| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 36.36 | 189.07 | 20.07 | 104.36 | 17.76 | 223.72 | 20.71 | 310.23 | 0.4432 | -616.2 | -361.0 | |
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back to the solar disc SDO HMI 2011-11-28 04:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.05 | 0.00 | 1.14 | 15.49 | 226.15 | 23.14 | 303.13 | 0.4541 | 870.0 | 509.5 | |
| 0.34 | 3.17 | 0.19 | 1.77 | 16.88 | 225.91 | 22.91 | 305.98 | 0.4622 | 864.8 | 747.0 | |
| 0.00 | 0.51 | 0.00 | 0.28 | 15.68 | 225.43 | 22.43 | 304.27 | 0.4464 | 470.0 | 406.5 | |
| 0.00 | 0.60 | 0.00 | 0.33 | 15.35 | 225.36 | 22.36 | 303.69 | 0.4428 | 679.0 | 551.9 | |
| 0.00 | 1.20 | 0.00 | 0.67 | 18.03 | 224.42 | 21.42 | 309.82 | 0.4540 | 62.0 | 34.1 | |
| 11.04 | 168.45 | 6.11 | 93.03 | 17.66 | 224.21 | 21.20 | 309.42 | 0.4480 | -1104.4 | -443.4 | |
| 0.94 | -6.00 | 0.52 | -6.00 | 17.57 | 223.90 | 20.89 | 309.65 | 0.4434 | -1115.3 | 999999 | |
| 1.20 | -6.00 | 0.66 | -6.00 | 18.19 | 223.81 | 20.80 | 310.88 | 0.4481 | -517.7 | 999999 | |
| 19.93 | -6.00 | 11.00 | -6.00 | 17.97 | 223.48 | 20.48 | 310.92 | 0.4422 | -1203.5 | 999999 | |
| 1.20 | 5.22 | 0.65 | 2.84 | 15.80 | 222.71 | 19.71 | 307.81 | 0.4125 | 613.6 | 125.5 | |
| 0.00 | 1.28 | 0.00 | 0.70 | 16.41 | 222.51 | 19.51 | 309.29 | 0.4157 | 557.0 | 488.2 | |
| 0.00 | 2.05 | 0.00 | 1.11 | 15.34 | 222.21 | 19.21 | 307.57 | 0.4020 | 1090.0 | 850.3 | |
| 1.71 | 1.97 | 0.94 | 1.08 | 19.82 | 221.58 | 18.58 | 316.78 | 0.4395 | -707.5 | -725.2 | |
| 0.00 | 1.20 | 0.00 | 0.66 | 19.29 | 221.39 | 18.38 | 316.18 | 0.4317 | -725.0 | -538.0 | |
| 0.00 | 1.37 | 0.00 | 0.75 | 19.69 | 221.43 | 18.43 | 316.79 | 0.4366 | -769.0 | -613.3 | |
| 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. | |