SDO HMI 2011-11-26 10:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.80 | 36.54 | 12.22 | 24.51 | 9.10 | 267.94 | 41.85 | 281.92 | 0.6749 | -603.7 | -440.0 | |
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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 |
| 4.36 | 4.71 | 3.13 | 3.38 | 10.08 | 271.96 | 45.87 | 282.53 | 0.7263 | -735.9 | -597.8 | |
| 2.40 | 3.08 | 1.70 | 2.19 | 10.22 | 271.30 | 45.21 | 282.83 | 0.7187 | -731.2 | -676.0 | |
| 1.71 | 3.08 | 1.20 | 2.17 | 8.34 | 270.99 | 44.90 | 280.27 | 0.7121 | 740.3 | 499.9 | |
| 0.00 | 1.20 | 0.00 | 0.81 | 8.71 | 268.47 | 42.38 | 281.22 | 0.6816 | 436.0 | 332.1 | |
| 9.33 | 13.01 | 6.19 | 8.63 | 8.31 | 267.41 | 41.32 | 280.83 | 0.6675 | -826.0 | -548.1 | |
| 0.00 | 3.85 | 0.00 | 2.53 | 10.06 | 266.54 | 40.45 | 283.63 | 0.6597 | -771.0 | -597.1 | |
| 0.00 | 0.86 | 0.00 | 0.55 | 10.15 | 264.83 | 38.74 | 284.21 | 0.6378 | -594.0 | -518.3 | |
| 0.00 | 1.45 | 0.00 | 0.93 | 10.66 | 264.71 | 38.62 | 285.03 | 0.6375 | -728.0 | -602.4 | |
| 0.00 | 0.60 | 0.00 | 0.38 | 9.17 | 263.82 | 37.73 | 282.95 | 0.6222 | -715.0 | -617.4 | |
| 0.00 | 0.94 | 0.00 | 0.59 | 9.27 | 263.64 | 37.55 | 283.14 | 0.6200 | -637.0 | -556.9 | |
| 0.00 | 0.94 | 0.00 | 0.59 | 7.95 | 263.45 | 37.36 | 281.08 | 0.6147 | -485.0 | -395.0 | |
| 0.00 | 1.11 | 0.00 | 0.69 | 8.02 | 263.19 | 37.10 | 281.24 | 0.6113 | -755.0 | -596.6 | |
| 0.00 | 1.71 | 0.00 | 1.07 | 8.97 | 263.15 | 37.06 | 282.80 | 0.6128 | -790.0 | -722.2 | |
| 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. | |