SDO HMI 2014-01-15 01:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 82.88 | 450.53 | 42.35 | 230.29 | -16.34 | 12.69 | 8.13 | 213.29 | 0.2475 | 1029.1 | 405.5 | |
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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 | 0.94 | 0.00 | 0.49 | -14.96 | 18.72 | 14.17 | 232.24 | 0.3004 | 648.0 | 471.9 | |
| 34.43 | 266.14 | 17.65 | 136.40 | -16.60 | 13.56 | 9.00 | 215.56 | 0.2590 | 1317.5 | 438.5 | |
| 7.31 | -2.00 | 3.74 | -2.00 | -16.63 | 13.16 | 8.60 | 214.27 | 0.2556 | 1377.6 | 999999 | |
| 4.42 | -2.00 | 2.26 | -2.00 | -16.70 | 12.82 | 8.26 | 213.08 | 0.2533 | 1078.3 | 999999 | |
| 0.00 | 3.91 | 0.00 | 1.99 | -15.77 | 12.47 | 7.91 | 214.15 | 0.2371 | 494.0 | 516.0 | |
| 0.00 | 1.02 | 0.00 | 0.52 | -16.61 | 12.32 | 7.76 | 211.67 | 0.2476 | 590.0 | 407.0 | |
| 0.00 | 5.87 | 0.00 | 2.98 | -15.26 | 12.20 | 7.65 | 214.53 | 0.2275 | 822.0 | 519.3 | |
| 0.00 | 0.85 | 0.00 | 0.43 | -14.66 | 11.75 | 7.20 | 214.51 | 0.2149 | -644.0 | -520.8 | |
| 36.72 | 161.08 | 18.70 | 82.06 | -16.05 | 11.74 | 7.18 | 211.00 | 0.2343 | 1264.6 | 422.9 | |
| 0.00 | 1.36 | 0.00 | 0.69 | -14.76 | 11.54 | 6.98 | 213.47 | 0.2142 | 932.0 | 617.8 | |
| 0.00 | 2.81 | 0.00 | 1.42 | -14.43 | 11.38 | 6.82 | 213.75 | 0.2080 | -890.0 | -689.9 | |
| 0.00 | 3.66 | 0.00 | 1.85 | -16.64 | 8.05 | 3.49 | 195.56 | 0.2186 | -904.0 | -702.3 | |
| 0.00 | 1.02 | 0.00 | 0.52 | -15.77 | 7.48 | 2.93 | 194.17 | 0.2017 | -835.0 | -670.5 | |
| 0.00 | 1.87 | 0.00 | 0.94 | -12.42 | 4.28 | -0.28 | 178.00 | 0.1377 | -831.0 | -670.4 | |
| 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. | |