SDO HMI 2014-01-14 20:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 84.29 | 446.50 | 42.86 | 227.05 | -16.39 | 12.77 | 5.46 | 203.74 | 0.2270 | 1066.3 | 428.2 | |
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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 |
| 38.92 | 267.57 | 19.83 | 136.31 | -16.59 | 13.55 | 6.24 | 206.43 | 0.2352 | 1475.8 | 472.9 | |
| 3.23 | -1.00 | 1.64 | -1.00 | -16.62 | 13.03 | 5.72 | 204.43 | 0.2319 | 1250.5 | 999999 | |
| 4.33 | -1.00 | 2.21 | -1.00 | -16.71 | 12.88 | 5.57 | 203.69 | 0.2322 | 1170.3 | 999999 | |
| 0.00 | 5.95 | 0.00 | 3.02 | -15.90 | 12.55 | 5.24 | 203.93 | 0.2174 | 864.0 | 547.9 | |
| 0.76 | 6.12 | 0.39 | 3.11 | -16.62 | 12.38 | 5.07 | 201.94 | 0.2276 | 848.2 | 686.9 | |
| 0.00 | 3.14 | 0.00 | 1.59 | -15.33 | 12.26 | 4.95 | 203.86 | 0.2065 | 702.0 | 600.5 | |
| 0.00 | 2.29 | 0.00 | 1.16 | -14.94 | 12.03 | 4.72 | 203.69 | 0.1989 | -486.0 | -310.6 | |
| 4.76 | 153.88 | 2.42 | 78.04 | -16.38 | 11.97 | 4.66 | 200.73 | 0.2213 | 1100.1 | 405.4 | |
| 32.29 | -8.00 | 16.37 | -8.00 | -16.05 | 11.81 | 4.50 | 200.63 | 0.2151 | 1374.4 | 999999 | |
| 0.00 | 1.36 | 0.00 | 0.69 | -14.53 | 11.54 | 4.23 | 202.28 | 0.1890 | -828.0 | -616.6 | |
| 0.00 | 1.19 | 0.00 | 0.60 | -14.53 | 11.32 | 4.01 | 201.26 | 0.1877 | -666.0 | -495.3 | |
| 0.00 | 1.78 | 0.00 | 0.90 | -16.45 | 8.13 | 0.82 | 183.78 | 0.2084 | -978.0 | -777.0 | |
| 0.00 | 0.93 | 0.00 | 0.47 | -15.73 | 7.51 | 0.20 | 181.01 | 0.1955 | -885.0 | -760.5 | |
| 0.00 | 1.10 | 0.00 | 0.56 | -16.96 | 6.03 | -1.28 | 174.36 | 0.2177 | -878.0 | -659.8 | |
| 0.00 | 1.19 | 0.00 | 0.60 | -17.30 | 5.82 | -1.49 | 173.58 | 0.2237 | -720.0 | -611.4 | |
| 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. | |