SOHO MDI 2000-10-27 17:35:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 94 | 568 | 85 | 507 | -22.78 | 307.12 | -50.26 | 121.52 | 0.8334 | -225.6 | -102.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14 | 67 | 12 | 57 | -23.94 | 309.99 | -47.40 | 124.09 | 0.8146 | -636.8 | -351.6 | |
| 16 | 91 | 14 | 80 | -23.61 | 308.30 | -49.08 | 122.94 | 0.8272 | -754.1 | -151.0 | |
| 24 | 156 | 20 | 134 | -22.05 | 308.49 | -48.89 | 121.28 | 0.8194 | -86.2 | -282.8 | |
| 0 | 7 | 0 | 6 | -20.30 | 308.01 | -49.37 | 119.09 | 0.8168 | 561.0 | 479.3 | |
| 0 | 5 | 0 | 5 | -21.24 | 307.20 | -50.18 | 119.81 | 0.8273 | 502.0 | 246.4 | |
| 0 | 8 | 0 | 7 | -22.30 | 306.68 | -50.70 | 120.77 | 0.8355 | -958.0 | -611.1 | |
| 0 | 2 | 0 | 2 | -21.61 | 306.83 | -50.55 | 120.06 | 0.8318 | 200.0 | 184.1 | |
| 7 | 51 | 7 | 45 | -20.81 | 306.68 | -50.70 | 119.11 | 0.8301 | 1034.6 | 667.0 | |
| 10 | 142 | 10 | 135 | -24.01 | 305.01 | -52.37 | 121.96 | 0.8548 | -599.1 | -27.0 | |
| 0 | 5 | 0 | 4 | -20.20 | 306.90 | -50.49 | 118.51 | 0.8262 | 779.0 | 791.8 | |
| 4 | -9 | 4 | -9 | -23.58 | 304.98 | -52.40 | 121.48 | 0.8536 | -909.6 | 999999 | |
| 0 | 4 | 0 | 3 | -22.41 | 305.62 | -51.76 | 120.46 | 0.8445 | -146.0 | -288.7 | |
| 8 | -8 | 7 | -8 | -20.63 | 306.24 | -51.14 | 118.72 | 0.8332 | 1064.9 | 999999 | |
| 11 | -9 | 11 | -9 | -23.65 | 304.52 | -52.86 | 121.37 | 0.8574 | -419.0 | 999999 | |
| 0 | 4 | 0 | 4 | -19.99 | 306.34 | -51.04 | 118.04 | 0.8302 | 425.0 | 461.8 | |
| 0 | 6 | 0 | 5 | -21.43 | 305.65 | -51.73 | 119.38 | 0.8409 | -303.0 | -109.0 | |
| 0 | 9 | 0 | 9 | -21.79 | 303.53 | -53.85 | 118.96 | 0.8591 | -1112.0 | -699.4 | |
| 0 | 11 | 0 | 11 | -21.76 | 302.69 | -54.70 | 118.62 | 0.8655 | -747.0 | -508.3 | |
| 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. | |