SDO HMI 2011-11-12 00:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 46.66 | 318.83 | 25.98 | 177.87 | 28.08 | 44.05 | -12.06 | 23.64 | 0.4615 | -1153.0 | -444.9 | |
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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 |
| 0.00 | 1.03 | 0.00 | 0.57 | 29.27 | 50.63 | -5.48 | 10.74 | 0.4486 | -664.0 | -495.0 | |
| 0.00 | 1.98 | 0.00 | 1.13 | 31.31 | 46.44 | -9.66 | 16.93 | 0.4944 | -915.0 | -732.7 | |
| 0.00 | 1.81 | 0.00 | 1.04 | 32.49 | 45.50 | -10.61 | 17.61 | 0.5154 | -210.0 | -176.6 | |
| 1.03 | 306.51 | 0.57 | 170.76 | 27.45 | 44.39 | -11.71 | 23.67 | 0.4506 | -1421.4 | -439.2 | |
| 38.74 | -4.00 | 21.57 | -4.00 | 27.90 | 44.14 | -11.97 | 23.66 | 0.4585 | -1368.4 | 999999 | |
| 1.21 | -4.00 | 0.67 | -4.00 | 28.36 | 44.02 | -12.09 | 23.42 | 0.4656 | -733.3 | 999999 | |
| 2.58 | -4.00 | 1.44 | -4.00 | 28.29 | 43.75 | -12.36 | 23.94 | 0.4663 | -897.6 | 999999 | |
| 1.72 | -4.00 | 0.96 | -4.00 | 28.00 | 43.58 | -12.53 | 24.52 | 0.4633 | -798.8 | 999999 | |
| 1.38 | -4.00 | 0.77 | -4.00 | 27.99 | 43.40 | -12.70 | 24.82 | 0.4644 | -806.0 | 999999 | |
| 0.00 | 1.38 | 0.00 | 0.84 | 36.62 | 41.49 | -14.61 | 20.16 | 0.5898 | -771.0 | -513.1 | |
| 0.00 | 1.21 | 0.00 | 0.74 | 37.11 | 40.66 | -15.44 | 20.81 | 0.6000 | -489.0 | -407.9 | |
| 0.00 | 2.15 | 0.00 | 1.21 | 28.27 | 41.50 | -14.61 | 27.62 | 0.4810 | -1013.0 | -773.7 | |
| 0.00 | 2.07 | 0.00 | 1.18 | 29.32 | 41.21 | -14.90 | 26.94 | 0.4968 | -899.0 | -668.0 | |
| 0.00 | 0.69 | 0.00 | 0.40 | 29.73 | 40.08 | -16.03 | 28.16 | 0.5100 | -718.0 | -611.5 | |
| 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. | |