SDO HMI 2014-11-29 10:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.07 | 22.85 | 3.72 | 13.69 | 16.80 | 152.39 | 31.17 | 298.91 | 0.5681 | 14.1 | -17.4 | |
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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 |
| 4.62 | 6.93 | 2.85 | 4.27 | 17.31 | 154.58 | 33.36 | 298.25 | 0.5983 | 862.1 | 625.2 | |
| 0.94 | 2.99 | 0.56 | 1.79 | 15.42 | 152.79 | 31.58 | 296.36 | 0.5655 | 940.8 | 718.8 | |
| 0.51 | 2.05 | 0.31 | 1.22 | 15.64 | 152.25 | 31.04 | 297.07 | 0.5598 | 799.3 | 696.6 | |
| 0.00 | 1.03 | 0.00 | 0.61 | 16.47 | 152.25 | 31.04 | 298.43 | 0.5645 | 716.0 | 571.5 | |
| 0.00 | 1.11 | 0.00 | 0.66 | 16.13 | 152.05 | 30.84 | 298.02 | 0.5599 | 780.0 | 601.2 | |
| 0.00 | 1.20 | 0.00 | 0.71 | 17.22 | 151.10 | 29.88 | 300.48 | 0.5544 | -756.0 | -693.9 | |
| 0.00 | 0.86 | 0.00 | 0.50 | 16.33 | 150.59 | 29.37 | 299.39 | 0.5424 | -707.0 | -580.9 | |
| 0.00 | 0.51 | 0.00 | 0.30 | 17.47 | 150.68 | 29.46 | 301.21 | 0.5507 | -615.0 | -497.8 | |
| 0.00 | 1.54 | 0.00 | 0.91 | 17.44 | 150.50 | 29.28 | 301.30 | 0.5482 | -787.0 | -662.7 | |
| 0.00 | 0.86 | 0.00 | 0.50 | 16.58 | 150.35 | 29.13 | 299.99 | 0.5408 | -737.0 | -649.7 | |
| 0.00 | 1.97 | 0.00 | 1.16 | 17.20 | 150.35 | 29.13 | 301.01 | 0.5447 | -986.0 | -754.7 | |
| 0.00 | 1.80 | 0.00 | 1.06 | 17.85 | 150.35 | 29.14 | 302.07 | 0.5491 | -746.0 | -561.0 | |
| 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. | |