SDO HMI 2014-09-10 12:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.99 | 52.49 | 17.97 | 41.43 | 9.63 | 147.01 | 51.66 | 276.55 | 0.7802 | 204.6 | -112.0 | |
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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 |
| 1.16 | 2.58 | 1.01 | 2.25 | 9.89 | 151.20 | 55.85 | 277.04 | 0.8237 | -508.6 | -319.6 | |
| 0.00 | 1.43 | 0.00 | 1.24 | 10.65 | 151.19 | 55.84 | 277.97 | 0.8233 | -463.0 | -405.2 | |
| 4.28 | 13.90 | 3.51 | 11.38 | 10.26 | 148.78 | 53.44 | 277.41 | 0.7993 | -634.1 | -604.5 | |
| 0.71 | -3.00 | 0.58 | -3.00 | 10.43 | 148.57 | 53.22 | 277.62 | 0.7970 | -691.4 | 999999 | |
| 0.00 | 0.98 | 0.00 | 0.79 | 9.20 | 147.72 | 52.38 | 276.04 | 0.7885 | -558.0 | -487.3 | |
| 0.00 | 1.34 | 0.00 | 1.07 | 9.50 | 147.54 | 52.19 | 276.41 | 0.7864 | -649.0 | -564.3 | |
| 0.00 | 1.16 | 0.00 | 0.92 | 9.79 | 147.35 | 52.01 | 276.78 | 0.7843 | -649.0 | -579.3 | |
| 0.00 | 0.89 | 0.00 | 0.70 | 10.35 | 146.88 | 51.54 | 277.49 | 0.7791 | -485.0 | -395.8 | |
| 0.00 | 4.01 | 0.00 | 3.10 | 8.88 | 146.08 | 50.73 | 275.55 | 0.7708 | 531.0 | 408.1 | |
| 16.84 | 22.99 | 12.87 | 17.57 | 9.27 | 145.48 | 50.13 | 276.04 | 0.7640 | 719.6 | 446.8 | |
| 0.00 | 1.16 | 0.00 | 0.89 | 10.09 | 145.50 | 50.16 | 277.12 | 0.7641 | 535.0 | 475.5 | |
| 0.00 | 1.07 | 0.00 | 0.79 | 7.95 | 143.64 | 48.30 | 274.20 | 0.7437 | 589.0 | 399.5 | |
| 0.00 | 0.98 | 0.00 | 0.73 | 9.96 | 144.01 | 48.66 | 276.91 | 0.7472 | 545.0 | 511.3 | |
| 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. | |