SDO HMI 2011-01-07 15:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.80 | 0.00 | 10.66 | -13.69 | 205.44 | 37.86 | 252.64 | 0.6270 | -704.0 | -634.8 | |
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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 | 0.76 | 0.00 | 0.49 | -13.90 | 206.82 | 39.24 | 252.74 | 0.6454 | -485.0 | -441.4 | |
| 0.00 | 1.87 | 0.00 | 1.21 | -14.08 | 206.71 | 39.12 | 252.42 | 0.6443 | -626.0 | -501.8 | |
| 0.00 | 0.59 | 0.00 | 0.38 | -13.61 | 206.49 | 38.91 | 253.08 | 0.6404 | -704.0 | -637.4 | |
| 0.00 | 0.76 | 0.00 | 0.49 | -13.70 | 205.89 | 38.30 | 252.78 | 0.6328 | -625.0 | -595.2 | |
| 0.00 | 1.19 | 0.00 | 0.75 | -13.86 | 205.45 | 37.87 | 252.38 | 0.6277 | -864.0 | -717.6 | |
| 0.00 | 1.95 | 0.00 | 1.24 | -13.59 | 205.40 | 37.82 | 252.79 | 0.6263 | -721.0 | -589.7 | |
| 0.00 | 1.27 | 0.00 | 0.80 | -13.36 | 205.17 | 37.59 | 253.08 | 0.6226 | -598.0 | -492.1 | |
| 0.00 | 1.53 | 0.00 | 0.97 | -13.63 | 205.14 | 37.56 | 252.64 | 0.6230 | -733.0 | -586.9 | |
| 0.00 | 1.19 | 0.00 | 0.75 | -13.87 | 205.19 | 37.61 | 252.28 | 0.6242 | -713.0 | -663.7 | |
| 0.00 | 3.82 | 0.00 | 2.40 | -13.47 | 204.84 | 37.26 | 252.82 | 0.6186 | -777.0 | -720.4 | |
| 0.00 | 1.87 | 0.00 | 1.18 | -13.86 | 204.88 | 37.30 | 252.21 | 0.6201 | -898.0 | -805.5 | |
| 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. | |