SDO HMI 2014-10-06 01:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 48.32 | 293.70 | 30.25 | 184.43 | -1.50 | 155.22 | 37.02 | 259.07 | 0.6152 | 821.4 | 330.9 | |
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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 |
| 33.56 | 267.43 | 21.13 | 168.40 | -1.53 | 155.51 | 37.31 | 259.13 | 0.6192 | 1098.1 | 341.8 | |
| 0.26 | -1.00 | 0.16 | -1.00 | -1.23 | 155.01 | 36.82 | 259.45 | 0.6117 | 1153.7 | 999999 | |
| 3.87 | -1.00 | 2.41 | -1.00 | -1.58 | 154.83 | 36.63 | 258.82 | 0.6103 | 1096.4 | 999999 | |
| 0.00 | 1.49 | 0.00 | 0.93 | -3.29 | 154.62 | 36.42 | 256.01 | 0.6132 | -138.0 | -179.4 | |
| 0.00 | 0.79 | 0.00 | 0.50 | -3.77 | 154.53 | 36.33 | 255.21 | 0.6137 | 471.0 | 437.8 | |
| 7.73 | 10.37 | 4.78 | 6.41 | -1.77 | 154.13 | 35.93 | 258.24 | 0.6013 | 906.9 | 701.9 | |
| 0.00 | 0.79 | 0.00 | 0.48 | -0.10 | 153.59 | 35.39 | 260.80 | 0.5889 | 762.0 | 650.6 | |
| 2.90 | 6.06 | 1.77 | 3.71 | -0.43 | 153.52 | 35.32 | 260.23 | 0.5889 | 896.5 | 720.3 | |
| 0.00 | 1.23 | 0.00 | 0.74 | -0.08 | 151.88 | 33.68 | 260.25 | 0.5648 | 755.0 | 681.4 | |
| 0.00 | 2.55 | 0.00 | 1.52 | -0.67 | 151.13 | 32.93 | 258.94 | 0.5560 | -758.0 | -640.8 | |
| 0.00 | 1.05 | 0.00 | 0.62 | -0.39 | 150.55 | 32.35 | 259.20 | 0.5469 | -681.0 | -547.2 | |
| 0.00 | 0.53 | 0.00 | 0.31 | -1.60 | 148.66 | 30.47 | 256.14 | 0.5241 | -622.0 | -609.8 | |
| 0.00 | 1.41 | 0.00 | 0.81 | -1.68 | 148.42 | 30.22 | 255.87 | 0.5209 | -655.0 | -428.2 | |
| 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. | |