SDO HMI 2014-10-05 03:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 66.46 | 335.87 | 36.58 | 184.95 | -1.35 | 154.91 | 24.61 | 253.04 | 0.4371 | 1028.6 | 383.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 48.53 | 297.62 | 26.78 | 164.24 | -1.38 | 155.24 | 24.94 | 253.23 | 0.4422 | 1318.5 | 379.4 | |
| 5.45 | -1.00 | 2.99 | -1.00 | -1.56 | 154.51 | 24.22 | 252.32 | 0.4322 | 1172.5 | 999999 | |
| 9.58 | 16.09 | 5.24 | 8.79 | -1.80 | 153.92 | 23.63 | 251.33 | 0.4247 | 1028.2 | 663.8 | |
| 0.00 | 0.97 | 0.00 | 0.53 | -1.12 | 153.62 | 23.33 | 252.63 | 0.4166 | 891.0 | 813.5 | |
| 0.00 | 0.88 | 0.00 | 0.48 | 0.24 | 153.56 | 23.26 | 255.75 | 0.4092 | 739.0 | 597.6 | |
| 2.90 | 9.23 | 1.57 | 5.00 | -0.21 | 153.36 | 23.06 | 254.56 | 0.4081 | 1062.4 | 833.5 | |
| 0.00 | 1.58 | 0.00 | 0.85 | 1.66 | 152.82 | 22.52 | 258.74 | 0.3921 | 879.0 | 698.2 | |
| 0.00 | 2.02 | 0.00 | 1.09 | 0.95 | 152.45 | 22.16 | 256.75 | 0.3891 | 834.0 | 742.8 | |
| 0.00 | 1.58 | 0.00 | 0.85 | 0.06 | 152.25 | 21.96 | 254.39 | 0.3899 | 784.0 | 582.4 | |
| 0.00 | 0.79 | 0.00 | 0.42 | -1.73 | 150.24 | 19.94 | 248.13 | 0.3690 | -636.0 | -496.2 | |
| 0.00 | 1.76 | 0.00 | 0.94 | -2.18 | 149.96 | 19.66 | 246.71 | 0.3676 | -808.0 | -719.2 | |
| 0.00 | 1.06 | 0.00 | 0.56 | -1.57 | 149.82 | 19.53 | 248.11 | 0.3617 | -823.0 | -552.1 | |
| 0.00 | 2.29 | 0.00 | 1.20 | -1.65 | 148.11 | 17.82 | 245.90 | 0.3365 | -845.0 | -668.6 | |
| 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. | |