SDO HMI 2011-10-26 08:59:00 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.21 | 44.48 | 4.41 | 26.99 | 14.80 | 241.33 | -34.56 | 71.26 | 0.5812 | -19.8 | 138.0 | |
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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 | 1.39 | 0.00 | 0.81 | 15.30 | 245.06 | -30.83 | 68.84 | 0.5321 | -838.0 | -677.1 | |
| 0.00 | 1.13 | 0.00 | 0.66 | 15.34 | 244.76 | -31.12 | 68.90 | 0.5364 | -764.0 | -667.5 | |
| 0.00 | 1.30 | 0.00 | 0.76 | 14.95 | 244.82 | -31.06 | 69.58 | 0.5340 | -656.0 | -424.3 | |
| 0.00 | 0.69 | 0.00 | 0.41 | 14.21 | 244.54 | -31.34 | 71.05 | 0.5352 | -670.0 | -517.4 | |
| 0.00 | 1.74 | 0.00 | 1.03 | 15.35 | 243.48 | -32.40 | 69.48 | 0.5539 | -85.0 | -176.1 | |
| 0.00 | 2.78 | 0.00 | 1.66 | 14.64 | 242.69 | -33.20 | 71.04 | 0.5623 | -426.0 | -302.8 | |
| 0.00 | 0.87 | 0.00 | 0.52 | 15.24 | 242.47 | -33.41 | 70.10 | 0.5672 | -571.0 | -503.6 | |
| 0.00 | 2.17 | 0.00 | 1.32 | 16.33 | 241.67 | -34.22 | 68.59 | 0.5819 | -981.0 | -787.0 | |
| 0.00 | 2.87 | 0.00 | 1.75 | 16.48 | 241.49 | -34.40 | 68.42 | 0.5848 | -910.0 | -769.3 | |
| 7.21 | 24.15 | 4.41 | 14.74 | 14.37 | 240.65 | -35.24 | 72.26 | 0.5891 | 865.5 | 606.9 | |
| 0.00 | 2.00 | 0.00 | 1.23 | 14.76 | 240.00 | -35.88 | 71.82 | 0.5988 | 727.0 | 595.6 | |
| 0.00 | 2.26 | 0.00 | 1.40 | 14.84 | 239.72 | -36.16 | 71.79 | 0.6027 | 565.0 | 485.0 | |
| 0.00 | 1.13 | 0.00 | 0.70 | 15.23 | 239.64 | -36.24 | 71.17 | 0.6049 | 467.0 | 418.8 | |
| 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. | |