SDO HMI 2014-04-14 23:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 44.12 | 261.82 | 23.00 | 136.58 | 12.21 | 263.01 | 3.29 | 349.54 | 0.3153 | -821.8 | -374.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.06 | 0.00 | 0.55 | 12.05 | 265.69 | 5.97 | 341.47 | 0.3214 | 772.0 | 613.5 | |
| 7.16 | 249.01 | 3.74 | 129.80 | 12.35 | 263.75 | 4.03 | 347.46 | 0.3176 | -1193.8 | -432.3 | |
| 13.17 | -2.00 | 6.87 | -2.00 | 12.16 | 263.69 | 3.97 | 347.52 | 0.3143 | -1370.9 | 999999 | |
| 5.75 | -2.00 | 2.99 | -2.00 | 11.91 | 263.56 | 3.84 | 347.73 | 0.3098 | -1538.0 | 999999 | |
| 17.77 | -2.00 | 9.26 | -2.00 | 12.10 | 263.28 | 3.57 | 348.71 | 0.3119 | -1343.9 | 999999 | |
| 0.27 | -2.00 | 0.14 | -2.00 | 12.44 | 263.29 | 3.57 | 348.91 | 0.3176 | -887.3 | 999999 | |
| 0.00 | 0.88 | 0.00 | 0.47 | 15.99 | 254.24 | -5.48 | 14.00 | 0.3811 | 597.0 | 503.8 | |
| 0.00 | 2.30 | 0.00 | 1.21 | 12.95 | 254.25 | -5.47 | 16.27 | 0.3331 | 801.0 | 622.4 | |
| 0.00 | 1.59 | 0.00 | 0.83 | 12.51 | 253.98 | -5.74 | 17.43 | 0.3274 | 750.0 | 475.2 | |
| 0.00 | 0.88 | 0.00 | 0.47 | 15.22 | 253.85 | -5.87 | 15.50 | 0.3707 | 699.0 | 536.5 | |
| 0.00 | 2.21 | 0.00 | 1.19 | 15.89 | 252.07 | -7.65 | 19.27 | 0.3896 | 767.0 | 574.7 | |
| 0.00 | 1.24 | 0.00 | 0.67 | 15.37 | 250.29 | -9.43 | 23.85 | 0.3923 | 855.0 | 612.2 | |
| 0.00 | 2.65 | 0.00 | 1.39 | 10.03 | 249.62 | -10.10 | 32.74 | 0.3207 | 398.0 | 376.3 | |
| 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. | |