SDO HMI 2014-04-06 15:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.88 | 26.42 | 0.44 | 13.09 | -8.01 | 7.27 | -2.47 | 142.91 | 0.0760 | -175.0 | -249.0 | |
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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 | 1.50 | 0.00 | 0.74 | -7.76 | 13.06 | 3.32 | 244.62 | 0.0638 | 866.0 | 574.8 | |
| 0.00 | 2.20 | 0.00 | 1.09 | -8.25 | 12.58 | 2.84 | 234.01 | 0.0608 | 1090.0 | 963.6 | |
| 0.00 | 1.06 | 0.00 | 0.52 | -10.02 | 10.36 | 0.62 | 189.19 | 0.0676 | 959.0 | 829.9 | |
| 0.88 | 1.76 | 0.44 | 0.87 | -9.69 | 10.12 | 0.38 | 186.17 | 0.0613 | 1009.8 | 887.1 | |
| 0.00 | 1.23 | 0.00 | 0.61 | -9.12 | 9.91 | 0.17 | 183.28 | 0.0510 | 944.0 | 777.3 | |
| 0.00 | 2.73 | 0.00 | 1.35 | -9.12 | 9.67 | -0.07 | 178.56 | 0.0509 | 819.0 | 631.4 | |
| 0.00 | 0.79 | 0.00 | 0.39 | -6.67 | 5.83 | -3.91 | 96.92 | 0.0685 | -888.0 | -732.1 | |
| 0.00 | 1.06 | 0.00 | 0.52 | -7.48 | 5.67 | -4.07 | 107.63 | 0.0741 | -1085.0 | -882.7 | |
| 0.00 | 2.99 | 0.00 | 1.49 | -6.91 | 5.47 | -4.27 | 99.51 | 0.0753 | -1158.0 | -966.8 | |
| 0.00 | 1.06 | 0.00 | 0.52 | -6.73 | 5.17 | -4.57 | 96.66 | 0.0801 | -790.0 | -601.3 | |
| 0.00 | 3.17 | 0.00 | 1.57 | -7.42 | 5.07 | -4.67 | 104.76 | 0.0839 | -1091.0 | -942.5 | |
| 0.00 | 2.82 | 0.00 | 1.40 | -7.59 | 4.94 | -4.80 | 106.42 | 0.0868 | -1087.0 | -886.6 | |
| 0.00 | 1.23 | 0.00 | 0.61 | -8.46 | 4.35 | -5.39 | 113.09 | 0.1014 | -951.0 | -757.4 | |
| 0.00 | 1.50 | 0.00 | 0.75 | -7.73 | 3.54 | -6.20 | 104.17 | 0.1108 | -1125.0 | -963.5 | |
| 0.00 | 1.32 | 0.00 | 0.66 | -7.73 | 3.36 | -6.38 | 103.78 | 0.1139 | -659.0 | -570.9 | |
| 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. | |