SDO HMI 2014-01-02 19:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.61 | 42.20 | 14.47 | 31.31 | -12.12 | 118.19 | -47.70 | 103.46 | 0.7446 | 512.7 | 264.1 | |
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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 | 1.02 | 0.00 | 0.67 | -14.68 | 126.09 | -39.80 | 108.86 | 0.6566 | 642.0 | 447.0 | |
| 0.00 | 1.87 | 0.00 | 1.21 | -10.00 | 125.89 | -39.99 | 101.71 | 0.6487 | 627.0 | 527.9 | |
| 0.00 | 1.02 | 0.00 | 0.69 | -15.29 | 123.88 | -42.01 | 109.08 | 0.6854 | 616.0 | 513.3 | |
| 0.00 | 0.59 | 0.00 | 0.41 | -8.48 | 122.01 | -43.88 | 98.91 | 0.6963 | 556.0 | 490.6 | |
| 7.05 | 19.11 | 5.10 | 13.86 | -11.41 | 119.35 | -46.54 | 102.67 | 0.7316 | 934.7 | 574.3 | |
| 1.27 | -5.00 | 0.92 | -5.00 | -11.17 | 119.18 | -46.71 | 102.31 | 0.7332 | 766.3 | 999999 | |
| 2.29 | -5.00 | 1.67 | -5.00 | -11.31 | 119.02 | -46.87 | 102.48 | 0.7353 | 572.7 | 999999 | |
| 0.00 | 1.44 | 0.00 | 1.05 | -11.73 | 118.93 | -46.96 | 103.03 | 0.7369 | 394.0 | 310.1 | |
| 0.00 | 0.76 | 0.00 | 0.57 | -14.33 | 117.95 | -47.94 | 106.34 | 0.7520 | 490.0 | 415.2 | |
| 9.00 | 11.38 | 6.78 | 8.57 | -12.35 | 117.29 | -48.60 | 103.61 | 0.7562 | 698.4 | 403.5 | |
| 0.00 | 1.44 | 0.00 | 1.22 | -14.12 | 112.26 | -53.63 | 105.15 | 0.8113 | -130.0 | -183.8 | |
| 0.00 | 1.02 | 0.00 | 0.86 | -13.90 | 112.07 | -53.82 | 104.86 | 0.8128 | -640.0 | -557.8 | |
| 0.00 | 1.36 | 0.00 | 1.17 | -13.84 | 111.31 | -54.58 | 104.68 | 0.8202 | -646.0 | -600.3 | |
| 0.00 | 1.19 | 0.00 | 1.03 | -13.98 | 111.21 | -54.68 | 104.85 | 0.8213 | -526.0 | -455.4 | |
| 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. | |