SDO HMI 2014-09-08 11:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.05 | 0.00 | 11.11 | -17.97 | 159.01 | 36.71 | 234.69 | 0.6983 | 259.4 | 199.6 | |
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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 | 0.89 | 0.00 | 0.64 | -17.30 | 161.64 | 39.33 | 237.33 | 0.7212 | 521.0 | 435.1 | |
| 0.00 | 0.98 | 0.00 | 0.70 | -17.98 | 161.16 | 38.86 | 236.19 | 0.7205 | 447.0 | 328.7 | |
| 0.00 | 0.80 | 0.00 | 0.58 | -19.26 | 161.26 | 38.96 | 234.74 | 0.7293 | 572.0 | 508.3 | |
| 0.00 | 1.16 | 0.00 | 0.83 | -18.86 | 160.86 | 38.56 | 234.94 | 0.7229 | 588.0 | 524.8 | |
| 0.00 | 1.70 | 0.00 | 1.19 | -17.50 | 160.47 | 38.16 | 236.32 | 0.7105 | 622.0 | 543.6 | |
| 0.00 | 0.80 | 0.00 | 0.57 | -18.61 | 160.67 | 38.37 | 235.11 | 0.7195 | 723.0 | 644.0 | |
| 0.00 | 1.07 | 0.00 | 0.76 | -18.38 | 160.33 | 38.02 | 235.15 | 0.7146 | 677.0 | 598.1 | |
| 0.00 | 0.89 | 0.00 | 0.62 | -17.91 | 159.93 | 37.62 | 235.44 | 0.7076 | 489.0 | 358.9 | |
| 0.00 | 1.25 | 0.00 | 0.90 | -20.61 | 160.54 | 38.24 | 232.67 | 0.7309 | 71.0 | 148.0 | |
| 0.00 | 0.71 | 0.00 | 0.48 | -16.28 | 157.66 | 35.36 | 235.85 | 0.6735 | 692.0 | 625.5 | |
| 0.00 | 1.61 | 0.00 | 1.09 | -18.17 | 157.30 | 34.99 | 233.22 | 0.6827 | -653.0 | -604.7 | |
| 0.00 | 1.25 | 0.00 | 0.83 | -16.38 | 156.84 | 34.53 | 235.10 | 0.6654 | 629.0 | 489.6 | |
| 0.00 | 0.98 | 0.00 | 0.66 | -18.82 | 156.21 | 33.90 | 231.57 | 0.6763 | -589.0 | -548.8 | |
| 0.00 | 0.98 | 0.00 | 0.63 | -16.03 | 154.69 | 32.38 | 233.84 | 0.6399 | -339.0 | -437.7 | |
| 0.00 | 0.98 | 0.00 | 0.63 | -16.45 | 154.66 | 32.35 | 233.26 | 0.6427 | -559.0 | -400.7 | |
| 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. | |