SDO HMI 2014-10-05 01:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 26.46 | 0.00 | 13.97 | -12.10 | 138.61 | 7.21 | 201.05 | 0.3456 | -123.4 | 76.8 | |
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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 | 0.97 | 0.00 | 0.51 | -11.50 | 143.10 | 11.71 | 212.91 | 0.3676 | 370.0 | 363.2 | |
| 0.00 | 1.32 | 0.00 | 0.70 | -11.02 | 141.34 | 9.95 | 209.48 | 0.3461 | 824.0 | 635.0 | |
| 0.00 | 7.65 | 0.00 | 4.01 | -10.18 | 140.36 | 8.96 | 208.18 | 0.3262 | 963.0 | 811.9 | |
| 0.00 | 0.79 | 0.00 | 0.41 | -10.11 | 140.17 | 8.78 | 207.77 | 0.3238 | 274.0 | 623.9 | |
| 0.00 | 0.88 | 0.00 | 0.46 | -11.71 | 140.00 | 8.61 | 205.16 | 0.3461 | 707.0 | 475.7 | |
| 0.00 | 1.49 | 0.00 | 0.79 | -12.63 | 139.75 | 8.36 | 203.44 | 0.3581 | 681.0 | 422.3 | |
| 0.00 | 1.41 | 0.00 | 0.75 | -12.90 | 139.11 | 7.71 | 201.52 | 0.3582 | 724.0 | 527.9 | |
| 0.00 | 1.14 | 0.00 | 0.61 | -14.81 | 138.61 | 7.21 | 198.48 | 0.3846 | -854.0 | -740.5 | |
| 0.00 | 2.37 | 0.00 | 1.31 | -18.27 | 138.67 | 7.28 | 196.02 | 0.4375 | -780.0 | -689.5 | |
| 0.00 | 1.76 | 0.00 | 0.93 | -13.07 | 137.62 | 6.23 | 197.52 | 0.3527 | -803.0 | -627.7 | |
| 0.00 | 0.79 | 0.00 | 0.43 | -15.95 | 137.01 | 5.62 | 193.84 | 0.3951 | -699.0 | -548.0 | |
| 0.00 | 1.76 | 0.00 | 0.92 | -12.51 | 136.07 | 4.67 | 193.71 | 0.3370 | -758.0 | -517.8 | |
| 0.00 | 1.49 | 0.00 | 0.77 | -9.82 | 135.08 | 3.69 | 192.69 | 0.2898 | -936.0 | -748.2 | |
| 0.00 | 1.23 | 0.00 | 0.64 | -10.01 | 134.96 | 3.57 | 192.15 | 0.2924 | -921.0 | -695.1 | |
| 0.00 | 1.41 | 0.00 | 0.73 | -10.93 | 131.95 | 0.55 | 181.81 | 0.3017 | -643.0 | -468.9 | |
| 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. | |