SOHO MDI 2002-08-07 09:35:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41 | 274 | 96 | 539 | -8.19 | 150.21 | 74.26 | 259.80 | 0.9667 | -175.2 | -87.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4 | 87 | 12 | 230 | -8.03 | 154.28 | 78.33 | 260.60 | 0.9838 | 28.8 | 76.1 | |
| 0 | 11 | 0 | 28 | -6.47 | 153.34 | 77.39 | 262.04 | 0.9800 | -444.0 | -344.1 | |
| 5 | -1 | 14 | -1 | -7.61 | 153.81 | 77.86 | 260.95 | 0.9821 | -247.2 | 999999 | |
| 14 | -1 | 38 | -1 | -8.46 | 154.19 | 78.24 | 260.15 | 0.9837 | -133.4 | 999999 | |
| 0 | 2 | 0 | 3 | -7.14 | 151.26 | 75.31 | 261.07 | 0.9726 | -247.0 | -235.8 | |
| 2 | 56 | 4 | 107 | -6.96 | 149.95 | 74.00 | 261.06 | 0.9671 | -534.2 | -376.6 | |
| 9 | -6 | 17 | -6 | -7.43 | 149.87 | 73.92 | 260.56 | 0.9670 | -481.7 | 999999 | |
| 0 | 5 | 0 | 8 | -9.35 | 148.03 | 72.08 | 258.31 | 0.9600 | 102.0 | 32.4 | |
| 0 | 4 | 0 | 6 | -6.21 | 145.89 | 69.94 | 261.20 | 0.9464 | -220.0 | -151.1 | |
| 3 | 38 | 5 | 55 | -8.50 | 144.63 | 68.68 | 258.59 | 0.9414 | 74.2 | -119.6 | |
| 0 | 6 | 0 | 8 | -6.97 | 143.88 | 67.93 | 260.07 | 0.9354 | 112.0 | 159.3 | |
| 2 | 40 | 3 | 60 | -10.36 | 144.88 | 68.93 | 256.69 | 0.9447 | -162.8 | -243.3 | |
| 2 | 17 | 3 | 23 | -7.58 | 143.54 | 67.59 | 259.36 | 0.9340 | 528.1 | 337.3 | |
| 0 | 4 | 0 | 6 | -10.41 | 143.80 | 67.84 | 256.43 | 0.9386 | -393.0 | -452.3 | |
| 0 | 2 | 0 | 2 | -9.22 | 142.06 | 66.10 | 257.35 | 0.9266 | 354.0 | 215.6 | |
| 0 | 2 | 0 | 3 | -9.41 | 141.53 | 65.58 | 257.04 | 0.9234 | 474.0 | 333.4 | |
| 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. | |