SDO HMI 2014-10-10 06:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 62.35 | 370.44 | 49.07 | 292.02 | -20.55 | 18.52 | -44.17 | 122.87 | 0.7791 | 902.3 | 225.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.23 | 0.00 | 0.94 | -21.83 | 21.00 | -41.68 | 125.76 | 0.7631 | -485.0 | -364.1 | |
| 0.00 | 1.05 | 0.00 | 0.80 | -20.21 | 20.31 | -42.37 | 123.49 | 0.7606 | 662.0 | 640.2 | |
| 0.88 | 356.50 | 0.67 | 281.29 | -20.36 | 20.04 | -42.64 | 123.51 | 0.7640 | 893.6 | 227.5 | |
| 3.16 | -3.00 | 2.44 | -3.00 | -20.44 | 19.40 | -43.28 | 123.24 | 0.7704 | 993.5 | 999999 | |
| 0.00 | 0.96 | 0.00 | 0.74 | -19.27 | 19.63 | -43.06 | 122.00 | 0.7623 | 632.0 | 511.8 | |
| 0.00 | 1.58 | 0.00 | 1.19 | -17.76 | 19.67 | -43.01 | 120.24 | 0.7542 | 770.0 | 664.8 | |
| 55.85 | -3.00 | 44.05 | -3.00 | -20.62 | 18.45 | -44.24 | 122.92 | 0.7801 | 1057.5 | 999999 | |
| 1.32 | 4.21 | 0.99 | 3.18 | -17.72 | 19.33 | -43.35 | 120.01 | 0.7573 | 677.3 | 479.5 | |
| 0.00 | 1.14 | 0.00 | 0.97 | -23.86 | 16.31 | -46.37 | 125.39 | 0.8143 | 496.0 | 423.4 | |
| 1.14 | -3.00 | 0.92 | -3.00 | -20.86 | 17.45 | -45.23 | 122.66 | 0.7903 | 146.8 | 999999 | |
| 0.00 | 0.70 | 0.00 | 0.54 | -17.84 | 17.89 | -44.79 | 119.38 | 0.7719 | 180.0 | 129.1 | |
| 0.00 | 1.67 | 0.00 | 1.28 | -16.69 | 18.07 | -44.61 | 118.11 | 0.7649 | -612.0 | -525.8 | |
| 0.00 | 1.40 | 0.00 | 1.09 | -17.86 | 17.57 | -45.11 | 119.25 | 0.7751 | -558.0 | -429.6 | |
| 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. | |