SDO HMI 2011-10-26 04:59:00 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.30 | 39.19 | 0.82 | 24.52 | 14.94 | 240.96 | -37.11 | 71.95 | 0.6154 | 27.9 | 313.4 | |
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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 |
| 0.00 | 1.13 | 0.00 | 0.68 | 14.31 | 244.34 | -33.74 | 71.86 | 0.5684 | -611.0 | -424.5 | |
| 0.00 | 1.04 | 0.00 | 0.64 | 15.33 | 243.40 | -34.67 | 70.48 | 0.5842 | -495.0 | -394.4 | |
| 0.00 | 1.65 | 0.00 | 1.01 | 14.81 | 242.71 | -35.36 | 71.60 | 0.5919 | -679.0 | -542.5 | |
| 0.00 | 1.91 | 0.00 | 1.19 | 16.09 | 241.46 | -36.62 | 69.96 | 0.6123 | -764.0 | -579.0 | |
| 0.00 | 5.04 | 0.00 | 3.16 | 16.42 | 241.34 | -36.73 | 69.47 | 0.6148 | -784.0 | -643.9 | |
| 0.00 | 1.39 | 0.00 | 0.87 | 14.90 | 241.51 | -36.56 | 71.84 | 0.6081 | 647.0 | 479.4 | |
| 0.00 | 1.22 | 0.00 | 0.76 | 14.75 | 241.54 | -36.53 | 72.08 | 0.6073 | 773.0 | 548.1 | |
| 1.30 | 19.90 | 0.82 | 12.46 | 14.52 | 240.58 | -37.49 | 72.74 | 0.6193 | 740.7 | 723.3 | |
| 0.00 | 1.56 | 0.00 | 0.99 | 14.48 | 240.43 | -37.64 | 72.84 | 0.6211 | 412.0 | 538.3 | |
| 0.00 | 3.39 | 0.00 | 2.15 | 15.00 | 239.93 | -38.14 | 72.17 | 0.6289 | 669.0 | 575.4 | |
| 0.00 | 0.96 | 0.00 | 0.61 | 14.90 | 239.64 | -38.43 | 72.42 | 0.6324 | 527.0 | 360.5 | |
| 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. | |