SDO HMI 2011-11-26 11:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.54 | 37.03 | 12.08 | 25.37 | 9.31 | 268.64 | 43.10 | 281.96 | 0.6906 | -534.6 | -257.6 | |
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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 | 1.45 | 0.00 | 1.14 | 13.29 | 275.65 | 50.11 | 285.95 | 0.7789 | 621.0 | 483.6 | |
| 3.85 | 4.96 | 2.79 | 3.60 | 10.10 | 271.99 | 46.44 | 282.45 | 0.7330 | -698.1 | -575.4 | |
| 0.00 | 1.28 | 0.00 | 0.93 | 11.21 | 271.90 | 46.36 | 283.98 | 0.7338 | -494.0 | -436.1 | |
| 1.54 | 4.28 | 1.09 | 3.04 | 8.29 | 270.99 | 45.45 | 280.13 | 0.7187 | 738.5 | 527.5 | |
| 1.54 | 2.31 | 1.10 | 1.65 | 10.23 | 271.27 | 45.73 | 282.76 | 0.7248 | -732.8 | -745.6 | |
| 0.00 | 1.11 | 0.00 | 0.76 | 8.75 | 268.50 | 42.96 | 281.19 | 0.6889 | 425.0 | 377.7 | |
| 10.01 | 12.15 | 6.70 | 8.13 | 8.29 | 267.42 | 41.88 | 280.71 | 0.6746 | -809.2 | -530.7 | |
| 0.60 | 3.08 | 0.40 | 2.04 | 10.04 | 266.59 | 41.04 | 283.47 | 0.6672 | -680.4 | -589.7 | |
| 0.00 | 1.11 | 0.00 | 0.72 | 10.64 | 264.71 | 39.17 | 284.86 | 0.6445 | -735.0 | -590.4 | |
| 0.00 | 1.28 | 0.00 | 0.82 | 9.19 | 263.81 | 38.27 | 282.84 | 0.6294 | -651.0 | -541.8 | |
| 0.00 | 1.37 | 0.00 | 0.87 | 9.25 | 263.59 | 38.04 | 283.00 | 0.6266 | -571.0 | -406.0 | |
| 0.00 | 1.20 | 0.00 | 0.75 | 8.07 | 263.22 | 37.67 | 281.19 | 0.6192 | -773.0 | -607.6 | |
| 0.00 | 1.45 | 0.00 | 0.92 | 8.96 | 263.17 | 37.63 | 282.64 | 0.6203 | -768.0 | -656.9 | |
| 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. | |