SDO HMI 2014-01-12 03:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 83.88 | 490.07 | 48.54 | 284.00 | -16.40 | 13.65 | -29.32 | 115.08 | 0.5206 | 1064.3 | 345.7 | |
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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 | 0.85 | -15.66 | 17.84 | -25.13 | 116.58 | 0.4591 | 684.0 | 620.4 | |
| 0.00 | 0.93 | 0.00 | 0.53 | -19.55 | 17.07 | -25.89 | 123.36 | 0.4947 | 703.0 | 551.7 | |
| 0.93 | 2.63 | 0.53 | 1.48 | -16.20 | 16.81 | -26.15 | 116.85 | 0.4764 | -748.1 | -623.7 | |
| 1.19 | 479.04 | 0.69 | 277.35 | -16.99 | 14.19 | -28.78 | 116.46 | 0.5164 | 602.4 | 363.1 | |
| 47.26 | -4.00 | 27.22 | -4.00 | -16.44 | 14.25 | -28.72 | 115.51 | 0.5128 | 1345.7 | 999999 | |
| 0.42 | -4.00 | 0.25 | -4.00 | -16.54 | 13.63 | -29.34 | 115.30 | 0.5216 | 867.4 | 999999 | |
| 4.25 | -4.00 | 2.46 | -4.00 | -16.45 | 13.54 | -29.43 | 115.07 | 0.5223 | 1022.8 | 999999 | |
| 7.22 | -4.00 | 4.20 | -4.00 | -16.47 | 13.25 | -29.71 | 114.93 | 0.5263 | 1140.6 | 999999 | |
| 22.61 | -4.00 | 13.19 | -4.00 | -16.24 | 12.83 | -30.14 | 114.27 | 0.5309 | 1169.1 | 999999 | |
| 0.00 | 1.10 | 0.00 | 0.68 | -14.59 | 7.06 | -35.91 | 108.79 | 0.6018 | -824.0 | -707.9 | |
| 0.00 | 2.55 | 0.00 | 1.61 | -15.26 | 5.82 | -37.14 | 109.43 | 0.6200 | -518.0 | -511.3 | |
| 0.00 | 1.44 | 0.00 | 0.94 | -18.26 | 4.33 | -38.64 | 113.47 | 0.6488 | -691.0 | -495.1 | |
| 0.00 | 0.85 | 0.00 | 0.56 | -18.15 | 3.35 | -39.61 | 112.94 | 0.6602 | -705.0 | -572.5 | |
| 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. | |