SDO HMI 2014-11-27 20:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 64.14 | 377.91 | 38.47 | 227.60 | 16.13 | 110.32 | -31.75 | 62.85 | 0.5701 | -985.9 | -312.5 | |
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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 |
| 63.46 | 363.04 | 38.06 | 217.90 | 16.12 | 110.62 | -31.45 | 62.71 | 0.5663 | -1393.7 | -356.5 | |
| 0.68 | -1.00 | 0.41 | -1.00 | 16.55 | 110.32 | -31.75 | 62.20 | 0.5724 | -761.5 | 999999 | |
| 0.00 | 0.86 | 0.00 | 0.53 | 16.55 | 107.82 | -34.26 | 63.72 | 0.6041 | -580.0 | -404.3 | |
| 0.00 | 2.22 | 0.00 | 1.39 | 16.63 | 106.97 | -35.10 | 64.06 | 0.6150 | 806.0 | 647.3 | |
| 0.00 | 0.51 | 0.00 | 0.32 | 16.88 | 106.84 | -35.23 | 63.75 | 0.6177 | 569.0 | 591.0 | |
| 0.00 | 1.28 | 0.00 | 0.82 | 16.18 | 105.31 | -36.76 | 65.59 | 0.6335 | 823.0 | 683.6 | |
| 0.00 | 1.62 | 0.00 | 1.05 | 16.88 | 104.69 | -37.38 | 64.85 | 0.6441 | 650.0 | 570.3 | |
| 0.00 | 0.94 | 0.00 | 0.62 | 16.81 | 103.53 | -38.54 | 65.51 | 0.6578 | 627.0 | 568.0 | |
| 0.00 | 1.11 | 0.00 | 0.74 | 16.55 | 102.35 | -39.72 | 66.40 | 0.6708 | 503.0 | 440.8 | |
| 0.00 | 1.54 | 0.00 | 1.03 | 15.59 | 101.98 | -40.09 | 67.92 | 0.6718 | 736.0 | 621.2 | |
| 0.00 | 1.71 | 0.00 | 1.14 | 15.77 | 101.86 | -40.21 | 67.70 | 0.6739 | 745.0 | 606.2 | |
| 0.00 | 3.08 | 0.00 | 2.06 | 15.59 | 101.62 | -40.45 | 68.07 | 0.6761 | 467.0 | 401.7 | |
| 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. | |