SDO HMI 2014-01-13 03:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.68 | 19.84 | 0.36 | 10.56 | 16.67 | 24.41 | -5.39 | 13.89 | 0.3728 | 290.4 | 267.8 | |
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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 | 0.77 | 0.00 | 0.40 | 16.05 | 28.08 | -1.72 | 4.72 | 0.3514 | -969.0 | -787.1 | |
| 0.00 | 1.96 | 0.00 | 1.03 | 16.15 | 27.90 | -1.90 | 5.20 | 0.3532 | -808.0 | -658.2 | |
| 0.68 | 2.47 | 0.36 | 1.31 | 16.71 | 27.61 | -2.18 | 5.80 | 0.3629 | -884.9 | -661.2 | |
| 0.00 | 0.77 | 0.00 | 0.41 | 16.91 | 26.13 | -3.67 | 9.58 | 0.3693 | 601.0 | 473.1 | |
| 0.00 | 1.02 | 0.00 | 0.54 | 15.56 | 25.63 | -4.17 | 11.61 | 0.3491 | -783.0 | -634.4 | |
| 0.00 | 1.02 | 0.00 | 0.54 | 16.89 | 24.56 | -5.24 | 13.58 | 0.3742 | 657.0 | 527.8 | |
| 0.00 | 1.11 | 0.00 | 0.59 | 15.83 | 23.78 | -6.02 | 16.31 | 0.3607 | 937.0 | 763.8 | |
| 0.00 | 1.19 | 0.00 | 0.63 | 16.08 | 23.74 | -6.05 | 16.20 | 0.3648 | 947.0 | 701.5 | |
| 0.00 | 1.70 | 0.00 | 0.90 | 16.05 | 23.38 | -6.42 | 17.16 | 0.3661 | 742.0 | 629.8 | |
| 0.00 | 0.94 | 0.00 | 0.50 | 15.96 | 23.16 | -6.64 | 17.77 | 0.3657 | 722.0 | 560.4 | |
| 0.00 | 1.19 | 0.00 | 0.64 | 17.01 | 22.66 | -7.14 | 18.09 | 0.3843 | 966.0 | 866.9 | |
| 0.00 | 1.28 | 0.00 | 0.69 | 17.45 | 22.24 | -7.56 | 18.69 | 0.3933 | 816.0 | 639.9 | |
| 0.00 | 3.06 | 0.00 | 1.64 | 16.73 | 22.08 | -7.72 | 19.71 | 0.3831 | 832.0 | 688.4 | |
| 0.00 | 1.36 | 0.00 | 0.74 | 19.38 | 21.84 | -7.96 | 18.01 | 0.4243 | 714.0 | 484.5 | |
| 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. | |