SDO HMI 2014-11-27 18:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 60.47 | 371.85 | 36.69 | 226.75 | 16.12 | 110.30 | -32.88 | 63.59 | 0.5842 | -843.3 | -311.1 | |
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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 |
| 59.61 | 353.21 | 36.17 | 214.54 | 16.09 | 110.63 | -32.55 | 63.46 | 0.5800 | -1361.0 | -367.4 | |
| 0.86 | -1.00 | 0.52 | -1.00 | 16.20 | 109.84 | -33.34 | 63.75 | 0.5907 | -527.7 | 999999 | |
| 0.00 | 1.45 | 0.00 | 0.91 | 16.48 | 107.95 | -35.23 | 64.36 | 0.6158 | -541.0 | -363.2 | |
| 0.00 | 3.08 | 0.00 | 1.95 | 16.60 | 107.09 | -36.09 | 64.64 | 0.6270 | 731.0 | 607.1 | |
| 0.00 | 0.94 | 0.00 | 0.60 | 16.29 | 106.73 | -36.44 | 65.29 | 0.6300 | 686.0 | 583.1 | |
| 0.00 | 1.03 | 0.00 | 0.66 | 17.85 | 106.34 | -36.84 | 63.16 | 0.6419 | 653.0 | 547.7 | |
| 0.00 | 0.60 | 0.00 | 0.39 | 16.58 | 105.35 | -37.83 | 65.52 | 0.6482 | 691.0 | 612.0 | |
| 0.00 | 1.88 | 0.00 | 1.22 | 16.27 | 105.30 | -37.87 | 66.00 | 0.6475 | 861.0 | 632.5 | |
| 0.00 | 1.45 | 0.00 | 0.95 | 16.78 | 104.71 | -38.47 | 65.51 | 0.6567 | 574.0 | 452.2 | |
| 0.00 | 0.60 | 0.00 | 0.40 | 17.08 | 103.68 | -39.50 | 65.55 | 0.6702 | 591.0 | 515.4 | |
| 0.00 | 2.39 | 0.00 | 1.60 | 16.86 | 103.50 | -39.68 | 65.94 | 0.6716 | 804.0 | 642.4 | |
| 0.00 | 2.05 | 0.00 | 1.38 | 16.39 | 102.68 | -40.49 | 66.95 | 0.6794 | 834.0 | 655.8 | |
| 0.00 | 0.86 | 0.00 | 0.58 | 16.54 | 102.36 | -40.82 | 66.87 | 0.6838 | 482.0 | 425.8 | |
| 0.00 | 0.86 | 0.00 | 0.58 | 16.07 | 102.11 | -41.07 | 67.62 | 0.6851 | 623.0 | 551.5 | |
| 0.00 | 1.45 | 0.00 | 0.99 | 15.76 | 101.82 | -41.36 | 68.17 | 0.6874 | 609.0 | 507.4 | |
| 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. | |