SDO HMI 2011-11-27 03:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.90 | 25.42 | 7.13 | 18.66 | 8.80 | 263.44 | 46.71 | 280.95 | 0.7282 | -269.7 | -59.1 | |
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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 | 1.20 | 0.00 | 1.06 | 9.99 | 272.45 | 55.72 | 281.11 | 0.8314 | -694.0 | -558.6 | |
| 0.00 | 1.28 | 0.00 | 1.10 | 8.16 | 271.23 | 54.50 | 279.00 | 0.8182 | 566.0 | 503.4 | |
| 1.45 | 1.80 | 1.26 | 1.55 | 10.52 | 271.42 | 54.69 | 281.86 | 0.8220 | -460.8 | -430.0 | |
| 7.45 | 8.13 | 5.87 | 6.41 | 8.38 | 267.55 | 50.82 | 279.64 | 0.7802 | -616.1 | -533.1 | |
| 0.00 | 1.45 | 0.00 | 1.15 | 9.55 | 267.64 | 50.91 | 281.12 | 0.7823 | -581.0 | -445.5 | |
| 0.00 | 0.60 | 0.00 | 0.44 | 9.23 | 263.85 | 47.12 | 281.23 | 0.7398 | -336.0 | -320.9 | |
| 0.00 | 1.11 | 0.00 | 0.82 | 9.38 | 263.79 | 47.06 | 281.44 | 0.7393 | -495.0 | -446.3 | |
| 0.00 | 2.23 | 0.00 | 1.51 | 9.21 | 259.43 | 42.70 | 281.98 | 0.6867 | -641.0 | -537.6 | |
| 0.00 | 0.77 | 0.00 | 0.51 | 7.62 | 258.13 | 41.39 | 279.88 | 0.6676 | -656.0 | -532.3 | |
| 0.00 | 1.63 | 0.00 | 0.98 | 8.74 | 250.96 | 34.23 | 283.32 | 0.5736 | 424.0 | 401.9 | |
| 0.00 | 0.94 | 0.00 | 0.57 | 8.47 | 250.90 | 34.17 | 282.88 | 0.5720 | 566.0 | 412.5 | |
| 0.00 | 2.05 | 0.00 | 1.23 | 7.97 | 250.42 | 33.69 | 282.15 | 0.5640 | 592.0 | 443.9 | |
| 0.00 | 2.23 | 0.00 | 1.33 | 8.19 | 249.93 | 33.20 | 282.67 | 0.5577 | 562.0 | 529.3 | |
| 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. | |