SDO HMI 2014-04-09 11:05:03 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 56.32 | 304.50 | 58.80 | 317.53 | 12.30 | 273.07 | -59.23 | 72.53 | 0.8807 | -280.4 | -57.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.71 | 0.00 | 0.66 | 12.78 | 277.23 | -55.07 | 70.79 | 0.8488 | 251.0 | 205.2 | |
| 4.50 | 23.36 | 5.72 | 29.56 | 15.27 | 268.07 | -64.23 | 70.60 | 0.9227 | 495.8 | 312.0 | |
| 0.00 | 0.97 | 0.00 | 1.08 | 13.71 | 271.49 | -60.81 | 71.40 | 0.8967 | -253.0 | -187.9 | |
| 0.00 | 0.44 | 0.00 | 0.52 | 14.15 | 269.94 | -62.36 | 71.33 | 0.9085 | 442.0 | 511.2 | |
| 0.00 | 1.76 | 0.00 | 2.19 | 14.66 | 268.56 | -63.75 | 71.13 | 0.9186 | 562.0 | 416.1 | |
| 39.14 | 220.40 | 38.14 | 214.97 | 11.30 | 275.15 | -57.15 | 73.07 | 0.8632 | -727.8 | -193.1 | |
| 1.23 | 51.04 | 1.51 | 61.96 | 14.38 | 268.95 | -63.35 | 71.33 | 0.9156 | 387.8 | 210.7 | |
| 1.85 | -7.00 | 2.24 | -7.00 | 14.21 | 269.09 | -63.21 | 71.48 | 0.9144 | 615.4 | 999999 | |
| 0.35 | 1.32 | 0.37 | 1.39 | 12.43 | 272.81 | -59.50 | 72.45 | 0.8844 | -432.5 | -405.5 | |
| 2.29 | -6.00 | 2.34 | -6.00 | 11.82 | 273.62 | -58.68 | 72.91 | 0.8768 | -184.5 | 999999 | |
| 0.00 | 2.12 | 0.00 | 2.66 | 14.41 | 268.13 | -64.17 | 71.49 | 0.9210 | 191.0 | 129.9 | |
| 6.96 | -7.00 | 8.48 | -7.00 | 13.89 | 268.90 | -63.40 | 71.86 | 0.9151 | 476.4 | 999999 | |
| 0.00 | 1.41 | 0.00 | 1.49 | 12.17 | 272.51 | -59.79 | 72.82 | 0.8861 | 17.0 | -41.6 | |
| 0.00 | 0.97 | 0.00 | 1.05 | 12.19 | 272.02 | -60.28 | 72.92 | 0.8899 | -2.0 | -43.3 | |
| 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. | |