SDO HMI 2014-10-05 01:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.73 | 0.00 | 11.50 | -18.41 | 105.49 | -25.91 | 135.31 | 0.5910 | 219.5 | 39.8 | |
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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 | 0.97 | 0.00 | 0.58 | -22.69 | 112.68 | -18.71 | 148.49 | 0.5684 | 712.0 | 631.4 | |
| 0.00 | 1.05 | 0.00 | 0.63 | -22.53 | 112.47 | -18.93 | 148.03 | 0.5681 | 746.0 | 616.0 | |
| 0.00 | 0.79 | 0.00 | 0.45 | -16.87 | 112.83 | -18.56 | 142.11 | 0.4981 | 564.0 | 550.7 | |
| 0.00 | 1.41 | 0.00 | 0.84 | -21.93 | 112.00 | -19.39 | 146.80 | 0.5647 | 110.0 | 133.0 | |
| 0.00 | 1.23 | 0.00 | 0.74 | -22.35 | 111.74 | -19.66 | 146.88 | 0.5717 | 136.0 | 283.9 | |
| 0.00 | 0.62 | 0.00 | 0.39 | -26.66 | 110.65 | -20.74 | 149.67 | 0.6290 | 520.0 | 455.7 | |
| 0.00 | 1.41 | 0.00 | 0.80 | -15.16 | 110.92 | -20.47 | 137.05 | 0.4975 | 657.0 | 505.6 | |
| 0.00 | 0.97 | 0.00 | 0.58 | -20.35 | 110.24 | -21.15 | 142.76 | 0.5611 | 468.0 | 366.4 | |
| 0.00 | 1.05 | 0.00 | 0.61 | -15.12 | 108.18 | -23.22 | 133.42 | 0.5260 | 626.0 | 508.2 | |
| 0.00 | 0.79 | 0.00 | 0.47 | -15.03 | 105.94 | -25.46 | 130.69 | 0.5496 | 804.0 | 718.4 | |
| 0.00 | 1.32 | 0.00 | 0.78 | -14.98 | 105.77 | -25.62 | 130.43 | 0.5509 | 677.0 | 497.7 | |
| 0.00 | 1.05 | 0.00 | 0.68 | -17.30 | 99.58 | -31.81 | 127.62 | 0.6376 | -784.0 | -705.8 | |
| 0.00 | 1.41 | 0.00 | 0.91 | -17.54 | 98.83 | -32.57 | 127.30 | 0.6475 | -687.0 | -598.1 | |
| 0.00 | 3.52 | 0.00 | 2.29 | -17.03 | 98.14 | -33.25 | 126.08 | 0.6510 | -676.0 | -581.8 | |
| 0.00 | 1.14 | 0.00 | 0.75 | -17.10 | 97.15 | -34.25 | 125.39 | 0.6621 | -581.0 | -461.9 | |
| 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. | |