SDO HMI 2014-10-31 23:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.11 | 95.41 | 20.63 | 78.59 | -4.58 | 83.96 | -52.40 | 99.10 | 0.8020 | 581.3 | 504.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.51 | 82.25 | 2.03 | 67.37 | -5.17 | 84.96 | -51.40 | 100.03 | 0.7927 | -206.5 | 556.6 | |
| 3.03 | -1.00 | 2.48 | -1.00 | -5.44 | 84.49 | -51.87 | 100.27 | 0.7981 | 832.5 | 999999 | |
| 0.00 | 2.08 | 0.00 | 1.70 | -5.75 | 84.40 | -51.96 | 100.63 | 0.7995 | 530.0 | 435.3 | |
| 10.48 | -1.00 | 8.59 | -1.00 | -4.43 | 84.21 | -52.15 | 98.96 | 0.7992 | 952.2 | 999999 | |
| 3.55 | -1.00 | 2.92 | -1.00 | -4.14 | 84.00 | -52.36 | 98.57 | 0.8010 | 787.5 | 999999 | |
| 0.00 | 2.68 | 0.00 | 2.24 | -5.25 | 83.58 | -52.78 | 99.85 | 0.8071 | 430.0 | 290.8 | |
| 0.00 | 1.04 | 0.00 | 0.86 | -3.11 | 83.79 | -52.57 | 97.24 | 0.8015 | 580.0 | 433.2 | |
| 4.59 | -1.00 | 3.81 | -1.00 | -4.02 | 83.62 | -52.74 | 98.34 | 0.8047 | 526.5 | 999999 | |
| 0.00 | 1.30 | 0.00 | 1.08 | -4.35 | 83.53 | -52.83 | 98.74 | 0.8061 | 278.0 | 203.0 | |
| 0.95 | 2.94 | 0.80 | 2.46 | -4.40 | 83.33 | -53.03 | 98.75 | 0.8082 | 345.7 | 170.4 | |
| 0.00 | 1.30 | 0.00 | 1.14 | -5.23 | 81.60 | -54.76 | 99.43 | 0.8267 | 521.0 | 434.3 | |
| 0.00 | 0.87 | 0.00 | 0.79 | -5.25 | 79.89 | -56.47 | 99.14 | 0.8429 | 447.0 | 380.1 | |
| 0.00 | 0.26 | 0.00 | 0.26 | -6.54 | 77.12 | -59.24 | 100.15 | 0.8693 | -347.0 | -346.3 | |
| 0.00 | 0.69 | 0.00 | 0.69 | -6.68 | 76.92 | -59.44 | 100.26 | 0.8712 | -203.0 | -241.9 | |
| 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. | |