SDO HMI 2014-10-15 22:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 61.66 | 403.12 | 39.44 | 257.84 | -21.14 | 16.92 | 28.99 | 225.65 | 0.6345 | 870.2 | 330.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.10 | 0.00 | 1.36 | -19.56 | 19.83 | 31.91 | 230.24 | 0.6502 | 510.0 | 396.5 | |
| 29.17 | 393.08 | 18.73 | 251.61 | -21.21 | 17.30 | 29.37 | 225.94 | 0.6386 | 1058.5 | 341.0 | |
| 30.04 | -2.00 | 19.15 | -2.00 | -21.04 | 16.75 | 28.82 | 225.62 | 0.6319 | 1272.7 | 999999 | |
| 2.45 | -2.00 | 1.56 | -2.00 | -21.51 | 16.67 | 28.74 | 224.98 | 0.6352 | 933.5 | 999999 | |
| 0.00 | 1.05 | 0.00 | 0.66 | -21.86 | 15.06 | 27.14 | 222.97 | 0.6233 | 455.0 | 475.4 | |
| 0.00 | 1.57 | 0.00 | 1.01 | -23.60 | 15.33 | 27.40 | 221.24 | 0.6420 | 529.0 | 385.1 | |
| 0.00 | 0.79 | 0.00 | 0.47 | -17.83 | 12.48 | 24.56 | 225.21 | 0.5596 | -562.0 | -451.0 | |
| 0.00 | 1.22 | 0.00 | 0.73 | -18.22 | 11.54 | 23.61 | 223.61 | 0.5538 | -601.0 | -506.2 | |
| 0.00 | 0.52 | 0.00 | 0.31 | -19.86 | 10.82 | 22.89 | 220.65 | 0.5638 | -542.0 | -457.7 | |
| 0.00 | 0.87 | 0.00 | 0.54 | -23.24 | 10.54 | 22.61 | 216.42 | 0.5973 | -589.0 | -478.8 | |
| 0.00 | 0.52 | 0.00 | 0.30 | -17.86 | 9.21 | 21.28 | 221.16 | 0.5270 | -606.0 | -477.5 | |
| 0.00 | 0.79 | 0.00 | 0.47 | -23.86 | 6.15 | 18.22 | 210.23 | 0.5701 | -615.0 | -449.6 | |
| 0.00 | 0.61 | 0.00 | 0.38 | -28.09 | 4.49 | 16.56 | 204.40 | 0.6110 | -612.0 | -418.1 | |
| 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. | |