SDO HMI 2014-10-14 08:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 72.69 | 462.46 | 40.84 | 259.85 | -20.90 | 17.29 | 8.48 | 197.01 | 0.4731 | 994.7 | 361.0 | |
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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 | 0.96 | 0.00 | 0.53 | -18.04 | 21.09 | 12.27 | 206.57 | 0.4536 | 736.0 | 513.7 | |
| 0.00 | 1.84 | 0.00 | 1.01 | -17.81 | 19.69 | 10.87 | 204.13 | 0.4411 | 834.0 | 699.1 | |
| 0.52 | 1.92 | 0.29 | 1.06 | -18.43 | 17.78 | 8.96 | 199.76 | 0.4388 | -832.8 | -698.4 | |
| 29.13 | 446.90 | 16.40 | 251.19 | -21.02 | 17.76 | 8.94 | 197.80 | 0.4767 | 1267.0 | 381.4 | |
| 0.00 | 1.05 | 0.00 | 0.60 | -22.27 | 17.71 | 8.89 | 196.87 | 0.4946 | -94.0 | -87.8 | |
| 0.00 | 1.75 | 0.00 | 0.97 | -19.58 | 17.52 | 8.70 | 198.35 | 0.4544 | 957.0 | 713.8 | |
| 43.04 | -4.00 | 24.15 | -4.00 | -20.87 | 17.10 | 8.29 | 196.66 | 0.4716 | 1400.3 | 999999 | |
| 0.00 | 0.87 | 0.00 | 0.48 | -17.91 | 16.20 | 7.38 | 196.85 | 0.4233 | -770.0 | -646.9 | |
| 0.00 | 1.05 | 0.00 | 0.57 | -17.97 | 15.94 | 7.13 | 196.26 | 0.4231 | -959.0 | -704.0 | |
| 0.00 | 1.57 | 0.00 | 0.86 | -18.82 | 15.12 | 6.30 | 193.96 | 0.4325 | -800.0 | -602.0 | |
| 0.00 | 1.14 | 0.00 | 0.64 | -21.61 | 14.49 | 5.67 | 191.24 | 0.4728 | -707.0 | -568.4 | |
| 0.00 | 2.62 | 0.00 | 1.47 | -21.77 | 7.30 | -1.52 | 176.97 | 0.4674 | -470.0 | -334.5 | |
| 0.00 | 0.79 | 0.00 | 0.47 | -27.91 | 7.11 | -1.70 | 177.30 | 0.5597 | -683.0 | -586.6 | |
| 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. | |