SDO HMI 2011-11-19 03:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.62 | 0.00 | 11.29 | 17.10 | 312.04 | -10.13 | 32.39 | 0.3130 | -635.0 | -544.4 | |
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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 | 2.83 | 0.00 | 1.46 | 17.94 | 317.48 | -4.70 | 16.22 | 0.2803 | -991.0 | -815.2 | |
| 0.00 | 1.37 | 0.00 | 0.71 | 17.60 | 316.43 | -5.75 | 20.02 | 0.2803 | -884.0 | -653.7 | |
| 0.00 | 1.12 | 0.00 | 0.58 | 17.35 | 316.22 | -5.96 | 21.01 | 0.2777 | -843.0 | -629.7 | |
| 0.00 | 1.03 | 0.00 | 0.52 | 13.06 | 316.21 | -5.96 | 28.66 | 0.2120 | -932.0 | -715.3 | |
| 0.00 | 1.03 | 0.00 | 0.53 | 17.35 | 315.87 | -6.30 | 22.11 | 0.2798 | -755.0 | -566.6 | |
| 0.00 | 1.72 | 0.00 | 0.90 | 19.44 | 314.34 | -7.84 | 23.68 | 0.3216 | -800.0 | -610.0 | |
| 0.00 | 2.49 | 0.00 | 1.29 | 16.50 | 311.65 | -10.52 | 35.66 | 0.3018 | -854.0 | -683.8 | |
| 0.00 | 1.37 | 0.00 | 0.71 | 16.19 | 311.39 | -10.79 | 36.96 | 0.3004 | -918.0 | -752.2 | |
| 0.00 | 0.94 | 0.00 | 0.49 | 17.10 | 311.18 | -11.00 | 35.63 | 0.3145 | -770.0 | -585.0 | |
| 0.00 | 1.20 | 0.00 | 0.63 | 18.08 | 309.91 | -12.27 | 36.70 | 0.3395 | -866.0 | -647.9 | |
| 0.00 | 2.66 | 0.00 | 1.40 | 18.17 | 309.74 | -12.44 | 36.90 | 0.3423 | -776.0 | -621.3 | |
| 0.00 | 1.03 | 0.00 | 0.55 | 18.22 | 308.58 | -13.59 | 39.21 | 0.3547 | -845.0 | -559.8 | |
| 0.00 | 0.77 | 0.00 | 0.42 | 19.31 | 306.06 | -16.12 | 41.88 | 0.3942 | -792.0 | -583.8 | |
| 0.00 | 1.20 | 0.00 | 0.64 | 14.78 | 304.69 | -17.48 | 53.34 | 0.3637 | 800.0 | 626.1 | |
| 0.00 | 0.86 | 0.00 | 0.46 | 11.40 | 301.97 | -20.20 | 64.87 | 0.3756 | 701.0 | 504.8 | |
| 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. | |