SDO HMI 2014-10-05 04:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.62 | 30.16 | 5.62 | 19.26 | 13.29 | 90.80 | -38.94 | 77.02 | 0.6291 | 191.2 | 47.3 | |
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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 | 1.06 | 0.00 | 0.59 | 9.26 | 102.41 | -27.34 | 82.42 | 0.4592 | -751.0 | -566.2 | |
| 0.00 | 1.14 | 0.00 | 0.66 | 12.52 | 98.98 | -30.76 | 76.48 | 0.5156 | -746.0 | -633.3 | |
| 0.00 | 1.93 | 0.00 | 1.14 | 14.49 | 97.46 | -32.28 | 73.25 | 0.5422 | -779.0 | -644.5 | |
| 0.00 | 1.41 | 0.00 | 0.83 | 7.83 | 97.13 | -32.62 | 85.66 | 0.5377 | -773.0 | -605.2 | |
| 0.00 | 1.32 | 0.00 | 0.79 | 10.71 | 95.06 | -34.68 | 80.57 | 0.5690 | -701.0 | -476.1 | |
| 0.00 | 1.76 | 0.00 | 1.06 | 10.96 | 94.73 | -35.02 | 80.17 | 0.5739 | -602.0 | -475.0 | |
| 0.00 | 0.70 | 0.00 | 0.44 | 9.24 | 92.34 | -37.40 | 83.30 | 0.6059 | -642.0 | -512.1 | |
| 0.00 | 0.97 | 0.00 | 0.63 | 16.63 | 89.31 | -40.44 | 72.04 | 0.6556 | 629.0 | 573.5 | |
| 0.00 | 0.97 | 0.00 | 0.63 | 12.98 | 89.19 | -40.56 | 77.62 | 0.6510 | 439.0 | 412.9 | |
| 8.62 | 12.13 | 5.62 | 7.91 | 13.25 | 89.09 | -40.65 | 77.22 | 0.6525 | 947.4 | 616.6 | |
| 0.00 | 1.93 | 0.00 | 1.29 | 15.37 | 87.67 | -42.08 | 74.26 | 0.6737 | 491.0 | 303.2 | |
| 0.00 | 1.85 | 0.00 | 1.24 | 15.08 | 87.06 | -42.68 | 74.80 | 0.6807 | 403.0 | 323.2 | |
| 0.00 | 0.79 | 0.00 | 0.53 | 12.53 | 87.55 | -42.20 | 78.50 | 0.6714 | 293.0 | 293.2 | |
| 0.00 | 1.23 | 0.00 | 0.86 | 19.49 | 85.37 | -44.38 | 68.86 | 0.7092 | 594.0 | 514.6 | |
| 0.00 | 0.97 | 0.00 | 0.66 | 14.59 | 86.59 | -43.16 | 75.59 | 0.6858 | 573.0 | 463.7 | |
| 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. | |