SDO HMI 2014-11-06 18:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.94 | 145.14 | 23.04 | 132.78 | 13.34 | 117.15 | 57.15 | 283.40 | 0.8420 | -542.9 | -244.1 | |
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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 |
| 23.30 | 125.38 | 21.72 | 116.86 | 13.91 | 117.84 | 57.84 | 284.05 | 0.8491 | -841.2 | -246.4 | |
| 0.00 | 1.81 | 0.00 | 1.58 | 12.35 | 115.38 | 55.38 | 282.38 | 0.8252 | -364.0 | -357.1 | |
| 0.00 | 2.85 | 0.00 | 2.30 | 7.73 | 112.39 | 52.38 | 276.82 | 0.7928 | -530.0 | -463.1 | |
| 0.52 | 8.89 | 0.42 | 7.16 | 8.15 | 112.22 | 52.21 | 277.37 | 0.7911 | -653.0 | -608.3 | |
| 1.12 | -4.00 | 0.90 | -4.00 | 8.02 | 112.00 | 51.99 | 277.20 | 0.7887 | -611.2 | 999999 | |
| 0.00 | 0.60 | 0.00 | 0.48 | 8.40 | 111.58 | 51.57 | 277.70 | 0.7844 | -299.0 | -264.4 | |
| 0.00 | 1.21 | 0.00 | 0.98 | 11.91 | 112.30 | 52.29 | 282.11 | 0.7940 | 541.0 | 508.2 | |
| 0.00 | 0.86 | 0.00 | 0.67 | 8.47 | 110.73 | 50.72 | 277.84 | 0.7751 | 431.0 | 375.3 | |
| 0.00 | 1.21 | 0.00 | 0.96 | 11.97 | 111.18 | 51.17 | 282.30 | 0.7823 | 382.0 | 292.3 | |
| 0.00 | 0.60 | 0.00 | 0.47 | 10.66 | 110.14 | 50.13 | 280.72 | 0.7699 | 598.0 | 558.1 | |
| 0.00 | 1.04 | 0.00 | 0.79 | 8.02 | 109.57 | 49.56 | 277.30 | 0.7621 | 652.0 | 584.2 | |
| 0.00 | 0.69 | 0.00 | 0.53 | 11.03 | 110.03 | 50.02 | 281.20 | 0.7691 | 400.0 | 405.9 | |
| 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. | |