SDO HMI 2011-11-13 09:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 56.10 | 378.88 | 31.74 | 214.11 | 16.15 | 64.00 | 26.00 | 298.87 | 0.4829 | -893.4 | -352.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.95 | 362.62 | 0.54 | 205.18 | 16.48 | 64.81 | 26.81 | 298.76 | 0.4954 | -442.1 | -388.0 | |
| 53.95 | -1.00 | 30.52 | -1.00 | 16.06 | 64.23 | 26.23 | 298.45 | 0.4851 | -1332.1 | 999999 | |
| 1.20 | -1.00 | 0.68 | -1.00 | 15.52 | 63.88 | 25.88 | 297.70 | 0.4770 | -1070.6 | 999999 | |
| 0.00 | 1.03 | 0.00 | 0.58 | 15.73 | 62.95 | 24.95 | 298.87 | 0.4657 | -788.0 | -615.8 | |
| 0.00 | 1.46 | 0.00 | 0.81 | 14.16 | 62.42 | 24.42 | 296.17 | 0.4486 | -840.0 | -688.8 | |
| 0.00 | 0.95 | 0.00 | 0.53 | 17.03 | 62.07 | 24.07 | 302.20 | 0.4629 | -785.0 | -597.2 | |
| 0.00 | 2.32 | 0.00 | 1.28 | 18.03 | 59.64 | 21.64 | 306.73 | 0.4394 | 621.0 | 575.4 | |
| 0.00 | 1.89 | 0.00 | 1.05 | 18.64 | 59.68 | 21.69 | 307.85 | 0.4453 | 836.0 | 685.8 | |
| 0.00 | 0.86 | 0.00 | 0.47 | 18.99 | 57.92 | 19.92 | 310.71 | 0.4268 | 693.0 | 479.7 | |
| 0.00 | 1.12 | 0.00 | 0.61 | 17.94 | 57.76 | 19.76 | 308.91 | 0.4151 | 864.0 | 690.2 | |
| 0.00 | 3.10 | 0.00 | 1.68 | 18.39 | 56.78 | 18.79 | 311.13 | 0.4075 | 739.0 | 594.8 | |
| 0.00 | 0.69 | 0.00 | 0.38 | 22.00 | 56.20 | 18.20 | 318.47 | 0.4386 | 605.0 | 522.5 | |
| 0.00 | 1.38 | 0.00 | 0.75 | 20.98 | 55.73 | 17.73 | 317.45 | 0.4224 | 751.0 | 628.2 | |
| 0.00 | 1.46 | 0.00 | 0.79 | 20.53 | 54.61 | 16.62 | 318.44 | 0.4054 | 743.0 | 626.5 | |
| 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. | |