SDO HMI 2014-11-28 02:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 67.76 | 396.39 | 39.34 | 230.87 | 16.16 | 110.41 | -28.35 | 60.36 | 0.5267 | -996.6 | -318.4 | |
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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 |
| 67.76 | 383.04 | 39.34 | 222.54 | 16.15 | 110.65 | -28.11 | 60.21 | 0.5236 | -1430.0 | -357.4 | |
| 0.00 | 0.94 | 0.00 | 0.56 | 15.52 | 108.28 | -30.48 | 63.02 | 0.5507 | 733.0 | 541.1 | |
| 0.00 | 1.37 | 0.00 | 0.84 | 16.10 | 105.35 | -33.42 | 63.90 | 0.5915 | 796.0 | 609.2 | |
| 0.00 | 1.11 | 0.00 | 0.68 | 16.43 | 105.21 | -33.56 | 63.45 | 0.5950 | 837.0 | 599.0 | |
| 0.00 | 1.71 | 0.00 | 1.06 | 16.03 | 104.65 | -34.11 | 64.40 | 0.5999 | 756.0 | 545.0 | |
| 0.00 | 1.03 | 0.00 | 0.64 | 17.10 | 103.91 | -34.85 | 63.16 | 0.6144 | 545.0 | 437.1 | |
| 0.00 | 1.63 | 0.00 | 1.02 | 16.72 | 103.69 | -35.08 | 63.85 | 0.6154 | 777.0 | 487.3 | |
| 0.00 | 0.86 | 0.00 | 0.54 | 16.78 | 102.99 | -35.77 | 64.14 | 0.6242 | 540.0 | 427.2 | |
| 0.00 | 2.22 | 0.00 | 1.41 | 16.44 | 102.68 | -36.08 | 64.82 | 0.6265 | 792.0 | 595.8 | |
| 0.00 | 1.11 | 0.00 | 0.71 | 16.62 | 102.45 | -36.31 | 64.66 | 0.6301 | 644.0 | 514.5 | |
| 0.00 | 1.37 | 0.00 | 0.87 | 15.85 | 101.93 | -36.84 | 66.08 | 0.6332 | 662.0 | 535.4 | |
| 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. | |