SDO HMI 2011-11-13 14:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 58.22 | 370.30 | 91.44 | 568.19 | 19.00 | 106.40 | 71.14 | 289.06 | 0.9474 | -379.3 | -190.7 | |
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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 |
| 9.98 | 183.00 | 17.24 | 310.67 | 19.03 | 108.65 | 73.39 | 288.96 | 0.9591 | 400.7 | 21.3 | |
| 21.50 | -1.00 | 36.05 | -1.00 | 19.05 | 108.13 | 72.87 | 289.01 | 0.9567 | -570.3 | 999999 | |
| 0.00 | 1.38 | 0.00 | 2.14 | 18.19 | 106.69 | 71.43 | 288.17 | 0.9493 | -370.0 | -351.1 | |
| 3.78 | -1.00 | 5.81 | -1.00 | 19.20 | 106.43 | 71.17 | 289.25 | 0.9482 | -513.2 | 999999 | |
| 0.00 | 1.63 | 0.00 | 2.54 | 20.17 | 106.56 | 71.31 | 290.26 | 0.9492 | -329.0 | -309.5 | |
| 17.63 | 153.93 | 24.96 | 212.36 | 18.47 | 104.69 | 69.43 | 288.59 | 0.9384 | -668.2 | -477.9 | |
| 3.01 | -6.00 | 4.15 | -6.00 | 19.32 | 104.03 | 68.77 | 289.53 | 0.9350 | -385.5 | 999999 | |
| 1.55 | -6.00 | 2.10 | -6.00 | 19.21 | 103.59 | 68.33 | 289.46 | 0.9323 | -792.6 | 999999 | |
| 0.77 | 11.78 | 1.13 | 17.22 | 21.15 | 105.12 | 69.86 | 291.41 | 0.9420 | -675.9 | -314.4 | |
| 0.00 | 6.11 | 0.00 | 8.00 | 20.23 | 102.71 | 67.46 | 290.62 | 0.9276 | -504.0 | -438.7 | |
| 0.00 | 3.96 | 0.00 | 5.18 | 20.70 | 102.64 | 67.39 | 291.14 | 0.9274 | -396.0 | -353.0 | |
| 0.00 | 3.18 | 0.00 | 3.98 | 19.43 | 101.55 | 66.29 | 289.87 | 0.9198 | -97.0 | -109.1 | |
| 0.00 | 0.86 | 0.00 | 1.01 | 19.60 | 99.92 | 64.66 | 290.22 | 0.9091 | 350.0 | 307.6 | |
| 0.00 | 3.44 | 0.00 | 4.00 | 19.69 | 99.54 | 64.28 | 290.35 | 0.9065 | 611.0 | 508.0 | |
| 0.00 | 1.03 | 0.00 | 1.09 | 17.94 | 96.70 | 61.45 | 288.73 | 0.8843 | 357.0 | 289.3 | |
| 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. | |