SDO HMI 2011-11-03 04:58:59 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.06 | 110.74 | 79.12 | 410.59 | 6.46 | 254.98 | 82.40 | 275.98 | 0.9879 | 326.9 | -39.9 | |
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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 |
| 0.69 | 63.41 | 3.65 | 331.40 | 5.62 | 257.47 | 84.89 | 275.26 | 0.9959 | 369.2 | 10.4 | |
| 8.13 | -1.00 | 41.34 | -1.00 | 6.14 | 257.39 | 84.81 | 275.77 | 0.9957 | 757.2 | 999999 | |
| 5.45 | -1.00 | 24.99 | -1.00 | 6.07 | 256.66 | 84.08 | 275.66 | 0.9944 | -305.4 | 999999 | |
| 1.12 | 31.32 | 1.99 | 54.45 | 7.89 | 246.73 | 74.16 | 277.01 | 0.9613 | 362.8 | -326.8 | |
| 0.00 | 2.34 | 0.00 | 3.75 | 7.59 | 245.00 | 72.42 | 276.63 | 0.9527 | -36.0 | -89.6 | |
| 0.00 | 1.56 | 0.00 | 2.52 | 7.94 | 245.15 | 72.58 | 277.00 | 0.9534 | -452.0 | -384.9 | |
| 0.78 | 7.18 | 1.21 | 11.05 | 8.29 | 244.41 | 71.84 | 277.35 | 0.9494 | -257.8 | 279.0 | |
| 2.42 | -7.00 | 3.72 | -7.00 | 8.04 | 244.20 | 71.63 | 277.07 | 0.9483 | 406.9 | 999999 | |
| 1.04 | -7.00 | 1.60 | -7.00 | 8.28 | 244.12 | 71.54 | 277.33 | 0.9478 | 286.1 | 999999 | |
| 0.00 | 0.61 | 0.00 | 0.93 | 8.70 | 244.21 | 71.63 | 277.77 | 0.9483 | -95.0 | 24.6 | |
| 0.00 | 1.30 | 0.00 | 1.98 | 8.50 | 244.02 | 71.45 | 277.56 | 0.9473 | 230.0 | 169.5 | |
| 0.00 | 1.38 | 0.00 | 2.16 | 11.10 | 244.52 | 71.94 | 280.31 | 0.9497 | 201.0 | 150.1 | |
| 0.43 | 1.64 | 0.62 | 2.35 | 8.45 | 242.61 | 70.03 | 277.46 | 0.9392 | 407.6 | 322.5 | |
| 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. | |