SDO HMI 2014-01-08 11:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.36 | 214.42 | 26.15 | 157.71 | 5.92 | 44.72 | -46.56 | 78.19 | 0.7394 | -918.4 | -247.3 | |
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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 | 1.36 | 0.00 | 0.71 | 8.57 | 78.52 | -12.76 | 45.63 | 0.3068 | -853.0 | -665.1 | |
| 0.00 | 1.27 | 0.00 | 0.72 | 9.63 | 65.73 | -25.55 | 61.93 | 0.4839 | -714.0 | -574.8 | |
| 0.00 | 1.36 | 0.00 | 0.82 | 10.41 | 59.18 | -32.10 | 65.68 | 0.5758 | -707.0 | -552.2 | |
| 0.00 | 1.10 | 0.00 | 0.68 | 11.71 | 58.63 | -32.65 | 63.99 | 0.5901 | -659.0 | -543.5 | |
| 0.00 | 0.51 | 0.00 | 0.33 | 14.04 | 54.04 | -37.24 | 63.40 | 0.6589 | -480.0 | -355.0 | |
| 0.00 | 0.85 | 0.00 | 0.55 | 9.40 | 53.40 | -37.87 | 70.44 | 0.6451 | -545.0 | -485.7 | |
| 0.00 | 1.10 | 0.00 | 0.78 | 12.04 | 48.19 | -43.09 | 69.03 | 0.7179 | -633.0 | -534.1 | |
| 0.00 | 1.36 | 0.00 | 0.95 | 10.63 | 48.33 | -42.95 | 70.86 | 0.7112 | -603.0 | -487.8 | |
| 0.00 | 1.02 | 0.00 | 0.73 | 12.26 | 47.93 | -43.35 | 68.84 | 0.7216 | -620.0 | -501.2 | |
| 0.00 | 0.93 | 0.00 | 0.67 | 11.96 | 47.95 | -43.33 | 69.23 | 0.7203 | -533.0 | -391.2 | |
| 35.36 | 203.56 | 26.15 | 150.77 | 5.69 | 44.20 | -47.08 | 78.79 | 0.7452 | -1026.9 | -232.2 | |
| 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. | |