SDO HMI 2014-01-14 08:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.82 | 110.40 | 88.51 | 542.59 | -10.11 | 98.71 | 84.81 | 260.24 | 0.9934 | 201.0 | 52.8 | |
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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 | 4.51 | 0.00 | 58.10 | -6.86 | 102.13 | 88.23 | 263.29 | 0.9994 | 115.0 | 143.5 | |
| 0.60 | 11.91 | 10.02 | 167.85 | -8.71 | 102.62 | 88.72 | 261.41 | 0.9996 | 264.0 | 75.2 | |
| 0.43 | -2.00 | 7.00 | -2.00 | -9.12 | 102.81 | 88.91 | 260.99 | 0.9997 | 204.8 | 999999 | |
| 13.44 | 58.85 | 50.19 | 225.71 | -10.87 | 96.93 | 83.02 | 259.62 | 0.9916 | 236.6 | -20.0 | |
| 0.00 | 2.30 | 0.00 | 6.87 | -9.78 | 95.02 | 81.11 | 260.82 | 0.9871 | 324.0 | 297.4 | |
| 0.43 | 3.40 | 1.26 | 10.07 | -11.46 | 95.08 | 81.17 | 259.11 | 0.9870 | 151.6 | 226.8 | |
| 1.53 | 7.23 | 4.03 | 18.69 | -10.96 | 93.72 | 79.82 | 259.68 | 0.9830 | -248.7 | -174.0 | |
| 2.13 | 4.25 | 6.00 | 12.11 | -12.62 | 94.50 | 80.59 | 257.95 | 0.9852 | 157.5 | 160.8 | |
| 0.00 | 1.79 | 0.00 | 4.98 | -13.33 | 94.36 | 80.45 | 257.24 | 0.9847 | 233.0 | 254.8 | |
| 0.43 | 1.62 | 1.04 | 3.92 | -12.54 | 92.82 | 78.91 | 258.10 | 0.9799 | -170.0 | -140.4 | |
| 0.00 | 0.94 | 0.00 | 2.18 | -12.87 | 92.41 | 78.50 | 257.78 | 0.9784 | -278.0 | -209.2 | |
| 0.00 | 6.63 | 0.00 | 15.76 | -14.20 | 92.60 | 78.69 | 256.42 | 0.9789 | 83.0 | 205.7 | |
| 0.00 | 0.51 | 0.00 | 1.16 | -13.97 | 92.00 | 78.10 | 256.67 | 0.9769 | -164.0 | -125.0 | |
| 3.83 | 6.46 | 8.97 | 15.19 | -14.55 | 92.42 | 78.51 | 256.07 | 0.9783 | 309.2 | 292.5 | |
| 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. | |