SDO HMI 2011-07-05 02:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 27.07 | 108.57 | 23.40 | 94.12 | 15.49 | 26.74 | 54.71 | 286.63 | 0.8228 | -337.8 | -245.2 | |
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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 | 1.09 | 0.00 | 1.01 | 16.12 | 29.17 | 57.14 | 287.04 | 0.8461 | -244.0 | -198.8 | |
| 0.00 | 0.64 | 0.00 | 0.59 | 17.01 | 29.17 | 57.14 | 288.08 | 0.8471 | -270.0 | -291.3 | |
| 0.00 | 1.00 | 0.00 | 0.92 | 17.27 | 28.83 | 56.79 | 288.45 | 0.8443 | -324.0 | -263.0 | |
| 15.90 | 78.22 | 14.05 | 68.88 | 15.35 | 27.52 | 55.49 | 286.34 | 0.8302 | -747.3 | -397.8 | |
| 3.63 | -4.00 | 3.17 | -4.00 | 14.99 | 27.10 | 55.07 | 285.97 | 0.8258 | -786.3 | 999999 | |
| 1.18 | 6.18 | 1.00 | 5.24 | 15.34 | 25.65 | 53.62 | 286.59 | 0.8123 | 250.8 | -211.8 | |
| 0.00 | 1.27 | 0.00 | 1.07 | 17.02 | 25.35 | 53.32 | 288.70 | 0.8117 | -458.0 | -424.0 | |
| 2.45 | 12.99 | 2.00 | 10.58 | 15.82 | 23.99 | 51.95 | 287.45 | 0.7965 | 478.3 | 400.2 | |
| 1.18 | -8.00 | 0.96 | -8.00 | 15.99 | 23.74 | 51.71 | 287.71 | 0.7942 | 670.0 | 999999 | |
| 0.00 | 1.73 | 0.00 | 1.40 | 16.21 | 23.72 | 51.68 | 287.99 | 0.7944 | 740.0 | 638.9 | |
| 2.73 | 3.45 | 2.22 | 2.81 | 16.68 | 23.84 | 51.81 | 288.55 | 0.7964 | 480.8 | 468.6 | |
| 0.00 | 2.00 | 0.00 | 1.62 | 16.43 | 23.70 | 51.66 | 288.27 | 0.7945 | 699.0 | 588.0 | |
| 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. | |