SDO HMI 2014-01-13 16:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.93 | 23.77 | 0.50 | 12.63 | 16.19 | 26.40 | 3.72 | 350.02 | 0.3610 | 10.5 | -45.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.12 | 0.00 | 1.13 | 15.60 | 29.83 | 7.14 | 340.67 | 0.3632 | -767.0 | -604.8 | |
| 0.00 | 3.57 | 0.00 | 1.90 | 15.82 | 29.46 | 6.78 | 341.78 | 0.3647 | -1073.0 | -881.8 | |
| 0.00 | 1.19 | 0.00 | 0.63 | 15.72 | 29.24 | 6.56 | 342.25 | 0.3621 | -845.0 | -612.1 | |
| 0.00 | 1.02 | 0.00 | 0.54 | 16.00 | 28.98 | 6.29 | 343.17 | 0.3652 | -855.0 | -659.8 | |
| 0.00 | 1.19 | 0.00 | 0.64 | 17.10 | 28.61 | 5.92 | 344.92 | 0.3807 | -654.0 | -543.8 | |
| 0.34 | 2.29 | 0.18 | 1.21 | 15.51 | 26.38 | 3.69 | 349.66 | 0.3474 | -1037.0 | -799.1 | |
| 0.00 | 1.36 | 0.00 | 0.72 | 15.73 | 26.32 | 3.64 | 349.94 | 0.3508 | -597.0 | -428.4 | |
| 0.59 | 2.29 | 0.32 | 1.23 | 17.41 | 25.62 | 2.93 | 352.52 | 0.3760 | 939.6 | 748.7 | |
| 0.00 | 1.61 | 0.00 | 0.85 | 16.08 | 25.59 | 2.91 | 352.07 | 0.3545 | 947.0 | 868.7 | |
| 0.00 | 1.44 | 0.00 | 0.77 | 16.93 | 24.59 | 1.90 | 355.01 | 0.3665 | 726.0 | 582.3 | |
| 0.00 | 1.02 | 0.00 | 0.54 | 16.36 | 22.99 | 0.30 | 359.19 | 0.3559 | 801.0 | 562.7 | |
| 0.00 | 2.72 | 0.00 | 1.44 | 15.95 | 22.86 | 0.17 | 359.52 | 0.3491 | 748.0 | 769.4 | |
| 0.00 | 1.19 | 0.00 | 0.63 | 17.18 | 22.46 | -0.22 | 0.58 | 0.3693 | 857.0 | 783.9 | |
| 0.00 | 0.76 | 0.00 | 0.40 | 16.11 | 22.16 | -0.53 | 1.46 | 0.3518 | 848.0 | 627.4 | |
| 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. | |