SDO HMI 2014-01-13 04:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 87.73 | 475.15 | 46.17 | 250.24 | -16.48 | 13.29 | -15.97 | 128.99 | 0.3406 | 1040.0 | 394.5 | |
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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 | 1.62 | 0.00 | 0.83 | -13.37 | 18.03 | -11.23 | 129.82 | 0.2478 | 837.0 | 567.7 | |
| 0.00 | 1.79 | 0.00 | 0.92 | -14.40 | 17.17 | -12.09 | 130.94 | 0.2697 | 1051.0 | 745.6 | |
| 0.00 | 0.51 | 0.00 | 0.26 | -14.39 | 15.23 | -14.02 | 126.93 | 0.2950 | -839.0 | -583.2 | |
| 56.79 | 297.80 | 29.82 | 156.26 | -16.56 | 13.90 | -15.36 | 130.13 | 0.3335 | 1383.4 | 473.9 | |
| 7.82 | 165.94 | 4.13 | 87.79 | -16.72 | 12.83 | -16.43 | 128.71 | 0.3486 | 1217.4 | 311.2 | |
| 23.12 | -5.00 | 12.22 | -5.00 | -16.29 | 12.45 | -16.80 | 127.09 | 0.3494 | 1323.5 | 999999 | |
| 0.00 | 1.02 | 0.00 | 0.57 | -18.73 | 5.08 | -24.17 | 123.28 | 0.4658 | -663.0 | -540.5 | |
| 0.00 | 1.45 | 0.00 | 0.80 | -14.89 | 5.07 | -24.18 | 115.54 | 0.4406 | -792.0 | -631.7 | |
| 0.00 | 0.34 | 0.00 | 0.19 | -19.05 | 4.45 | -24.80 | 123.27 | 0.4762 | -607.0 | -679.0 | |
| 0.00 | 0.85 | 0.00 | 0.48 | -19.09 | 3.93 | -25.33 | 122.87 | 0.4833 | -634.0 | -530.7 | |
| 0.00 | 0.85 | 0.00 | 0.48 | -18.12 | 3.98 | -25.27 | 121.09 | 0.4758 | -728.0 | -531.8 | |
| 0.00 | 0.85 | 0.00 | 0.48 | -18.55 | 3.32 | -25.93 | 121.34 | 0.4874 | -807.0 | -708.7 | |
| 0.00 | 2.13 | 0.00 | 1.18 | -12.43 | 3.31 | -25.94 | 109.10 | 0.4540 | -854.0 | -722.6 | |
| 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. | |