SDO HMI 2014-11-28 05:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.11 | 35.96 | 8.13 | 26.41 | -23.27 | 95.18 | -41.94 | 123.77 | 0.7407 | 76.3 | 86.3 | |
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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 | 0.86 | 0.00 | 0.61 | -24.13 | 97.97 | -39.16 | 126.36 | 0.7179 | 581.0 | 474.2 | |
| 0.00 | 0.77 | 0.00 | 0.55 | -23.94 | 97.45 | -39.67 | 125.82 | 0.7219 | 647.0 | 568.2 | |
| 4.19 | 8.73 | 2.99 | 6.23 | -23.32 | 97.08 | -40.04 | 124.85 | 0.7221 | 778.8 | 491.2 | |
| 2.22 | 8.39 | 1.62 | 6.09 | -23.79 | 96.18 | -40.94 | 124.92 | 0.7335 | 787.8 | 591.7 | |
| 0.00 | 1.28 | 0.00 | 0.93 | -23.40 | 96.25 | -40.87 | 124.47 | 0.7308 | 638.0 | 565.5 | |
| 0.00 | 0.51 | 0.00 | 0.38 | -23.13 | 94.88 | -42.24 | 123.40 | 0.7428 | 506.0 | 370.3 | |
| 3.59 | 6.08 | 2.67 | 4.52 | -23.17 | 94.34 | -42.78 | 123.17 | 0.7483 | -757.7 | -624.9 | |
| 0.00 | 0.26 | 0.00 | 0.19 | -23.12 | 93.34 | -43.78 | 122.61 | 0.7578 | -251.0 | -418.3 | |
| 0.00 | 0.94 | 0.00 | 0.74 | -25.30 | 92.00 | -45.12 | 124.56 | 0.7802 | -629.0 | -445.9 | |
| 1.11 | 5.05 | 0.85 | 3.86 | -23.16 | 92.65 | -44.47 | 122.33 | 0.7646 | -624.0 | -526.7 | |
| 0.00 | 0.86 | 0.00 | 0.63 | -20.90 | 93.54 | -43.58 | 119.98 | 0.7458 | -469.0 | -429.2 | |
| 0.00 | 1.20 | 0.00 | 0.89 | -21.38 | 93.23 | -43.89 | 120.43 | 0.7510 | -280.0 | -209.4 | |
| 0.00 | 1.03 | 0.00 | 0.79 | -20.99 | 91.59 | -45.53 | 119.21 | 0.7657 | -488.0 | -402.5 | |
| 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. | |