SDO HMI 2014-11-26 21:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 55.79 | 338.72 | 39.67 | 242.32 | 16.00 | 110.33 | -44.37 | 68.97 | 0.7224 | -890.7 | -253.8 | |
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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 | 1.45 | 0.00 | 1.07 | 20.70 | 109.90 | -44.80 | 62.94 | 0.7424 | -348.0 | -265.7 | |
| 54.16 | 327.43 | 38.50 | 233.29 | 15.96 | 110.57 | -44.13 | 68.96 | 0.7196 | -1229.0 | -279.4 | |
| 1.63 | -2.00 | 1.17 | -2.00 | 16.44 | 109.82 | -44.87 | 68.55 | 0.7294 | -427.4 | 999999 | |
| 0.00 | 1.71 | 0.00 | 1.32 | 17.56 | 106.57 | -48.12 | 68.09 | 0.7675 | 480.0 | 406.6 | |
| 0.00 | 0.77 | 0.00 | 0.60 | 16.47 | 105.83 | -48.87 | 69.68 | 0.7726 | 627.0 | 581.8 | |
| 0.00 | 0.60 | 0.00 | 0.47 | 16.31 | 105.74 | -48.96 | 69.90 | 0.7732 | 681.0 | 571.9 | |
| 0.00 | 1.20 | 0.00 | 0.96 | 16.48 | 104.44 | -50.26 | 70.02 | 0.7869 | 433.0 | 448.5 | |
| 0.00 | 0.86 | 0.00 | 0.68 | 16.35 | 104.43 | -50.27 | 70.18 | 0.7867 | 621.0 | 549.6 | |
| 0.00 | 1.03 | 0.00 | 0.83 | 15.60 | 103.62 | -51.08 | 71.30 | 0.7934 | -237.0 | -108.8 | |
| 0.00 | 1.11 | 0.00 | 0.93 | 15.55 | 102.24 | -52.46 | 71.67 | 0.8070 | 435.0 | 394.8 | |
| 0.00 | 0.51 | 0.00 | 0.43 | 15.12 | 102.19 | -52.51 | 72.20 | 0.8067 | 489.0 | 440.7 | |
| 0.00 | 2.05 | 0.00 | 1.74 | 15.50 | 101.49 | -53.21 | 71.87 | 0.8142 | 397.0 | 304.8 | |
| 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. | |