SDO HMI 2014-10-01 22:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.51 | 129.57 | 42.88 | 350.62 | -16.15 | 249.32 | 76.69 | 252.05 | 0.9805 | -7.4 | 68.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.99 | 0.00 | 26.01 | -17.67 | 256.51 | 83.88 | 251.70 | 0.9981 | 171.0 | 71.7 | |
| 0.00 | 3.70 | 0.00 | 13.11 | -16.48 | 252.14 | 79.51 | 252.23 | 0.9907 | 207.0 | 231.3 | |
| 0.00 | 10.65 | 0.00 | 66.97 | -18.04 | 254.83 | 82.20 | 251.09 | 0.9962 | 113.0 | 77.8 | |
| 0.00 | 5.37 | 0.00 | 15.76 | -16.03 | 250.49 | 77.86 | 252.41 | 0.9865 | 211.0 | 196.6 | |
| 0.00 | 5.46 | 0.00 | 15.15 | -15.62 | 249.95 | 77.32 | 252.73 | 0.9847 | 249.0 | 214.1 | |
| 0.00 | 0.26 | 0.00 | 0.68 | -15.03 | 249.24 | 76.61 | 253.20 | 0.9823 | 342.0 | 312.3 | |
| 0.00 | 1.85 | 0.00 | 8.68 | -18.18 | 253.78 | 81.15 | 250.80 | 0.9946 | 96.0 | 63.0 | |
| 2.20 | 13.20 | 5.44 | 32.42 | -15.84 | 248.56 | 75.93 | 252.27 | 0.9806 | 391.4 | 321.3 | |
| 1.41 | -8.00 | 3.47 | -8.00 | -16.08 | 248.45 | 75.81 | 252.01 | 0.9804 | 72.6 | 999999 | |
| 3.43 | 75.09 | 7.25 | 147.67 | -14.95 | 246.66 | 74.02 | 252.81 | 0.9733 | 514.9 | -47.2 | |
| 5.11 | -10.00 | 9.82 | -10.00 | -14.73 | 245.24 | 72.61 | 252.77 | 0.9674 | -415.2 | 999999 | |
| 3.08 | 7.57 | 7.00 | 17.11 | -16.93 | 247.29 | 74.66 | 250.94 | 0.9771 | 377.1 | 251.5 | |
| 0.44 | 3.43 | 0.91 | 7.06 | -16.44 | 246.07 | 73.44 | 251.20 | 0.9722 | 91.4 | -106.5 | |
| 4.84 | -10.00 | 8.99 | -10.00 | -15.01 | 244.65 | 72.02 | 252.37 | 0.9652 | -725.3 | 999999 | |
| 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. | |