| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 40.96 | 80.54 | 21.39 | 42.27 | -23.30 | 179.97 | -10.81 | 148.46 | 0.3295 | -143.1 | -546.3 | |
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back to the solar disc SDO HMI 2011-03-01 13:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.99 | 22.42 | 8.79 | 11.61 | -21.74 | 181.87 | -8.91 | 150.32 | 0.2918 | 1021.5 | 521.7 | |
| 5.61 | 5.78 | 2.91 | 3.00 | -22.19 | 181.36 | -9.42 | 149.77 | 0.3024 | 894.6 | 718.0 | |
| 0.00 | 1.21 | 0.00 | 0.63 | -22.33 | 180.79 | -9.99 | 148.59 | 0.3092 | 737.0 | 478.3 | |
| 0.00 | 2.50 | 0.00 | 1.32 | -24.79 | 179.97 | -10.81 | 150.76 | 0.3501 | -671.0 | -687.0 | |
| 0.69 | 2.76 | 0.36 | 1.45 | -23.70 | 179.87 | -10.92 | 148.78 | 0.3360 | -975.8 | -864.5 | |
| 1.55 | 3.28 | 0.81 | 1.72 | -23.30 | 179.87 | -10.91 | 148.09 | 0.3305 | -967.5 | -893.2 | |
| 1.55 | 1.98 | 0.81 | 1.04 | -22.65 | 179.82 | -10.96 | 146.83 | 0.3221 | -729.0 | -736.6 | |
| 0.00 | 1.03 | 0.00 | 0.55 | -24.69 | 179.31 | -11.47 | 149.17 | 0.3540 | -897.0 | -795.2 | |
| 0.00 | 3.62 | 0.00 | 1.92 | -24.78 | 179.14 | -11.64 | 148.94 | 0.3567 | -957.0 | -723.5 | |
| 0.00 | 1.98 | 0.00 | 1.05 | -24.93 | 178.89 | -11.89 | 148.65 | 0.3608 | -773.0 | -644.2 | |
| 11.12 | 30.79 | 5.88 | 16.29 | -24.15 | 178.83 | -11.95 | 147.26 | 0.3509 | -1086.1 | -775.2 | |
| 0.00 | 1.12 | 0.00 | 0.59 | -23.49 | 178.53 | -12.25 | 145.48 | 0.3449 | -955.0 | -762.4 | |
| 0.00 | 1.21 | 0.00 | 0.64 | -23.64 | 178.48 | -12.30 | 145.65 | 0.3474 | -969.0 | -749.9 | |
| 3.45 | -11.00 | 1.83 | -11.00 | -24.23 | 178.32 | -12.46 | 146.34 | 0.3565 | -834.6 | 999999 | |
| 0.00 | 0.86 | 0.00 | 0.46 | -23.69 | 178.14 | -12.64 | 145.04 | 0.3512 | -831.0 | -696.1 | |
| 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. | |