SDO HMI 2014-10-09 14:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 13.33 | 0.00 | 8.55 | -19.90 | 99.57 | 28.07 | 224.78 | 0.6318 | 31.9 | -95.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.61 | 0.00 | 0.42 | -13.23 | 110.43 | 38.93 | 243.13 | 0.6881 | 514.0 | 534.7 | |
| 0.00 | 0.79 | 0.00 | 0.54 | -13.41 | 110.22 | 38.73 | 242.78 | 0.6867 | 591.0 | 525.1 | |
| 0.00 | 1.23 | 0.00 | 0.88 | -18.38 | 111.38 | 39.89 | 237.17 | 0.7266 | 468.0 | 437.1 | |
| 0.00 | 0.70 | 0.00 | 0.49 | -15.91 | 110.51 | 39.02 | 239.69 | 0.7036 | 370.0 | 363.5 | |
| 0.00 | 0.35 | 0.00 | 0.24 | -15.93 | 110.23 | 38.74 | 239.50 | 0.7007 | 403.0 | 385.8 | |
| 0.00 | 0.53 | 0.00 | 0.39 | -22.18 | 111.18 | 39.69 | 232.56 | 0.7471 | 443.0 | 403.2 | |
| 0.00 | 0.26 | 0.00 | 0.18 | -16.71 | 107.65 | 36.16 | 236.78 | 0.6778 | 417.0 | 464.7 | |
| 0.00 | 0.70 | 0.00 | 0.46 | -17.10 | 106.16 | 34.66 | 235.20 | 0.6643 | 515.0 | 458.2 | |
| 0.00 | 1.14 | 0.00 | 0.72 | -19.27 | 99.96 | 28.46 | 227.08 | 0.6166 | -697.0 | -450.8 | |
| 0.00 | 2.28 | 0.00 | 1.36 | -19.15 | 94.33 | 22.84 | 221.07 | 0.5603 | -630.0 | -504.4 | |
| 0.00 | 1.58 | 0.00 | 0.93 | -19.83 | 92.48 | 20.98 | 217.89 | 0.5506 | -753.0 | -643.1 | |
| 0.00 | 0.70 | 0.00 | 0.40 | -18.96 | 89.04 | 17.54 | 214.09 | 0.5107 | -214.0 | -196.1 | |
| 0.00 | 1.67 | 0.00 | 1.03 | -27.15 | 87.42 | 15.93 | 204.07 | 0.6011 | -646.0 | -580.3 | |
| 0.00 | 0.79 | 0.00 | 0.51 | -31.68 | 84.89 | 13.39 | 197.85 | 0.6454 | -334.0 | -284.0 | |
| 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. | |