SDO HMI 2014-01-14 13:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.59 | 49.08 | 11.46 | 27.26 | 16.39 | 28.21 | 17.04 | 321.65 | 0.4546 | -262.2 | -163.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.41 | 16.92 | 6.96 | 9.49 | 16.15 | 30.22 | 19.05 | 318.02 | 0.4706 | -980.2 | -629.8 | |
| 0.00 | 1.11 | 0.00 | 0.62 | 16.46 | 29.92 | 18.75 | 318.91 | 0.4710 | -498.0 | -399.5 | |
| 0.00 | 1.87 | 0.00 | 1.04 | 15.80 | 29.86 | 18.69 | 318.02 | 0.4629 | -964.0 | -729.4 | |
| 0.00 | 2.98 | 0.00 | 1.66 | 16.01 | 29.65 | 18.48 | 318.66 | 0.4632 | -888.0 | -759.2 | |
| 1.79 | 4.68 | 0.99 | 2.60 | 15.87 | 29.09 | 17.92 | 319.31 | 0.4559 | -972.0 | -746.5 | |
| 2.64 | 5.27 | 1.46 | 2.93 | 15.99 | 28.68 | 17.51 | 320.13 | 0.4531 | -1036.5 | -809.5 | |
| 0.00 | 1.45 | 0.00 | 0.80 | 16.18 | 28.57 | 17.40 | 320.58 | 0.4542 | -860.0 | -696.6 | |
| 0.00 | 1.45 | 0.00 | 0.79 | 16.84 | 25.78 | 14.61 | 326.25 | 0.4363 | 896.0 | 688.0 | |
| 0.00 | 0.85 | 0.00 | 0.48 | 20.28 | 26.06 | 14.89 | 329.94 | 0.4831 | 662.0 | 573.8 | |
| 1.87 | 5.95 | 1.03 | 3.28 | 17.22 | 25.75 | 14.58 | 326.81 | 0.4410 | 899.2 | 668.6 | |
| 0.43 | -10.00 | 0.23 | -10.00 | 17.09 | 25.64 | 14.47 | 326.83 | 0.4384 | 968.4 | 999999 | |
| 1.45 | 2.55 | 0.79 | 1.40 | 16.98 | 24.84 | 13.67 | 328.16 | 0.4301 | 905.2 | 776.8 | |
| 0.00 | 1.19 | 0.00 | 0.65 | 16.21 | 24.24 | 13.07 | 328.29 | 0.4150 | 852.0 | 706.1 | |
| 0.00 | 1.79 | 0.00 | 0.96 | 15.90 | 22.68 | 11.51 | 331.04 | 0.3982 | 920.0 | 826.1 | |
| 0.00 | 1.02 | 0.00 | 0.56 | 18.42 | 20.60 | 9.43 | 338.17 | 0.4199 | 718.0 | 586.1 | |
| 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. | |