SDO HMI 2014-07-07 11:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 31.07 | 158.71 | 17.97 | 92.46 | 6.72 | 203.59 | -31.68 | 82.96 | 0.5276 | -686.9 | -373.8 | |
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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 |
| 7.81 | 11.99 | 4.49 | 6.89 | 7.14 | 204.94 | -30.34 | 81.93 | 0.5082 | -980.8 | -573.2 | |
| 23.26 | 126.37 | 13.48 | 73.26 | 6.50 | 203.98 | -31.29 | 83.32 | 0.5217 | -1227.7 | -438.7 | |
| 0.00 | 1.64 | 0.00 | 0.95 | 8.44 | 203.50 | -31.77 | 79.72 | 0.5314 | -839.0 | -573.3 | |
| 0.00 | 1.09 | 0.00 | 0.64 | 8.59 | 203.45 | -31.82 | 79.45 | 0.5324 | -701.0 | -631.4 | |
| 0.00 | 1.36 | 0.00 | 0.80 | 7.66 | 203.13 | -32.14 | 81.25 | 0.5356 | -753.0 | -605.9 | |
| 0.00 | 3.72 | 0.00 | 2.19 | 8.05 | 202.92 | -32.36 | 80.56 | 0.5393 | -251.0 | -315.2 | |
| 0.00 | 2.45 | 0.00 | 1.44 | 7.59 | 202.92 | -32.35 | 81.41 | 0.5386 | -674.0 | -466.7 | |
| 0.00 | 0.64 | 0.00 | 0.37 | 8.20 | 202.80 | -32.48 | 80.31 | 0.5413 | -543.0 | -476.3 | |
| 0.00 | 0.91 | 0.00 | 0.54 | 8.05 | 202.00 | -33.28 | 80.73 | 0.5525 | -552.0 | -459.8 | |
| 0.00 | 1.27 | 0.00 | 0.79 | 6.15 | 198.21 | -37.07 | 84.48 | 0.6043 | 733.0 | 627.6 | |
| 0.00 | 0.64 | 0.00 | 0.40 | 8.30 | 197.66 | -37.62 | 81.00 | 0.6138 | 655.0 | 520.9 | |
| 0.00 | 3.00 | 0.00 | 1.88 | 7.81 | 197.48 | -37.80 | 81.83 | 0.6157 | 890.0 | 623.4 | |
| 0.00 | 1.36 | 0.00 | 0.87 | 9.03 | 196.66 | -38.61 | 79.97 | 0.6281 | 679.0 | 584.6 | |
| 0.00 | 1.27 | 0.00 | 0.81 | 6.89 | 196.74 | -38.53 | 83.38 | 0.6248 | 618.0 | 493.4 | |
| 0.00 | 1.00 | 0.00 | 0.63 | 6.46 | 196.63 | -38.65 | 84.09 | 0.6262 | 419.0 | 312.4 | |
| 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. | |