SDO HMI 2014-01-09 10:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.71 | 0.00 | 10.12 | -15.10 | 112.52 | 33.87 | 248.70 | 0.5784 | -336.3 | -289.3 | |
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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 | 0.60 | 0.00 | 0.43 | -10.90 | 125.42 | 46.76 | 258.75 | 0.7317 | 431.0 | 459.9 | |
| 0.00 | 0.60 | 0.00 | 0.40 | -14.24 | 121.33 | 42.67 | 253.37 | 0.6880 | 588.0 | 504.6 | |
| 0.00 | 1.28 | 0.00 | 0.83 | -12.31 | 118.78 | 40.12 | 255.64 | 0.6523 | 655.0 | 538.5 | |
| 0.00 | 1.53 | 0.00 | 0.98 | -12.00 | 117.74 | 39.09 | 255.90 | 0.6382 | 631.0 | 535.7 | |
| 0.00 | 0.60 | 0.00 | 0.37 | -12.26 | 115.79 | 37.13 | 255.01 | 0.6130 | -444.0 | -455.4 | |
| 0.00 | 0.94 | 0.00 | 0.56 | -14.01 | 112.24 | 33.59 | 250.92 | 0.5702 | -749.0 | -617.4 | |
| 0.00 | 0.34 | 0.00 | 0.20 | -14.29 | 111.13 | 32.47 | 249.96 | 0.5560 | -753.0 | -576.0 | |
| 0.00 | 0.85 | 0.00 | 0.50 | -16.38 | 109.97 | 31.31 | 245.73 | 0.5491 | -571.0 | -559.0 | |
| 0.00 | 1.79 | 0.00 | 1.06 | -17.23 | 110.05 | 31.39 | 244.33 | 0.5542 | -573.0 | -503.5 | |
| 0.00 | 2.64 | 0.00 | 1.56 | -17.17 | 109.86 | 31.20 | 244.31 | 0.5514 | -498.0 | -513.8 | |
| 0.00 | 0.85 | 0.00 | 0.50 | -16.63 | 109.69 | 31.03 | 245.14 | 0.5465 | -711.0 | -587.5 | |
| 0.00 | 0.77 | 0.00 | 0.45 | -16.67 | 109.48 | 30.82 | 244.95 | 0.5439 | -750.0 | -597.4 | |
| 0.00 | 1.45 | 0.00 | 0.85 | -16.74 | 109.24 | 30.58 | 244.69 | 0.5411 | -710.0 | -612.5 | |
| 0.00 | 1.19 | 0.00 | 0.70 | -17.12 | 108.81 | 30.15 | 243.76 | 0.5373 | -842.0 | -741.3 | |
| 0.00 | 1.28 | 0.00 | 0.73 | -13.58 | 107.17 | 28.52 | 249.31 | 0.4981 | -749.0 | -628.0 | |
| 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. | |