SDO HMI 2011-11-29 06:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41.30 | 162.73 | 29.79 | 117.16 | 15.86 | 233.45 | 44.71 | 290.98 | 0.7271 | -754.5 | -281.5 | |
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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 |
| 1.97 | 2.39 | 1.47 | 1.78 | 16.68 | 235.26 | 46.53 | 291.49 | 0.7495 | -516.7 | -551.6 | |
| 0.00 | 3.68 | 0.00 | 2.76 | 17.57 | 235.42 | 46.69 | 292.60 | 0.7537 | -519.0 | -373.8 | |
| 1.45 | 2.48 | 1.09 | 1.86 | 17.73 | 235.25 | 46.51 | 292.86 | 0.7523 | -595.6 | -424.4 | |
| 1.45 | 5.64 | 1.09 | 4.22 | 17.98 | 235.15 | 46.42 | 293.21 | 0.7520 | -367.4 | -563.6 | |
| 0.00 | 1.71 | 0.00 | 1.28 | 18.26 | 234.93 | 46.20 | 293.65 | 0.7505 | -439.0 | -368.2 | |
| 26.77 | 124.94 | 19.18 | 89.64 | 15.41 | 233.39 | 44.65 | 290.40 | 0.7252 | -1002.7 | -237.6 | |
| 1.28 | 2.48 | 0.95 | 1.84 | 19.20 | 234.23 | 45.49 | 295.11 | 0.7461 | 557.2 | 404.5 | |
| 5.56 | 8.81 | 4.00 | 6.32 | 16.64 | 233.26 | 44.53 | 292.09 | 0.7274 | -593.2 | -612.9 | |
| 2.82 | -6.00 | 2.01 | -6.00 | 15.79 | 232.80 | 44.07 | 291.10 | 0.7197 | -892.4 | 999999 | |
| 0.00 | 3.42 | 0.00 | 2.44 | 16.31 | 232.86 | 44.13 | 291.78 | 0.7219 | -884.0 | -730.2 | |
| 0.00 | 2.48 | 0.00 | 1.73 | 15.25 | 231.81 | 43.07 | 290.69 | 0.7067 | -780.0 | -617.2 | |
| 0.00 | 0.77 | 0.00 | 0.56 | 19.13 | 232.70 | 43.96 | 295.58 | 0.7295 | -486.0 | -403.0 | |
| 0.00 | 1.03 | 0.00 | 0.74 | 19.38 | 232.52 | 43.79 | 295.98 | 0.7285 | -515.0 | -448.9 | |
| 0.00 | 1.62 | 0.00 | 1.12 | 15.26 | 231.18 | 42.45 | 290.92 | 0.6994 | 464.0 | 306.8 | |
| 0.00 | 1.28 | 0.00 | 0.87 | 16.41 | 229.70 | 40.96 | 293.08 | 0.6859 | -675.0 | -501.3 | |
| 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. | |