SDO HMI 2014-01-08 05:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.42 | 21.90 | 0.22 | 12.26 | -17.61 | 71.90 | -22.65 | 125.38 | 0.4433 | 65.6 | -17.9 | |
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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 | 1.78 | 0.00 | 0.94 | -19.49 | 82.82 | -11.73 | 144.75 | 0.3335 | 722.0 | 628.3 | |
| 0.42 | 2.63 | 0.22 | 1.39 | -19.53 | 81.76 | -12.79 | 142.53 | 0.3444 | 915.2 | 782.7 | |
| 0.00 | 1.44 | 0.00 | 0.75 | -13.06 | 79.92 | -14.63 | 123.45 | 0.2961 | -891.0 | -780.1 | |
| 0.00 | 1.53 | 0.00 | 0.81 | -16.61 | 76.98 | -17.57 | 127.78 | 0.3676 | 898.0 | 492.0 | |
| 0.00 | 1.19 | 0.00 | 0.63 | -15.88 | 76.40 | -18.15 | 125.27 | 0.3685 | 764.0 | 575.3 | |
| 0.00 | 1.36 | 0.00 | 0.73 | -13.82 | 74.34 | -20.21 | 117.86 | 0.3812 | -909.0 | -686.9 | |
| 0.00 | 1.27 | 0.00 | 0.70 | -19.83 | 73.64 | -20.91 | 129.80 | 0.4388 | 774.0 | 636.2 | |
| 0.00 | 1.87 | 0.00 | 1.03 | -20.17 | 73.56 | -20.99 | 130.33 | 0.4429 | 881.0 | 586.6 | |
| 0.00 | 1.02 | 0.00 | 0.57 | -20.58 | 72.89 | -21.66 | 130.26 | 0.4547 | 618.0 | 504.8 | |
| 0.00 | 2.04 | 0.00 | 1.14 | -15.01 | 69.42 | -25.13 | 115.98 | 0.4583 | -668.0 | -567.6 | |
| 0.00 | 3.31 | 0.00 | 1.84 | -12.62 | 68.69 | -25.86 | 110.51 | 0.4564 | -834.0 | -657.1 | |
| 0.00 | 0.51 | 0.00 | 0.35 | -24.17 | 53.45 | -41.10 | 121.15 | 0.7032 | -580.0 | -535.5 | |
| 0.00 | 1.10 | 0.00 | 0.78 | -23.21 | 52.36 | -42.19 | 119.39 | 0.7108 | -625.0 | -582.8 | |
| 0.00 | 0.85 | 0.00 | 0.60 | -23.04 | 52.20 | -42.35 | 119.10 | 0.7118 | -334.0 | -396.6 | |
| 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. | |