SDO HMI 2014-09-26 19:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.21 | 0.00 | 10.13 | 7.11 | 207.36 | -32.91 | 87.66 | 0.5417 | 173.4 | 160.8 | |
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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 |
| 0.00 | 3.35 | 0.00 | 1.91 | 6.51 | 210.40 | -29.87 | 88.98 | 0.4969 | -648.0 | -590.6 | |
| 0.00 | 0.97 | 0.00 | 0.55 | 5.90 | 210.37 | -29.90 | 90.19 | 0.4979 | -778.0 | -584.1 | |
| 0.00 | 0.97 | 0.00 | 0.56 | 6.24 | 208.94 | -31.33 | 89.37 | 0.5190 | -795.0 | -654.4 | |
| 0.00 | 0.97 | 0.00 | 0.57 | 5.07 | 208.05 | -32.22 | 91.48 | 0.5334 | -670.0 | -538.7 | |
| 0.00 | 0.62 | 0.00 | 0.37 | 5.95 | 206.81 | -33.46 | 89.67 | 0.5506 | 522.0 | 515.0 | |
| 0.00 | 4.68 | 0.00 | 2.78 | 7.70 | 206.38 | -33.89 | 86.47 | 0.5558 | 587.0 | 636.9 | |
| 0.00 | 1.06 | 0.00 | 0.63 | 7.44 | 206.07 | -34.20 | 86.93 | 0.5603 | 524.0 | 468.2 | |
| 0.00 | 0.62 | 0.00 | 0.37 | 8.10 | 205.98 | -34.30 | 85.75 | 0.5616 | 631.0 | 558.1 | |
| 0.00 | 0.97 | 0.00 | 0.58 | 7.43 | 205.85 | -34.42 | 86.95 | 0.5635 | 696.0 | 536.5 | |
| 0.00 | 0.97 | 0.00 | 0.58 | 9.06 | 205.51 | -34.76 | 84.04 | 0.5683 | 681.0 | 577.7 | |
| 0.00 | 1.15 | 0.00 | 0.69 | 6.87 | 205.68 | -34.59 | 87.92 | 0.5662 | 648.0 | 504.1 | |
| 0.00 | 0.88 | 0.00 | 0.54 | 8.01 | 204.72 | -35.55 | 85.88 | 0.5794 | 683.0 | 554.0 | |
| 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. | |