SDO HMI 2014-11-28 22:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.04 | 0.00 | 9.86 | -23.24 | 94.29 | -33.49 | 129.07 | 0.6543 | -93.2 | -21.8 | |
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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 | 0.43 | 0.00 | 0.26 | -19.95 | 100.57 | -27.22 | 129.81 | 0.5619 | 588.0 | 445.4 | |
| 0.00 | 2.22 | 0.00 | 1.40 | -23.25 | 97.70 | -30.08 | 131.75 | 0.6197 | 892.0 | 682.0 | |
| 0.00 | 1.11 | 0.00 | 0.71 | -23.13 | 96.80 | -30.99 | 130.82 | 0.6280 | 744.0 | 581.4 | |
| 0.00 | 0.94 | 0.00 | 0.59 | -21.19 | 96.94 | -30.85 | 128.34 | 0.6118 | -690.0 | -507.9 | |
| 0.00 | 3.08 | 0.00 | 2.01 | -23.57 | 94.73 | -33.05 | 129.75 | 0.6525 | 733.0 | 491.2 | |
| 0.00 | 3.16 | 0.00 | 2.10 | -24.08 | 93.34 | -34.45 | 129.35 | 0.6702 | -661.0 | -522.7 | |
| 0.00 | 0.77 | 0.00 | 0.51 | -22.94 | 93.17 | -34.61 | 127.78 | 0.6642 | -556.0 | -439.0 | |
| 0.00 | 1.11 | 0.00 | 0.75 | -24.48 | 92.66 | -35.13 | 129.37 | 0.6798 | -713.0 | -603.1 | |
| 0.00 | 0.34 | 0.00 | 0.22 | -20.31 | 92.93 | -34.85 | 124.11 | 0.6497 | -656.0 | -614.2 | |
| 0.00 | 0.77 | 0.00 | 0.51 | -19.23 | 91.35 | -36.43 | 121.60 | 0.6607 | -179.0 | -219.1 | |
| 0.00 | 1.11 | 0.00 | 0.80 | -25.27 | 88.01 | -39.78 | 127.32 | 0.7299 | -527.0 | -446.8 | |
| 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. | |