SDO HMI 2014-04-07 09:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 72.75 | 435.19 | 39.23 | 234.75 | 12.73 | 13.44 | 13.61 | 324.41 | 0.3963 | -1095.6 | -394.0 | |
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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 | 0.57 | 10.95 | 14.26 | 14.43 | 319.94 | 0.3818 | -614.0 | -584.8 | |
| 2.20 | 413.34 | 1.19 | 223.02 | 12.99 | 13.71 | 13.88 | 324.29 | 0.4021 | -912.7 | -420.9 | |
| 0.00 | 2.20 | 0.00 | 1.17 | 10.62 | 13.55 | 13.72 | 320.79 | 0.3704 | 442.0 | 521.3 | |
| 67.38 | -2.00 | 36.33 | -2.00 | 12.67 | 13.53 | 13.70 | 324.15 | 0.3963 | -1495.4 | 999999 | |
| 3.17 | -2.00 | 1.71 | -2.00 | 13.33 | 13.19 | 13.36 | 325.80 | 0.4017 | -1033.1 | 999999 | |
| 0.00 | 0.97 | 0.00 | 0.53 | 14.73 | 13.05 | 13.22 | 328.00 | 0.4191 | 651.0 | 556.2 | |
| 0.00 | 3.35 | 0.00 | 1.82 | 14.72 | 12.77 | 12.93 | 328.55 | 0.4166 | 693.0 | 637.4 | |
| 0.00 | 0.70 | 0.00 | 0.38 | 14.62 | 12.60 | 12.77 | 328.75 | 0.4139 | 764.0 | 574.2 | |
| 0.00 | 0.97 | 0.00 | 0.51 | 8.87 | 12.23 | 12.40 | 320.46 | 0.3347 | 733.0 | 518.5 | |
| 0.00 | 0.88 | 0.00 | 0.47 | 12.31 | 11.84 | 12.01 | 327.13 | 0.3762 | -624.0 | -494.4 | |
| 0.00 | 1.06 | 0.00 | 0.57 | 14.77 | 11.85 | 12.01 | 330.45 | 0.4098 | -685.0 | -517.8 | |
| 0.00 | 4.84 | 0.00 | 2.62 | 14.60 | 11.49 | 11.66 | 330.98 | 0.4047 | -854.0 | -677.6 | |
| 0.00 | 2.03 | 0.00 | 1.07 | 11.32 | 11.08 | 11.25 | 327.34 | 0.3559 | 819.0 | 638.9 | |
| 0.00 | 1.85 | 0.00 | 1.00 | 14.62 | 11.17 | 11.34 | 331.67 | 0.4026 | -917.0 | -701.9 | |
| 0.00 | 1.94 | 0.00 | 1.02 | 11.42 | 9.74 | 9.91 | 330.69 | 0.3461 | 643.0 | 419.4 | |
| 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. | |