SDO HMI 2011-11-26 08:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.30 | 39.89 | 11.63 | 26.57 | 8.98 | 268.54 | 41.36 | 281.81 | 0.6683 | -546.0 | -258.4 | |
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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 |
| 4.11 | 5.65 | 2.89 | 3.97 | 10.08 | 271.86 | 44.68 | 282.74 | 0.7121 | -763.5 | -634.2 | |
| 0.00 | 0.94 | 0.00 | 0.66 | 11.26 | 271.66 | 44.48 | 284.42 | 0.7118 | -540.0 | -437.1 | |
| 2.23 | 3.42 | 1.55 | 2.38 | 10.18 | 271.29 | 44.11 | 283.00 | 0.7054 | -812.1 | -733.1 | |
| 1.03 | 3.77 | 0.71 | 2.60 | 8.34 | 270.91 | 43.73 | 280.44 | 0.6979 | 753.1 | 603.0 | |
| 0.00 | 1.03 | 0.00 | 0.71 | 9.05 | 270.89 | 43.71 | 281.47 | 0.6987 | 419.0 | 394.4 | |
| 0.00 | 0.77 | 0.00 | 0.54 | 10.37 | 271.11 | 43.93 | 283.29 | 0.7036 | -580.0 | -660.8 | |
| 0.00 | 0.94 | 0.00 | 0.65 | 9.20 | 270.88 | 43.69 | 281.69 | 0.6987 | 409.0 | 282.5 | |
| 0.00 | 2.14 | 0.00 | 1.46 | 8.61 | 270.42 | 43.23 | 280.92 | 0.6921 | 659.0 | 525.7 | |
| 9.93 | 12.16 | 6.48 | 7.93 | 8.31 | 267.40 | 40.22 | 281.03 | 0.6532 | -846.9 | -655.5 | |
| 0.00 | 2.40 | 0.00 | 1.55 | 9.93 | 266.56 | 39.38 | 283.70 | 0.6456 | -919.0 | -704.5 | |
| 0.00 | 1.03 | 0.00 | 0.64 | 3.99 | 263.94 | 36.75 | 274.65 | 0.6012 | -683.0 | -533.9 | |
| 0.00 | 1.54 | 0.00 | 0.96 | 9.26 | 263.65 | 36.47 | 283.42 | 0.6053 | -747.0 | -636.1 | |
| 0.00 | 1.11 | 0.00 | 0.69 | 7.68 | 263.47 | 36.29 | 280.86 | 0.5996 | -612.0 | -486.5 | |
| 0.00 | 1.71 | 0.00 | 1.06 | 8.97 | 263.32 | 36.13 | 283.03 | 0.6001 | -746.0 | -607.8 | |
| 0.00 | 1.28 | 0.00 | 0.77 | 9.16 | 260.27 | 33.09 | 284.30 | 0.5584 | -597.0 | -420.3 | |
| 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. | |