SDO HMI 2014-01-06 03:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.68 | 13.82 | 0.44 | 9.71 | -16.17 | 78.35 | -43.63 | 109.65 | 0.7025 | 59.3 | 12.5 | |
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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 | 0.85 | 0.00 | 0.55 | -21.29 | 85.01 | -36.97 | 119.39 | 0.6455 | 568.0 | 506.1 | |
| 0.68 | 2.46 | 0.44 | 1.61 | -19.06 | 83.30 | -38.68 | 115.33 | 0.6559 | 790.2 | 608.3 | |
| 0.00 | 1.27 | 0.00 | 0.83 | -13.18 | 82.04 | -39.94 | 106.12 | 0.6531 | -423.0 | -400.9 | |
| 0.00 | 1.53 | 0.00 | 1.00 | -13.18 | 81.84 | -40.14 | 106.06 | 0.6555 | -369.0 | -448.2 | |
| 0.00 | 1.02 | 0.00 | 0.68 | -13.09 | 80.57 | -41.41 | 105.63 | 0.6713 | -592.0 | -416.7 | |
| 0.00 | 0.68 | 0.00 | 0.46 | -14.92 | 79.71 | -42.27 | 108.08 | 0.6861 | 673.0 | 571.0 | |
| 0.00 | 0.85 | 0.00 | 0.58 | -12.95 | 79.38 | -42.60 | 105.15 | 0.6858 | -607.0 | -494.5 | |
| 0.00 | 0.93 | 0.00 | 0.65 | -14.57 | 78.58 | -43.40 | 107.29 | 0.6988 | -516.0 | -399.5 | |
| 0.00 | 0.76 | 0.00 | 0.54 | -16.46 | 77.35 | -44.63 | 109.60 | 0.7176 | 650.0 | 556.2 | |
| 0.00 | 1.10 | 0.00 | 0.79 | -15.86 | 76.87 | -45.11 | 108.66 | 0.7217 | 489.0 | 411.5 | |
| 0.00 | 0.68 | 0.00 | 0.54 | -21.58 | 72.63 | -49.35 | 115.01 | 0.7808 | 376.0 | 349.0 | |
| 0.00 | 0.42 | 0.00 | 0.34 | -21.08 | 71.97 | -50.01 | 114.21 | 0.7860 | 360.0 | 331.6 | |
| 0.00 | 0.68 | 0.00 | 0.50 | -13.12 | 74.38 | -47.60 | 104.45 | 0.7450 | -432.0 | -404.4 | |
| 0.00 | 0.59 | 0.00 | 0.64 | -17.16 | 59.44 | -62.54 | 107.47 | 0.8907 | -458.0 | -388.9 | |
| 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. | |