SDO HMI 2014-01-10 17:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.46 | 0.00 | 9.27 | -19.98 | 66.10 | 4.46 | 196.13 | 0.3473 | -335.1 | -220.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.10 | 0.00 | 0.59 | -12.81 | 81.33 | 19.69 | 244.62 | 0.3653 | -651.0 | -537.5 | |
| 0.00 | 0.85 | 0.00 | 0.45 | -13.20 | 81.27 | 19.63 | 243.57 | 0.3668 | -702.0 | -565.2 | |
| 0.00 | 0.93 | 0.00 | 0.50 | -13.06 | 81.16 | 19.52 | 243.82 | 0.3643 | -882.0 | -691.4 | |
| 0.00 | 0.76 | 0.00 | 0.42 | -19.67 | 81.49 | 19.85 | 229.54 | 0.4220 | 725.0 | 593.6 | |
| 0.00 | 1.95 | 0.00 | 1.03 | -16.74 | 76.83 | 15.19 | 228.54 | 0.3362 | 918.0 | 831.4 | |
| 0.00 | 1.10 | 0.00 | 0.58 | -21.60 | 73.08 | 11.44 | 211.38 | 0.3557 | 799.0 | 642.8 | |
| 0.00 | 1.95 | 0.00 | 1.04 | -22.67 | 71.32 | 9.67 | 205.87 | 0.3569 | 761.0 | 591.7 | |
| 0.00 | 1.70 | 0.00 | 0.86 | -16.53 | 63.60 | 1.96 | 188.64 | 0.2191 | -873.0 | -699.5 | |
| 0.00 | 1.02 | 0.00 | 0.52 | -16.23 | 59.76 | -1.88 | 171.49 | 0.2138 | -962.0 | -835.2 | |
| 0.00 | 1.70 | 0.00 | 0.87 | -18.89 | 58.61 | -3.03 | 168.92 | 0.2617 | -858.0 | -734.4 | |
| 0.00 | 1.10 | 0.00 | 0.59 | -25.14 | 52.73 | -8.91 | 158.72 | 0.3881 | -898.0 | -777.5 | |
| 0.00 | 0.93 | 0.00 | 0.50 | -25.22 | 51.97 | -9.68 | 157.19 | 0.3940 | -737.0 | -592.0 | |
| 0.00 | 1.10 | 0.00 | 0.59 | -25.06 | 51.45 | -10.19 | 155.94 | 0.3949 | -648.0 | -585.2 | |
| 0.00 | 1.27 | 0.00 | 0.73 | -30.45 | 45.82 | -15.82 | 152.24 | 0.5066 | -684.0 | -594.7 | |
| 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. | |