SDO HMI 2014-10-16 13:00:30 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 56.40 | 351.27 | 39.62 | 247.03 | -21.12 | 16.65 | 36.95 | 232.28 | 0.7111 | 926.1 | 295.7 | |
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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 | 1.57 | 0.00 | 1.11 | -17.15 | 19.53 | 39.83 | 239.04 | 0.7160 | 690.0 | 526.9 | |
| 0.00 | 1.40 | 0.00 | 0.99 | -17.40 | 19.39 | 39.69 | 238.65 | 0.7159 | 385.0 | 344.6 | |
| 27.85 | 334.25 | 19.69 | 235.44 | -21.21 | 17.04 | 37.34 | 232.47 | 0.7153 | 998.5 | 302.7 | |
| 0.26 | -3.00 | 0.18 | -3.00 | -20.62 | 16.67 | 36.96 | 232.91 | 0.7079 | 1130.3 | 999999 | |
| 24.80 | -3.00 | 17.37 | -3.00 | -21.07 | 16.47 | 36.77 | 232.23 | 0.7090 | 1246.1 | 999999 | |
| 2.53 | 5.76 | 1.74 | 3.97 | -21.44 | 14.99 | 35.29 | 230.70 | 0.6971 | 775.7 | 628.9 | |
| 0.00 | 1.40 | 0.00 | 0.96 | -21.86 | 14.71 | 35.01 | 230.00 | 0.6974 | 245.0 | 315.1 | |
| 0.00 | 0.61 | 0.00 | 0.41 | -20.58 | 13.90 | 34.20 | 230.91 | 0.6803 | 461.0 | 489.6 | |
| 0.00 | 1.57 | 0.00 | 1.05 | -21.06 | 13.02 | 33.32 | 229.63 | 0.6751 | -365.0 | -404.3 | |
| 0.96 | 2.53 | 0.64 | 1.69 | -21.37 | 12.68 | 32.97 | 228.97 | 0.6742 | -589.5 | -452.3 | |
| 0.00 | 0.96 | 0.00 | 0.62 | -18.82 | 10.96 | 31.26 | 230.68 | 0.6372 | -578.0 | -428.5 | |
| 0.00 | 1.22 | 0.00 | 0.79 | -28.23 | 2.08 | 22.38 | 211.27 | 0.6486 | -347.0 | -417.8 | |
| 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. | |