SDO HMI 2014-10-07 03:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 36.53 | 153.17 | 41.16 | 176.70 | -12.31 | 165.83 | 61.93 | 253.00 | 0.9024 | 253.1 | 50.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.79 | 121.54 | 22.48 | 145.60 | -12.49 | 167.05 | 63.14 | 253.13 | 0.9119 | 530.1 | 94.2 | |
| 7.90 | -1.00 | 9.21 | -1.00 | -12.04 | 166.38 | 62.48 | 253.44 | 0.9066 | 724.1 | 999999 | |
| 0.00 | 0.26 | 0.00 | 0.30 | -11.58 | 165.80 | 61.89 | 253.80 | 0.9017 | 452.0 | 471.0 | |
| 0.00 | 1.49 | 0.00 | 1.70 | -12.01 | 165.77 | 61.87 | 253.32 | 0.9022 | 447.0 | 520.6 | |
| 0.00 | 1.41 | 0.00 | 1.58 | -12.04 | 165.39 | 61.49 | 253.20 | 0.8995 | 666.0 | 587.5 | |
| 0.00 | 0.53 | 0.00 | 0.57 | -13.78 | 163.70 | 59.79 | 250.86 | 0.8904 | -222.0 | -182.7 | |
| 0.00 | 2.11 | 0.00 | 2.25 | -13.85 | 163.42 | 59.51 | 250.71 | 0.8884 | -281.0 | -228.8 | |
| 0.00 | 1.32 | 0.00 | 1.34 | -11.63 | 162.28 | 58.38 | 252.83 | 0.8749 | 316.0 | 248.7 | |
| 0.00 | 0.79 | 0.00 | 0.80 | -11.78 | 162.22 | 58.31 | 252.64 | 0.8747 | 355.0 | 293.6 | |
| 6.59 | 11.42 | 6.38 | 11.08 | -11.57 | 160.71 | 56.80 | 252.45 | 0.8619 | -611.8 | -373.3 | |
| 0.00 | 1.67 | 0.00 | 1.60 | -11.90 | 160.25 | 56.35 | 251.94 | 0.8588 | -285.0 | -293.7 | |
| 3.25 | 5.36 | 3.09 | 5.10 | -11.97 | 159.94 | 56.04 | 251.78 | 0.8563 | -606.6 | -428.6 | |
| 0.00 | 4.04 | 0.00 | 3.66 | -12.43 | 157.88 | 53.97 | 250.60 | 0.8394 | -682.0 | -548.1 | |
| 0.00 | 1.23 | 0.00 | 1.12 | -13.27 | 157.77 | 53.87 | 249.61 | 0.8408 | -627.0 | -580.7 | |
| 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. | |