SDO HMI 2014-03-30 07:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.90 | 43.75 | 10.48 | 23.04 | -24.28 | 116.05 | 9.57 | 206.40 | 0.3421 | -43.1 | 108.7 | |
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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 | 1.23 | 0.00 | 0.65 | -23.59 | 117.70 | 11.22 | 211.28 | 0.3450 | 821.0 | 660.3 | |
| 0.00 | 1.84 | 0.00 | 0.98 | -24.51 | 117.48 | 11.00 | 209.35 | 0.3558 | 800.0 | 651.4 | |
| 9.82 | 16.66 | 5.18 | 8.78 | -23.98 | 117.00 | 10.52 | 209.09 | 0.3446 | 1034.2 | 602.3 | |
| 0.00 | 0.88 | 0.00 | 0.46 | -23.54 | 116.90 | 10.42 | 209.54 | 0.3377 | -701.0 | -546.7 | |
| 0.00 | 0.88 | 0.00 | 0.46 | -24.43 | 116.77 | 10.29 | 207.90 | 0.3491 | 699.0 | 540.2 | |
| 0.00 | 1.75 | 0.00 | 0.93 | -24.27 | 116.69 | 10.21 | 207.95 | 0.3463 | 540.0 | 465.0 | |
| 0.00 | 2.63 | 0.00 | 1.39 | -24.72 | 116.32 | 9.85 | 206.48 | 0.3499 | 571.0 | 462.4 | |
| 0.00 | 1.05 | 0.00 | 0.55 | -23.85 | 115.56 | 9.08 | 205.91 | 0.3319 | -803.0 | -671.8 | |
| 0.00 | 0.61 | 0.00 | 0.32 | -24.29 | 115.39 | 8.91 | 204.88 | 0.3371 | -820.0 | -577.1 | |
| 0.00 | 0.79 | 0.00 | 0.41 | -24.10 | 115.31 | 8.83 | 204.94 | 0.3338 | -911.0 | -729.9 | |
| 10.08 | 14.47 | 5.30 | 7.61 | -24.62 | 114.82 | 8.34 | 203.05 | 0.3381 | -1066.1 | -746.1 | |
| 0.00 | 0.96 | 0.00 | 0.50 | -24.66 | 111.17 | 4.69 | 193.50 | 0.3199 | -785.0 | -709.4 | |
| 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. | |