SDO HMI 2014-04-25 05:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 47.59 | 320.16 | 34.70 | 232.91 | 18.08 | 166.14 | 41.80 | 300.15 | 0.7350 | -649.4 | -287.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.16 | 0.00 | 0.86 | 19.22 | 166.93 | 42.59 | 301.10 | 0.7487 | 123.0 | 131.4 | |
| 37.36 | 304.86 | 27.24 | 222.15 | 17.94 | 166.28 | 41.94 | 299.89 | 0.7357 | -1061.6 | -323.1 | |
| 9.79 | -2.00 | 7.15 | -2.00 | 18.52 | 166.20 | 41.86 | 300.66 | 0.7378 | -936.0 | 999999 | |
| 0.00 | 1.60 | 0.00 | 1.17 | 19.31 | 165.58 | 41.24 | 301.96 | 0.7357 | -201.0 | -170.7 | |
| 0.00 | 0.71 | 0.00 | 0.51 | 17.63 | 164.75 | 40.41 | 300.35 | 0.7184 | -550.0 | -505.5 | |
| 0.00 | 0.71 | 0.00 | 0.49 | 16.57 | 163.69 | 39.35 | 299.62 | 0.7014 | 468.0 | 410.0 | |
| 0.00 | 1.78 | 0.00 | 1.26 | 19.05 | 163.90 | 39.57 | 302.64 | 0.7173 | 528.0 | 444.3 | |
| 0.00 | 0.36 | 0.00 | 0.25 | 19.00 | 163.60 | 39.26 | 302.76 | 0.7139 | 345.0 | 359.2 | |
| 0.44 | 5.16 | 0.31 | 3.58 | 17.99 | 163.12 | 38.78 | 301.79 | 0.7032 | 610.2 | 585.6 | |
| 0.00 | 0.36 | 0.00 | 0.25 | 18.29 | 163.12 | 38.78 | 302.16 | 0.7048 | 319.0 | 329.0 | |
| 0.00 | 1.16 | 0.00 | 0.80 | 18.72 | 162.66 | 38.32 | 303.00 | 0.7026 | 564.0 | 488.6 | |
| 0.00 | 0.44 | 0.00 | 0.31 | 18.40 | 162.17 | 37.83 | 302.91 | 0.6955 | 613.0 | 562.0 | |
| 0.00 | 0.80 | 0.00 | 0.56 | 19.29 | 162.29 | 37.95 | 303.95 | 0.7021 | 499.0 | 425.6 | |
| 0.00 | 0.62 | 0.00 | 0.43 | 20.48 | 161.69 | 37.35 | 305.83 | 0.7033 | 513.0 | 444.3 | |
| 0.00 | 0.44 | 0.00 | 0.29 | 16.34 | 159.91 | 35.57 | 301.72 | 0.6585 | 617.0 | 558.8 | |
| 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. | |