SDO HMI 2014-04-03 11:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.31 | 57.73 | 15.12 | 39.15 | -8.09 | 8.13 | -43.39 | 95.06 | 0.6842 | 257.1 | 210.2 | |
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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 | 0.79 | 0.00 | 0.50 | -9.17 | 12.70 | -38.82 | 96.69 | 0.6254 | 582.0 | 422.2 | |
| 0.00 | 1.05 | 0.00 | 0.68 | -5.80 | 10.99 | -40.54 | 91.42 | 0.6491 | 573.0 | 418.7 | |
| 15.20 | 30.58 | 10.00 | 20.08 | -8.53 | 10.08 | -41.44 | 95.65 | 0.6600 | 886.6 | 463.6 | |
| 0.00 | 4.92 | 0.00 | 3.26 | -8.61 | 9.50 | -42.02 | 95.76 | 0.6676 | 565.0 | 495.8 | |
| 1.14 | 2.64 | 0.76 | 1.76 | -8.53 | 9.22 | -42.30 | 95.64 | 0.6711 | 568.8 | 470.6 | |
| 0.00 | 0.97 | 0.00 | 0.65 | -7.78 | 8.87 | -42.65 | 94.53 | 0.6757 | 505.0 | 497.9 | |
| 0.00 | 1.23 | 0.00 | 0.83 | -8.71 | 8.49 | -43.03 | 95.92 | 0.6804 | 525.0 | 498.4 | |
| 0.00 | 0.62 | 0.00 | 0.45 | -5.90 | 4.21 | -47.31 | 92.11 | 0.7340 | -541.0 | -481.0 | |
| 5.97 | 9.40 | 4.36 | 6.87 | -7.44 | 3.87 | -47.65 | 94.23 | 0.7371 | -734.7 | -477.6 | |
| 0.00 | 1.58 | 0.00 | 1.16 | -7.14 | 3.51 | -48.01 | 93.84 | 0.7415 | -542.0 | -377.3 | |
| 0.00 | 1.23 | 0.00 | 0.90 | -5.89 | 3.67 | -47.85 | 92.13 | 0.7403 | -370.0 | -357.1 | |
| 0.00 | 1.14 | 0.00 | 0.84 | -7.15 | 3.24 | -48.29 | 93.86 | 0.7447 | -470.0 | -373.7 | |
| 0.00 | 1.58 | 0.00 | 1.17 | -6.99 | 3.12 | -48.40 | 93.65 | 0.7461 | -463.0 | -385.8 | |
| 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. | |