SDO HMI 2014-09-08 05:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.55 | 56.57 | 16.06 | 94.84 | -9.54 | 196.56 | 70.96 | 257.58 | 0.9549 | 186.5 | -53.9 | |
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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 |
| 4.02 | 38.28 | 7.22 | 69.88 | -9.49 | 198.02 | 72.42 | 257.92 | 0.9628 | 396.9 | -5.5 | |
| 3.12 | -1.00 | 5.65 | -1.00 | -9.83 | 198.00 | 72.40 | 257.57 | 0.9630 | 425.5 | 999999 | |
| 0.00 | 0.27 | 0.00 | 0.45 | -9.09 | 196.82 | 71.23 | 258.10 | 0.9567 | 434.0 | 441.0 | |
| 0.00 | 0.71 | 0.00 | 1.17 | -8.99 | 196.48 | 70.89 | 258.15 | 0.9549 | 549.0 | 494.5 | |
| 0.00 | 0.80 | 0.00 | 1.29 | -8.72 | 196.08 | 70.49 | 258.35 | 0.9526 | 510.0 | 465.9 | |
| 0.00 | 1.34 | 0.00 | 2.06 | -9.04 | 195.13 | 69.54 | 257.83 | 0.9479 | 274.0 | 295.9 | |
| 0.00 | 0.27 | 0.00 | 0.40 | -9.46 | 194.70 | 69.10 | 257.31 | 0.9460 | 346.0 | 306.3 | |
| 0.00 | 0.98 | 0.00 | 1.33 | -8.78 | 192.44 | 66.85 | 257.55 | 0.9321 | -90.0 | -85.1 | |
| 0.80 | 2.41 | 1.11 | 3.32 | -10.56 | 192.45 | 66.85 | 255.68 | 0.9344 | -194.7 | -116.4 | |
| 0.00 | 1.34 | 0.00 | 1.71 | -8.11 | 191.21 | 65.62 | 258.01 | 0.9235 | -361.0 | -329.9 | |
| 0.54 | 6.51 | 0.70 | 8.50 | -9.07 | 191.46 | 65.87 | 257.04 | 0.9264 | -456.2 | -452.8 | |
| 0.00 | 1.25 | 0.00 | 1.62 | -9.25 | 191.38 | 65.78 | 256.83 | 0.9261 | -584.0 | -450.1 | |
| 0.00 | 0.27 | 0.00 | 0.35 | -9.71 | 191.32 | 65.73 | 256.33 | 0.9264 | -317.0 | -252.7 | |
| 1.07 | 2.14 | 1.38 | 2.76 | -9.58 | 191.05 | 65.46 | 256.41 | 0.9244 | -595.5 | -548.7 | |
| 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. | |