SDO HMI 2014-09-27 11:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.65 | 0.00 | 11.71 | 6.81 | 207.57 | -23.91 | 88.76 | 0.4044 | -97.1 | -8.4 | |
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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 | 2.12 | 0.00 | 1.12 | 6.40 | 210.33 | -21.15 | 90.04 | 0.3601 | -695.0 | -658.1 | |
| 0.00 | 1.06 | 0.00 | 0.56 | 6.60 | 210.26 | -21.22 | 89.45 | 0.3611 | -762.0 | -576.2 | |
| 0.00 | 1.15 | 0.00 | 0.62 | 6.45 | 208.73 | -22.75 | 89.72 | 0.3859 | -732.0 | -569.4 | |
| 0.00 | 0.62 | 0.00 | 0.33 | 7.59 | 208.68 | -22.80 | 86.75 | 0.3865 | -530.0 | -376.0 | |
| 0.00 | 1.24 | 0.00 | 0.66 | 6.32 | 208.51 | -22.97 | 90.03 | 0.3896 | -484.0 | -444.9 | |
| 0.00 | 1.15 | 0.00 | 0.62 | 4.57 | 208.48 | -23.00 | 94.49 | 0.3924 | -718.0 | -473.4 | |
| 0.00 | 1.50 | 0.00 | 0.81 | 6.74 | 207.90 | -23.58 | 88.89 | 0.3991 | -709.0 | -588.3 | |
| 0.00 | 1.77 | 0.00 | 0.95 | 6.53 | 207.84 | -23.64 | 89.42 | 0.4001 | -677.0 | -561.4 | |
| 0.00 | 1.15 | 0.00 | 0.62 | 7.08 | 207.42 | -24.07 | 88.02 | 0.4066 | -757.0 | -608.3 | |
| 0.00 | 1.50 | 0.00 | 0.82 | 5.98 | 207.07 | -24.41 | 90.68 | 0.4128 | 794.0 | 635.9 | |
| 0.00 | 2.91 | 0.00 | 1.59 | 6.89 | 206.63 | -24.85 | 88.44 | 0.4192 | 832.0 | 630.1 | |
| 0.00 | 2.83 | 0.00 | 1.55 | 7.13 | 206.08 | -25.40 | 87.83 | 0.4278 | 978.0 | 686.5 | |
| 0.00 | 0.53 | 0.00 | 0.29 | 9.08 | 205.91 | -25.57 | 83.28 | 0.4309 | 612.0 | 468.7 | |
| 0.00 | 0.88 | 0.00 | 0.49 | 8.37 | 205.49 | -25.99 | 84.97 | 0.4370 | 753.0 | 651.6 | |
| 0.00 | 1.24 | 0.00 | 0.68 | 8.42 | 205.25 | -26.23 | 84.87 | 0.4408 | 638.0 | 565.9 | |
| 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. | |