SDO HMI 2014-01-11 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 |
| 0.00 | 18.76 | 0.00 | 10.42 | -18.42 | 63.84 | 18.12 | 225.91 | 0.4400 | -760.4 | -607.2 | |
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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 | 1.53 | 0.00 | 0.94 | -13.66 | 81.26 | 35.55 | 252.57 | 0.5944 | -614.0 | -432.7 | |
| 0.00 | 1.53 | 0.00 | 0.92 | -12.67 | 79.92 | 34.21 | 253.80 | 0.5734 | -725.0 | -508.3 | |
| 0.00 | 1.02 | 0.00 | 0.61 | -12.41 | 79.59 | 33.88 | 254.13 | 0.5681 | -854.0 | -787.4 | |
| 0.00 | 1.44 | 0.00 | 0.82 | -14.44 | 72.92 | 27.21 | 247.28 | 0.4821 | -643.0 | -515.6 | |
| 0.00 | 0.68 | 0.00 | 0.38 | -14.62 | 72.88 | 27.17 | 246.89 | 0.4823 | -576.0 | -523.2 | |
| 0.00 | 4.25 | 0.00 | 2.28 | -15.49 | 65.35 | 19.64 | 238.35 | 0.3822 | -840.0 | -684.8 | |
| 0.00 | 1.02 | 0.00 | 0.54 | -16.91 | 62.64 | 16.93 | 231.36 | 0.3583 | -753.0 | -614.3 | |
| 0.00 | 0.85 | 0.00 | 0.45 | -19.10 | 58.40 | 12.69 | 218.75 | 0.3331 | -761.0 | -628.3 | |
| 0.00 | 1.61 | 0.00 | 0.84 | -18.68 | 57.99 | 12.28 | 218.70 | 0.3236 | -827.0 | -656.1 | |
| 0.00 | 1.10 | 0.00 | 0.59 | -24.18 | 51.91 | 6.19 | 196.07 | 0.3573 | -924.0 | -705.8 | |
| 0.00 | 1.61 | 0.00 | 0.86 | -26.31 | 49.60 | 3.89 | 189.19 | 0.3828 | -845.0 | -548.1 | |
| 0.00 | 0.85 | 0.00 | 0.47 | -29.36 | 42.37 | -3.34 | 173.18 | 0.4299 | -751.0 | -640.6 | |
| 0.00 | 1.27 | 0.00 | 0.72 | -31.98 | 39.17 | -6.54 | 168.28 | 0.4781 | -772.0 | -605.7 | |
| 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. | |