SDO HMI 2011-05-05 02:59:07 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 50.85 | 309.66 | 27.11 | 165.25 | 17.92 | 61.22 | 2.03 | 354.72 | 0.3734 | -814.4 | -408.8 | |
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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 | 1.16 | 0.00 | 0.63 | 19.22 | 63.42 | 4.23 | 349.89 | 0.3987 | -733.0 | -570.9 | |
| 43.61 | 294.93 | 23.24 | 157.23 | 17.74 | 61.44 | 2.26 | 354.16 | 0.3706 | -1388.1 | -449.1 | |
| 1.52 | -2.00 | 0.81 | -2.00 | 18.20 | 61.42 | 2.23 | 354.36 | 0.3779 | -609.9 | 999999 | |
| 0.00 | 1.25 | 0.00 | 0.67 | 18.79 | 61.26 | 2.08 | 354.89 | 0.3872 | -478.0 | -312.5 | |
| 5.72 | -2.00 | 3.06 | -2.00 | 18.13 | 60.97 | 1.79 | 355.47 | 0.3762 | -933.4 | 999999 | |
| 0.00 | 0.89 | 0.00 | 0.48 | 18.72 | 60.98 | 1.79 | 355.58 | 0.3857 | -269.0 | -343.2 | |
| 0.00 | 1.61 | 0.00 | 0.86 | 18.95 | 59.57 | 0.39 | 359.05 | 0.3883 | -754.0 | -568.6 | |
| 0.00 | 2.32 | 0.00 | 1.24 | 18.43 | 57.21 | -1.97 | 4.93 | 0.3812 | 1017.0 | 739.3 | |
| 0.00 | 0.63 | 0.00 | 0.34 | 18.72 | 57.02 | -2.17 | 5.34 | 0.3862 | 687.0 | 488.7 | |
| 0.00 | 0.89 | 0.00 | 0.48 | 18.63 | 56.28 | -2.90 | 7.17 | 0.3860 | 730.0 | 568.5 | |
| 0.00 | 1.43 | 0.00 | 0.80 | 23.22 | 56.06 | -3.12 | 6.29 | 0.4589 | 701.0 | 596.7 | |
| 0.00 | 0.89 | 0.00 | 0.50 | 23.36 | 55.93 | -3.26 | 6.52 | 0.4612 | 728.0 | 555.9 | |
| 0.00 | 1.34 | 0.00 | 0.72 | 19.02 | 55.86 | -3.32 | 8.05 | 0.3932 | 755.0 | 500.9 | |
| 0.00 | 0.80 | 0.00 | 0.45 | 23.67 | 55.62 | -3.56 | 7.04 | 0.4665 | 594.0 | 492.0 | |
| 0.00 | 1.52 | 0.00 | 0.85 | 23.53 | 55.43 | -3.76 | 7.46 | 0.4648 | 780.0 | 587.1 | |
| 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. | |