SDO HMI 2014-05-09 01:00:37 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.27 | 126.33 | 35.39 | 195.88 | -13.63 | 229.96 | -71.54 | 103.25 | 0.9439 | 331.3 | 141.3 | |
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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 | 0.98 | 0.00 | 1.05 | -10.56 | 239.05 | -62.46 | 100.16 | 0.8874 | 530.0 | 444.5 | |
| 0.00 | 0.98 | 0.00 | 1.08 | -9.34 | 238.11 | -63.40 | 98.77 | 0.8946 | 342.0 | 301.8 | |
| 12.80 | 86.22 | 15.81 | 107.14 | -11.67 | 234.96 | -66.54 | 101.27 | 0.9178 | 804.1 | 289.2 | |
| 3.04 | -3.00 | 3.86 | -3.00 | -11.45 | 234.35 | -67.15 | 101.02 | 0.9218 | 252.8 | 999999 | |
| 0.00 | 0.72 | 0.00 | 0.93 | -12.62 | 233.74 | -67.77 | 102.27 | 0.9260 | 159.0 | 211.6 | |
| 1.70 | -3.00 | 2.15 | -3.00 | -11.21 | 234.39 | -67.12 | 100.75 | 0.9215 | 235.8 | 999999 | |
| 0.00 | 0.63 | 0.00 | 0.84 | -7.88 | 233.07 | -68.43 | 97.15 | 0.9300 | -152.0 | -154.9 | |
| 5.73 | 26.59 | 13.57 | 63.58 | -17.05 | 223.13 | -78.37 | 106.73 | 0.9787 | 82.8 | 22.7 | |
| 0.00 | 0.27 | 0.00 | 0.57 | -15.64 | 224.47 | -77.03 | 105.29 | 0.9739 | -40.0 | -47.0 | |
| 0.00 | 1.97 | 0.00 | 4.24 | -15.48 | 224.39 | -77.12 | 105.12 | 0.9742 | -204.0 | -155.0 | |
| 0.00 | 1.52 | 0.00 | 3.19 | -15.16 | 224.78 | -76.73 | 104.79 | 0.9727 | -264.0 | -306.0 | |
| 0.00 | 5.37 | 0.00 | 11.04 | -13.89 | 225.08 | -76.42 | 103.48 | 0.9715 | -223.0 | -167.0 | |
| 0.00 | 0.81 | 0.00 | 1.72 | -13.61 | 224.55 | -76.96 | 103.20 | 0.9736 | -143.0 | -191.9 | |
| 0.00 | 0.27 | 0.00 | 0.50 | -11.51 | 226.47 | -75.04 | 101.02 | 0.9656 | -286.0 | -299.0 | |
| 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. | |