SDO HMI 2014-04-04 19:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.50 | 0.00 | 8.99 | 5.38 | 25.49 | -8.43 | 34.47 | 0.2527 | -387.2 | -298.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.35 | 0.00 | 0.18 | 0.68 | 29.91 | -4.01 | 29.85 | 0.1412 | -378.0 | -367.8 | |
| 0.00 | 0.88 | 0.00 | 0.45 | 6.06 | 29.47 | -4.45 | 19.79 | 0.2290 | -809.0 | -654.9 | |
| 0.00 | 1.32 | 0.00 | 0.67 | 6.13 | 29.29 | -4.63 | 20.43 | 0.2311 | -849.0 | -739.9 | |
| 0.00 | 0.97 | 0.00 | 0.49 | 3.44 | 29.31 | -4.62 | 25.36 | 0.1885 | -905.0 | -731.9 | |
| 0.00 | 2.37 | 0.00 | 1.20 | 4.27 | 28.85 | -5.07 | 25.65 | 0.2047 | -1027.0 | -801.6 | |
| 0.00 | 0.88 | 0.00 | 0.44 | 3.06 | 27.71 | -6.21 | 33.59 | 0.1963 | -853.0 | -664.7 | |
| 0.00 | 1.49 | 0.00 | 0.76 | 3.28 | 27.29 | -6.64 | 34.74 | 0.2035 | -1025.0 | -792.2 | |
| 0.00 | 1.32 | 0.00 | 0.67 | 4.63 | 26.67 | -7.25 | 33.59 | 0.2285 | -722.0 | -518.8 | |
| 0.00 | 1.32 | 0.00 | 0.67 | 1.64 | 25.66 | -8.27 | 46.22 | 0.1999 | -1033.0 | -740.7 | |
| 0.00 | 1.23 | 0.00 | 0.63 | 4.25 | 25.55 | -8.37 | 38.48 | 0.2344 | -890.0 | -616.3 | |
| 0.00 | 0.97 | 0.00 | 0.51 | 8.70 | 21.72 | -12.20 | 39.10 | 0.3328 | 939.0 | 735.1 | |
| 0.00 | 1.67 | 0.00 | 0.88 | 9.36 | 21.61 | -12.32 | 38.14 | 0.3424 | 712.0 | 525.6 | |
| 0.00 | 1.41 | 0.00 | 0.74 | 8.46 | 20.36 | -13.56 | 42.58 | 0.3443 | 677.0 | 473.6 | |
| 0.00 | 1.32 | 0.00 | 0.70 | 7.13 | 18.12 | -15.80 | 49.73 | 0.3557 | 742.0 | 616.5 | |
| 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. | |