SDO HMI 2011-11-12 04:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 31.60 | 122.38 | 21.11 | 83.44 | -25.38 | 87.40 | 33.49 | 226.55 | 0.6877 | -5.7 | 170.0 | |
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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 | 1.55 | 0.00 | 1.16 | -26.99 | 93.21 | 39.30 | 228.93 | 0.7509 | -426.0 | -374.8 | |
| 0.00 | 1.21 | 0.00 | 0.87 | -25.73 | 91.48 | 37.57 | 229.23 | 0.7276 | -692.0 | -578.1 | |
| 12.49 | 92.58 | 8.63 | 64.07 | -25.20 | 88.84 | 34.93 | 227.98 | 0.6997 | 921.5 | 292.5 | |
| 1.55 | -3.00 | 1.07 | -3.00 | -25.53 | 88.55 | 34.64 | 227.38 | 0.6993 | 920.6 | 999999 | |
| 1.55 | -3.00 | 1.07 | -3.00 | -25.83 | 88.53 | 34.62 | 227.01 | 0.7014 | 520.9 | 999999 | |
| 2.41 | -3.00 | 1.66 | -3.00 | -25.79 | 88.27 | 34.36 | 226.87 | 0.6987 | 776.2 | 999999 | |
| 0.00 | 1.46 | 0.00 | 1.00 | -25.35 | 87.42 | 33.51 | 226.72 | 0.6876 | 682.0 | 608.9 | |
| 0.00 | 0.86 | 0.00 | 0.57 | -25.48 | 84.96 | 31.05 | 224.56 | 0.6660 | -565.0 | -458.9 | |
| 0.00 | 0.86 | 0.00 | 0.55 | -24.52 | 82.22 | 28.30 | 223.20 | 0.6325 | -582.0 | -468.9 | |
| 0.00 | 1.21 | 0.00 | 0.78 | -25.78 | 82.46 | 28.55 | 221.96 | 0.6460 | -662.0 | -466.4 | |
| 0.00 | 1.72 | 0.00 | 1.11 | -25.56 | 81.88 | 27.97 | 221.67 | 0.6388 | -555.0 | -441.4 | |
| 3.44 | 19.72 | 2.19 | 12.58 | -25.07 | 81.46 | 27.55 | 221.82 | 0.6306 | -873.7 | -628.4 | |
| 10.16 | -12.00 | 6.49 | -12.00 | -25.44 | 81.44 | 27.53 | 221.37 | 0.6338 | -868.5 | 999999 | |
| 0.00 | 1.21 | 0.00 | 0.75 | -24.11 | 80.50 | 26.59 | 222.01 | 0.6128 | -600.0 | -479.8 | |
| 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. | |