SDO HMI 2014-10-10 09:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.76 | 0.00 | 7.90 | 12.49 | 59.37 | -1.67 | 254.89 | 0.1535 | -219.5 | -137.1 | |
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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 | 1.40 | 0.00 | 0.71 | 16.94 | 68.53 | 7.49 | 326.35 | 0.2260 | -926.0 | -736.1 | |
| 0.00 | 1.40 | 0.00 | 0.70 | 12.78 | 66.77 | 5.73 | 319.78 | 0.1515 | -915.0 | -690.2 | |
| 0.00 | 1.40 | 0.00 | 0.70 | 11.30 | 63.74 | 2.70 | 332.62 | 0.1008 | -973.0 | -749.0 | |
| 0.00 | 0.53 | 0.00 | 0.26 | 10.37 | 63.30 | 2.26 | 331.97 | 0.0830 | -873.0 | -667.3 | |
| 0.00 | 0.96 | 0.00 | 0.48 | 14.20 | 63.06 | 2.02 | 346.20 | 0.1441 | -870.0 | -648.1 | |
| 0.00 | 1.67 | 0.00 | 0.83 | 14.44 | 62.82 | 1.78 | 348.17 | 0.1473 | -894.0 | -680.3 | |
| 0.00 | 0.96 | 0.00 | 0.48 | 10.35 | 62.73 | 1.68 | 338.24 | 0.0783 | -877.0 | -691.0 | |
| 0.00 | 1.05 | 0.00 | 0.52 | 7.69 | 55.36 | -5.68 | 74.82 | 0.1021 | 898.0 | 619.1 | |
| 0.00 | 0.96 | 0.00 | 0.49 | 16.70 | 55.08 | -5.96 | 28.55 | 0.2091 | -757.0 | -561.6 | |
| 0.00 | 1.31 | 0.00 | 0.66 | 13.70 | 55.16 | -5.88 | 37.21 | 0.1653 | 937.0 | 750.3 | |
| 0.00 | 1.05 | 0.00 | 0.53 | 12.49 | 52.78 | -8.26 | 51.71 | 0.1796 | 647.0 | 524.5 | |
| 0.00 | 1.84 | 0.00 | 0.92 | 9.55 | 52.71 | -8.34 | 67.38 | 0.1556 | 845.0 | 592.3 | |
| 0.00 | 1.23 | 0.00 | 0.62 | 10.77 | 50.61 | -10.44 | 65.38 | 0.1966 | 905.0 | 747.7 | |
| 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. | |