SDO HMI 2011-11-26 00:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 47.77 | 309.19 | 24.86 | 161.06 | 17.59 | 223.29 | -8.27 | 26.35 | 0.3100 | -763.2 | -408.7 | |
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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 |
| 0.00 | 2.31 | 0.00 | 1.20 | 18.80 | 227.47 | -4.08 | 12.82 | 0.3052 | -892.0 | -709.4 | |
| 0.00 | 1.03 | 0.00 | 0.54 | 18.86 | 225.49 | -6.06 | 18.58 | 0.3150 | 980.0 | 854.5 | |
| 0.00 | 1.03 | 0.00 | 0.54 | 19.07 | 225.45 | -6.10 | 18.46 | 0.3186 | 859.0 | 691.9 | |
| 0.00 | 2.57 | 0.00 | 1.34 | 19.13 | 224.76 | -6.80 | 20.32 | 0.3234 | 758.0 | 538.7 | |
| 16.52 | 242.32 | 8.57 | 126.04 | 17.22 | 223.87 | -7.69 | 25.34 | 0.3000 | -1290.0 | -472.4 | |
| 0.00 | 2.74 | 0.00 | 1.44 | 19.72 | 223.56 | -7.99 | 22.78 | 0.3396 | -1178.0 | -790.9 | |
| 23.03 | -5.00 | 11.99 | -5.00 | 17.64 | 223.32 | -8.24 | 26.24 | 0.3103 | -1335.9 | 999999 | |
| 0.00 | 3.51 | 0.00 | 1.85 | 19.22 | 222.61 | -8.95 | 25.83 | 0.3386 | -866.0 | -500.3 | |
| 8.22 | 42.37 | 4.30 | 22.19 | 17.85 | 222.11 | -9.45 | 29.09 | 0.3227 | -1058.8 | -352.1 | |
| 0.00 | 1.80 | 0.00 | 0.94 | 17.51 | 221.81 | -9.74 | 30.40 | 0.3203 | -530.0 | -530.1 | |
| 0.00 | 1.46 | 0.00 | 0.76 | 17.79 | 221.77 | -9.79 | 30.06 | 0.3246 | -382.0 | -259.9 | |
| 0.00 | 1.63 | 0.00 | 0.84 | 15.67 | 221.32 | -10.24 | 35.04 | 0.2995 | 889.0 | 730.8 | |
| 0.00 | 1.03 | 0.00 | 0.54 | 17.54 | 220.99 | -10.56 | 32.39 | 0.3278 | 806.0 | 521.9 | |
| 0.00 | 1.37 | 0.00 | 0.71 | 15.52 | 220.70 | -10.86 | 36.93 | 0.3034 | 855.0 | 615.6 | |
| 0.00 | 2.82 | 0.00 | 1.50 | 18.77 | 219.77 | -11.79 | 33.14 | 0.3553 | 735.0 | 548.9 | |
| 0.00 | 1.20 | 0.00 | 0.63 | 18.40 | 219.48 | -12.08 | 34.39 | 0.3530 | 698.0 | 571.4 | |
| 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. | |