SDO HMI 2014-03-02 06:47:43 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.69 | 26.00 | 0.37 | 14.10 | 7.30 | 134.68 | 19.01 | 307.57 | 0.4088 | 281.1 | 322.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.95 | 0.00 | 0.54 | 5.28 | 141.46 | 25.79 | 295.23 | 0.4809 | -766.0 | -590.4 | |
| 0.00 | 1.47 | 0.00 | 0.83 | 5.22 | 141.06 | 25.39 | 295.49 | 0.4750 | -908.0 | -698.7 | |
| 0.00 | 1.90 | 0.00 | 1.05 | 4.37 | 139.32 | 23.65 | 295.48 | 0.4449 | -939.0 | -695.9 | |
| 0.00 | 1.12 | 0.00 | 0.61 | 7.01 | 136.43 | 20.76 | 304.07 | 0.4265 | 811.0 | 693.7 | |
| 0.00 | 1.47 | 0.00 | 0.80 | 7.43 | 136.32 | 20.65 | 305.03 | 0.4289 | 738.0 | 645.5 | |
| 0.00 | 1.21 | 0.00 | 0.66 | 7.59 | 136.30 | 20.63 | 305.36 | 0.4300 | 615.0 | 551.8 | |
| 0.00 | 1.64 | 0.00 | 0.90 | 8.51 | 135.61 | 19.94 | 308.04 | 0.4300 | -1067.0 | -792.8 | |
| 0.00 | 0.78 | 0.00 | 0.42 | 8.49 | 135.16 | 19.49 | 308.64 | 0.4243 | -782.0 | -649.7 | |
| 0.00 | 1.90 | 0.00 | 1.03 | 6.87 | 134.55 | 18.87 | 306.41 | 0.4008 | 841.0 | 702.1 | |
| 0.00 | 1.21 | 0.00 | 0.65 | 7.85 | 133.93 | 18.25 | 309.31 | 0.4027 | 811.0 | 654.5 | |
| 0.69 | 6.22 | 0.37 | 3.35 | 8.20 | 133.18 | 17.51 | 311.15 | 0.3972 | 1045.1 | 827.4 | |
| 0.00 | 0.69 | 0.00 | 0.37 | 7.46 | 132.46 | 16.79 | 310.93 | 0.3807 | 766.0 | 532.0 | |
| 0.00 | 1.30 | 0.00 | 0.69 | 8.05 | 130.77 | 15.10 | 315.15 | 0.3673 | 855.0 | 706.7 | |
| 0.00 | 1.55 | 0.00 | 0.83 | 8.23 | 130.65 | 14.98 | 315.72 | 0.3680 | 1020.0 | 757.9 | |
| 0.00 | 2.59 | 0.00 | 1.37 | 7.24 | 130.46 | 14.79 | 314.15 | 0.3544 | 893.0 | 591.0 | |
| 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. | |