SDO HMI 2014-01-12 22:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 70.93 | 482.47 | 37.98 | 258.98 | -16.47 | 13.09 | -19.45 | 124.04 | 0.3866 | 1019.8 | 398.6 | |
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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 | 0.93 | 0.00 | 0.48 | -13.83 | 19.89 | -12.65 | 128.16 | 0.2717 | 943.0 | 788.6 | |
| 0.93 | 2.55 | 0.49 | 1.33 | -14.44 | 17.06 | -15.48 | 124.61 | 0.3154 | 1095.1 | 895.9 | |
| 39.25 | 458.44 | 20.95 | 245.45 | -16.54 | 14.04 | -18.51 | 125.29 | 0.3744 | 1473.7 | 443.5 | |
| 0.00 | 1.61 | 0.00 | 0.87 | -17.61 | 13.20 | -19.34 | 126.53 | 0.3946 | 655.0 | 435.2 | |
| 0.00 | 1.10 | 0.00 | 0.59 | -16.06 | 13.04 | -19.50 | 122.91 | 0.3838 | 294.0 | 307.3 | |
| 7.56 | -3.00 | 4.06 | -3.00 | -16.69 | 12.94 | -19.60 | 124.21 | 0.3902 | 1233.5 | 999999 | |
| 23.19 | -3.00 | 12.48 | -3.00 | -16.29 | 12.56 | -19.98 | 122.84 | 0.3921 | 1324.6 | 999999 | |
| 0.00 | 2.21 | 0.00 | 1.23 | -16.14 | 7.56 | -24.98 | 117.55 | 0.4595 | -780.0 | -669.8 | |
| 0.00 | 1.53 | 0.00 | 0.88 | -19.18 | 4.65 | -27.89 | 120.92 | 0.5171 | -873.0 | -657.4 | |
| 0.00 | 1.02 | 0.00 | 0.59 | -19.38 | 4.51 | -28.04 | 121.17 | 0.5203 | -689.0 | -605.5 | |
| 0.00 | 1.36 | 0.00 | 0.79 | -19.16 | 4.16 | -28.38 | 120.51 | 0.5233 | -278.0 | -388.0 | |
| 0.00 | 1.70 | 0.00 | 0.96 | -12.76 | 5.04 | -27.50 | 108.99 | 0.4783 | -406.0 | -323.8 | |
| 0.00 | 5.52 | 0.00 | 3.22 | -18.46 | 3.37 | -29.18 | 118.71 | 0.5294 | -721.0 | -583.3 | |
| 0.00 | 0.85 | 0.00 | 0.50 | -20.04 | 2.36 | -30.18 | 120.71 | 0.5515 | -671.0 | -559.3 | |
| 0.00 | 3.65 | 0.00 | 2.09 | -12.45 | 3.18 | -29.36 | 107.49 | 0.5040 | -550.0 | -616.0 | |
| 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. | |