SDO HMI 2014-11-30 08:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.25 | 0.00 | 9.19 | -22.87 | 92.43 | -16.70 | 146.71 | 0.4848 | -700.5 | -612.8 | |
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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 | 1.37 | 0.00 | 0.75 | -20.57 | 94.42 | -14.71 | 147.05 | 0.4390 | -828.0 | -725.8 | |
| 0.00 | 1.11 | 0.00 | 0.61 | -20.63 | 94.18 | -14.95 | 146.73 | 0.4418 | -752.0 | -575.0 | |
| 0.00 | 1.11 | 0.00 | 0.63 | -24.09 | 93.28 | -15.84 | 149.50 | 0.4931 | -836.0 | -697.8 | |
| 0.00 | 1.20 | 0.00 | 0.68 | -24.25 | 92.79 | -16.34 | 148.93 | 0.4990 | -547.0 | -479.8 | |
| 0.00 | 1.88 | 0.00 | 1.07 | -24.09 | 92.68 | -16.45 | 148.57 | 0.4979 | -542.0 | -605.9 | |
| 0.00 | 2.65 | 0.00 | 1.51 | -23.70 | 92.63 | -16.50 | 148.04 | 0.4934 | -809.0 | -706.0 | |
| 0.00 | 1.11 | 0.00 | 0.64 | -24.25 | 92.45 | -16.68 | 148.43 | 0.5017 | -399.0 | -342.4 | |
| 0.00 | 1.54 | 0.00 | 0.86 | -20.71 | 91.93 | -17.19 | 143.14 | 0.4629 | -836.0 | -682.2 | |
| 0.00 | 2.31 | 0.00 | 1.29 | -20.58 | 91.75 | -17.38 | 142.68 | 0.4631 | -706.0 | -509.9 | |
| 0.00 | 0.60 | 0.00 | 0.35 | -25.68 | 90.35 | -18.78 | 147.07 | 0.5358 | -611.0 | -496.9 | |
| 0.00 | 1.37 | 0.00 | 0.80 | -25.12 | 90.10 | -19.03 | 146.09 | 0.5312 | -840.0 | -772.1 | |
| 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. | |