SDO HMI 2014-09-07 04:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41.95 | 96.50 | 38.58 | 88.33 | -9.29 | 194.34 | 54.99 | 253.98 | 0.8425 | -20.0 | 143.5 | |
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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 | 0.71 | 0.00 | 0.70 | -9.01 | 196.76 | 57.41 | 255.03 | 0.8634 | 170.0 | 128.4 | |
| 11.07 | 42.50 | 10.79 | 41.00 | -9.49 | 196.60 | 57.25 | 254.44 | 0.8631 | 332.4 | 430.1 | |
| 5.09 | -2.00 | 4.90 | -2.00 | -9.23 | 196.25 | 56.90 | 254.63 | 0.8596 | 764.2 | 999999 | |
| 4.64 | -2.00 | 4.47 | -2.00 | -9.47 | 196.14 | 56.79 | 254.33 | 0.8591 | 740.4 | 999999 | |
| 0.00 | 1.52 | 0.00 | 1.42 | -8.91 | 195.28 | 55.93 | 254.72 | 0.8504 | 630.0 | 502.3 | |
| 0.98 | 2.68 | 0.92 | 2.51 | -9.18 | 195.23 | 55.88 | 254.40 | 0.8506 | 557.0 | 399.5 | |
| 0.00 | 0.45 | 0.00 | 0.41 | -8.92 | 194.84 | 55.50 | 254.58 | 0.8466 | 560.0 | 518.2 | |
| 0.80 | 1.87 | 0.72 | 1.68 | -8.09 | 193.81 | 54.46 | 255.23 | 0.8353 | -385.3 | -293.2 | |
| 0.00 | 0.80 | 0.00 | 0.71 | -8.77 | 193.16 | 53.81 | 254.25 | 0.8309 | -191.0 | -182.0 | |
| 0.00 | 0.89 | 0.00 | 0.79 | -9.14 | 193.03 | 53.68 | 253.78 | 0.8306 | -108.0 | -128.7 | |
| 0.00 | 1.52 | 0.00 | 1.34 | -9.05 | 192.86 | 53.51 | 253.82 | 0.8288 | -385.0 | -305.8 | |
| 0.00 | 0.71 | 0.00 | 0.61 | -8.33 | 191.94 | 52.59 | 254.38 | 0.8183 | -550.0 | -468.8 | |
| 19.37 | 40.53 | 16.78 | 35.17 | -9.32 | 192.09 | 52.74 | 253.27 | 0.8223 | -645.9 | -71.3 | |
| 0.00 | 1.07 | 0.00 | 0.92 | -8.45 | 191.86 | 52.52 | 254.22 | 0.8178 | -528.0 | -471.0 | |
| 0.00 | 1.25 | 0.00 | 1.07 | -8.63 | 191.75 | 52.40 | 253.97 | 0.8172 | -588.0 | -491.5 | |
| 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. | |