SDO HMI 2014-09-06 18:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.64 | 48.90 | 12.61 | 72.58 | -20.55 | 78.81 | -66.05 | 114.86 | 0.9437 | -6.7 | -148.7 | |
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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 |
| 0.62 | 2.14 | 0.81 | 2.76 | -20.67 | 82.36 | -62.49 | 115.99 | 0.9249 | 424.9 | 325.2 | |
| 0.00 | 1.52 | 0.00 | 2.00 | -20.45 | 81.67 | -63.19 | 115.55 | 0.9285 | 558.0 | 338.7 | |
| 0.00 | 6.96 | 0.00 | 9.40 | -20.48 | 81.14 | -63.72 | 115.42 | 0.9316 | -138.0 | -42.6 | |
| 1.78 | 4.64 | 2.55 | 6.67 | -21.67 | 80.10 | -64.76 | 116.34 | 0.9395 | 458.7 | 227.1 | |
| 3.03 | 4.46 | 4.36 | 6.40 | -21.29 | 79.88 | -64.98 | 115.90 | 0.9401 | 89.1 | 56.2 | |
| 0.00 | 1.34 | 0.00 | 1.66 | -17.66 | 82.37 | -62.49 | 112.87 | 0.9189 | 402.0 | 349.6 | |
| 0.00 | 0.98 | 0.00 | 1.35 | -19.13 | 80.22 | -64.64 | 113.77 | 0.9344 | -95.0 | -132.4 | |
| 0.00 | 2.23 | 0.00 | 3.24 | -19.94 | 79.20 | -65.66 | 114.33 | 0.9414 | -465.0 | -464.8 | |
| 2.94 | 20.88 | 4.48 | 31.47 | -20.13 | 78.16 | -66.70 | 114.24 | 0.9471 | -371.7 | -358.1 | |
| 0.27 | -9.00 | 0.41 | -9.00 | -19.86 | 78.23 | -66.63 | 113.98 | 0.9464 | -472.3 | 999999 | |
| 0.00 | 3.75 | 0.00 | 7.63 | -22.12 | 73.35 | -71.51 | 115.05 | 0.9709 | 35.0 | -34.6 | |
| 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. | |