SDO HMI 2014-04-14 18:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 66.80 | 409.45 | 35.56 | 217.84 | 11.76 | 274.89 | 12.41 | 324.74 | 0.3662 | -1013.9 | -368.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.12 | 0.00 | 1.13 | 8.72 | 279.32 | 16.84 | 310.43 | 0.3778 | -772.0 | -590.3 | |
| 65.30 | 386.48 | 34.76 | 205.72 | 11.71 | 275.17 | 12.69 | 324.00 | 0.3674 | -1495.4 | -428.0 | |
| 1.50 | -2.00 | 0.80 | -2.00 | 11.98 | 274.62 | 12.13 | 325.64 | 0.3658 | -882.6 | 999999 | |
| 0.00 | 2.56 | 0.00 | 1.34 | 10.04 | 273.57 | 11.08 | 324.84 | 0.3301 | -996.0 | -723.8 | |
| 0.00 | 0.88 | 0.00 | 0.47 | 12.73 | 270.61 | 8.13 | 336.31 | 0.3448 | 711.0 | 582.6 | |
| 0.00 | 3.00 | 0.00 | 1.59 | 12.92 | 270.37 | 7.89 | 337.16 | 0.3461 | 695.0 | 729.1 | |
| 0.00 | 3.89 | 0.00 | 2.05 | 13.04 | 270.03 | 7.55 | 338.18 | 0.3458 | 954.0 | 826.3 | |
| 0.00 | 1.94 | 0.00 | 1.02 | 13.13 | 269.51 | 7.02 | 339.66 | 0.3441 | 1064.0 | 846.7 | |
| 0.00 | 3.80 | 0.00 | 2.02 | 14.55 | 268.05 | 5.57 | 344.77 | 0.3590 | 832.0 | 742.4 | |
| 0.00 | 0.62 | 0.00 | 0.33 | 17.14 | 267.91 | 5.42 | 346.86 | 0.3990 | 374.0 | 523.3 | |
| 0.00 | 0.80 | 0.00 | 0.41 | 11.69 | 267.61 | 5.13 | 343.61 | 0.3116 | 772.0 | 612.8 | |
| 0.00 | 2.12 | 0.00 | 1.12 | 13.65 | 267.63 | 5.14 | 345.23 | 0.3430 | 854.0 | 754.2 | |
| 0.00 | 1.24 | 0.00 | 0.64 | 11.74 | 265.98 | 3.50 | 348.69 | 0.3060 | 991.0 | 902.2 | |
| 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. | |