SDO HMI 2011-12-14 18:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 73.43 | 398.68 | 38.46 | 208.64 | -18.18 | 352.18 | 7.70 | 203.11 | 0.3263 | 1085.2 | 442.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.45 | 0.00 | 0.77 | -18.75 | 355.31 | 10.82 | 209.98 | 0.3574 | -769.0 | -533.4 | |
| 0.00 | 1.11 | 0.00 | 0.59 | -19.28 | 354.23 | 9.75 | 206.75 | 0.3565 | -806.0 | -599.1 | |
| 0.00 | 1.79 | 0.00 | 0.94 | -18.78 | 353.00 | 8.52 | 204.43 | 0.3406 | -77.0 | -23.8 | |
| 50.11 | 358.42 | 26.20 | 187.52 | -17.82 | 352.36 | 7.88 | 204.02 | 0.3219 | 1461.2 | 442.9 | |
| 16.25 | -4.00 | 8.55 | -4.00 | -19.03 | 352.07 | 7.58 | 201.75 | 0.3383 | 1028.5 | 999999 | |
| 0.34 | -4.00 | 0.18 | -4.00 | -17.82 | 351.80 | 7.31 | 202.48 | 0.3183 | 1083.5 | 999999 | |
| 0.00 | 1.79 | 0.00 | 0.92 | -15.22 | 351.45 | 6.97 | 205.18 | 0.2764 | -853.0 | -694.8 | |
| 3.66 | 15.82 | 1.92 | 8.29 | -18.66 | 351.46 | 6.97 | 200.56 | 0.3290 | 1195.1 | 679.8 | |
| 0.00 | 1.36 | 0.00 | 0.72 | -19.19 | 351.48 | 6.99 | 200.03 | 0.3372 | 804.0 | 617.4 | |
| 1.62 | -8.00 | 0.85 | -8.00 | -18.81 | 351.37 | 6.88 | 200.15 | 0.3309 | 941.1 | 999999 | |
| 1.45 | 12.17 | 0.76 | 6.40 | -19.56 | 350.96 | 6.47 | 198.28 | 0.3402 | 926.0 | 858.8 | |
| 0.00 | 2.64 | 0.00 | 1.36 | -15.80 | 350.70 | 6.22 | 201.93 | 0.2802 | -680.0 | -438.2 | |
| 0.00 | 1.11 | 0.00 | 0.58 | -19.56 | 350.11 | 5.62 | 196.02 | 0.3361 | 958.0 | 775.2 | |
| 0.00 | 1.02 | 0.00 | 0.55 | -22.90 | 346.84 | 2.35 | 185.74 | 0.3797 | 771.0 | 561.9 | |
| 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. | |