SDO HMI 2014-01-07 19:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.11 | 0.00 | 9.17 | -16.55 | 74.14 | -25.90 | 118.54 | 0.4767 | -13.2 | -62.7 | |
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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 | 2.46 | 0.00 | 1.30 | -10.80 | 81.32 | -18.72 | 111.75 | 0.3410 | -728.0 | -728.1 | |
| 0.00 | 0.76 | 0.00 | 0.42 | -20.67 | 78.61 | -21.43 | 130.80 | 0.4535 | 773.0 | 587.9 | |
| 0.00 | 2.97 | 0.00 | 1.60 | -13.28 | 79.04 | -21.00 | 115.92 | 0.3895 | -798.0 | -628.9 | |
| 0.00 | 0.85 | 0.00 | 0.46 | -13.28 | 78.06 | -21.98 | 115.02 | 0.4037 | -822.0 | -688.5 | |
| 0.00 | 1.02 | 0.00 | 0.57 | -13.90 | 74.41 | -25.63 | 113.47 | 0.4597 | -730.0 | -605.2 | |
| 0.00 | 1.10 | 0.00 | 0.62 | -17.15 | 73.87 | -26.18 | 119.44 | 0.4860 | 630.0 | 484.8 | |
| 0.00 | 1.61 | 0.00 | 0.93 | -20.43 | 73.20 | -26.84 | 124.74 | 0.5170 | 785.0 | 612.5 | |
| 0.00 | 1.44 | 0.00 | 0.84 | -21.11 | 73.03 | -27.01 | 125.73 | 0.5240 | 656.0 | 573.0 | |
| 0.00 | 2.12 | 0.00 | 1.23 | -20.71 | 73.00 | -27.04 | 125.03 | 0.5214 | 887.0 | 715.7 | |
| 0.00 | 0.42 | 0.00 | 0.25 | -12.50 | 68.69 | -31.35 | 107.60 | 0.5350 | -523.0 | -595.6 | |
| 0.00 | 1.36 | 0.00 | 0.95 | -18.73 | 57.05 | -42.99 | 113.05 | 0.7042 | -275.0 | -320.1 | |
| 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. | |