SDO HMI 2014-11-10 14:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.05 | 0.00 | 8.38 | -9.30 | 338.28 | -31.19 | 112.44 | 0.5547 | 115.2 | 46.2 | |
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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 | 1.29 | 0.00 | 0.74 | -9.94 | 342.56 | -26.92 | 116.67 | 0.5011 | 703.0 | 568.4 | |
| 0.00 | 1.21 | 0.00 | 0.69 | -9.94 | 342.35 | -27.12 | 116.51 | 0.5039 | 819.0 | 676.7 | |
| 0.00 | 1.29 | 0.00 | 0.74 | -5.68 | 341.28 | -28.20 | 107.74 | 0.4957 | 730.0 | 560.0 | |
| 0.00 | 0.78 | 0.00 | 0.45 | -6.69 | 340.40 | -29.08 | 109.14 | 0.5130 | 754.0 | 569.0 | |
| 0.00 | 0.86 | 0.00 | 0.51 | -11.45 | 339.82 | -29.65 | 117.12 | 0.5469 | 765.0 | 637.5 | |
| 0.00 | 1.38 | 0.00 | 0.80 | -6.80 | 339.91 | -29.56 | 109.04 | 0.5204 | 633.0 | 378.7 | |
| 0.00 | 1.03 | 0.00 | 0.60 | -6.89 | 339.80 | -29.67 | 109.14 | 0.5223 | 612.0 | 461.8 | |
| 0.00 | 1.64 | 0.00 | 1.00 | -10.05 | 336.48 | -33.00 | 112.57 | 0.5829 | -823.0 | -682.5 | |
| 0.00 | 0.95 | 0.00 | 0.59 | -12.21 | 335.98 | -33.50 | 115.67 | 0.6007 | -563.0 | -441.2 | |
| 0.00 | 0.43 | 0.00 | 0.27 | -10.81 | 334.85 | -34.62 | 112.82 | 0.6077 | -360.0 | -305.2 | |
| 0.00 | 1.64 | 0.00 | 1.02 | -10.70 | 334.54 | -34.94 | 112.47 | 0.6112 | -608.0 | -554.4 | |
| 0.00 | 0.52 | 0.00 | 0.32 | -9.54 | 334.43 | -35.05 | 110.62 | 0.6073 | -572.0 | -531.7 | |
| 0.00 | 1.03 | 0.00 | 0.65 | -10.76 | 333.68 | -35.80 | 112.09 | 0.6225 | -593.0 | -479.6 | |
| 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. | |