SDO HMI 2014-01-06 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 | 14.24 | 0.00 | 8.50 | -17.43 | 79.97 | -31.03 | 116.85 | 0.5531 | 437.2 | 344.7 | |
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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 | 2.97 | 0.00 | 1.72 | -18.68 | 83.39 | -27.61 | 121.17 | 0.5153 | 886.0 | 678.5 | |
| 0.00 | 1.19 | 0.00 | 0.69 | -19.50 | 83.17 | -27.84 | 122.42 | 0.5235 | 732.0 | 544.4 | |
| 0.00 | 0.93 | 0.00 | 0.54 | -18.88 | 83.21 | -27.79 | 121.39 | 0.5189 | 526.0 | 540.6 | |
| 0.00 | 1.10 | 0.00 | 0.64 | -18.79 | 83.05 | -27.95 | 121.10 | 0.5203 | 618.0 | 531.0 | |
| 0.00 | 1.10 | 0.00 | 0.64 | -19.17 | 82.48 | -28.52 | 121.32 | 0.5300 | 689.0 | 564.9 | |
| 0.00 | 2.21 | 0.00 | 1.30 | -13.84 | 79.81 | -31.19 | 110.23 | 0.5380 | -786.0 | -543.1 | |
| 0.00 | 0.93 | 0.00 | 0.55 | -12.84 | 79.64 | -31.36 | 108.35 | 0.5368 | -586.0 | -463.5 | |
| 0.00 | 0.85 | 0.00 | 0.52 | -16.84 | 76.69 | -34.31 | 113.83 | 0.5921 | 724.0 | 617.9 | |
| 0.00 | 0.76 | 0.00 | 0.49 | -18.43 | 74.23 | -36.77 | 115.15 | 0.6297 | 726.0 | 647.1 | |
| 0.00 | 0.93 | 0.00 | 0.60 | -19.08 | 73.83 | -37.18 | 115.95 | 0.6374 | 670.0 | 513.6 | |
| 0.00 | 1.27 | 0.00 | 0.81 | -17.07 | 74.06 | -36.95 | 113.00 | 0.6266 | 610.0 | 499.4 | |
| 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. | |