SDO HMI 2014-09-24 18:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 25.38 | 0.00 | 14.57 | -15.53 | 246.45 | -20.77 | 137.69 | 0.5094 | -813.7 | -679.7 | |
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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 | 2.12 | 0.00 | 1.22 | -15.68 | 247.12 | -20.10 | 138.82 | 0.5044 | -971.0 | -729.3 | |
| 0.00 | 2.39 | 0.00 | 1.37 | -16.01 | 247.02 | -20.20 | 139.12 | 0.5091 | -574.0 | -519.9 | |
| 0.00 | 1.24 | 0.00 | 0.71 | -15.13 | 247.11 | -20.11 | 138.05 | 0.4984 | -941.0 | -691.7 | |
| 0.00 | 0.80 | 0.00 | 0.45 | -14.25 | 247.20 | -20.02 | 136.93 | 0.4879 | -790.0 | -664.6 | |
| 0.00 | 1.33 | 0.00 | 0.76 | -15.75 | 246.95 | -20.27 | 138.67 | 0.5070 | -944.0 | -768.7 | |
| 0.00 | 2.47 | 0.00 | 1.42 | -15.26 | 246.93 | -20.29 | 137.98 | 0.5017 | -954.0 | -836.4 | |
| 0.00 | 1.15 | 0.00 | 0.66 | -15.96 | 246.73 | -20.49 | 138.64 | 0.5114 | -591.0 | -478.9 | |
| 0.00 | 1.50 | 0.00 | 0.86 | -15.64 | 246.53 | -20.69 | 137.94 | 0.5099 | -654.0 | -501.0 | |
| 0.00 | 1.24 | 0.00 | 0.71 | -15.72 | 246.15 | -21.07 | 137.53 | 0.5146 | -701.0 | -539.1 | |
| 0.00 | 1.50 | 0.00 | 0.86 | -15.17 | 246.11 | -21.11 | 136.72 | 0.5091 | -804.0 | -659.1 | |
| 0.00 | 1.24 | 0.00 | 0.71 | -15.01 | 245.99 | -21.23 | 136.35 | 0.5086 | -864.0 | -737.1 | |
| 0.00 | 3.36 | 0.00 | 1.94 | -15.93 | 245.89 | -21.33 | 137.47 | 0.5194 | -710.0 | -548.8 | |
| 0.00 | 5.04 | 0.00 | 2.90 | -15.38 | 245.85 | -21.37 | 136.66 | 0.5139 | -1080.0 | -847.4 | |
| 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. | |