SDO HMI 2014-12-04 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 |
| 0.00 | 11.53 | 0.00 | 7.57 | 13.09 | 18.12 | -38.83 | 70.23 | 0.6494 | -485.3 | -397.8 | |
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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 | 1.11 | 0.00 | 0.65 | 11.11 | 26.49 | -30.47 | 69.55 | 0.5332 | -589.0 | -434.8 | |
| 0.00 | 0.85 | 0.00 | 0.52 | 16.79 | 24.33 | -32.62 | 61.34 | 0.5905 | -637.0 | -560.8 | |
| 0.00 | 0.77 | 0.00 | 0.47 | 15.01 | 23.67 | -33.29 | 64.56 | 0.5893 | -574.0 | -469.8 | |
| 0.00 | 0.94 | 0.00 | 0.57 | 6.02 | 22.67 | -34.28 | 80.08 | 0.5709 | -237.0 | -264.3 | |
| 0.00 | 0.94 | 0.00 | 0.60 | 15.18 | 19.96 | -37.00 | 66.26 | 0.6368 | -565.0 | -503.1 | |
| 0.00 | 1.54 | 0.00 | 1.03 | 15.69 | 17.02 | -39.94 | 66.85 | 0.6745 | -518.0 | -462.4 | |
| 0.00 | 1.20 | 0.00 | 0.79 | 13.53 | 17.41 | -39.55 | 69.81 | 0.6619 | -688.0 | -528.4 | |
| 0.00 | 0.68 | 0.00 | 0.45 | 9.49 | 17.26 | -39.69 | 75.88 | 0.6519 | -535.0 | -489.0 | |
| 0.00 | 0.60 | 0.00 | 0.39 | 8.92 | 17.18 | -39.77 | 76.77 | 0.6516 | -695.0 | -686.7 | |
| 0.00 | 1.28 | 0.00 | 0.84 | 8.92 | 16.99 | -39.97 | 76.82 | 0.6541 | -682.0 | -580.7 | |
| 0.00 | 0.68 | 0.00 | 0.45 | 9.21 | 16.40 | -40.56 | 76.52 | 0.6624 | -514.0 | -405.2 | |
| 0.00 | 0.94 | 0.00 | 0.81 | 21.41 | 4.81 | -52.15 | 63.90 | 0.8208 | 410.0 | 354.7 | |
| 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. | |