SDO HMI 2011-12-09 13:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30.92 | 119.54 | 29.40 | 112.81 | 9.00 | 355.28 | -57.85 | 79.29 | 0.8527 | -254.7 | -154.3 | |
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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 |
| 2.81 | 93.21 | 2.56 | 85.78 | 8.77 | 356.50 | -56.63 | 79.43 | 0.8418 | -694.5 | -258.9 | |
| 6.56 | -1.00 | 6.01 | -1.00 | 9.16 | 356.35 | -56.78 | 78.99 | 0.8435 | -876.4 | 999999 | |
| 4.26 | -1.00 | 3.92 | -1.00 | 9.49 | 356.21 | -56.92 | 78.62 | 0.8452 | -662.0 | 999999 | |
| 6.56 | -1.00 | 6.08 | -1.00 | 9.07 | 355.93 | -57.20 | 79.15 | 0.8473 | -443.8 | 999999 | |
| 1.53 | 2.98 | 1.46 | 2.84 | 8.99 | 354.93 | -58.19 | 79.37 | 0.8562 | -274.6 | -105.4 | |
| 4.52 | 6.65 | 4.36 | 6.41 | 8.72 | 354.43 | -58.70 | 79.73 | 0.8604 | -357.0 | -157.8 | |
| 0.00 | 0.60 | 0.00 | 0.59 | 8.99 | 353.77 | -59.36 | 79.49 | 0.8663 | -237.0 | -228.9 | |
| 0.00 | 1.53 | 0.00 | 1.51 | 7.73 | 353.67 | -59.46 | 80.95 | 0.8662 | 575.0 | 454.6 | |
| 1.02 | 2.47 | 1.06 | 2.55 | 9.11 | 352.16 | -60.97 | 79.52 | 0.8799 | 522.6 | 464.7 | |
| 0.00 | 0.51 | 0.00 | 0.54 | 8.55 | 351.31 | -61.81 | 80.24 | 0.8864 | 571.0 | 540.7 | |
| 0.00 | 1.70 | 0.00 | 1.83 | 8.43 | 350.90 | -62.23 | 80.41 | 0.8896 | 692.0 | 592.2 | |
| 3.66 | 6.48 | 3.95 | 6.97 | 8.07 | 350.74 | -62.39 | 80.83 | 0.8906 | 529.7 | 512.9 | |
| 0.00 | 0.77 | 0.00 | 0.84 | 8.79 | 350.53 | -62.60 | 80.04 | 0.8927 | 258.0 | 312.6 | |
| 0.00 | 0.77 | 0.00 | 0.85 | 8.76 | 350.14 | -62.98 | 80.11 | 0.8957 | 292.0 | 279.2 | |
| 0.00 | 1.87 | 0.00 | 2.10 | 8.64 | 349.71 | -63.42 | 80.28 | 0.8989 | 229.0 | 156.2 | |
| 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. | |