SDO HMI 2011-11-11 19:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 43.46 | 279.88 | 44.81 | 291.31 | -14.74 | 117.82 | 58.95 | 250.78 | 0.8731 | 640.3 | 197.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.20 | 105.85 | 1.50 | 131.25 | -14.67 | 123.64 | 64.77 | 252.47 | 0.9195 | 295.4 | 145.6 | |
| 2.84 | -1.00 | 3.52 | -1.00 | -14.88 | 123.46 | 64.60 | 252.22 | 0.9186 | 373.8 | 999999 | |
| 1.64 | -1.00 | 2.00 | -1.00 | -14.73 | 123.10 | 64.23 | 252.30 | 0.9160 | 736.9 | 999999 | |
| 0.00 | 1.55 | 0.00 | 1.87 | -14.35 | 122.82 | 63.95 | 252.66 | 0.9136 | 419.0 | 415.8 | |
| 4.82 | -1.00 | 5.97 | -1.00 | -15.40 | 123.33 | 64.47 | 251.63 | 0.9184 | 381.6 | 999999 | |
| 5.25 | -1.00 | 6.41 | -1.00 | -15.10 | 123.02 | 64.15 | 251.89 | 0.9159 | 735.4 | 999999 | |
| 11.45 | 69.54 | 12.60 | 76.64 | -11.08 | 120.82 | 61.95 | 255.86 | 0.8951 | 746.9 | 205.0 | |
| 0.34 | 1.64 | 0.35 | 1.67 | -14.70 | 117.75 | 58.88 | 251.19 | 0.8768 | -310.8 | -219.1 | |
| 0.00 | 1.46 | 0.00 | 1.37 | -14.42 | 114.60 | 55.74 | 250.73 | 0.8500 | -446.0 | -336.8 | |
| 14.46 | 96.65 | 11.32 | 76.02 | -17.68 | 105.78 | 46.91 | 243.93 | 0.7769 | 967.9 | 288.9 | |
| 0.00 | 0.95 | 0.00 | 0.75 | -18.79 | 105.85 | 46.99 | 242.62 | 0.7819 | 497.0 | 358.1 | |
| 1.03 | -10.00 | 0.81 | -10.00 | -18.30 | 105.54 | 46.67 | 243.08 | 0.7769 | 577.8 | 999999 | |
| 0.43 | 2.24 | 0.33 | 1.74 | -19.41 | 104.61 | 45.75 | 241.33 | 0.7723 | 588.2 | 403.4 | |
| 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. | |