SDO HMI 2014-12-07 11:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 62.44 | 370.79 | 31.96 | 189.79 | -3.64 | 1.12 | -14.12 | 104.98 | 0.2533 | 1029.2 | 393.7 | |
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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 | 1.19 | 0.00 | 0.60 | -5.28 | 5.15 | -10.09 | 118.16 | 0.1988 | 877.0 | 727.0 | |
| 0.00 | 1.28 | 0.00 | 0.65 | -4.27 | 4.21 | -11.04 | 111.66 | 0.2064 | 880.0 | 588.7 | |
| 0.00 | 1.19 | 0.00 | 0.61 | -7.24 | 3.84 | -11.40 | 123.00 | 0.2349 | 917.0 | 667.3 | |
| 0.00 | 1.28 | 0.00 | 0.65 | -6.23 | 2.59 | -12.65 | 116.76 | 0.2450 | -712.0 | -558.1 | |
| 0.00 | 1.54 | 0.00 | 0.79 | -6.52 | 2.40 | -12.84 | 117.50 | 0.2501 | -1098.0 | -845.8 | |
| 31.90 | 349.56 | 16.31 | 178.89 | -3.79 | 1.45 | -13.79 | 105.85 | 0.2483 | 1433.7 | 406.5 | |
| 0.60 | -6.00 | 0.31 | -6.00 | -3.14 | 0.95 | -14.30 | 102.84 | 0.2540 | 787.9 | 999999 | |
| 28.58 | -6.00 | 14.64 | -6.00 | -3.50 | 0.79 | -14.45 | 104.05 | 0.2580 | 1361.3 | 999999 | |
| 0.00 | 1.28 | 0.00 | 0.66 | -1.75 | 0.29 | -14.95 | 97.06 | 0.2610 | 854.0 | 731.8 | |
| 0.51 | 3.07 | 0.26 | 1.58 | -2.43 | 0.25 | -14.99 | 99.62 | 0.2633 | 862.5 | 596.0 | |
| 0.00 | 2.81 | 0.00 | 1.45 | -4.56 | 0.09 | -15.15 | 107.25 | 0.2740 | 983.0 | 795.2 | |
| 0.00 | 1.28 | 0.00 | 0.66 | -1.43 | 359.90 | -15.35 | 95.67 | 0.2671 | -810.0 | -714.1 | |
| 0.00 | 2.47 | 0.00 | 1.28 | -4.41 | 359.79 | -15.45 | 106.43 | 0.2782 | 652.0 | 649.7 | |
| 0.00 | 0.77 | 0.00 | 0.39 | -1.66 | 359.68 | -15.56 | 96.47 | 0.2711 | -675.0 | -611.7 | |
| 0.85 | 3.07 | 0.44 | 1.58 | -1.52 | 359.10 | -16.14 | 95.71 | 0.2806 | -713.8 | -529.4 | |
| 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. | |