SDO HMI 2014-09-07 10:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 43.02 | 142.73 | 44.00 | 144.50 | -9.23 | 194.55 | 58.49 | 255.06 | 0.8722 | 151.4 | 6.0 | |
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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 | 0.27 | 0.00 | 0.29 | -8.33 | 196.97 | 60.91 | 256.71 | 0.8903 | 255.0 | 207.7 | |
| 5.53 | 70.88 | 6.04 | 76.58 | -9.52 | 197.05 | 60.99 | 255.42 | 0.8931 | 412.7 | 97.6 | |
| 8.57 | -2.00 | 9.27 | -2.00 | -9.22 | 196.84 | 60.78 | 255.70 | 0.8909 | 691.5 | 999999 | |
| 12.85 | -2.00 | 13.67 | -2.00 | -9.19 | 196.33 | 60.27 | 255.60 | 0.8869 | 771.4 | 999999 | |
| 0.00 | 0.71 | 0.00 | 0.74 | -8.82 | 195.55 | 59.49 | 255.81 | 0.8801 | 495.0 | 504.9 | |
| 0.00 | 4.91 | 0.00 | 4.89 | -9.59 | 194.03 | 57.97 | 254.54 | 0.8693 | 575.0 | 508.1 | |
| 0.00 | 1.79 | 0.00 | 1.77 | -9.20 | 193.93 | 57.87 | 254.95 | 0.8676 | 258.0 | 202.9 | |
| 0.00 | 0.80 | 0.00 | 0.78 | -7.91 | 193.50 | 57.44 | 256.29 | 0.8614 | -232.0 | -184.9 | |
| 0.00 | 5.80 | 0.00 | 5.53 | -8.97 | 192.67 | 56.61 | 254.86 | 0.8565 | -373.0 | -262.7 | |
| 0.00 | 1.16 | 0.00 | 1.09 | -8.79 | 192.13 | 56.07 | 254.91 | 0.8513 | -372.0 | -311.1 | |
| 5.00 | 49.54 | 4.69 | 46.47 | -9.12 | 192.04 | 55.98 | 254.51 | 0.8513 | -515.5 | -66.3 | |
| 0.00 | 1.43 | 0.00 | 1.32 | -8.13 | 191.82 | 55.76 | 255.58 | 0.8471 | -388.0 | -338.8 | |
| 0.00 | 3.39 | 0.00 | 3.15 | -8.69 | 191.78 | 55.72 | 254.93 | 0.8480 | -646.0 | -588.2 | |
| 0.00 | 2.05 | 0.00 | 1.89 | -8.29 | 191.58 | 55.52 | 255.32 | 0.8453 | -656.0 | -527.1 | |
| 11.07 | -11.00 | 10.33 | -11.00 | -9.40 | 191.72 | 55.66 | 254.09 | 0.8492 | -752.2 | 999999 | |
| 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. | |