SDO HMI 2014-01-09 19:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.23 | 0.00 | 9.66 | -19.41 | 65.96 | -7.74 | 163.70 | 0.3336 | -69.6 | -102.3 | |
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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 | 1.02 | 0.00 | 0.53 | -19.75 | 81.57 | 7.87 | 205.31 | 0.3027 | 864.0 | 681.9 | |
| 0.00 | 1.78 | 0.00 | 0.90 | -13.59 | 80.44 | 6.74 | 214.26 | 0.2035 | -699.0 | -609.8 | |
| 0.00 | 1.53 | 0.00 | 0.78 | -17.43 | 77.09 | 3.39 | 193.62 | 0.2405 | 825.0 | 614.4 | |
| 0.00 | 1.95 | 0.00 | 1.00 | -18.89 | 75.62 | 1.92 | 187.01 | 0.2604 | 784.0 | 483.5 | |
| 0.00 | 0.76 | 0.00 | 0.39 | -19.60 | 74.75 | 1.05 | 183.66 | 0.2709 | 786.0 | 652.3 | |
| 0.00 | 1.10 | 0.00 | 0.56 | -17.95 | 74.19 | 0.48 | 181.90 | 0.2426 | 903.0 | 771.3 | |
| 0.00 | 1.02 | 0.00 | 0.52 | -18.43 | 73.01 | -0.70 | 177.35 | 0.2510 | -884.0 | -737.7 | |
| 0.00 | 1.44 | 0.00 | 0.74 | -12.10 | 62.85 | -10.86 | 127.71 | 0.2339 | 941.0 | 714.8 | |
| 0.00 | 1.78 | 0.00 | 0.94 | -18.33 | 59.29 | -14.41 | 136.60 | 0.3454 | -755.0 | -517.7 | |
| 0.00 | 1.10 | 0.00 | 0.59 | -19.26 | 58.43 | -15.27 | 136.91 | 0.3656 | -919.0 | -734.8 | |
| 0.00 | 1.36 | 0.00 | 0.76 | -24.57 | 54.05 | -19.66 | 139.27 | 0.4708 | -641.0 | -507.9 | |
| 0.00 | 1.27 | 0.00 | 0.71 | -24.19 | 53.94 | -19.76 | 138.53 | 0.4678 | -750.0 | -682.1 | |
| 0.00 | 1.36 | 0.00 | 0.76 | -24.18 | 53.63 | -20.07 | 138.11 | 0.4709 | -866.0 | -768.5 | |
| 0.00 | 0.76 | 0.00 | 0.48 | -27.61 | 42.24 | -31.47 | 131.54 | 0.6203 | -564.0 | -453.1 | |
| 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. | |