SDO HMI 2014-05-29 16:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.22 | 169.57 | 16.14 | 85.07 | -8.99 | 25.10 | -3.61 | 156.63 | 0.1555 | 1071.2 | 452.9 | |
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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 |
| 9.75 | 153.61 | 4.88 | 76.98 | -9.06 | 25.76 | -2.95 | 160.13 | 0.1502 | 1198.1 | 433.2 | |
| 22.47 | -1.00 | 11.26 | -1.00 | -8.97 | 25.42 | -3.29 | 157.83 | 0.1508 | 1330.7 | 999999 | |
| 0.00 | 1.08 | 0.00 | 0.54 | -9.18 | 23.48 | -5.23 | 147.74 | 0.1695 | 905.0 | 625.0 | |
| 0.00 | 1.44 | 0.00 | 0.73 | -10.19 | 23.43 | -5.28 | 150.51 | 0.1848 | 793.0 | 628.9 | |
| 0.00 | 1.26 | 0.00 | 0.63 | -8.78 | 23.36 | -5.35 | 145.83 | 0.1648 | 794.0 | 610.8 | |
| 0.00 | 3.07 | 0.00 | 1.55 | -9.82 | 23.10 | -5.61 | 147.92 | 0.1823 | 941.0 | 865.5 | |
| 0.00 | 2.98 | 0.00 | 1.50 | -9.54 | 23.07 | -5.64 | 146.95 | 0.1786 | 997.0 | 908.7 | |
| 0.00 | 1.08 | 0.00 | 0.55 | -9.97 | 22.94 | -5.77 | 147.65 | 0.1860 | 906.0 | 810.2 | |
| 0.00 | 1.44 | 0.00 | 0.73 | -9.85 | 22.63 | -6.08 | 145.93 | 0.1871 | 709.0 | 456.0 | |
| 0.00 | 1.99 | 0.00 | 1.01 | -1.98 | 15.35 | -13.36 | 94.44 | 0.2326 | 946.0 | 763.2 | |
| 0.00 | 1.62 | 0.00 | 0.85 | -11.94 | 13.12 | -15.59 | 125.95 | 0.3262 | -891.0 | -672.2 | |
| 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. | |