SDO HMI 2014-12-01 15:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.54 | 128.75 | 33.12 | 227.82 | -13.90 | 165.17 | 73.05 | 255.24 | 0.9612 | 347.1 | 126.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.94 | 18.11 | 2.01 | 38.51 | -12.44 | 168.19 | 76.07 | 257.00 | 0.9738 | 187.0 | 22.3 | |
| 1.79 | -1.00 | 3.77 | -1.00 | -12.28 | 167.93 | 75.81 | 257.15 | 0.9727 | 396.0 | 999999 | |
| 0.00 | 0.26 | 0.00 | 0.51 | -12.69 | 167.18 | 75.06 | 256.67 | 0.9698 | 197.0 | 132.0 | |
| 0.00 | 1.03 | 0.00 | 1.84 | -11.36 | 165.59 | 73.48 | 257.92 | 0.9624 | 312.0 | 216.1 | |
| 0.00 | 0.26 | 0.00 | 0.46 | -11.73 | 165.74 | 73.62 | 257.56 | 0.9632 | 233.0 | 281.7 | |
| 1.20 | 102.68 | 2.08 | 177.23 | -13.69 | 164.87 | 72.76 | 255.45 | 0.9600 | 118.4 | 170.3 | |
| 2.05 | -6.00 | 3.58 | -6.00 | -13.94 | 164.86 | 72.74 | 255.19 | 0.9600 | 153.2 | 999999 | |
| 12.56 | -6.00 | 21.68 | -6.00 | -14.39 | 164.71 | 72.60 | 254.70 | 0.9595 | 572.8 | 999999 | |
| 0.00 | 1.62 | 0.00 | 2.34 | -12.57 | 161.28 | 69.16 | 256.28 | 0.9405 | -457.0 | -384.2 | |
| 0.00 | 1.28 | 0.00 | 1.84 | -12.78 | 161.23 | 69.11 | 256.05 | 0.9403 | -383.0 | -327.3 | |
| 0.00 | 1.45 | 0.00 | 2.28 | -15.50 | 162.75 | 70.64 | 253.35 | 0.9503 | 95.0 | 147.9 | |
| 0.00 | 1.03 | 0.00 | 1.41 | -14.57 | 160.07 | 67.95 | 254.02 | 0.9347 | -383.0 | -340.2 | |
| 0.00 | 1.03 | 0.00 | 1.40 | -14.35 | 159.93 | 67.81 | 254.24 | 0.9337 | -422.0 | -427.8 | |
| 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. | |