SDO HMI 2014-10-05 10:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.05 | 29.17 | 5.64 | 17.64 | 13.02 | 91.80 | -34.66 | 76.69 | 0.5712 | 31.4 | 29.2 | |
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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 | 1.05 | 0.00 | 0.57 | 9.89 | 102.72 | -23.74 | 80.19 | 0.4043 | -715.0 | -614.4 | |
| 0.00 | 1.05 | 0.00 | 0.57 | 9.62 | 102.27 | -24.19 | 80.94 | 0.4108 | -590.0 | -534.5 | |
| 0.00 | 0.70 | 0.00 | 0.39 | 12.94 | 99.10 | -27.36 | 74.45 | 0.4669 | -651.0 | -545.1 | |
| 0.00 | 0.70 | 0.00 | 0.39 | 12.40 | 99.09 | -27.37 | 75.60 | 0.4655 | -663.0 | -433.8 | |
| 0.00 | 0.97 | 0.00 | 0.55 | 14.59 | 97.41 | -29.05 | 71.80 | 0.4967 | -743.0 | -638.2 | |
| 0.00 | 0.79 | 0.00 | 0.45 | 6.87 | 97.00 | -29.47 | 87.53 | 0.4908 | -639.0 | -498.8 | |
| 0.00 | 1.14 | 0.00 | 0.65 | 8.22 | 96.44 | -30.02 | 84.79 | 0.4992 | -719.0 | -561.2 | |
| 0.00 | 1.85 | 0.00 | 1.06 | 10.31 | 95.54 | -30.92 | 80.75 | 0.5143 | -765.0 | -433.8 | |
| 0.00 | 0.97 | 0.00 | 0.56 | 10.75 | 95.28 | -31.19 | 79.94 | 0.5188 | -754.0 | -515.3 | |
| 0.00 | 0.97 | 0.00 | 0.56 | 11.00 | 94.89 | -31.57 | 79.53 | 0.5248 | -552.0 | -487.1 | |
| 0.00 | 0.79 | 0.00 | 0.50 | 19.45 | 88.83 | -37.63 | 66.83 | 0.6285 | 668.0 | 516.9 | |
| 0.00 | 1.67 | 0.00 | 1.08 | 21.26 | 87.90 | -38.57 | 64.44 | 0.6463 | 659.0 | 465.3 | |
| 9.05 | 14.59 | 5.64 | 9.09 | 13.21 | 89.16 | -37.30 | 76.69 | 0.6085 | 905.9 | 585.0 | |
| 0.00 | 0.79 | 0.00 | 0.50 | 13.31 | 88.72 | -37.75 | 76.62 | 0.6146 | 311.0 | 355.4 | |
| 0.00 | 1.14 | 0.00 | 0.72 | 13.44 | 88.06 | -38.40 | 76.52 | 0.6235 | 661.0 | 552.3 | |
| 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. | |