SDO HMI 2014-01-13 23:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.96 | 0.00 | 11.29 | 16.64 | 27.38 | 8.55 | 338.40 | 0.3895 | 34.7 | -165.9 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.44 | 0.00 | 0.77 | 14.98 | 29.92 | 11.10 | 330.66 | 0.3812 | -764.0 | -632.2 | |
| 0.00 | 4.16 | 0.00 | 2.24 | 15.89 | 29.88 | 11.06 | 331.93 | 0.3936 | -1070.0 | -870.6 | |
| 0.00 | 0.93 | 0.00 | 0.50 | 16.04 | 29.58 | 10.75 | 332.77 | 0.3935 | -666.0 | -559.6 | |
| 0.00 | 1.44 | 0.00 | 0.78 | 16.12 | 28.68 | 9.85 | 334.84 | 0.3883 | -787.0 | -669.2 | |
| 0.00 | 1.27 | 0.00 | 0.69 | 17.22 | 28.52 | 9.69 | 336.39 | 0.4033 | -757.0 | -633.4 | |
| 0.00 | 1.87 | 0.00 | 1.00 | 15.27 | 28.39 | 9.56 | 334.50 | 0.3740 | -761.0 | -591.2 | |
| 0.00 | 1.19 | 0.00 | 0.65 | 17.83 | 28.33 | 9.51 | 337.40 | 0.4109 | -729.0 | -618.3 | |
| 0.00 | 1.27 | 0.00 | 0.71 | 20.97 | 26.54 | 7.72 | 343.68 | 0.4481 | 532.0 | 367.9 | |
| 0.00 | 0.51 | 0.00 | 0.28 | 20.25 | 26.12 | 7.30 | 344.04 | 0.4355 | 750.0 | 638.5 | |
| 0.00 | 1.27 | 0.00 | 0.69 | 17.45 | 25.66 | 6.83 | 343.04 | 0.3908 | 966.0 | 828.9 | |
| 0.00 | 1.19 | 0.00 | 0.63 | 16.02 | 25.39 | 6.56 | 342.53 | 0.3675 | 830.0 | 607.1 | |
| 0.00 | 1.36 | 0.00 | 0.73 | 17.06 | 24.83 | 6.01 | 344.70 | 0.3811 | 661.0 | 551.5 | |
| 0.00 | 1.02 | 0.00 | 0.54 | 16.04 | 23.45 | 4.62 | 347.51 | 0.3596 | 847.0 | 708.7 | |
| 0.00 | 0.85 | 0.00 | 0.45 | 15.91 | 23.04 | 4.22 | 348.49 | 0.3562 | 783.0 | 689.1 | |
| 0.00 | 1.19 | 0.00 | 0.63 | 16.48 | 22.93 | 4.11 | 349.10 | 0.3649 | 685.0 | 488.9 | |
| 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. | |