SDO HMI 2014-01-09 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 | 19.93 | 0.00 | 10.60 | -18.93 | 66.03 | -6.01 | 172.58 | 0.3332 | -294.7 | -371.7 | |
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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 | 0.93 | 0.00 | 0.49 | -19.73 | 81.62 | 9.58 | 209.94 | 0.3152 | 798.0 | 663.5 | |
| 0.00 | 0.85 | 0.00 | 0.44 | -19.58 | 81.52 | 9.47 | 209.93 | 0.3122 | 622.0 | 498.8 | |
| 0.00 | 1.19 | 0.00 | 0.60 | -13.09 | 81.15 | 9.11 | 224.15 | 0.2223 | -715.0 | -610.7 | |
| 0.00 | 2.12 | 0.00 | 1.08 | -13.45 | 80.43 | 8.38 | 220.69 | 0.2185 | -821.0 | -745.3 | |
| 0.00 | 1.53 | 0.00 | 0.77 | -12.62 | 80.04 | 7.99 | 222.02 | 0.2036 | -823.0 | -701.1 | |
| 0.00 | 1.27 | 0.00 | 0.65 | -18.33 | 75.23 | 3.19 | 192.02 | 0.2543 | 845.0 | 697.8 | |
| 0.00 | 0.68 | 0.00 | 0.35 | -19.59 | 74.88 | 2.83 | 189.83 | 0.2740 | 352.0 | 393.4 | |
| 0.00 | 1.10 | 0.00 | 0.56 | -17.94 | 74.23 | 2.19 | 188.57 | 0.2448 | 984.0 | 749.3 | |
| 0.00 | 1.36 | 0.00 | 0.69 | -14.31 | 68.94 | -3.11 | 163.64 | 0.1875 | -876.0 | -706.8 | |
| 0.00 | 1.61 | 0.00 | 0.85 | -19.22 | 58.58 | -13.46 | 140.25 | 0.3453 | -939.0 | -757.0 | |
| 0.00 | 2.29 | 0.00 | 1.19 | -15.46 | 58.68 | -13.37 | 131.98 | 0.3011 | -880.0 | -701.1 | |
| 0.00 | 0.93 | 0.00 | 0.54 | -29.08 | 53.59 | -18.46 | 147.05 | 0.5108 | -654.0 | -560.8 | |
| 0.00 | 1.78 | 0.00 | 0.99 | -24.24 | 53.88 | -18.17 | 140.85 | 0.4522 | -989.0 | -809.9 | |
| 0.00 | 0.68 | 0.00 | 0.37 | -20.48 | 51.36 | -20.69 | 131.01 | 0.4406 | -691.0 | -596.8 | |
| 0.00 | 1.61 | 0.00 | 1.03 | -28.70 | 40.53 | -31.51 | 132.95 | 0.6287 | -633.0 | -485.3 | |
| 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. | |