SDO HMI 2011-11-07 15:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 43.97 | 286.96 | 40.84 | 270.15 | 9.57 | 55.58 | -58.24 | 81.05 | 0.8497 | -550.8 | -211.4 | |
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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 |
| 24.06 | 237.83 | 21.68 | 216.81 | 9.29 | 57.00 | -56.81 | 81.33 | 0.8376 | -933.0 | -211.9 | |
| 4.05 | 11.38 | 3.77 | 10.61 | 12.04 | 55.96 | -57.85 | 78.11 | 0.8483 | 433.0 | -38.8 | |
| 0.00 | 0.60 | 0.00 | 0.56 | 10.79 | 56.31 | -57.50 | 79.57 | 0.8445 | -206.0 | -214.6 | |
| 0.00 | 0.86 | 0.00 | 0.79 | 10.26 | 56.47 | -57.35 | 80.20 | 0.8429 | -367.0 | -311.9 | |
| 0.86 | -1.00 | 0.79 | -1.00 | 8.85 | 56.61 | -57.20 | 81.87 | 0.8411 | -495.4 | 999999 | |
| 9.40 | -1.00 | 8.66 | -1.00 | 9.52 | 56.22 | -57.60 | 81.08 | 0.8450 | -375.0 | 999999 | |
| 1.29 | -1.00 | 1.19 | -1.00 | 8.68 | 56.26 | -57.55 | 82.07 | 0.8444 | -277.7 | 999999 | |
| 0.00 | 0.60 | 0.00 | 0.57 | 11.35 | 55.44 | -58.37 | 78.96 | 0.8526 | -587.0 | -552.6 | |
| 0.00 | 1.72 | 0.00 | 1.64 | 11.18 | 55.15 | -58.66 | 79.17 | 0.8552 | -609.0 | -551.2 | |
| 4.31 | 23.71 | 4.75 | 26.04 | 9.40 | 50.25 | -63.56 | 81.35 | 0.8954 | -622.0 | -460.5 | |
| 0.00 | 2.41 | 0.00 | 2.68 | 9.09 | 50.08 | -63.73 | 81.70 | 0.8967 | -440.0 | -306.4 | |
| 0.00 | 1.64 | 0.00 | 1.84 | 9.85 | 49.75 | -64.06 | 80.85 | 0.8993 | -174.0 | -147.9 | |
| 0.00 | 0.60 | 0.00 | 0.79 | 12.52 | 45.83 | -67.98 | 77.99 | 0.9269 | 381.0 | 351.7 | |
| 0.00 | 5.61 | 0.00 | 7.82 | 12.77 | 44.33 | -69.48 | 77.75 | 0.9362 | 622.0 | 394.8 | |
| 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. | |