SDO HMI 2014-01-11 14:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 73.34 | 453.44 | 45.89 | 284.66 | -16.31 | 13.69 | -36.44 | 111.45 | 0.6146 | 891.9 | 292.2 | |
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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 | 0.85 | 0.00 | 0.50 | -17.37 | 18.75 | -31.37 | 115.63 | 0.5533 | 772.0 | 616.0 | |
| 49.37 | 442.07 | 30.70 | 276.63 | -16.34 | 14.29 | -35.84 | 111.73 | 0.6071 | 1194.2 | 314.3 | |
| 1.87 | -2.00 | 1.17 | -2.00 | -16.13 | 13.61 | -36.52 | 111.12 | 0.6151 | 905.8 | 999999 | |
| 2.89 | -2.00 | 1.82 | -2.00 | -16.30 | 13.42 | -36.71 | 111.32 | 0.6181 | 1057.2 | 999999 | |
| 16.15 | -2.00 | 10.19 | -2.00 | -16.10 | 13.04 | -37.09 | 110.87 | 0.6223 | 1002.9 | 999999 | |
| 2.04 | -2.00 | 1.29 | -2.00 | -16.06 | 12.63 | -37.50 | 110.64 | 0.6274 | 510.5 | 999999 | |
| 0.00 | 0.93 | 0.00 | 0.64 | -16.58 | 7.50 | -42.62 | 109.76 | 0.6920 | -715.0 | -653.8 | |
| 0.00 | 2.72 | 0.00 | 1.96 | -19.39 | 4.97 | -45.15 | 112.91 | 0.7284 | -727.0 | -540.3 | |
| 1.02 | 2.97 | 0.72 | 2.09 | -15.37 | 5.71 | -44.41 | 107.60 | 0.7103 | -707.0 | -411.0 | |
| 0.00 | 0.85 | 0.00 | 0.62 | -19.03 | 4.57 | -45.56 | 112.31 | 0.7320 | -577.0 | -498.7 | |
| 0.00 | 1.10 | 0.00 | 0.80 | -17.86 | 4.61 | -45.52 | 110.76 | 0.7286 | -639.0 | -475.5 | |
| 0.00 | 0.93 | 0.00 | 0.68 | -18.16 | 4.42 | -45.71 | 111.11 | 0.7314 | -601.0 | -545.3 | |
| 0.00 | 1.02 | 0.00 | 0.74 | -17.17 | 4.21 | -45.91 | 109.72 | 0.7314 | -356.0 | -283.0 | |
| 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. | |