SDO HMI 2014-04-06 00:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.14 | 20.32 | 0.57 | 10.27 | -7.85 | 6.89 | -11.08 | 99.91 | 0.1956 | -343.2 | -153.9 | |
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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 | 1.14 | 0.00 | 0.57 | -8.06 | 11.55 | -6.42 | 106.02 | 0.1157 | 1020.0 | 767.3 | |
| 1.14 | 4.75 | 0.57 | 2.38 | -9.80 | 9.80 | -8.17 | 114.09 | 0.1541 | 1086.5 | 808.0 | |
| 0.00 | 1.94 | 0.00 | 0.97 | -6.23 | 9.81 | -8.15 | 90.14 | 0.1417 | 705.0 | 594.4 | |
| 0.00 | 0.79 | 0.00 | 0.40 | -11.53 | 6.08 | -11.89 | 114.96 | 0.2236 | 734.0 | 556.3 | |
| 0.00 | 1.23 | 0.00 | 0.62 | -7.23 | 5.83 | -12.13 | 95.24 | 0.2104 | -849.0 | -648.1 | |
| 0.00 | 0.97 | 0.00 | 0.49 | -6.60 | 5.73 | -12.24 | 92.21 | 0.2117 | -894.0 | -723.5 | |
| 0.00 | 0.88 | 0.00 | 0.45 | -7.16 | 5.34 | -12.63 | 94.76 | 0.2187 | -715.0 | -591.0 | |
| 0.00 | 0.97 | 0.00 | 0.49 | -7.27 | 5.09 | -12.88 | 95.20 | 0.2230 | -885.0 | -693.6 | |
| 0.00 | 1.94 | 0.00 | 0.98 | -6.91 | 5.01 | -12.96 | 93.56 | 0.2241 | -786.0 | -764.2 | |
| 0.00 | 1.58 | 0.00 | 0.81 | -7.51 | 4.77 | -13.20 | 96.13 | 0.2287 | -771.0 | -663.8 | |
| 0.00 | 1.58 | 0.00 | 0.81 | -7.05 | 4.69 | -13.28 | 94.13 | 0.2295 | -969.0 | -817.6 | |
| 0.00 | 1.58 | 0.00 | 0.81 | -6.65 | 4.05 | -13.92 | 92.31 | 0.2402 | -953.0 | -811.3 | |
| 0.00 | 0.97 | 0.00 | 0.49 | -7.32 | 3.53 | -14.44 | 95.01 | 0.2493 | -570.0 | -456.0 | |
| 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. | |