SDO HMI 2011-11-21 13:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 60.09 | 343.97 | 58.97 | 337.26 | 14.65 | 231.34 | -59.01 | 74.21 | 0.8623 | -275.1 | -132.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.40 | 209.15 | 18.54 | 191.74 | 14.31 | 233.93 | -56.42 | 74.28 | 0.8408 | -986.8 | -260.9 | |
| 0.00 | 1.20 | 0.00 | 1.07 | 12.11 | 234.54 | -55.81 | 76.82 | 0.8328 | 389.0 | 288.5 | |
| 12.09 | -1.00 | 11.11 | -1.00 | 14.63 | 233.52 | -56.82 | 73.95 | 0.8448 | -586.0 | 999999 | |
| 1.20 | -1.00 | 1.11 | -1.00 | 14.23 | 233.40 | -56.95 | 74.44 | 0.8455 | -415.9 | 999999 | |
| 1.71 | -1.00 | 1.60 | -1.00 | 14.40 | 232.99 | -57.35 | 74.30 | 0.8493 | -175.0 | 999999 | |
| 7.97 | 41.49 | 7.29 | 37.94 | 12.51 | 233.53 | -56.82 | 76.47 | 0.8426 | -582.7 | -316.9 | |
| 0.00 | 6.17 | 0.00 | 6.83 | 16.35 | 227.45 | -62.90 | 72.76 | 0.8963 | 117.0 | 97.4 | |
| 0.00 | 1.54 | 0.00 | 1.69 | 15.49 | 227.72 | -62.62 | 73.68 | 0.8936 | 447.0 | 387.1 | |
| 0.00 | 1.11 | 0.00 | 1.28 | 17.36 | 226.48 | -63.87 | 71.74 | 0.9041 | -369.0 | -289.2 | |
| 0.00 | 2.23 | 0.00 | 2.58 | 17.64 | 226.30 | -64.05 | 71.46 | 0.9056 | -343.0 | -281.3 | |
| 0.00 | 0.86 | 0.00 | 0.95 | 15.70 | 227.34 | -63.01 | 73.49 | 0.8966 | 437.0 | 357.9 | |
| 14.49 | 66.51 | 16.75 | 77.23 | 15.75 | 226.12 | -64.23 | 73.55 | 0.9055 | 618.9 | 202.4 | |
| 0.00 | 1.71 | 0.00 | 2.14 | 18.35 | 224.31 | -66.04 | 70.90 | 0.9196 | -464.0 | -434.2 | |
| 2.23 | 12.00 | 2.57 | 13.81 | 15.26 | 226.19 | -64.16 | 74.09 | 0.9047 | 415.7 | 202.6 | |
| 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. | |