SDO HMI 2014-05-26 07:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.92 | 0.00 | 9.61 | -18.49 | 49.73 | -23.62 | 128.23 | 0.4823 | 447.3 | 368.6 | |
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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 | 1.35 | 0.00 | 0.74 | -17.98 | 54.99 | -18.36 | 133.79 | 0.4167 | 856.0 | 608.3 | |
| 0.00 | 1.35 | 0.00 | 0.73 | -15.96 | 53.96 | -19.39 | 128.43 | 0.4091 | 736.0 | 642.6 | |
| 0.00 | 0.99 | 0.00 | 0.54 | -15.67 | 53.32 | -20.03 | 126.99 | 0.4146 | 637.0 | 592.0 | |
| 0.00 | 0.54 | 0.00 | 0.29 | -15.79 | 53.21 | -20.14 | 127.09 | 0.4172 | 691.0 | 586.0 | |
| 0.00 | 1.26 | 0.00 | 0.69 | -15.16 | 53.14 | -20.21 | 125.74 | 0.4125 | 733.0 | 584.7 | |
| 0.00 | 1.53 | 0.00 | 0.83 | -14.88 | 53.13 | -20.22 | 125.15 | 0.4102 | 763.0 | 548.9 | |
| 0.00 | 1.44 | 0.00 | 0.80 | -18.53 | 52.41 | -20.94 | 131.20 | 0.4522 | 729.0 | 560.9 | |
| 0.00 | 0.45 | 0.00 | 0.25 | -19.20 | 52.12 | -21.24 | 131.98 | 0.4621 | 622.0 | 458.0 | |
| 0.00 | 1.17 | 0.00 | 0.67 | -22.52 | 51.15 | -22.20 | 136.08 | 0.5052 | 685.0 | 553.8 | |
| 0.00 | 1.08 | 0.00 | 0.61 | -20.06 | 50.98 | -22.37 | 132.02 | 0.4831 | 752.0 | 657.1 | |
| 0.00 | 1.35 | 0.00 | 0.75 | -15.24 | 50.93 | -22.42 | 123.28 | 0.4419 | 666.0 | 511.8 | |
| 0.00 | 1.44 | 0.00 | 0.87 | -20.26 | 43.29 | -30.07 | 124.82 | 0.5746 | 772.0 | 607.2 | |
| 0.00 | 0.90 | 0.00 | 0.55 | -21.74 | 42.49 | -30.86 | 126.40 | 0.5941 | -680.0 | -604.2 | |
| 0.00 | 0.81 | 0.00 | 0.50 | -22.09 | 42.14 | -31.21 | 126.64 | 0.6006 | -697.0 | -549.7 | |
| 0.00 | 1.26 | 0.00 | 0.79 | -22.66 | 40.83 | -32.52 | 126.47 | 0.6191 | -555.0 | -453.0 | |
| 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. | |