SDO HMI 2013-08-23 10:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 45.65 | 272.84 | 26.55 | 158.56 | -7.05 | 139.52 | 28.30 | 244.14 | 0.5250 | 814.6 | 342.1 | |
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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 | 1.80 | 0.00 | 1.07 | -9.14 | 140.58 | 29.36 | 241.56 | 0.5526 | 658.0 | 419.7 | |
| 45.65 | 257.99 | 26.55 | 150.03 | -6.98 | 139.64 | 28.42 | 244.36 | 0.5260 | 1283.9 | 381.3 | |
| 0.00 | 0.99 | 0.00 | 0.57 | -4.83 | 139.49 | 28.26 | 248.05 | 0.5108 | -506.0 | -482.0 | |
| 0.00 | 0.90 | 0.00 | 0.53 | -9.57 | 138.90 | 27.68 | 239.38 | 0.5343 | 747.0 | 620.5 | |
| 0.00 | 0.99 | 0.00 | 0.56 | -5.11 | 138.51 | 27.28 | 246.77 | 0.4988 | -652.0 | -499.7 | |
| 0.00 | 0.81 | 0.00 | 0.46 | -6.39 | 137.65 | 26.42 | 243.68 | 0.4953 | 554.0 | 555.4 | |
| 0.00 | 1.08 | 0.00 | 0.62 | -6.98 | 137.61 | 26.39 | 242.59 | 0.4989 | 821.0 | 568.2 | |
| 0.00 | 1.17 | 0.00 | 0.69 | -13.55 | 137.65 | 26.42 | 231.97 | 0.5513 | -669.0 | -525.6 | |
| 0.00 | 1.53 | 0.00 | 0.87 | -6.91 | 136.79 | 25.56 | 241.96 | 0.4873 | -673.0 | -446.8 | |
| 0.00 | 1.35 | 0.00 | 0.79 | -13.08 | 136.69 | 25.46 | 231.64 | 0.5361 | -690.0 | -620.5 | |
| 0.00 | 2.25 | 0.00 | 1.25 | -5.19 | 135.46 | 24.24 | 243.92 | 0.4570 | -705.0 | -572.7 | |
| 0.00 | 1.35 | 0.00 | 0.76 | -9.77 | 135.16 | 23.93 | 235.19 | 0.4888 | -838.0 | -723.2 | |
| 0.00 | 0.63 | 0.00 | 0.36 | -10.03 | 135.18 | 23.95 | 234.79 | 0.4913 | -732.0 | -666.0 | |
| 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. | |