SDO HMI 2014-11-07 00:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.64 | 28.22 | 3.47 | 14.60 | 4.53 | 72.48 | 15.79 | 274.77 | 0.2763 | 60.4 | 25.0 | |
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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 | 0.26 | 0.00 | 0.14 | 3.73 | 77.12 | 20.42 | 270.51 | 0.3498 | -6.0 | -5.0 | |
| 0.00 | 2.85 | 0.00 | 1.51 | -2.29 | 76.19 | 19.50 | 252.98 | 0.3504 | -17.0 | 0.7 | |
| 0.00 | 0.78 | 0.00 | 0.41 | -3.92 | 75.56 | 18.87 | 247.96 | 0.3496 | 4.0 | 2.4 | |
| 5.35 | 9.75 | 2.80 | 5.10 | 5.64 | 75.43 | 18.74 | 276.39 | 0.3232 | -1046.2 | -797.2 | |
| 1.29 | 2.59 | 0.67 | 1.35 | 5.42 | 74.67 | 17.98 | 275.88 | 0.3103 | -852.9 | -743.1 | |
| 0.00 | 2.16 | 0.00 | 1.12 | 5.17 | 73.54 | 16.85 | 275.35 | 0.2912 | -749.0 | -572.7 | |
| 0.00 | 1.12 | 0.00 | 0.58 | 5.56 | 71.90 | 15.21 | 277.26 | 0.2644 | 746.0 | 542.5 | |
| 0.00 | 1.64 | 0.00 | 0.83 | 5.72 | 67.31 | 10.62 | 280.78 | 0.1875 | 844.0 | 630.0 | |
| 0.00 | 2.24 | 0.00 | 1.13 | 6.06 | 66.59 | 9.90 | 283.37 | 0.1765 | 966.0 | 704.7 | |
| 0.00 | 2.50 | 0.00 | 1.26 | 5.02 | 66.57 | 9.88 | 277.50 | 0.1732 | 663.0 | 625.6 | |
| 0.00 | 1.12 | 0.00 | 0.56 | 6.63 | 65.93 | 9.24 | 287.56 | 0.1681 | 856.0 | 647.1 | |
| 0.00 | 1.21 | 0.00 | 0.61 | 6.40 | 65.54 | 8.84 | 286.88 | 0.1604 | 1007.0 | 777.6 | |
| 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. | |