SDO HMI 2014-09-28 07:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.45 | 0.00 | 7.87 | 6.56 | 206.97 | -13.50 | 90.55 | 0.2341 | 277.7 | 349.0 | |
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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 | 1.06 | 0.00 | 0.53 | 5.76 | 210.79 | -9.69 | 95.88 | 0.1691 | -903.0 | -706.2 | |
| 0.00 | 0.71 | 0.00 | 0.36 | 6.51 | 209.51 | -10.96 | 91.09 | 0.1898 | -752.0 | -563.0 | |
| 0.00 | 0.62 | 0.00 | 0.31 | 6.21 | 209.21 | -11.26 | 92.60 | 0.1953 | -918.0 | -724.0 | |
| 0.00 | 1.32 | 0.00 | 0.67 | 6.62 | 207.81 | -12.66 | 90.25 | 0.2188 | -913.0 | -674.5 | |
| 0.00 | 2.21 | 0.00 | 1.12 | 5.72 | 207.68 | -12.80 | 94.32 | 0.2220 | 897.0 | 745.2 | |
| 0.00 | 0.53 | 0.00 | 0.27 | 5.71 | 207.37 | -13.11 | 94.22 | 0.2273 | 421.0 | 551.0 | |
| 0.00 | 2.03 | 0.00 | 1.04 | 8.00 | 206.52 | -13.95 | 84.32 | 0.2410 | 913.0 | 767.7 | |
| 0.00 | 1.06 | 0.00 | 0.54 | 8.21 | 206.20 | -14.27 | 83.59 | 0.2466 | 953.0 | 724.8 | |
| 0.00 | 0.79 | 0.00 | 0.41 | 8.68 | 206.06 | -14.41 | 81.72 | 0.2498 | 894.0 | 776.9 | |
| 0.00 | 1.41 | 0.00 | 0.72 | 8.56 | 205.94 | -14.53 | 82.27 | 0.2515 | 673.0 | 592.4 | |
| 0.00 | 1.24 | 0.00 | 0.63 | 4.38 | 205.90 | -14.57 | 98.88 | 0.2550 | 764.0 | 601.0 | |
| 0.00 | 1.32 | 0.00 | 0.68 | 4.07 | 205.57 | -14.91 | 99.82 | 0.2616 | 809.0 | 544.7 | |
| 0.00 | 1.15 | 0.00 | 0.59 | 6.62 | 204.53 | -15.94 | 89.85 | 0.2741 | 772.0 | 571.5 | |
| 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. | |