SDO HMI 2013-03-29 06:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 49.87 | 256.23 | 26.59 | 136.57 | 14.84 | 255.26 | -1.99 | 5.22 | 0.3700 | -1033.2 | -382.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.61 | 0.00 | 0.32 | 13.00 | 259.22 | 1.98 | 354.29 | 0.3398 | -364.0 | -473.0 | |
| 0.00 | 3.42 | 0.00 | 1.80 | 13.60 | 256.95 | -0.29 | 0.82 | 0.3482 | -804.0 | -737.0 | |
| 24.80 | 237.38 | 13.22 | 126.65 | 14.99 | 255.65 | -1.59 | 4.17 | 0.3717 | -1297.4 | -362.6 | |
| 0.00 | 1.49 | 0.00 | 0.77 | 9.79 | 255.43 | -1.81 | 6.27 | 0.2864 | -826.0 | -673.3 | |
| 0.00 | 2.72 | 0.00 | 1.43 | 13.01 | 255.35 | -1.89 | 5.45 | 0.3398 | -1174.0 | -920.4 | |
| 24.54 | -3.00 | 13.09 | -3.00 | 14.96 | 255.00 | -2.25 | 5.86 | 0.3722 | -1233.4 | 999999 | |
| 0.00 | 1.23 | 0.00 | 0.66 | 16.19 | 254.80 | -2.44 | 6.02 | 0.3923 | -469.0 | -324.1 | |
| 0.53 | -3.00 | 0.28 | -3.00 | 15.22 | 254.56 | -2.68 | 6.91 | 0.3772 | -637.7 | 999999 | |
| 0.00 | 1.05 | 0.00 | 0.55 | 12.22 | 254.41 | -2.84 | 8.50 | 0.3287 | -974.0 | -858.7 | |
| 0.00 | 1.49 | 0.00 | 0.78 | 12.82 | 254.22 | -3.03 | 8.77 | 0.3391 | -850.0 | -721.1 | |
| 0.00 | 4.38 | 0.00 | 2.30 | 12.48 | 253.88 | -3.36 | 9.90 | 0.3343 | -738.0 | -652.7 | |
| 0.00 | 0.70 | 0.00 | 0.37 | 11.95 | 253.06 | -4.18 | 12.61 | 0.3283 | -969.0 | -842.9 | |
| 0.00 | 0.88 | 0.00 | 0.47 | 15.41 | 251.60 | -5.64 | 14.17 | 0.3890 | 731.0 | 618.7 | |
| 0.00 | 0.88 | 0.00 | 0.47 | 14.91 | 250.34 | -6.91 | 17.56 | 0.3868 | 680.0 | 549.3 | |
| 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. | |