SDO HMI 2014-10-10 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 |
| 41.06 | 176.29 | 64.55 | 284.19 | -15.21 | 123.28 | 69.39 | 251.76 | 0.9517 | 171.5 | 111.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.79 | 125.41 | 1.40 | 214.86 | -14.46 | 125.34 | 71.45 | 252.95 | 0.9614 | 204.4 | 113.4 | |
| 2.89 | -1.00 | 5.11 | -1.00 | -14.70 | 125.23 | 71.35 | 252.69 | 0.9612 | 148.6 | 999999 | |
| 11.03 | -1.00 | 19.24 | -1.00 | -15.20 | 124.84 | 70.96 | 252.10 | 0.9599 | 208.1 | 999999 | |
| 8.58 | -1.00 | 14.30 | -1.00 | -14.99 | 124.02 | 70.13 | 252.16 | 0.9557 | 570.3 | 999999 | |
| 3.15 | -1.00 | 5.06 | -1.00 | -14.45 | 123.45 | 69.57 | 252.59 | 0.9524 | 683.8 | 999999 | |
| 0.00 | 0.88 | 0.00 | 1.38 | -14.98 | 123.02 | 69.13 | 251.96 | 0.9507 | 421.0 | 449.0 | |
| 0.00 | 1.75 | 0.00 | 2.73 | -15.11 | 122.76 | 68.87 | 251.77 | 0.9495 | 286.0 | 396.0 | |
| 0.00 | 2.19 | 0.00 | 3.31 | -15.07 | 122.13 | 68.25 | 251.67 | 0.9462 | 642.0 | 481.8 | |
| 0.00 | 2.89 | 0.00 | 4.29 | -15.22 | 121.73 | 67.85 | 251.43 | 0.9442 | 577.0 | 478.9 | |
| 0.00 | 2.80 | 0.00 | 4.01 | -15.97 | 120.68 | 66.80 | 250.42 | 0.9394 | 261.0 | 244.7 | |
| 0.00 | 1.66 | 0.00 | 2.34 | -15.78 | 120.40 | 66.51 | 250.55 | 0.9375 | 153.0 | 131.8 | |
| 8.93 | 16.38 | 12.07 | 22.19 | -15.32 | 119.56 | 65.68 | 250.84 | 0.9320 | -150.6 | 239.9 | |
| 0.00 | 1.49 | 0.00 | 1.97 | -15.23 | 119.06 | 65.17 | 250.80 | 0.9289 | -485.0 | -410.1 | |
| 0.00 | 0.26 | 0.00 | 0.35 | -15.43 | 119.10 | 65.22 | 250.61 | 0.9294 | -507.0 | -502.3 | |
| 2.10 | 11.03 | 2.75 | 14.55 | -16.79 | 118.39 | 64.50 | 249.01 | 0.9272 | -432.0 | -21.6 | |
| 3.59 | 8.76 | 4.62 | 11.24 | -17.06 | 117.90 | 64.02 | 248.60 | 0.9247 | -450.0 | -345.2 | |
| 0.00 | 0.79 | 0.00 | 0.97 | -16.16 | 116.86 | 62.98 | 249.28 | 0.9165 | -313.0 | -336.1 | |
| 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. | |