SDO HMI 2011-11-15 00:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.08 | 40.77 | 6.36 | 23.45 | 8.57 | 346.30 | -30.25 | 78.08 | 0.5110 | 177.9 | 155.2 | |
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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 | 1.03 | 0.00 | 0.56 | 7.31 | 351.66 | -24.89 | 78.96 | 0.4272 | -683.0 | -477.9 | |
| 1.89 | 9.03 | 1.06 | 5.05 | 7.97 | 349.35 | -27.20 | 78.28 | 0.4643 | -944.3 | -851.7 | |
| 2.15 | -2.00 | 1.21 | -2.00 | 8.17 | 348.93 | -27.62 | 78.01 | 0.4712 | -755.5 | 999999 | |
| 0.00 | 1.12 | 0.00 | 0.63 | 7.96 | 348.81 | -27.74 | 78.49 | 0.4724 | -742.0 | -543.1 | |
| 0.00 | 0.95 | 0.00 | 0.54 | 8.56 | 346.43 | -30.12 | 78.02 | 0.5094 | 635.0 | 549.7 | |
| 0.00 | 1.38 | 0.00 | 0.79 | 8.61 | 346.04 | -30.51 | 78.04 | 0.5152 | 697.0 | 589.4 | |
| 0.00 | 1.46 | 0.00 | 0.84 | 8.19 | 345.91 | -30.65 | 78.89 | 0.5163 | 965.0 | 811.5 | |
| 1.63 | 18.83 | 0.95 | 10.91 | 8.42 | 345.71 | -30.84 | 78.50 | 0.5196 | 983.5 | 696.5 | |
| 2.06 | -8.00 | 1.19 | -8.00 | 8.21 | 345.66 | -30.89 | 78.91 | 0.5199 | 974.2 | 999999 | |
| 3.35 | -8.00 | 1.95 | -8.00 | 8.33 | 345.47 | -31.08 | 78.74 | 0.5229 | 862.8 | 999999 | |
| 0.00 | 0.95 | 0.00 | 0.55 | 8.52 | 344.96 | -31.59 | 78.51 | 0.5307 | -365.0 | -377.8 | |
| 0.00 | 2.92 | 0.00 | 1.71 | 8.66 | 344.74 | -31.81 | 78.30 | 0.5343 | -859.0 | -714.8 | |
| 0.00 | 1.12 | 0.00 | 0.66 | 9.20 | 343.69 | -32.86 | 77.61 | 0.5506 | 676.0 | 469.1 | |
| 0.00 | 1.98 | 0.00 | 1.21 | 13.60 | 341.89 | -34.67 | 70.63 | 0.5882 | 547.0 | 461.7 | |
| 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. | |