SDO HMI 2014-10-09 16:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 24.11 | 0.00 | 13.52 | -21.06 | 74.17 | 3.78 | 188.01 | 0.4713 | 76.1 | 267.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.98 | 0.00 | 1.67 | -19.98 | 80.59 | 10.20 | 200.70 | 0.4726 | 834.0 | 642.8 | |
| 0.00 | 0.88 | 0.00 | 0.50 | -21.49 | 80.63 | 10.24 | 199.62 | 0.4944 | 702.0 | 523.2 | |
| 0.00 | 3.51 | 0.00 | 1.95 | -19.42 | 79.43 | 9.04 | 198.93 | 0.4585 | 735.0 | 610.6 | |
| 0.00 | 1.58 | 0.00 | 0.89 | -21.16 | 79.30 | 8.91 | 197.46 | 0.4832 | 900.0 | 677.9 | |
| 0.00 | 3.86 | 0.00 | 2.12 | -19.05 | 74.18 | 3.79 | 188.32 | 0.4334 | 853.0 | 642.0 | |
| 0.00 | 2.45 | 0.00 | 1.33 | -17.07 | 73.92 | 3.53 | 188.45 | 0.4017 | 888.0 | 653.9 | |
| 0.00 | 1.23 | 0.00 | 0.71 | -24.54 | 73.43 | 3.04 | 185.38 | 0.5161 | 518.0 | 424.0 | |
| 0.00 | 2.10 | 0.00 | 1.20 | -23.87 | 68.93 | -1.46 | 177.34 | 0.5043 | -277.0 | -300.6 | |
| 0.00 | 0.70 | 0.00 | 0.40 | -24.53 | 68.56 | -1.83 | 176.74 | 0.5146 | -573.0 | -394.0 | |
| 0.00 | 0.88 | 0.00 | 0.52 | -26.94 | 67.68 | -2.71 | 175.59 | 0.5510 | -723.0 | -567.6 | |
| 0.00 | 0.88 | 0.00 | 0.49 | -22.02 | 67.69 | -2.70 | 174.73 | 0.4775 | -779.0 | -611.5 | |
| 0.00 | 0.96 | 0.00 | 0.55 | -23.63 | 67.62 | -2.77 | 174.92 | 0.5021 | -624.0 | -513.9 | |
| 0.00 | 1.05 | 0.00 | 0.58 | -20.47 | 66.70 | -3.70 | 172.35 | 0.4553 | -786.0 | -549.8 | |
| 0.00 | 1.05 | 0.00 | 0.61 | -25.00 | 66.07 | -4.32 | 172.49 | 0.5250 | -603.0 | -515.8 | |
| 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. | |