SDO HMI 2014-11-03 01:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.26 | 44.11 | 4.92 | 23.86 | -16.91 | 99.05 | -9.84 | 156.42 | 0.3999 | -28.3 | 191.0 | |
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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 |
| 7.44 | 14.88 | 3.95 | 7.90 | -16.28 | 103.55 | -5.34 | 165.67 | 0.3624 | 1057.7 | 732.7 | |
| 0.00 | 1.12 | 0.00 | 0.60 | -16.56 | 100.51 | -8.38 | 158.46 | 0.3819 | 839.0 | 785.4 | |
| 1.82 | 11.85 | 0.97 | 6.36 | -16.66 | 100.16 | -8.73 | 157.75 | 0.3855 | 1156.5 | 883.8 | |
| 0.00 | 1.04 | 0.00 | 0.56 | -16.72 | 99.84 | -9.04 | 157.09 | 0.3885 | 579.0 | 511.8 | |
| 0.00 | 1.64 | 0.00 | 0.88 | -16.45 | 98.50 | -10.38 | 153.82 | 0.3935 | -797.0 | -580.1 | |
| 0.00 | 1.12 | 0.00 | 0.61 | -16.27 | 98.20 | -10.69 | 152.94 | 0.3930 | -718.0 | -499.9 | |
| 0.00 | 1.21 | 0.00 | 0.66 | -17.35 | 95.97 | -12.92 | 149.73 | 0.4251 | -885.0 | -726.3 | |
| 0.00 | 0.95 | 0.00 | 0.52 | -16.93 | 94.65 | -14.23 | 146.72 | 0.4304 | -891.0 | -627.5 | |
| 0.00 | 3.63 | 0.00 | 2.01 | -17.90 | 93.90 | -14.99 | 146.65 | 0.4495 | -781.0 | -702.1 | |
| 0.00 | 1.38 | 0.00 | 0.77 | -17.49 | 93.58 | -15.31 | 145.55 | 0.4471 | -853.0 | -677.5 | |
| 0.00 | 1.04 | 0.00 | 0.56 | -13.42 | 93.44 | -15.44 | 139.21 | 0.3981 | -868.0 | -670.1 | |
| 0.00 | 0.87 | 0.00 | 0.48 | -16.13 | 91.50 | -17.39 | 140.17 | 0.4501 | -719.0 | -595.2 | |
| 0.00 | 1.82 | 0.00 | 1.04 | -19.55 | 90.84 | -18.04 | 143.84 | 0.4966 | -215.0 | -305.8 | |
| 0.00 | 1.56 | 0.00 | 0.91 | -21.77 | 89.45 | -19.44 | 144.55 | 0.5350 | -469.0 | -286.7 | |
| 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. | |