SDO HMI 2014-11-27 09:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 52.04 | 366.76 | 33.54 | 237.78 | 16.04 | 110.28 | -37.84 | 66.32 | 0.6458 | -815.6 | -285.0 | |
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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 | 0.34 | 0.00 | 0.22 | 17.32 | 110.52 | -37.60 | 64.35 | 0.6485 | -6.0 | -76.2 | |
| 50.93 | 352.04 | 32.81 | 227.19 | 16.03 | 110.62 | -37.50 | 66.21 | 0.6418 | -1215.1 | -325.1 | |
| 1.11 | -2.00 | 0.73 | -2.00 | 16.48 | 109.89 | -38.23 | 65.88 | 0.6525 | -497.3 | 999999 | |
| 0.00 | 0.77 | 0.00 | 0.52 | 16.50 | 107.07 | -41.05 | 67.03 | 0.6862 | 444.0 | 379.2 | |
| 0.00 | 1.54 | 0.00 | 1.08 | 16.38 | 105.10 | -43.02 | 67.93 | 0.7086 | 651.0 | 486.3 | |
| 0.00 | 2.14 | 0.00 | 1.51 | 16.44 | 104.58 | -43.54 | 68.04 | 0.7148 | 482.0 | 441.0 | |
| 0.00 | 1.71 | 0.00 | 1.21 | 16.31 | 104.49 | -43.63 | 68.24 | 0.7154 | 591.0 | 498.0 | |
| 0.00 | 1.54 | 0.00 | 1.12 | 16.35 | 102.83 | -45.29 | 68.74 | 0.7342 | 722.0 | 547.1 | |
| 0.00 | 1.20 | 0.00 | 0.88 | 16.31 | 102.17 | -45.95 | 68.99 | 0.7412 | 561.0 | 442.4 | |
| 0.00 | 2.40 | 0.00 | 1.77 | 15.66 | 101.74 | -46.38 | 69.97 | 0.7442 | 572.0 | 552.0 | |
| 0.00 | 0.94 | 0.00 | 0.69 | 15.08 | 101.82 | -46.30 | 70.72 | 0.7419 | 346.0 | 425.5 | |
| 0.00 | 2.14 | 0.00 | 1.59 | 15.50 | 101.52 | -46.60 | 70.24 | 0.7463 | 357.0 | 317.5 | |
| 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. | |