SDO HMI 2014-05-27 13:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.79 | 149.00 | 15.12 | 87.60 | -8.77 | 24.97 | -31.86 | 104.49 | 0.5407 | 575.6 | 375.0 | |
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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 | 1.08 | 0.00 | 0.63 | -9.47 | 25.90 | -30.93 | 106.11 | 0.5297 | 205.0 | 155.3 | |
| 10.28 | 137.84 | 6.02 | 80.69 | -8.91 | 25.45 | -31.38 | 104.90 | 0.5343 | 1196.9 | 436.1 | |
| 3.25 | -2.00 | 1.90 | -2.00 | -8.67 | 25.48 | -31.35 | 104.46 | 0.5333 | 1180.5 | 999999 | |
| 1.53 | -2.00 | 0.90 | -2.00 | -8.42 | 25.39 | -31.44 | 103.98 | 0.5338 | 861.8 | 999999 | |
| 9.83 | -2.00 | 5.77 | -2.00 | -8.79 | 25.18 | -31.65 | 104.57 | 0.5379 | 1016.7 | 999999 | |
| 0.90 | -2.00 | 0.53 | -2.00 | -8.69 | 24.75 | -32.08 | 104.23 | 0.5437 | 779.6 | 999999 | |
| 0.00 | 1.89 | 0.00 | 1.12 | -8.84 | 24.19 | -32.64 | 104.30 | 0.5521 | 529.0 | 418.0 | |
| 0.00 | 1.35 | 0.00 | 0.83 | -9.05 | 21.76 | -35.07 | 103.86 | 0.5867 | 516.0 | 377.6 | |
| 0.00 | 0.99 | 0.00 | 0.61 | -7.14 | 20.74 | -36.09 | 100.39 | 0.5964 | -645.0 | -498.3 | |
| 0.00 | 0.72 | 0.00 | 0.45 | -5.82 | 20.48 | -36.35 | 98.14 | 0.5979 | -592.0 | -552.9 | |
| 0.00 | 1.62 | 0.00 | 1.02 | -8.87 | 19.48 | -37.35 | 102.91 | 0.6171 | -771.0 | -585.6 | |
| 0.00 | 1.08 | 0.00 | 0.69 | -7.97 | 18.69 | -38.14 | 101.28 | 0.6259 | -584.0 | -437.3 | |
| 0.00 | 1.35 | 0.00 | 0.87 | -8.64 | 18.14 | -38.69 | 102.20 | 0.6345 | -609.0 | -542.2 | |
| 0.00 | 1.08 | 0.00 | 0.69 | -8.63 | 17.91 | -38.92 | 102.14 | 0.6376 | -668.0 | -543.7 | |
| 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. | |