SDO HMI 2013-08-18 16:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 43.28 | 278.28 | 26.97 | 173.66 | -7.07 | 139.17 | -34.83 | 111.10 | 0.6097 | 676.5 | 282.6 | |
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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 | 0.90 | 0.00 | 0.55 | -8.87 | 141.67 | -32.32 | 115.51 | 0.5875 | 555.0 | 460.9 | |
| 0.00 | 1.35 | 0.00 | 0.83 | -9.36 | 141.00 | -33.00 | 115.77 | 0.5989 | -593.0 | -589.6 | |
| 0.00 | 2.88 | 0.00 | 1.80 | -9.82 | 140.21 | -33.79 | 115.92 | 0.6115 | 661.0 | 620.3 | |
| 1.17 | 256.32 | 0.73 | 159.49 | -7.32 | 139.61 | -34.38 | 111.75 | 0.6052 | 974.5 | 338.7 | |
| 40.22 | -4.00 | 25.01 | -4.00 | -6.90 | 139.32 | -34.68 | 110.93 | 0.6069 | 1116.8 | 999999 | |
| 0.00 | 3.06 | 0.00 | 1.96 | -9.91 | 138.39 | -35.60 | 114.87 | 0.6343 | -876.0 | -673.9 | |
| 0.00 | 2.52 | 0.00 | 1.69 | -13.93 | 136.67 | -37.32 | 119.32 | 0.6772 | -633.0 | -593.0 | |
| 0.00 | 1.08 | 0.00 | 0.73 | -13.84 | 136.22 | -37.78 | 118.90 | 0.6817 | -693.0 | -594.0 | |
| 0.00 | 1.53 | 0.00 | 0.98 | -7.09 | 137.11 | -36.88 | 109.98 | 0.6360 | 740.0 | 575.5 | |
| 1.89 | 5.31 | 1.23 | 3.45 | -6.83 | 135.98 | -38.02 | 109.01 | 0.6491 | -770.3 | -611.8 | |
| 0.00 | 0.54 | 0.00 | 0.35 | -6.46 | 135.93 | -38.06 | 108.44 | 0.6480 | -631.0 | -613.0 | |
| 0.00 | 1.53 | 0.00 | 1.00 | -6.57 | 135.69 | -38.30 | 108.49 | 0.6516 | -506.0 | -482.5 | |
| 0.00 | 1.26 | 0.00 | 0.83 | -3.68 | 134.18 | -39.82 | 103.59 | 0.6597 | -707.0 | -588.3 | |
| 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. | |