SDO HMI 2014-10-10 09:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 57.41 | 382.71 | 43.98 | 293.57 | -20.61 | 18.32 | -42.72 | 123.75 | 0.7659 | 765.2 | 234.9 | |
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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 | 1.49 | 0.00 | 1.11 | -21.81 | 21.03 | -40.01 | 126.78 | 0.7475 | -540.0 | -423.5 | |
| 0.00 | 0.61 | 0.00 | 0.45 | -19.97 | 20.67 | -40.38 | 124.40 | 0.7402 | 797.0 | 666.4 | |
| 1.84 | 367.65 | 1.39 | 282.01 | -20.40 | 19.34 | -41.70 | 124.10 | 0.7553 | 1012.1 | 238.6 | |
| 0.00 | 0.79 | 0.00 | 0.58 | -19.15 | 19.70 | -41.34 | 122.84 | 0.7450 | 455.0 | 459.9 | |
| 0.00 | 0.61 | 0.00 | 0.46 | -19.30 | 19.53 | -41.52 | 122.91 | 0.7475 | 519.0 | 473.4 | |
| 0.70 | 1.93 | 0.51 | 1.41 | -17.62 | 19.69 | -41.35 | 120.98 | 0.7368 | 688.1 | 629.5 | |
| 50.49 | -3.00 | 38.72 | -3.00 | -20.64 | 18.35 | -42.70 | 123.80 | 0.7659 | 957.1 | 999999 | |
| 0.79 | 4.12 | 0.58 | 3.02 | -17.71 | 19.28 | -41.76 | 120.87 | 0.7414 | 530.0 | 542.1 | |
| 3.33 | -3.00 | 2.58 | -3.00 | -21.20 | 18.01 | -43.03 | 124.25 | 0.7719 | 322.3 | 999999 | |
| 0.00 | 0.70 | 0.00 | 0.58 | -23.93 | 16.37 | -44.67 | 126.38 | 0.8004 | 316.0 | 341.8 | |
| 0.26 | -3.00 | 0.20 | -3.00 | -20.49 | 17.70 | -43.35 | 123.25 | 0.7711 | 469.7 | 999999 | |
| 0.00 | 0.70 | 0.00 | 0.53 | -17.82 | 17.93 | -43.11 | 120.23 | 0.7554 | 424.0 | 332.6 | |
| 0.00 | 1.31 | 0.00 | 0.98 | -16.67 | 18.09 | -42.95 | 118.94 | 0.7482 | -561.0 | -485.9 | |
| 0.00 | 1.75 | 0.00 | 1.61 | -24.63 | 11.26 | -49.78 | 124.54 | 0.8447 | -177.0 | -141.6 | |
| 0.00 | 1.05 | 0.00 | 0.83 | -14.20 | 14.06 | -46.98 | 113.98 | 0.7780 | -447.0 | -364.9 | |
| 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. | |