SDO HMI 2014-10-03 20:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.83 | 0.00 | 12.95 | -19.11 | 107.84 | -39.51 | 124.35 | 0.7297 | 345.8 | 271.9 | |
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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 | 2.37 | 0.00 | 1.66 | -22.31 | 112.07 | -35.28 | 130.96 | 0.7099 | 178.0 | 185.4 | |
| 0.00 | 1.14 | 0.00 | 0.81 | -22.32 | 111.43 | -35.92 | 130.49 | 0.7159 | 139.0 | 261.9 | |
| 0.00 | 0.62 | 0.00 | 0.41 | -16.88 | 112.70 | -34.65 | 124.86 | 0.6653 | 704.0 | 600.9 | |
| 0.00 | 0.70 | 0.00 | 0.50 | -22.61 | 111.14 | -36.21 | 130.61 | 0.7207 | 485.0 | 439.9 | |
| 0.00 | 3.34 | 0.00 | 2.20 | -15.84 | 112.26 | -35.08 | 123.19 | 0.6630 | 798.0 | 497.4 | |
| 0.00 | 3.16 | 0.00 | 2.44 | -25.00 | 107.38 | -39.97 | 130.63 | 0.7695 | 573.0 | 453.8 | |
| 0.00 | 0.26 | 0.00 | 0.18 | -13.98 | 110.40 | -36.95 | 119.44 | 0.6721 | 270.0 | 349.3 | |
| 0.00 | 0.88 | 0.00 | 0.61 | -15.58 | 108.65 | -38.70 | 120.39 | 0.7005 | 650.0 | 582.9 | |
| 0.00 | 1.05 | 0.00 | 0.70 | -11.56 | 109.39 | -37.96 | 115.52 | 0.6701 | 471.0 | 385.1 | |
| 0.00 | 0.35 | 0.00 | 0.26 | -17.84 | 106.27 | -41.08 | 121.74 | 0.7377 | 541.0 | 525.2 | |
| 0.00 | 0.88 | 0.00 | 0.65 | -17.59 | 105.29 | -42.06 | 120.86 | 0.7462 | 458.0 | 364.4 | |
| 0.00 | 0.97 | 0.00 | 0.77 | -16.59 | 100.61 | -46.74 | 117.23 | 0.7871 | -658.0 | -596.7 | |
| 0.00 | 2.11 | 0.00 | 1.76 | -16.65 | 98.44 | -48.91 | 116.31 | 0.8077 | -113.0 | -149.3 | |
| 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. | |