SDO HMI 2014-01-16 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 |
| 68.87 | 386.23 | 37.50 | 210.17 | -16.27 | 12.17 | 21.87 | 239.83 | 0.4151 | 889.9 | 387.7 | |
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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 |
| 36.22 | 222.95 | 19.85 | 122.25 | -16.55 | 13.09 | 22.80 | 240.27 | 0.4295 | 1183.9 | 391.0 | |
| 1.19 | -1.00 | 0.65 | -1.00 | -16.69 | 12.57 | 22.28 | 239.47 | 0.4234 | 1145.4 | 999999 | |
| 0.00 | 2.04 | 0.00 | 1.11 | -15.83 | 12.04 | 21.75 | 240.80 | 0.4101 | 399.0 | 434.4 | |
| 0.00 | 0.77 | 0.00 | 0.41 | -14.76 | 11.53 | 21.24 | 242.71 | 0.3959 | -602.0 | -318.6 | |
| 31.46 | 146.00 | 17.00 | 78.81 | -15.81 | 11.42 | 21.12 | 240.18 | 0.4013 | 1271.7 | 492.9 | |
| 0.00 | 1.28 | 0.00 | 0.69 | -17.11 | 11.53 | 21.23 | 237.46 | 0.4124 | 742.0 | 527.5 | |
| 0.00 | 0.60 | 0.00 | 0.32 | -14.65 | 11.07 | 20.77 | 242.50 | 0.3885 | 779.0 | 733.0 | |
| 0.00 | 4.00 | 0.00 | 2.10 | -15.20 | 7.21 | 16.92 | 236.44 | 0.3385 | -844.0 | -655.4 | |
| 0.00 | 1.02 | 0.00 | 0.53 | -16.44 | 5.17 | 14.88 | 229.98 | 0.3230 | -790.0 | -555.9 | |
| 0.00 | 1.87 | 0.00 | 0.98 | -16.23 | 5.06 | 14.77 | 230.30 | 0.3195 | -765.0 | -690.2 | |
| 0.00 | 1.19 | 0.00 | 0.63 | -19.15 | 4.28 | 13.98 | 222.10 | 0.3419 | -828.0 | -606.6 | |
| 0.00 | 1.19 | 0.00 | 0.61 | -12.31 | 3.41 | 13.11 | 238.61 | 0.2608 | -899.0 | -733.6 | |
| 0.00 | 3.32 | 0.00 | 1.73 | -19.66 | 0.86 | 10.56 | 213.56 | 0.3137 | -785.0 | -623.0 | |
| 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. | |