SDO HMI 2014-10-03 14:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 44.16 | 157.89 | 27.05 | 96.79 | -13.26 | 120.23 | -30.43 | 123.34 | 0.5921 | 488.1 | 203.8 | |
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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 |
| 31.49 | 132.37 | 19.17 | 80.60 | -13.02 | 120.82 | -29.84 | 123.49 | 0.5835 | 975.9 | 319.8 | |
| 7.48 | -1.00 | 4.58 | -1.00 | -13.35 | 120.52 | -30.14 | 123.72 | 0.5895 | 578.0 | 999999 | |
| 0.26 | -1.00 | 0.16 | -1.00 | -13.55 | 120.42 | -30.24 | 123.92 | 0.5921 | -50.7 | 999999 | |
| 0.00 | 3.52 | 0.00 | 2.18 | -13.72 | 119.72 | -30.94 | 123.55 | 0.6016 | 534.0 | 326.5 | |
| 0.00 | 1.50 | 0.00 | 0.92 | -11.72 | 118.70 | -31.96 | 119.83 | 0.5997 | 721.0 | 617.0 | |
| 2.46 | 4.75 | 1.57 | 3.02 | -15.04 | 118.00 | -32.65 | 123.98 | 0.6306 | -705.4 | -556.7 | |
| 0.00 | 1.41 | 0.00 | 0.88 | -13.31 | 118.14 | -32.52 | 121.69 | 0.6170 | -723.0 | -615.8 | |
| 1.32 | 3.08 | 0.84 | 1.96 | -14.80 | 117.79 | -32.87 | 123.48 | 0.6314 | -592.7 | -521.7 | |
| 0.00 | 0.88 | 0.00 | 0.56 | -13.97 | 117.74 | -32.92 | 122.30 | 0.6261 | 539.0 | 332.4 | |
| 0.62 | 2.55 | 0.39 | 1.60 | -12.67 | 117.76 | -32.90 | 120.48 | 0.6171 | -750.6 | -572.4 | |
| 0.00 | 3.96 | 0.00 | 2.57 | -14.74 | 116.27 | -34.39 | 122.23 | 0.6480 | -704.0 | -641.2 | |
| 0.00 | 1.32 | 0.00 | 0.85 | -14.24 | 116.06 | -34.60 | 121.40 | 0.6472 | -458.0 | -330.6 | |
| 0.53 | 2.55 | 0.34 | 1.65 | -13.42 | 115.90 | -34.76 | 120.17 | 0.6438 | -718.5 | -625.0 | |
| 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. | |