SDO HMI 2014-12-10 07:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 56.61 | 322.35 | 30.55 | 174.08 | -3.82 | 1.08 | 23.19 | 261.04 | 0.3995 | 1014.8 | 362.0 | |
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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 | 1.45 | 0.00 | 0.83 | -3.11 | 7.78 | 29.89 | 264.27 | 0.5022 | 749.0 | 556.4 | |
| 35.13 | 293.11 | 19.01 | 158.46 | -4.00 | 1.41 | 23.52 | 260.69 | 0.4051 | 1308.1 | 407.7 | |
| 0.77 | -2.00 | 0.41 | -2.00 | -3.47 | 1.14 | 23.24 | 261.92 | 0.3996 | 678.9 | 999999 | |
| 0.51 | 1.79 | 0.28 | 0.96 | -2.58 | 0.99 | 23.10 | 264.10 | 0.3957 | 868.8 | 708.3 | |
| 0.00 | 1.28 | 0.00 | 0.69 | -2.88 | 1.00 | 23.10 | 263.36 | 0.3963 | 787.0 | 641.0 | |
| 1.11 | 3.67 | 0.60 | 1.97 | -1.55 | 0.94 | 23.05 | 266.72 | 0.3938 | -1007.2 | -788.2 | |
| 15.60 | -2.00 | 8.40 | -2.00 | -3.80 | 0.79 | 22.90 | 260.98 | 0.3948 | 1359.1 | 999999 | |
| 0.00 | 1.45 | 0.00 | 0.78 | -2.38 | 0.76 | 22.87 | 264.58 | 0.3917 | 640.0 | 551.1 | |
| 0.00 | 1.02 | 0.00 | 0.55 | -1.61 | 0.72 | 22.83 | 266.54 | 0.3902 | -817.0 | -666.2 | |
| 0.00 | 0.94 | 0.00 | 0.50 | -5.07 | 359.71 | 21.82 | 257.25 | 0.3812 | 976.0 | 900.9 | |
| 0.00 | 1.02 | 0.00 | 0.55 | -2.76 | 359.59 | 21.69 | 263.27 | 0.3734 | 744.0 | 494.8 | |
| 0.00 | 1.45 | 0.00 | 0.77 | -1.82 | 359.16 | 21.27 | 265.73 | 0.3651 | 1057.0 | 880.4 | |
| 0.68 | 2.73 | 0.36 | 1.45 | -2.73 | 358.92 | 21.03 | 263.16 | 0.3625 | 832.5 | 529.5 | |
| 0.00 | 1.19 | 0.00 | 0.63 | -3.68 | 358.87 | 20.98 | 260.55 | 0.3638 | 756.0 | 644.6 | |
| 2.81 | 11.25 | 1.49 | 5.94 | -3.12 | 358.01 | 20.12 | 261.77 | 0.3485 | -1079.2 | -910.4 | |
| 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. | |