SDO HMI 2014-10-04 21:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 65.55 | 354.99 | 35.17 | 190.63 | -1.39 | 154.82 | 21.22 | 250.15 | 0.3864 | 1000.5 | 413.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 45.52 | 302.79 | 24.49 | 162.93 | -1.39 | 155.17 | 21.57 | 250.51 | 0.3916 | 1424.9 | 413.2 | |
| 0.00 | 1.32 | 0.00 | 0.71 | -2.56 | 154.80 | 21.20 | 247.39 | 0.3930 | 639.0 | 468.6 | |
| 5.01 | -1.00 | 2.68 | -1.00 | -1.57 | 154.50 | 20.90 | 249.44 | 0.3825 | 1260.1 | 999999 | |
| 3.60 | 24.25 | 1.93 | 12.94 | -1.91 | 153.96 | 20.36 | 248.07 | 0.3764 | 961.6 | 575.8 | |
| 2.81 | -4.00 | 1.50 | -4.00 | -1.73 | 153.86 | 20.26 | 248.43 | 0.3738 | 1175.8 | 999999 | |
| 1.76 | -4.00 | 0.94 | -4.00 | -1.72 | 153.70 | 20.10 | 248.28 | 0.3713 | 1091.3 | 999999 | |
| 0.00 | 4.13 | 0.00 | 2.20 | -1.05 | 153.66 | 20.06 | 249.93 | 0.3667 | 1035.0 | 943.3 | |
| 0.00 | 1.67 | 0.00 | 0.89 | 0.09 | 153.66 | 20.06 | 252.91 | 0.3604 | 924.0 | 663.1 | |
| 6.85 | 12.04 | 3.63 | 6.37 | -0.25 | 153.18 | 19.58 | 251.56 | 0.3548 | 1064.0 | 715.9 | |
| 0.00 | 1.14 | 0.00 | 0.60 | 0.80 | 152.64 | 19.04 | 253.94 | 0.3410 | 757.0 | 580.5 | |
| 0.00 | 1.05 | 0.00 | 0.55 | -2.05 | 151.35 | 17.75 | 244.69 | 0.3386 | 713.0 | 500.9 | |
| 0.00 | 0.53 | 0.00 | 0.28 | -2.41 | 150.23 | 16.63 | 242.18 | 0.3247 | -588.0 | -522.5 | |
| 0.00 | 0.97 | 0.00 | 0.51 | -2.43 | 150.07 | 16.47 | 241.88 | 0.3226 | -704.0 | -592.3 | |
| 0.00 | 1.67 | 0.00 | 0.87 | -1.71 | 150.06 | 16.46 | 243.89 | 0.3169 | -721.0 | -540.7 | |
| 0.00 | 1.41 | 0.00 | 0.73 | -2.25 | 150.01 | 16.41 | 242.29 | 0.3202 | -881.0 | -797.8 | |
| 0.00 | 1.23 | 0.00 | 0.64 | -1.52 | 149.91 | 16.31 | 244.20 | 0.3131 | -755.0 | -665.2 | |
| 0.00 | 0.79 | 0.00 | 0.41 | -1.67 | 149.75 | 16.15 | 243.55 | 0.3119 | -1007.0 | -832.7 | |
| 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. | |