SDO HMI 2014-04-10 13:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.58 | 0.00 | 11.74 | -21.14 | 321.17 | 3.13 | 191.94 | 0.2985 | -1.6 | -208.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.50 | 0.00 | 0.78 | -13.92 | 332.96 | 14.91 | 240.36 | 0.2886 | 680.0 | 568.1 | |
| 0.00 | 1.15 | 0.00 | 0.59 | -15.61 | 332.40 | 14.35 | 234.40 | 0.2949 | 843.0 | 697.8 | |
| 0.00 | 0.79 | 0.00 | 0.41 | -15.76 | 332.34 | 14.30 | 233.87 | 0.2955 | 726.0 | 693.8 | |
| 0.00 | 1.23 | 0.00 | 0.65 | -19.77 | 331.81 | 13.77 | 222.82 | 0.3309 | 797.0 | 688.1 | |
| 0.00 | 1.23 | 0.00 | 0.65 | -21.38 | 330.57 | 12.52 | 216.96 | 0.3373 | 717.0 | 502.9 | |
| 0.00 | 0.71 | 0.00 | 0.36 | -18.04 | 328.54 | 10.49 | 219.35 | 0.2743 | 815.0 | 542.6 | |
| 0.00 | 1.59 | 0.00 | 0.82 | -19.63 | 325.47 | 7.43 | 207.16 | 0.2679 | 913.0 | 721.0 | |
| 0.00 | 1.15 | 0.00 | 0.59 | -20.44 | 318.60 | 0.55 | 182.07 | 0.2515 | -912.0 | -690.2 | |
| 0.00 | 3.88 | 0.00 | 2.02 | -23.78 | 317.13 | -0.91 | 177.27 | 0.3080 | -630.0 | -650.5 | |
| 0.00 | 2.91 | 0.00 | 1.51 | -22.68 | 316.10 | -1.95 | 173.79 | 0.2909 | -895.0 | -794.5 | |
| 0.00 | 1.15 | 0.00 | 0.60 | -23.50 | 316.02 | -2.02 | 173.87 | 0.3046 | -564.0 | -486.5 | |
| 0.00 | 1.23 | 0.00 | 0.64 | -22.33 | 315.78 | -2.27 | 172.62 | 0.2858 | -907.0 | -707.9 | |
| 0.00 | 1.15 | 0.00 | 0.60 | -23.74 | 315.33 | -2.72 | 171.92 | 0.3102 | -787.0 | -625.9 | |
| 0.00 | 2.91 | 0.00 | 1.52 | -23.26 | 313.14 | -4.90 | 165.23 | 0.3094 | -819.0 | -729.2 | |
| 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. | |