SDO HMI 2014-04-07 11:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 76.16 | 413.45 | 41.28 | 224.15 | 12.75 | 13.45 | 14.71 | 322.30 | 0.4069 | -1170.2 | -397.3 | |
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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 | 1.67 | 0.00 | 0.90 | 10.38 | 13.62 | 14.88 | 318.06 | 0.3795 | 770.0 | 595.5 | |
| 71.59 | 397.33 | 38.80 | 215.44 | 12.70 | 13.52 | 14.78 | 322.10 | 0.4070 | -1436.1 | -421.6 | |
| 0.00 | 1.76 | 0.00 | 0.94 | 10.62 | 13.25 | 14.51 | 319.19 | 0.3785 | 732.0 | 525.0 | |
| 3.87 | -2.00 | 2.10 | -2.00 | 13.33 | 13.18 | 14.44 | 323.69 | 0.4116 | -994.6 | 999999 | |
| 0.00 | 3.35 | 0.00 | 1.83 | 14.88 | 12.71 | 13.97 | 326.76 | 0.4274 | 739.0 | 686.8 | |
| 0.00 | 0.97 | 0.00 | 0.52 | 12.28 | 11.73 | 12.99 | 324.99 | 0.3844 | -751.0 | -542.4 | |
| 0.00 | 0.44 | 0.00 | 0.24 | 14.80 | 11.87 | 13.13 | 328.25 | 0.4192 | -626.0 | -521.4 | |
| 0.00 | 0.44 | 0.00 | 0.24 | 11.80 | 11.51 | 12.77 | 324.70 | 0.3762 | -574.0 | -517.2 | |
| 0.00 | 1.50 | 0.00 | 0.82 | 14.76 | 11.65 | 12.91 | 328.64 | 0.4168 | -670.0 | -570.6 | |
| 0.70 | 3.52 | 0.38 | 1.91 | 14.56 | 11.28 | 12.54 | 329.10 | 0.4111 | -970.9 | -745.4 | |
| 0.00 | 2.47 | 0.00 | 1.31 | 11.31 | 10.99 | 12.25 | 325.06 | 0.3649 | 695.0 | 592.8 | |
| 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. | |