SDO HMI 2014-07-09 02:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37.59 | 185.17 | 18.93 | 93.07 | 6.27 | 204.45 | -9.29 | 74.04 | 0.1678 | -585.5 | -416.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.36 | 0.00 | 0.18 | 9.72 | 206.41 | -7.33 | 50.12 | 0.1646 | -600.0 | -605.0 | |
| 0.00 | 0.91 | 0.00 | 0.46 | 10.92 | 206.29 | -7.45 | 45.34 | 0.1798 | -967.0 | -819.6 | |
| 0.00 | 1.63 | 0.00 | 0.82 | 10.12 | 206.25 | -7.49 | 48.90 | 0.1712 | -838.0 | -739.7 | |
| 1.63 | 3.09 | 0.82 | 1.55 | 7.12 | 205.75 | -8.00 | 66.54 | 0.1512 | -1102.6 | -800.2 | |
| 24.16 | 152.39 | 12.12 | 76.48 | 6.20 | 204.92 | -8.82 | 73.91 | 0.1593 | -1433.4 | -458.7 | |
| 0.00 | 1.00 | 0.00 | 0.50 | 6.51 | 202.74 | -11.00 | 75.27 | 0.1970 | -589.0 | -501.0 | |
| 0.00 | 2.45 | 0.00 | 1.24 | 6.81 | 202.64 | -11.10 | 73.90 | 0.1999 | -822.0 | -584.3 | |
| 0.00 | 1.00 | 0.00 | 0.50 | 5.78 | 202.47 | -11.27 | 79.20 | 0.1988 | -631.0 | -464.8 | |
| 0.00 | 0.91 | 0.00 | 0.46 | 5.44 | 202.42 | -11.33 | 80.92 | 0.1989 | -827.0 | -680.4 | |
| 0.54 | 2.36 | 0.28 | 1.20 | 7.23 | 202.00 | -11.74 | 72.76 | 0.2123 | -847.2 | -706.5 | |
| 8.81 | 12.35 | 4.47 | 6.26 | 5.61 | 201.57 | -12.17 | 80.67 | 0.2136 | 1090.8 | 592.7 | |
| 2.45 | 4.09 | 1.24 | 2.07 | 6.16 | 201.56 | -12.18 | 78.15 | 0.2154 | 981.3 | 645.7 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 5.60 | 198.29 | -15.45 | 82.47 | 0.2687 | 708.0 | 607.6 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 8.21 | 197.69 | -16.05 | 73.55 | 0.2866 | 897.0 | 735.5 | |
| 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. | |