SDO HMI 2014-01-12 03:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.94 | 0.00 | 9.02 | -20.23 | 63.43 | 20.46 | 225.99 | 0.4679 | -414.0 | -302.8 | |
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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 | 1.19 | 0.00 | 0.75 | -12.72 | 80.28 | 37.31 | 254.67 | 0.6154 | -565.0 | -478.8 | |
| 0.00 | 1.19 | 0.00 | 0.74 | -12.39 | 79.69 | 36.73 | 255.06 | 0.6068 | -741.0 | -638.1 | |
| 0.00 | 1.44 | 0.00 | 0.87 | -18.84 | 74.64 | 31.67 | 242.17 | 0.5641 | 649.0 | 481.5 | |
| 0.00 | 0.93 | 0.00 | 0.55 | -23.42 | 71.05 | 28.08 | 232.09 | 0.5496 | 500.0 | 440.5 | |
| 0.00 | 1.27 | 0.00 | 0.71 | -14.36 | 69.28 | 26.31 | 246.93 | 0.4687 | -683.0 | -471.1 | |
| 0.00 | 1.27 | 0.00 | 0.75 | -23.30 | 70.80 | 27.83 | 232.06 | 0.5459 | 667.0 | 555.5 | |
| 0.00 | 1.36 | 0.00 | 0.72 | -18.00 | 58.38 | 15.42 | 226.46 | 0.3503 | -844.0 | -689.4 | |
| 0.00 | 1.19 | 0.00 | 0.63 | -19.19 | 58.30 | 15.33 | 223.80 | 0.3623 | -679.0 | -527.9 | |
| 0.00 | 1.10 | 0.00 | 0.59 | -19.01 | 58.15 | 15.18 | 223.91 | 0.3586 | -781.0 | -582.2 | |
| 0.00 | 0.93 | 0.00 | 0.49 | -18.53 | 53.58 | 10.61 | 215.16 | 0.3045 | -715.0 | -612.5 | |
| 0.00 | 1.27 | 0.00 | 0.67 | -22.35 | 52.68 | 9.71 | 206.59 | 0.3501 | -679.0 | -480.8 | |
| 0.00 | 0.68 | 0.00 | 0.36 | -24.95 | 52.01 | 9.05 | 201.92 | 0.3836 | -587.0 | -575.2 | |
| 0.00 | 0.93 | 0.00 | 0.52 | -30.82 | 52.10 | 9.13 | 196.92 | 0.4703 | -637.0 | -571.7 | |
| 0.00 | 1.19 | 0.00 | 0.67 | -32.07 | 39.10 | -3.87 | 173.02 | 0.4723 | -701.0 | -514.1 | |
| 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. | |