SDO HMI 2014-09-03 18:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.71 | 0.00 | 10.92 | 8.99 | 181.35 | -3.14 | 221.23 | 0.1181 | -319.0 | -439.3 | |
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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 | 1.16 | 0.00 | 0.58 | 5.24 | 189.60 | 5.12 | 249.07 | 0.0956 | -906.0 | -696.2 | |
| 0.00 | 3.22 | 0.00 | 1.60 | 6.05 | 187.20 | 2.72 | 246.81 | 0.0516 | -1100.0 | -879.1 | |
| 0.00 | 1.25 | 0.00 | 0.62 | 5.76 | 185.90 | 1.41 | 223.94 | 0.0356 | -1090.0 | -880.6 | |
| 0.00 | 3.04 | 0.00 | 1.51 | 10.90 | 185.92 | 1.44 | 338.98 | 0.0691 | -867.0 | -749.0 | |
| 0.00 | 0.98 | 0.00 | 0.49 | 12.02 | 185.74 | 1.26 | 345.58 | 0.0868 | -694.0 | -487.5 | |
| 0.00 | 0.71 | 0.00 | 0.36 | 11.54 | 185.62 | 1.13 | 345.54 | 0.0781 | -844.0 | -727.8 | |
| 0.00 | 1.07 | 0.00 | 0.53 | 11.02 | 185.34 | 0.85 | 347.54 | 0.0682 | -1122.0 | -918.8 | |
| 0.00 | 4.47 | 0.00 | 2.21 | 6.00 | 185.20 | 0.72 | 210.32 | 0.0247 | -485.0 | -679.1 | |
| 0.00 | 0.45 | 0.00 | 0.22 | 11.23 | 185.21 | 0.73 | 349.84 | 0.0714 | -602.0 | -643.6 | |
| 0.00 | 1.61 | 0.00 | 0.82 | 8.75 | 171.93 | -12.55 | 82.14 | 0.2178 | 158.0 | 187.0 | |
| 0.00 | 0.54 | 0.00 | 0.27 | 11.36 | 171.04 | -13.45 | 71.66 | 0.2412 | 866.0 | 606.5 | |
| 0.00 | 0.98 | 0.00 | 0.52 | 12.90 | 165.20 | -19.28 | 71.81 | 0.3403 | 748.0 | 590.2 | |
| 0.00 | 1.07 | 0.00 | 0.57 | 15.57 | 164.87 | -19.62 | 64.80 | 0.3590 | 612.0 | 501.3 | |
| 0.00 | 1.16 | 0.00 | 0.62 | 12.85 | 163.98 | -20.50 | 72.78 | 0.3589 | 860.0 | 669.9 | |
| 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. | |