SDO HMI 2014-11-03 04:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.29 | 0.00 | 13.20 | -20.15 | 78.99 | -28.25 | 132.49 | 0.6031 | 693.2 | 562.2 | |
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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 | 2.86 | 0.00 | 1.69 | -20.95 | 85.08 | -22.16 | 139.99 | 0.5500 | 834.0 | 660.2 | |
| 0.00 | 0.87 | 0.00 | 0.51 | -20.72 | 84.94 | -22.29 | 139.54 | 0.5489 | 706.0 | 467.7 | |
| 0.00 | 1.12 | 0.00 | 0.65 | -16.54 | 84.65 | -22.59 | 133.42 | 0.5090 | 702.0 | 645.7 | |
| 0.00 | 1.21 | 0.00 | 0.74 | -20.01 | 79.60 | -27.64 | 132.68 | 0.5952 | 782.0 | 466.1 | |
| 0.00 | 0.26 | 0.00 | 0.16 | -20.45 | 79.26 | -27.97 | 132.92 | 0.6024 | 521.0 | 568.3 | |
| 0.00 | 0.52 | 0.00 | 0.32 | -20.46 | 78.83 | -28.41 | 132.52 | 0.6070 | 708.0 | 636.5 | |
| 0.00 | 1.21 | 0.00 | 0.76 | -20.66 | 78.68 | -28.56 | 132.63 | 0.6103 | 734.0 | 615.2 | |
| 0.00 | 2.34 | 0.00 | 1.46 | -20.51 | 78.49 | -28.75 | 132.26 | 0.6109 | 704.0 | 616.3 | |
| 0.00 | 2.16 | 0.00 | 1.35 | -20.58 | 78.22 | -29.02 | 132.10 | 0.6143 | 485.0 | 354.7 | |
| 0.00 | 1.12 | 0.00 | 0.71 | -20.01 | 76.88 | -30.36 | 130.14 | 0.6234 | 873.0 | 716.5 | |
| 0.00 | 1.38 | 0.00 | 0.88 | -20.35 | 76.62 | -30.61 | 130.35 | 0.6288 | 675.0 | 546.4 | |
| 0.00 | 2.08 | 0.00 | 1.32 | -20.19 | 76.36 | -30.88 | 129.92 | 0.6303 | 633.0 | 605.9 | |
| 0.00 | 0.52 | 0.00 | 0.33 | -19.90 | 76.35 | -30.89 | 129.53 | 0.6281 | 826.0 | 708.5 | |
| 0.00 | 1.82 | 0.00 | 1.16 | -19.79 | 75.93 | -31.30 | 129.02 | 0.6316 | 616.0 | 471.5 | |
| 0.00 | 1.82 | 0.00 | 1.16 | -19.74 | 75.57 | -31.66 | 128.65 | 0.6350 | 599.0 | 511.0 | |
| 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. | |