SOHO MDI 2000-04-03 01:35:33 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 79 | 457 | 57 | 334 | -14.15 | 269.20 | 47.40 | 256.60 | 0.7354 | 182.3 | 34.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 2 | 0 | 2 | -14.27 | 276.16 | 54.35 | 257.03 | 0.8104 | -414.0 | -324.2 | |
| 0 | 4 | 0 | 3 | -14.28 | 274.73 | 52.93 | 256.94 | 0.7961 | -568.0 | -457.8 | |
| 18 | 189 | 14 | 144 | -13.12 | 272.05 | 50.24 | 258.26 | 0.7670 | -1036.9 | -470.0 | |
| 4 | -3 | 3 | -3 | -13.79 | 271.12 | 49.31 | 257.31 | 0.7572 | -962.1 | 999999 | |
| 0 | 3 | 0 | 3 | -14.37 | 270.92 | 49.11 | 256.54 | 0.7554 | -563.0 | -504.8 | |
| 3 | -3 | 2 | -3 | -13.40 | 270.58 | 48.78 | 257.79 | 0.7509 | -807.3 | 999999 | |
| 4 | -3 | 3 | -3 | -13.87 | 270.65 | 48.85 | 257.17 | 0.7520 | -1018.4 | 999999 | |
| 2 | 8 | 2 | 6 | -13.49 | 269.52 | 47.71 | 257.59 | 0.7389 | -939.0 | -807.6 | |
| 2 | 46 | 2 | 33 | -14.17 | 268.99 | 47.18 | 256.62 | 0.7334 | 559.9 | -95.8 | |
| 3 | -9 | 2 | -9 | -14.03 | 268.77 | 46.97 | 256.79 | 0.7308 | -191.5 | 999999 | |
| 0 | 4 | 0 | 3 | -15.53 | 267.79 | 45.98 | 254.60 | 0.7210 | 329.0 | 373.8 | |
| 16 | 201 | 11 | 140 | -14.68 | 267.03 | 45.23 | 255.68 | 0.7111 | 1000.6 | 639.3 | |
| 15 | -12 | 10 | -12 | -15.07 | 266.62 | 44.82 | 255.08 | 0.7067 | 1298.3 | 999999 | |
| 7 | -12 | 5 | -12 | -15.23 | 266.04 | 44.24 | 254.76 | 0.7000 | 1283.4 | 999999 | |
| 5 | -12 | 3 | -12 | -15.34 | 265.68 | 43.87 | 254.55 | 0.6958 | 1196.4 | 999999 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |