SDO HMI 2014-01-02 17:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.64 | 40.58 | 15.54 | 31.41 | -12.23 | 117.17 | -49.83 | 103.33 | 0.7683 | 395.2 | 162.2 | |
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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 | 1.27 | 0.00 | 0.85 | -14.72 | 126.03 | -40.97 | 108.57 | 0.6713 | 480.0 | 435.3 | |
| 0.00 | 1.19 | 0.00 | 0.90 | -15.01 | 118.54 | -48.46 | 107.13 | 0.7588 | 553.0 | 444.8 | |
| 11.64 | 19.71 | 8.61 | 14.58 | -11.36 | 119.23 | -47.77 | 102.43 | 0.7457 | 796.9 | 549.8 | |
| 0.85 | -3.00 | 0.63 | -3.00 | -11.50 | 119.06 | -47.93 | 102.60 | 0.7478 | 463.6 | 999999 | |
| 0.00 | 1.02 | 0.00 | 0.78 | -14.34 | 117.90 | -49.09 | 106.15 | 0.7646 | 425.0 | 401.9 | |
| 8.15 | 10.36 | 6.30 | 8.01 | -12.32 | 117.16 | -49.84 | 103.41 | 0.7699 | 650.6 | 339.3 | |
| 0.00 | 1.27 | 0.00 | 1.07 | -13.42 | 113.30 | -53.70 | 104.29 | 0.8112 | 315.0 | 262.9 | |
| 0.00 | 0.76 | 0.00 | 0.68 | -13.82 | 111.36 | -55.63 | 104.54 | 0.8303 | -534.0 | -531.1 | |
| 0.00 | 1.19 | 0.00 | 1.05 | -13.96 | 111.20 | -55.79 | 104.69 | 0.8319 | -490.0 | -458.1 | |
| 0.00 | 0.68 | 0.00 | 0.60 | -13.59 | 111.12 | -55.88 | 104.25 | 0.8324 | -422.0 | -369.4 | |
| 0.00 | 1.61 | 0.00 | 1.42 | -12.37 | 111.48 | -55.51 | 102.82 | 0.8279 | -591.0 | -484.1 | |
| 0.00 | 0.59 | 0.00 | 0.53 | -11.75 | 110.93 | -56.07 | 102.01 | 0.8327 | -444.0 | -422.3 | |
| 0.00 | 0.93 | 0.00 | 0.94 | -12.99 | 106.67 | -60.33 | 103.14 | 0.8714 | -450.0 | -356.1 | |
| 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. | |