SDO HMI 2014-07-19 22:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 31.92 | 107.14 | 17.70 | 59.39 | -21.68 | 67.89 | -2.50 | 174.88 | 0.4498 | 139.9 | 24.8 | |
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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 |
| 17.78 | 48.98 | 9.82 | 27.09 | -21.51 | 69.41 | -0.98 | 177.95 | 0.4448 | 1137.6 | 436.3 | |
| 0.00 | 7.62 | 0.00 | 4.19 | -20.97 | 69.15 | -1.23 | 177.35 | 0.4364 | 460.0 | 688.5 | |
| 2.63 | 6.89 | 1.45 | 3.80 | -21.27 | 68.82 | -1.56 | 176.69 | 0.4415 | 913.5 | 635.2 | |
| 0.00 | 0.82 | 0.00 | 0.45 | -21.48 | 68.39 | -1.99 | 175.82 | 0.4451 | 640.0 | 487.2 | |
| 0.36 | 2.09 | 0.20 | 1.15 | -21.24 | 67.87 | -2.51 | 174.68 | 0.4421 | 677.8 | 534.5 | |
| 0.00 | 0.91 | 0.00 | 0.50 | -21.85 | 67.63 | -2.75 | 174.32 | 0.4520 | -749.0 | -575.3 | |
| 0.00 | 1.36 | 0.00 | 0.76 | -22.40 | 67.39 | -2.99 | 173.96 | 0.4609 | -592.0 | -436.8 | |
| 0.00 | 1.09 | 0.00 | 0.61 | -21.99 | 66.25 | -4.14 | 171.55 | 0.4569 | -400.0 | -450.2 | |
| 0.00 | 2.63 | 0.00 | 1.47 | -22.27 | 66.14 | -4.24 | 171.43 | 0.4613 | -758.0 | -645.1 | |
| 0.00 | 9.71 | 0.00 | 5.39 | -21.66 | 65.90 | -4.49 | 170.71 | 0.4525 | -973.0 | -807.8 | |
| 0.00 | 5.26 | 0.00 | 2.93 | -22.13 | 65.88 | -4.50 | 170.86 | 0.4599 | -847.0 | -640.3 | |
| 0.00 | 1.36 | 0.00 | 0.76 | -22.00 | 65.59 | -4.80 | 170.23 | 0.4586 | -646.0 | -729.3 | |
| 1.81 | 3.36 | 1.01 | 1.87 | -22.07 | 65.36 | -5.03 | 169.79 | 0.4603 | -997.0 | -856.5 | |
| 3.72 | 15.06 | 2.08 | 8.42 | -22.48 | 65.27 | -5.11 | 169.80 | 0.4667 | -825.6 | -703.9 | |
| 5.62 | -14.00 | 3.14 | -14.00 | -22.31 | 65.08 | -5.30 | 169.35 | 0.4647 | -906.0 | 999999 | |
| 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. | |