SDO HMI 2014-03-04 13:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 23.85 | 0.00 | 15.40 | 9.71 | 121.05 | 35.12 | 297.06 | 0.6307 | -92.5 | -265.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.43 | 0.00 | 0.31 | 6.77 | 130.35 | 44.43 | 286.52 | 0.7274 | -593.0 | -506.0 | |
| 0.00 | 1.21 | 0.00 | 0.84 | 4.93 | 129.17 | 43.24 | 284.51 | 0.7074 | -575.0 | -507.1 | |
| 0.00 | 3.11 | 0.00 | 2.21 | 7.81 | 129.32 | 43.39 | 288.33 | 0.7193 | -696.0 | -608.5 | |
| 0.00 | 0.86 | 0.00 | 0.62 | 9.49 | 129.52 | 43.60 | 290.44 | 0.7282 | -589.0 | -557.5 | |
| 0.00 | 3.37 | 0.00 | 2.36 | 6.48 | 128.87 | 42.94 | 286.74 | 0.7092 | -760.0 | -668.2 | |
| 0.00 | 2.07 | 0.00 | 1.50 | 11.17 | 129.23 | 43.31 | 292.74 | 0.7320 | -88.0 | -119.8 | |
| 0.00 | 0.69 | 0.00 | 0.45 | 10.46 | 122.50 | 36.57 | 295.50 | 0.6515 | -607.0 | -536.1 | |
| 0.00 | 2.25 | 0.00 | 1.43 | 13.20 | 119.38 | 33.45 | 301.50 | 0.6317 | -707.0 | -570.8 | |
| 0.00 | 2.77 | 0.00 | 1.72 | 14.37 | 116.59 | 30.67 | 305.40 | 0.6084 | -607.0 | -484.3 | |
| 0.00 | 1.56 | 0.00 | 0.88 | 7.82 | 111.08 | 25.15 | 300.48 | 0.4907 | 628.0 | 455.3 | |
| 0.00 | 0.69 | 0.00 | 0.39 | 9.07 | 110.31 | 24.38 | 303.49 | 0.4908 | 699.0 | 573.8 | |
| 0.00 | 1.04 | 0.00 | 0.61 | 15.06 | 109.83 | 23.90 | 313.32 | 0.5398 | 571.0 | 423.2 | |
| 0.00 | 1.64 | 0.00 | 0.91 | 8.96 | 106.84 | 20.91 | 307.52 | 0.4464 | 547.0 | 375.5 | |
| 0.00 | 1.04 | 0.00 | 0.56 | 10.62 | 102.45 | 16.52 | 317.17 | 0.4128 | 674.0 | 466.6 | |
| 0.00 | 1.12 | 0.00 | 0.61 | 10.05 | 102.32 | 16.39 | 316.43 | 0.4049 | 715.0 | 571.8 | |
| 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. | |