SDO HMI 2014-06-30 02:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41.87 | 317.16 | 85.69 | 658.53 | -20.32 | 259.01 | -73.85 | 111.77 | 0.9704 | 76.6 | -126.7 | |
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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 |
| 5.36 | 18.71 | 8.50 | 29.68 | -21.19 | 263.57 | -69.29 | 113.37 | 0.9514 | 544.7 | 298.6 | |
| 0.91 | 123.97 | 1.52 | 232.12 | -21.38 | 262.51 | -70.35 | 113.38 | 0.9567 | 186.4 | -373.1 | |
| 3.36 | -2.00 | 5.73 | -2.00 | -21.26 | 262.14 | -70.72 | 113.20 | 0.9583 | 98.9 | 999999 | |
| 0.00 | 2.27 | 0.00 | 4.36 | -22.58 | 260.30 | -72.56 | 114.25 | 0.9673 | -376.0 | -305.2 | |
| 0.00 | 1.36 | 0.00 | 2.64 | -22.39 | 260.11 | -72.75 | 114.02 | 0.9679 | -513.0 | -462.9 | |
| 3.72 | 7.27 | 7.54 | 14.74 | -22.25 | 259.37 | -73.49 | 113.78 | 0.9707 | -319.0 | -208.2 | |
| 4.18 | -2.00 | 8.12 | -2.00 | -21.60 | 259.92 | -72.94 | 113.19 | 0.9681 | -466.9 | 999999 | |
| 0.54 | 1.73 | 0.96 | 3.04 | -20.24 | 261.34 | -71.52 | 112.02 | 0.9611 | -108.0 | -43.6 | |
| 0.00 | 4.09 | 0.00 | 9.22 | -22.83 | 257.90 | -74.96 | 114.14 | 0.9764 | -77.0 | -63.8 | |
| 23.80 | 152.04 | 53.32 | 347.19 | -19.29 | 257.43 | -75.43 | 110.49 | 0.9762 | 164.5 | 31.1 | |
| 0.00 | 5.72 | 0.00 | 15.54 | -20.41 | 255.12 | -77.74 | 111.34 | 0.9841 | -121.0 | -157.1 | |
| 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. | |