SDO HMI 2013-01-09 04:58:54 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 40.62 | 228.50 | 24.99 | 140.24 | -24.63 | 249.78 | 30.82 | 232.14 | 0.5919 | 598.2 | 281.1 | |
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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 | 1.19 | 0.00 | 0.73 | -18.63 | 252.97 | 34.01 | 243.50 | 0.5945 | -592.0 | -507.9 | |
| 0.00 | 0.85 | 0.00 | 0.53 | -22.22 | 252.80 | 33.84 | 237.86 | 0.6111 | -640.0 | -561.4 | |
| 1.70 | 215.09 | 1.04 | 132.38 | -24.13 | 250.05 | 31.08 | 233.11 | 0.5914 | 1048.6 | 340.8 | |
| 36.88 | -3.00 | 22.70 | -3.00 | -24.70 | 250.09 | 31.13 | 232.30 | 0.5958 | 1183.5 | 999999 | |
| 1.02 | -3.00 | 0.63 | -3.00 | -25.06 | 249.58 | 30.62 | 231.38 | 0.5928 | 870.5 | 999999 | |
| 1.02 | -3.00 | 0.62 | -3.00 | -25.14 | 249.34 | 30.38 | 231.08 | 0.5906 | 712.5 | 999999 | |
| 0.00 | 1.44 | 0.00 | 0.86 | -25.39 | 246.05 | 27.09 | 227.87 | 0.5569 | -671.0 | -488.2 | |
| 0.00 | 1.10 | 0.00 | 0.66 | -25.34 | 245.86 | 26.89 | 227.77 | 0.5543 | -727.0 | -603.3 | |
| 0.00 | 0.93 | 0.00 | 0.56 | -25.69 | 245.72 | 26.76 | 227.12 | 0.5559 | -583.0 | -459.5 | |
| 0.00 | 1.02 | 0.00 | 0.58 | -22.14 | 243.29 | 24.33 | 230.24 | 0.4984 | -832.0 | -643.1 | |
| 0.00 | 1.70 | 0.00 | 0.97 | -22.45 | 243.24 | 24.28 | 229.67 | 0.5005 | -578.0 | -485.1 | |
| 0.00 | 0.85 | 0.00 | 0.48 | -22.34 | 242.87 | 23.91 | 229.47 | 0.4953 | -749.0 | -607.1 | |
| 0.00 | 1.36 | 0.00 | 0.77 | -21.84 | 242.64 | 23.68 | 230.05 | 0.4883 | -730.0 | -619.0 | |
| 0.00 | 0.76 | 0.00 | 0.44 | -24.01 | 242.10 | 23.13 | 225.90 | 0.5018 | -605.0 | -416.1 | |
| 0.00 | 2.21 | 0.00 | 1.28 | -25.89 | 241.90 | 22.94 | 222.83 | 0.5178 | -708.0 | -518.2 | |
| 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. | |