SDO HMI 2014-03-05 05:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.15 | 40.72 | 11.66 | 40.04 | 7.75 | 135.19 | 58.06 | 283.41 | 0.8658 | -5.2 | 249.7 | |
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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 |
| 6.14 | 8.65 | 6.78 | 9.56 | 7.26 | 138.99 | 61.86 | 281.90 | 0.8958 | -527.9 | -323.6 | |
| 2.85 | 7.52 | 2.85 | 7.49 | 7.06 | 135.83 | 58.70 | 282.43 | 0.8704 | -378.7 | -340.5 | |
| 0.00 | 0.95 | 0.00 | 0.93 | 7.12 | 134.98 | 57.85 | 282.71 | 0.8633 | 352.0 | 243.2 | |
| 0.43 | 1.47 | 0.42 | 1.43 | 7.38 | 134.87 | 57.74 | 283.04 | 0.8629 | 354.2 | 232.4 | |
| 0.00 | 1.38 | 0.00 | 1.32 | 6.54 | 134.20 | 57.07 | 282.26 | 0.8554 | 410.0 | 294.9 | |
| 0.00 | 1.12 | 0.00 | 1.07 | 7.12 | 134.14 | 57.01 | 282.93 | 0.8561 | 418.0 | 412.0 | |
| 0.00 | 0.52 | 0.00 | 0.49 | 6.77 | 134.08 | 56.95 | 282.56 | 0.8548 | 433.0 | 420.2 | |
| 0.00 | 0.69 | 0.00 | 0.66 | 8.62 | 133.86 | 56.73 | 284.72 | 0.8568 | 385.0 | 333.0 | |
| 0.00 | 0.78 | 0.00 | 0.74 | 8.76 | 133.73 | 56.60 | 284.91 | 0.8559 | 430.0 | 382.6 | |
| 0.00 | 0.78 | 0.00 | 0.73 | 7.96 | 133.49 | 56.36 | 284.08 | 0.8521 | 282.0 | 273.6 | |
| 0.00 | 1.38 | 0.00 | 1.30 | 8.71 | 133.33 | 56.20 | 284.98 | 0.8524 | 222.0 | 336.8 | |
| 1.73 | 15.48 | 1.61 | 14.32 | 8.52 | 132.96 | 55.83 | 284.86 | 0.8487 | 693.7 | 544.5 | |
| 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. | |