SDO HMI 2014-04-02 08:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.38 | 0.00 | 8.44 | -27.04 | 79.95 | 13.59 | 208.67 | 0.4266 | -560.0 | -443.0 | |
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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 | 0.97 | 0.00 | 0.59 | -21.66 | 99.59 | 33.23 | 241.28 | 0.5830 | 680.0 | 573.1 | |
| 0.00 | 1.32 | 0.00 | 0.76 | -27.04 | 89.72 | 23.36 | 224.50 | 0.5060 | 862.0 | 650.9 | |
| 0.00 | 1.05 | 0.00 | 0.58 | -27.32 | 83.59 | 17.23 | 216.15 | 0.4481 | -549.0 | -533.8 | |
| 0.00 | 1.41 | 0.00 | 0.78 | -27.13 | 83.31 | 16.96 | 216.00 | 0.4434 | -723.0 | -461.7 | |
| 0.00 | 1.67 | 0.00 | 0.91 | -26.23 | 82.55 | 16.19 | 216.18 | 0.4255 | -912.0 | -650.9 | |
| 0.00 | 0.79 | 0.00 | 0.43 | -28.82 | 79.37 | 13.01 | 207.27 | 0.4324 | -757.0 | -628.9 | |
| 0.00 | 1.14 | 0.00 | 0.63 | -29.29 | 78.76 | 12.40 | 205.65 | 0.4345 | -841.0 | -725.5 | |
| 0.00 | 0.97 | 0.00 | 0.52 | -28.98 | 75.93 | 9.57 | 200.74 | 0.4126 | -759.0 | -594.1 | |
| 0.00 | 1.14 | 0.00 | 0.62 | -29.28 | 75.68 | 9.32 | 199.96 | 0.4155 | -950.0 | -771.1 | |
| 0.00 | 1.32 | 0.00 | 0.71 | -27.58 | 74.78 | 8.42 | 199.77 | 0.3854 | -746.0 | -643.8 | |
| 0.00 | 1.58 | 0.00 | 0.83 | -24.45 | 72.60 | 6.24 | 197.75 | 0.3262 | -973.0 | -733.9 | |
| 0.00 | 1.05 | 0.00 | 0.56 | -26.49 | 72.03 | 5.67 | 194.48 | 0.3556 | -820.0 | -694.8 | |
| 0.00 | 0.97 | 0.00 | 0.52 | -29.32 | 68.15 | 1.79 | 184.01 | 0.3909 | -792.0 | -640.5 | |
| 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. | |