SDO HMI 2014-04-24 23:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.52 | 56.18 | 21.39 | 55.32 | -10.37 | 187.66 | 60.02 | 260.75 | 0.8647 | 215.9 | -48.3 | |
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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 |
| 6.76 | 32.36 | 6.89 | 33.16 | -10.08 | 188.98 | 61.33 | 261.12 | 0.8763 | 540.3 | -12.6 | |
| 6.40 | -1.00 | 6.53 | -1.00 | -10.32 | 188.93 | 61.29 | 260.84 | 0.8760 | 514.1 | 999999 | |
| 4.27 | 6.93 | 4.30 | 7.00 | -9.46 | 188.59 | 60.95 | 261.83 | 0.8731 | 602.1 | 320.9 | |
| 0.00 | 0.62 | 0.00 | 0.58 | -10.85 | 185.84 | 58.20 | 260.19 | 0.8492 | -221.0 | -205.7 | |
| 0.00 | 1.51 | 0.00 | 1.38 | -10.20 | 185.07 | 57.43 | 260.94 | 0.8420 | -532.0 | -425.2 | |
| 0.00 | 2.40 | 0.00 | 2.20 | -10.83 | 185.20 | 57.56 | 260.19 | 0.8433 | -492.0 | -423.7 | |
| 0.00 | 1.24 | 0.00 | 1.13 | -11.13 | 184.89 | 57.24 | 259.83 | 0.8405 | -398.0 | -307.1 | |
| 4.09 | 5.96 | 3.67 | 5.34 | -10.83 | 184.40 | 56.76 | 260.18 | 0.8358 | -589.2 | -407.0 | |
| 0.00 | 2.49 | 0.00 | 2.22 | -12.16 | 184.13 | 56.49 | 258.56 | 0.8337 | -153.0 | -148.4 | |
| 0.00 | 0.36 | 0.00 | 0.31 | -11.25 | 182.70 | 55.06 | 259.61 | 0.8196 | -282.0 | -461.5 | |
| 0.00 | 2.31 | 0.00 | 2.00 | -12.24 | 182.94 | 55.30 | 258.40 | 0.8223 | 700.0 | 441.4 | |
| 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. | |