SDO HMI 2014-11-28 06:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.23 | 35.07 | 8.91 | 25.57 | -23.46 | 95.24 | -41.34 | 124.32 | 0.7355 | 139.5 | 122.3 | |
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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 | 0.68 | 0.00 | 0.48 | -24.00 | 97.51 | -39.07 | 126.25 | 0.7163 | 534.0 | 489.0 | |
| 4.36 | 7.87 | 3.09 | 5.57 | -23.32 | 97.13 | -39.45 | 125.18 | 0.7162 | 786.0 | 518.6 | |
| 2.48 | 8.56 | 1.79 | 6.17 | -23.76 | 96.21 | -40.37 | 125.19 | 0.7277 | 764.0 | 545.6 | |
| 0.00 | 1.37 | 0.00 | 0.98 | -23.40 | 96.26 | -40.32 | 124.77 | 0.7253 | 729.0 | 565.8 | |
| 0.00 | 1.11 | 0.00 | 0.81 | -24.52 | 95.61 | -40.97 | 125.78 | 0.7376 | 513.0 | 355.1 | |
| 0.00 | 1.28 | 0.00 | 0.94 | -23.13 | 94.90 | -41.67 | 123.69 | 0.7372 | 155.0 | 148.5 | |
| 0.00 | 1.28 | 0.00 | 0.95 | -23.85 | 94.49 | -42.09 | 124.36 | 0.7449 | 456.0 | 353.1 | |
| 2.74 | 5.99 | 2.02 | 4.41 | -23.17 | 94.32 | -42.25 | 123.44 | 0.7431 | -749.9 | -649.3 | |
| 0.00 | 1.11 | 0.00 | 0.87 | -25.30 | 91.97 | -44.61 | 124.81 | 0.7755 | -632.0 | -514.7 | |
| 2.65 | 4.96 | 2.01 | 3.76 | -23.20 | 92.68 | -43.90 | 122.64 | 0.7592 | -612.2 | -516.4 | |
| 0.00 | 0.86 | 0.00 | 0.63 | -21.22 | 93.14 | -43.43 | 120.44 | 0.7457 | -587.0 | -450.7 | |
| 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. | |