SDO HMI 2011-11-28 08:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 25.32 | 0.00 | 13.46 | 17.85 | 214.18 | 13.35 | 322.54 | 0.3633 | 557.1 | 468.3 | |
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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 | 1.03 | 0.00 | 0.56 | 18.09 | 218.64 | 17.82 | 314.96 | 0.4129 | 976.0 | 700.4 | |
| 0.00 | 1.71 | 0.00 | 0.92 | 17.82 | 217.77 | 16.94 | 315.85 | 0.4001 | 827.0 | 640.1 | |
| 0.00 | 1.20 | 0.00 | 0.66 | 21.19 | 217.14 | 16.32 | 322.52 | 0.4324 | 669.0 | 497.6 | |
| 0.00 | 0.68 | 0.00 | 0.36 | 15.83 | 215.44 | 14.62 | 316.09 | 0.3517 | -896.0 | -675.4 | |
| 0.00 | 3.34 | 0.00 | 1.77 | 16.35 | 215.42 | 14.60 | 317.19 | 0.3574 | -755.0 | -486.6 | |
| 0.00 | 2.14 | 0.00 | 1.13 | 17.47 | 213.98 | 13.15 | 322.18 | 0.3556 | 815.0 | 583.1 | |
| 0.00 | 1.54 | 0.00 | 0.81 | 17.47 | 213.63 | 12.80 | 322.92 | 0.3521 | 864.0 | 668.7 | |
| 0.00 | 3.51 | 0.00 | 1.85 | 17.28 | 213.30 | 12.47 | 323.29 | 0.3465 | 730.0 | 716.5 | |
| 0.00 | 1.71 | 0.00 | 0.91 | 17.87 | 213.27 | 12.45 | 324.38 | 0.3538 | 842.0 | 714.2 | |
| 0.00 | 2.22 | 0.00 | 1.18 | 17.90 | 212.99 | 12.17 | 325.04 | 0.3516 | 856.0 | 689.4 | |
| 0.00 | 1.45 | 0.00 | 0.77 | 17.78 | 212.95 | 12.13 | 324.92 | 0.3496 | 847.0 | 612.5 | |
| 0.00 | 2.91 | 0.00 | 1.53 | 17.44 | 212.55 | 11.72 | 325.22 | 0.3413 | 742.0 | 670.5 | |
| 0.00 | 1.88 | 0.00 | 1.01 | 21.24 | 211.73 | 10.90 | 332.74 | 0.3865 | 725.0 | 606.5 | |
| 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. | |