SDO HMI 2014-09-24 01:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.62 | 0.00 | 9.17 | -15.15 | 286.74 | 10.19 | 204.23 | 0.4302 | 701.3 | 562.7 | |
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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 |
| 0.00 | 0.97 | 0.00 | 0.56 | -10.03 | 301.42 | 24.87 | 235.75 | 0.5030 | 588.0 | 493.2 | |
| 0.00 | 0.71 | 0.00 | 0.40 | -9.19 | 299.72 | 23.16 | 235.26 | 0.4745 | 635.0 | 620.6 | |
| 0.00 | 0.88 | 0.00 | 0.50 | -10.28 | 299.63 | 23.08 | 233.28 | 0.4831 | 744.0 | 674.1 | |
| 0.00 | 2.03 | 0.00 | 1.10 | -12.22 | 290.68 | 14.13 | 216.22 | 0.4055 | 775.0 | 586.5 | |
| 0.00 | 0.53 | 0.00 | 0.29 | -11.25 | 290.41 | 13.86 | 217.16 | 0.3906 | 419.0 | 542.3 | |
| 0.00 | 1.06 | 0.00 | 0.55 | -8.30 | 286.81 | 10.26 | 213.90 | 0.3172 | 747.0 | 581.2 | |
| 0.00 | 2.12 | 0.00 | 1.22 | -21.70 | 287.04 | 10.49 | 199.47 | 0.5096 | 768.0 | 585.8 | |
| 0.00 | 1.06 | 0.00 | 0.61 | -22.96 | 282.78 | 6.22 | 191.31 | 0.5109 | 569.0 | 401.9 | |
| 0.00 | 1.06 | 0.00 | 0.55 | -10.09 | 282.32 | 5.77 | 198.63 | 0.3111 | 811.0 | 601.7 | |
| 0.00 | 1.15 | 0.00 | 0.61 | -13.61 | 281.93 | 5.37 | 194.51 | 0.3650 | 832.0 | 625.5 | |
| 0.00 | 1.15 | 0.00 | 0.67 | -23.96 | 282.16 | 5.61 | 189.85 | 0.5240 | 616.0 | 417.7 | |
| 0.00 | 1.06 | 0.00 | 0.57 | -14.12 | 281.29 | 4.73 | 192.52 | 0.3706 | 762.0 | 618.7 | |
| 0.00 | 1.42 | 0.00 | 0.80 | -21.10 | 279.98 | 3.43 | 186.75 | 0.4763 | 689.0 | 510.6 | |
| 0.00 | 1.42 | 0.00 | 0.74 | -10.71 | 278.25 | 1.70 | 185.47 | 0.3072 | 863.0 | 624.9 | |
| 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. | |