SDO HMI 2014-11-28 23:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 69.09 | 411.72 | 36.98 | 220.75 | 16.34 | 110.46 | -16.77 | 46.49 | 0.3833 | -1097.4 | -377.9 | |
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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 | 1.03 | 0.00 | 0.54 | 16.19 | 112.44 | -14.80 | 43.37 | 0.3588 | 775.0 | 546.7 | |
| 0.00 | 1.37 | 0.00 | 0.72 | 15.49 | 112.07 | -15.16 | 45.48 | 0.3550 | -276.0 | -326.2 | |
| 0.00 | 0.86 | 0.00 | 0.46 | 18.56 | 111.30 | -15.93 | 40.99 | 0.3985 | 714.0 | 528.8 | |
| 69.09 | 397.51 | 36.98 | 212.91 | 16.34 | 110.63 | -16.60 | 46.27 | 0.3811 | -1559.7 | -417.2 | |
| 0.00 | 0.77 | 0.00 | 0.42 | 16.99 | 106.79 | -20.45 | 50.66 | 0.4338 | 657.0 | 619.0 | |
| 0.00 | 1.37 | 0.00 | 0.75 | 16.29 | 106.34 | -20.89 | 52.58 | 0.4329 | 735.0 | 674.3 | |
| 0.00 | 1.45 | 0.00 | 0.81 | 17.26 | 104.86 | -22.37 | 52.54 | 0.4598 | 849.0 | 696.9 | |
| 0.00 | 1.62 | 0.00 | 0.91 | 17.38 | 104.64 | -22.59 | 52.57 | 0.4636 | 651.0 | 576.1 | |
| 0.00 | 1.80 | 0.00 | 1.01 | 16.55 | 103.54 | -23.69 | 55.31 | 0.4704 | 634.0 | 558.2 | |
| 0.00 | 2.74 | 0.00 | 1.54 | 15.80 | 102.42 | -24.81 | 57.80 | 0.4792 | 640.0 | 498.5 | |
| 0.00 | 1.20 | 0.00 | 0.68 | 15.37 | 101.90 | -25.33 | 59.09 | 0.4829 | 740.0 | 665.7 | |
| 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. | |