SDO HMI 2014-07-08 12:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.16 | 173.59 | 13.05 | 90.26 | 6.54 | 204.11 | -17.38 | 79.81 | 0.3031 | -632.4 | -365.4 | |
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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 | 1.00 | 0.00 | 0.52 | 10.88 | 206.02 | -15.48 | 63.94 | 0.2930 | -692.0 | -474.5 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 6.44 | 205.97 | -15.52 | 79.14 | 0.2719 | -967.0 | -779.3 | |
| 0.00 | 1.73 | 0.00 | 0.89 | 10.79 | 205.76 | -15.73 | 64.58 | 0.2961 | -939.0 | -739.0 | |
| 1.00 | 5.09 | 0.52 | 2.63 | 7.11 | 205.54 | -15.95 | 77.05 | 0.2811 | -1169.4 | -883.3 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 11.35 | 204.63 | -16.86 | 64.33 | 0.3169 | -866.0 | -638.1 | |
| 24.16 | 148.52 | 12.53 | 77.00 | 6.33 | 204.51 | -16.98 | 80.33 | 0.2958 | -1358.2 | -433.7 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 8.59 | 203.12 | -18.37 | 73.99 | 0.3255 | -740.0 | -557.3 | |
| 0.00 | 2.18 | 0.00 | 1.15 | 6.91 | 201.34 | -20.15 | 79.93 | 0.3488 | 757.0 | 587.0 | |
| 0.00 | 1.27 | 0.00 | 0.68 | 7.89 | 200.24 | -21.25 | 77.70 | 0.3689 | 781.0 | 642.1 | |
| 0.00 | 2.63 | 0.00 | 1.40 | 6.24 | 200.09 | -21.40 | 82.22 | 0.3676 | 215.0 | 241.0 | |
| 0.00 | 1.45 | 0.00 | 0.79 | 7.78 | 197.82 | -23.67 | 79.01 | 0.4069 | 840.0 | 633.6 | |
| 0.00 | 1.73 | 0.00 | 0.94 | 5.90 | 197.38 | -24.11 | 83.71 | 0.4105 | 796.0 | 659.8 | |
| 0.00 | 1.27 | 0.00 | 0.69 | 8.80 | 197.08 | -24.41 | 76.86 | 0.4212 | 754.0 | 636.0 | |
| 0.00 | 1.64 | 0.00 | 0.89 | 6.30 | 197.19 | -24.30 | 82.79 | 0.4140 | 844.0 | 666.6 | |
| 0.00 | 1.18 | 0.00 | 0.65 | 8.83 | 196.91 | -24.58 | 76.87 | 0.4239 | 370.0 | 407.5 | |
| 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. | |