| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 45.17 | 271.95 | 33.83 | 204.33 | 17.50 | 222.92 | -47.08 | 68.24 | 0.7543 | -550.7 | -215.6 | |
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back to the solar disc SDO HMI 2011-11-23 02:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.40 | 242.90 | 24.11 | 181.69 | 17.43 | 223.43 | -46.57 | 68.19 | 0.7487 | -1093.8 | -288.6 | |
| 9.51 | -1.00 | 7.22 | -1.00 | 17.96 | 222.51 | -47.49 | 67.77 | 0.7599 | -586.1 | 999999 | |
| 0.43 | -1.00 | 0.33 | -1.00 | 18.78 | 221.97 | -48.03 | 66.88 | 0.7677 | -262.4 | 999999 | |
| 0.00 | 0.34 | 0.00 | 0.26 | 17.76 | 221.97 | -48.02 | 68.18 | 0.7650 | -156.0 | -188.5 | |
| 0.00 | 0.69 | 0.00 | 0.54 | 19.78 | 220.71 | -49.29 | 65.99 | 0.7831 | 554.0 | 537.2 | |
| 0.00 | 2.49 | 0.00 | 1.89 | 16.13 | 222.02 | -47.98 | 70.26 | 0.7605 | -437.0 | -248.6 | |
| 0.86 | 12.94 | 0.65 | 9.92 | 16.53 | 221.84 | -48.16 | 69.80 | 0.7633 | -256.6 | 294.0 | |
| 0.00 | 2.23 | 0.00 | 1.69 | 15.79 | 221.99 | -48.01 | 70.71 | 0.7601 | 741.0 | 568.3 | |
| 1.97 | -7.00 | 1.52 | -7.00 | 16.45 | 221.45 | -48.55 | 69.99 | 0.7674 | 407.7 | 999999 | |
| 0.00 | 0.94 | 0.00 | 0.75 | 18.71 | 220.04 | -49.96 | 67.52 | 0.7871 | 364.0 | 387.0 | |
| 0.00 | 0.94 | 0.00 | 0.73 | 16.16 | 220.79 | -49.21 | 70.53 | 0.7736 | 697.0 | 588.9 | |
| 0.00 | 1.37 | 0.00 | 1.08 | 16.40 | 220.28 | -49.72 | 70.36 | 0.7794 | 678.0 | 598.4 | |
| 0.00 | 1.54 | 0.00 | 1.25 | 17.54 | 219.08 | -50.92 | 69.22 | 0.7940 | 632.0 | 546.4 | |
| 0.00 | 1.20 | 0.00 | 0.97 | 17.17 | 219.07 | -50.92 | 69.68 | 0.7933 | 545.0 | 473.8 | |
| 0.00 | 1.46 | 0.00 | 1.17 | 16.74 | 219.24 | -50.76 | 70.17 | 0.7908 | 432.0 | 339.2 | |
| 0.00 | 1.71 | 0.00 | 1.41 | 17.77 | 218.59 | -51.41 | 69.04 | 0.7993 | 281.0 | 221.1 | |
| 0.00 | 1.20 | 0.00 | 0.98 | 17.53 | 218.68 | -51.31 | 69.32 | 0.7979 | 380.0 | 297.8 | |
| 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. | |