SDO HMI 2011-12-16 02:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 49.28 | 332.19 | 28.24 | 190.41 | -18.25 | 352.16 | 25.26 | 233.66 | 0.5052 | 974.6 | 407.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.28 | 0.00 | 0.76 | -19.99 | 355.76 | 28.85 | 234.17 | 0.5616 | -772.0 | -622.8 | |
| 0.00 | 1.19 | 0.00 | 0.70 | -19.19 | 354.25 | 27.35 | 234.10 | 0.5378 | -820.0 | -702.3 | |
| 0.00 | 1.11 | 0.00 | 0.62 | -15.15 | 351.85 | 24.94 | 238.85 | 0.4776 | -639.0 | -458.2 | |
| 41.62 | 308.52 | 23.84 | 176.87 | -18.06 | 352.22 | 25.32 | 234.04 | 0.5044 | 1315.3 | 414.8 | |
| 4.34 | -4.00 | 2.50 | -4.00 | -19.08 | 352.35 | 25.45 | 232.46 | 0.5141 | 949.9 | 999999 | |
| 1.28 | 1.79 | 0.73 | 1.02 | -19.58 | 351.12 | 24.22 | 230.36 | 0.5039 | 776.3 | 756.3 | |
| 2.04 | 2.81 | 1.17 | 1.60 | -19.21 | 351.03 | 24.12 | 230.87 | 0.4996 | 912.8 | 708.0 | |
| 0.00 | 1.19 | 0.00 | 0.68 | -19.68 | 350.90 | 23.99 | 229.96 | 0.5022 | 797.0 | 698.7 | |
| 0.00 | 3.66 | 0.00 | 2.10 | -19.96 | 350.84 | 23.93 | 229.44 | 0.5040 | 863.0 | 683.4 | |
| 0.00 | 1.28 | 0.00 | 0.73 | -19.27 | 350.70 | 23.79 | 230.40 | 0.4963 | 985.0 | 886.2 | |
| 0.00 | 1.87 | 0.00 | 1.08 | -21.62 | 350.95 | 24.04 | 226.96 | 0.5203 | 585.0 | 481.8 | |
| 0.00 | 2.04 | 0.00 | 1.16 | -19.62 | 350.41 | 23.50 | 229.51 | 0.4960 | 890.0 | 719.5 | |
| 0.00 | 3.15 | 0.00 | 1.80 | -19.96 | 350.43 | 23.52 | 228.98 | 0.4993 | 925.0 | 722.2 | |
| 0.00 | 2.30 | 0.00 | 1.29 | -17.76 | 349.66 | 22.76 | 231.81 | 0.4707 | -912.0 | -609.5 | |
| 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. | |