SDO HMI 2014-01-12 15:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.01 | 0.00 | 8.63 | -23.12 | 57.63 | 21.22 | 223.83 | 0.5008 | -446.5 | -412.3 | |
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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 | 0.74 | -14.37 | 72.90 | 36.49 | 251.81 | 0.6087 | -597.0 | -434.9 | |
| 0.00 | 0.93 | 0.00 | 0.59 | -22.86 | 71.14 | 34.73 | 237.78 | 0.6228 | 618.0 | 501.4 | |
| 0.00 | 0.85 | 0.00 | 0.54 | -23.24 | 71.13 | 34.73 | 237.22 | 0.6249 | 569.0 | 455.1 | |
| 0.00 | 2.46 | 0.00 | 1.42 | -16.51 | 65.12 | 28.71 | 244.42 | 0.5128 | -688.0 | -518.9 | |
| 0.00 | 0.93 | 0.00 | 0.51 | -16.19 | 58.50 | 22.09 | 239.64 | 0.4204 | -756.0 | -686.3 | |
| 0.00 | 2.12 | 0.00 | 1.17 | -18.99 | 58.19 | 21.78 | 233.57 | 0.4379 | -765.0 | -673.4 | |
| 0.00 | 1.27 | 0.00 | 0.70 | -24.44 | 52.54 | 16.14 | 216.07 | 0.4315 | -728.0 | -584.5 | |
| 0.00 | 1.19 | 0.00 | 0.68 | -30.87 | 51.65 | 15.24 | 206.65 | 0.5052 | -602.0 | -473.5 | |
| 0.00 | 1.53 | 0.00 | 0.88 | -33.71 | 46.72 | 10.31 | 196.83 | 0.5165 | -708.0 | -484.3 | |
| 0.00 | 1.44 | 0.00 | 0.79 | -29.30 | 43.20 | 6.80 | 193.70 | 0.4375 | -655.0 | -538.1 | |
| 0.00 | 1.10 | 0.00 | 0.61 | -29.50 | 41.75 | 5.35 | 190.77 | 0.4358 | -600.0 | -523.6 | |
| 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. | |