SDO HMI 2014-10-02 12:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.23 | 70.33 | 13.20 | 40.21 | -10.34 | 140.26 | -24.69 | 124.36 | 0.5005 | 482.8 | 315.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.76 | 0.00 | 1.04 | -17.43 | 142.45 | -22.50 | 137.58 | 0.5434 | 460.0 | 382.1 | |
| 0.00 | 0.88 | 0.00 | 0.50 | -11.71 | 141.04 | -23.92 | 127.56 | 0.5028 | 695.0 | 586.1 | |
| 0.00 | 0.53 | 0.00 | 0.30 | -12.15 | 140.45 | -24.50 | 127.59 | 0.5136 | 717.0 | 528.3 | |
| 3.08 | 47.45 | 1.75 | 27.00 | -9.79 | 140.53 | -24.42 | 123.80 | 0.4922 | 1058.1 | 402.0 | |
| 5.19 | 11.88 | 2.94 | 6.73 | -9.19 | 140.58 | -24.37 | 122.82 | 0.4867 | 992.1 | 735.3 | |
| 6.51 | -4.00 | 3.71 | -4.00 | -9.98 | 140.42 | -24.54 | 124.00 | 0.4953 | 849.2 | 999999 | |
| 8.45 | -4.00 | 4.80 | -4.00 | -9.61 | 140.45 | -24.51 | 123.39 | 0.4918 | 967.8 | 999999 | |
| 0.00 | 0.97 | 0.00 | 0.56 | -11.55 | 139.94 | -25.01 | 126.05 | 0.5144 | 873.0 | 734.0 | |
| 0.00 | 1.14 | 0.00 | 0.67 | -13.56 | 139.07 | -25.88 | 128.21 | 0.5421 | -628.0 | -475.9 | |
| 0.00 | 1.14 | 0.00 | 0.69 | -15.72 | 138.20 | -26.75 | 130.39 | 0.5710 | -675.0 | -520.5 | |
| 0.00 | 1.85 | 0.00 | 1.10 | -13.88 | 137.72 | -27.23 | 127.28 | 0.5605 | -670.0 | -496.8 | |
| 0.00 | 1.41 | 0.00 | 0.83 | -12.73 | 137.83 | -27.12 | 125.68 | 0.5496 | -737.0 | -612.9 | |
| 0.00 | 0.26 | 0.00 | 0.16 | -14.63 | 137.48 | -27.47 | 128.12 | 0.5696 | -655.0 | -583.7 | |
| 0.00 | 1.06 | 0.00 | 0.63 | -12.48 | 136.68 | -28.28 | 124.18 | 0.5613 | -744.0 | -669.2 | |
| 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. | |