SDO HMI 2014-09-16 06:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.48 | 212.70 | 45.47 | 281.20 | 15.44 | 88.51 | 69.10 | 283.79 | 0.9288 | 503.9 | 190.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.22 | 154.29 | 34.88 | 205.05 | 14.84 | 88.63 | 69.22 | 283.15 | 0.9297 | 683.3 | 233.8 | |
| 2.04 | 22.40 | 2.79 | 30.48 | 16.80 | 89.24 | 69.83 | 285.28 | 0.9331 | -4.3 | 13.6 | |
| 0.00 | 2.31 | 0.00 | 3.08 | 17.55 | 88.77 | 69.36 | 286.07 | 0.9301 | -89.0 | -83.8 | |
| 0.00 | 0.27 | 0.00 | 0.35 | 17.12 | 88.41 | 69.00 | 285.60 | 0.9279 | 157.0 | 180.0 | |
| 0.00 | 1.16 | 0.00 | 1.52 | 17.34 | 88.41 | 69.00 | 285.84 | 0.9279 | 121.0 | 117.2 | |
| 0.00 | 1.16 | 0.00 | 1.50 | 17.29 | 88.02 | 68.60 | 285.78 | 0.9255 | 121.0 | 155.0 | |
| 0.00 | 0.89 | 0.00 | 1.20 | 18.83 | 89.18 | 69.76 | 287.45 | 0.9325 | -266.0 | -235.5 | |
| 4.89 | 15.91 | 6.22 | 20.34 | 17.27 | 87.57 | 68.16 | 285.76 | 0.9226 | 557.7 | 261.3 | |
| 0.00 | 4.27 | 0.00 | 5.31 | 16.58 | 87.04 | 67.63 | 285.00 | 0.9193 | 555.0 | 420.6 | |
| 0.00 | 3.91 | 0.00 | 5.13 | 18.76 | 88.38 | 68.97 | 287.37 | 0.9277 | -592.0 | -444.4 | |
| 0.00 | 1.24 | 0.00 | 1.52 | 16.67 | 86.53 | 67.12 | 285.09 | 0.9158 | 228.0 | 237.6 | |
| 1.33 | 3.20 | 1.58 | 3.80 | 15.76 | 85.74 | 66.33 | 284.08 | 0.9105 | 454.3 | 374.6 | |
| 0.00 | 0.71 | 0.00 | 0.79 | 13.61 | 83.89 | 64.48 | 281.66 | 0.8974 | -490.0 | -465.2 | |
| 0.00 | 0.71 | 0.00 | 0.82 | 17.03 | 85.03 | 65.62 | 285.48 | 0.9055 | 397.0 | 365.5 | |
| 0.00 | 0.27 | 0.00 | 0.31 | 17.71 | 85.43 | 66.02 | 286.23 | 0.9083 | 306.0 | 345.7 | |
| 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. | |