SDO HMI 2014-05-26 00:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.13 | 0.00 | 8.34 | -18.35 | 48.79 | -28.41 | 123.27 | 0.5398 | 503.3 | 416.9 | |
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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 |
| 0.00 | 1.53 | 0.00 | 0.86 | -15.71 | 53.16 | -24.04 | 122.40 | 0.4664 | 814.0 | 602.8 | |
| 0.00 | 1.44 | 0.00 | 0.82 | -18.26 | 52.48 | -24.72 | 126.32 | 0.4948 | 682.0 | 555.2 | |
| 0.00 | 1.53 | 0.00 | 0.88 | -19.47 | 52.08 | -25.12 | 127.93 | 0.5095 | 753.0 | 572.2 | |
| 0.00 | 1.08 | 0.00 | 0.62 | -18.38 | 52.25 | -24.95 | 126.30 | 0.4986 | 731.0 | 615.3 | |
| 0.00 | 0.54 | 0.00 | 0.31 | -19.56 | 51.92 | -25.28 | 127.93 | 0.5122 | 272.0 | 372.2 | |
| 0.00 | 0.63 | 0.00 | 0.36 | -19.04 | 51.18 | -26.01 | 126.35 | 0.5168 | 553.0 | 375.3 | |
| 0.00 | 1.98 | 0.00 | 1.12 | -15.15 | 51.17 | -26.03 | 119.53 | 0.4887 | 583.0 | 492.8 | |
| 0.00 | 0.81 | 0.00 | 0.46 | -15.09 | 50.94 | -26.26 | 119.20 | 0.4914 | 619.0 | 477.3 | |
| 0.00 | 2.25 | 0.00 | 1.42 | -20.41 | 43.16 | -34.03 | 122.13 | 0.6217 | 745.0 | 568.1 | |
| 0.00 | 0.99 | 0.00 | 0.63 | -20.64 | 43.03 | -34.17 | 122.37 | 0.6246 | 413.0 | 362.5 | |
| 0.00 | 1.35 | 0.00 | 0.86 | -20.01 | 42.13 | -35.07 | 120.90 | 0.6315 | -629.0 | -508.1 | |
| 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. | |