SDO HMI 2014-11-28 23:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 12.74 | 0.00 | 8.31 | -23.36 | 94.00 | -33.24 | 129.40 | 0.6524 | -123.1 | -114.7 | |
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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 | 1.62 | 0.00 | 1.02 | -23.28 | 97.70 | -29.54 | 132.27 | 0.6143 | 840.0 | 720.9 | |
| 0.00 | 0.51 | 0.00 | 0.32 | -23.13 | 96.81 | -30.43 | 131.29 | 0.6222 | 612.0 | 601.8 | |
| 0.00 | 1.37 | 0.00 | 0.85 | -21.23 | 96.82 | -30.41 | 128.74 | 0.6072 | -628.0 | -581.7 | |
| 0.00 | 0.60 | 0.00 | 0.39 | -23.77 | 94.93 | -32.30 | 130.58 | 0.6462 | 364.0 | 429.9 | |
| 0.00 | 1.62 | 0.00 | 1.05 | -23.54 | 94.73 | -32.51 | 130.13 | 0.6466 | 858.0 | 685.2 | |
| 0.00 | 0.60 | 0.00 | 0.38 | -22.08 | 94.93 | -32.30 | 128.37 | 0.6339 | -774.0 | -594.0 | |
| 0.00 | 1.11 | 0.00 | 0.74 | -24.11 | 93.28 | -33.95 | 129.76 | 0.6654 | -729.0 | -599.6 | |
| 0.00 | 1.20 | 0.00 | 0.78 | -22.46 | 93.30 | -33.93 | 127.63 | 0.6537 | -584.0 | -428.9 | |
| 0.00 | 1.54 | 0.00 | 1.03 | -24.48 | 92.66 | -34.58 | 129.76 | 0.6742 | -720.0 | -633.1 | |
| 0.00 | 1.03 | 0.00 | 0.68 | -23.15 | 92.00 | -35.23 | 127.61 | 0.6718 | -73.0 | -153.4 | |
| 0.00 | 1.54 | 0.00 | 1.07 | -24.49 | 89.55 | -37.68 | 127.65 | 0.7050 | -520.0 | -480.5 | |
| 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. | |