SDO HMI 2014-04-04 06:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.33 | 45.30 | 8.40 | 26.43 | -8.36 | 9.04 | -32.03 | 95.63 | 0.5291 | 570.6 | 489.8 | |
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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 | 1.85 | 0.00 | 1.04 | -8.76 | 12.59 | -28.48 | 96.65 | 0.4764 | 931.0 | 694.1 | |
| 0.00 | 0.79 | 0.00 | 0.45 | -8.78 | 12.38 | -28.69 | 96.67 | 0.4796 | 621.0 | 562.9 | |
| 0.00 | 1.06 | 0.00 | 0.60 | -5.80 | 11.83 | -29.23 | 90.49 | 0.4879 | 780.0 | 659.4 | |
| 0.00 | 0.53 | 0.00 | 0.30 | -4.16 | 11.43 | -29.63 | 87.20 | 0.4958 | 800.0 | 695.2 | |
| 5.89 | 8.09 | 3.38 | 4.64 | -8.35 | 10.56 | -30.50 | 95.65 | 0.5067 | 1029.1 | 724.8 | |
| 0.26 | 10.11 | 0.15 | 5.85 | -8.55 | 9.84 | -31.23 | 96.00 | 0.5175 | 1003.0 | 735.3 | |
| 1.58 | -6.00 | 0.92 | -6.00 | -8.57 | 9.66 | -31.41 | 96.03 | 0.5202 | 988.4 | 999999 | |
| 0.97 | 10.55 | 0.56 | 6.13 | -8.86 | 9.49 | -31.58 | 96.58 | 0.5229 | 998.0 | 592.9 | |
| 2.73 | -8.00 | 1.59 | -8.00 | -9.00 | 9.29 | -31.77 | 96.83 | 0.5258 | 816.6 | 999999 | |
| 0.00 | 0.88 | 0.00 | 0.51 | -7.16 | 9.28 | -31.78 | 93.32 | 0.5255 | 728.0 | 626.8 | |
| 0.00 | 3.96 | 0.00 | 2.31 | -8.04 | 8.96 | -32.11 | 95.00 | 0.5304 | 291.0 | 310.2 | |
| 0.00 | 0.79 | 0.00 | 0.46 | -8.67 | 8.86 | -32.20 | 96.18 | 0.5320 | 531.0 | 527.8 | |
| 0.00 | 0.88 | 0.00 | 0.54 | -11.65 | 4.91 | -36.15 | 101.06 | 0.5909 | 515.0 | 472.9 | |
| 2.90 | 5.28 | 1.80 | 3.27 | -7.60 | 3.95 | -37.12 | 94.19 | 0.6020 | -871.1 | -619.9 | |
| 0.00 | 0.53 | 0.00 | 0.33 | -6.32 | 3.69 | -37.38 | 92.07 | 0.6060 | -529.0 | -490.7 | |
| 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. | |