 0.00 | 1.9862E+08 | 24.83 | |||
55 | 040a | Engineering and data acquistion | 300 | 0.08 | 48 | 3 | 16 | 10 | RAW | 5.2915E+07 | 1.0575E+08 | 13.22 | 352.51 | 1.9862E+08 | 24.83 | |
56 | 050a | Scattered backgrd monitor #1 | 3600 | 1.00 | 120 | 3 | 40 | 3 | BOTH | 1.9480E+07 | 3.8768E+07 | 4.85 | 10.77 | 2.3835E+09 | 297.94 | |
57 | 055a | Scattered backgrd monitor #2 | 3600 | 1.00 | 120 | 3 | 40 | 3 | BOTH | 1.9480E+07 | 3.8768E+07 | 4.85 | 10.77 | 2.3835E+09 | 297.94 | |
58 | 060a | Scattered backgrd monitor #3 | 3600 | 1.00 | 120 | 3 | 40 | 3 | BOTH | 1.9480E+07 | 3.8768E+07 | 4.85 | 10.77 | 2.3835E+09 | 297.94 | |
59 | 065a | Scattered backgrd monitor #4 | 3600 | 1.00 | 120 | 3 | 40 | 3 | BOTH | 1.9480E+07 | 3.8768E+07 | 4.85 | 10.77 | 2.3835E+09 | 297.94 | |
60 | 070a | Scattered backgrd monitor #5 | 3600 | 1.00 | 120 | 3 | 40 | 3,10 | BOTH | 2.4242E+07 | 4.8292E+07 | 6.04 | 13.41 | 2.3835E+09 | 297.94 | |
61 | Misc new or forgotten tasks | 21600 | 6.00 | 1.4301E+10 | 1787.62 | Placeholder | ||||||||||
(eg 4 sec darks, scan speed optimization) | ||||||||||||||||
Totals: | 1.4490E+05 | 4.2145E+10 | 8.4050E+10 | 10506.27 | 3.6066E+11 | 45082.68 | ||||||||||
Prime DCEs = | 7.4867E+04 | |||||||||||||||
Notes: | These data volumes are estimates only. | 16 bit quantization used. | DG = Data Group | Header
size per DG = 4800 bits -- this is approximate because data is grouped in a way that is
not always equal to a DG. Header goes with the data group Compression factor is applied to pixel data only, not header, and is assumed to be 0.5. Max data is for highest data collection rate for total time estimated for task. It is an upper limit of data for the task Maximum data rate estimate = Raw mode and 3 second exposures. H = header volume C = compression factor t(exp) = exposure time (seconds) |
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Data rates used: | = (128x128x2 + 32x32x8 + 20x2x8)x16xCxt(exp) + H | |||||||||||||||
Raw data for 1 DG | =660,480xCxt(exp) + 4800 bits per DG | |||||||||||||||
= [128x128x2 + (32x32x8 + 20x2x8)xt(exp)]x16xC + H | ||||||||||||||||
SUR data for 1 DG | = [524,288 + 136,192xt(exp)]xC + 4800 bits per DG | |||||||||||||||
Si:As array is sampled at 2 Hz; the Ge:Ga arrays are sampled at 8 Hz maximum (co-addition of samples is possible and will reduce data rate) | ||||||||||||||||
Prepared by: | ||||||||||||||||
William B. Latter | ||||||||||||||||
SSC/MIPS Instrument Scientist |
Last Updated on 11/16/99
By Marcia Rieke
Email: mrieke@as.arizona.edu