SDO HMI 2014-11-03 05:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.67 | 33.48 | 7.25 | 17.98 | -16.84 | 99.22 | -7.47 | 161.68 | 0.3856 | 62.3 | -119.2 | |
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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 |
| 4.50 | 12.46 | 2.38 | 6.60 | -16.27 | 103.72 | -2.98 | 171.88 | 0.3543 | 1042.4 | 754.0 | |
| 0.00 | 1.04 | 0.00 | 0.55 | -16.02 | 103.56 | -3.13 | 171.36 | 0.3506 | 601.0 | 520.2 | |
| 4.76 | -1.00 | 2.52 | -1.00 | -16.34 | 103.53 | -3.16 | 171.40 | 0.3558 | 1002.7 | 999999 | |
| 4.41 | 6.32 | 2.35 | 3.37 | -16.64 | 100.22 | -6.47 | 163.08 | 0.3726 | 1146.4 | 870.0 | |
| 0.00 | 1.47 | 0.00 | 0.79 | -16.77 | 100.00 | -6.69 | 162.64 | 0.3756 | 745.0 | 692.7 | |
| 0.00 | 0.78 | 0.00 | 0.42 | -17.42 | 95.93 | -10.76 | 154.10 | 0.4095 | -785.0 | -681.8 | |
| 0.00 | 1.12 | 0.00 | 0.61 | -16.75 | 95.69 | -11.00 | 152.82 | 0.4018 | -801.0 | -633.5 | |
| 0.00 | 1.12 | 0.00 | 0.61 | -16.96 | 94.72 | -11.97 | 151.08 | 0.4119 | -933.0 | -708.9 | |
| 0.00 | 1.38 | 0.00 | 0.76 | -18.05 | 94.14 | -12.55 | 151.25 | 0.4314 | -836.0 | -639.1 | |
| 0.00 | 1.21 | 0.00 | 0.66 | -17.67 | 93.84 | -12.85 | 150.23 | 0.4285 | -723.0 | -604.1 | |
| 0.00 | 2.34 | 0.00 | 1.28 | -18.06 | 93.78 | -12.91 | 150.58 | 0.4342 | -820.0 | -697.2 | |
| 0.00 | 1.56 | 0.00 | 0.85 | -17.84 | 93.58 | -13.12 | 149.92 | 0.4328 | -786.0 | -622.4 | |
| 0.00 | 0.69 | 0.00 | 0.38 | -18.10 | 93.52 | -13.17 | 150.14 | 0.4367 | -727.0 | -582.6 | |
| 0.00 | 0.95 | 0.00 | 0.51 | -13.35 | 93.50 | -13.20 | 143.41 | 0.3743 | -674.0 | -516.0 | |
| 0.00 | 1.04 | 0.00 | 0.59 | -20.05 | 91.04 | -15.65 | 148.14 | 0.4821 | -764.0 | -623.9 | |
| 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. | |