SDO HMI 2014-10-31 21:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.56 | 81.48 | 24.17 | 69.17 | -4.61 | 83.80 | -53.66 | 98.90 | 0.8147 | 586.1 | 448.1 | |
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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 | 0.78 | 0.00 | 0.64 | -3.87 | 85.13 | -52.33 | 98.23 | 0.8002 | 388.0 | 370.7 | |
| 2.42 | 12.47 | 2.01 | 10.40 | -5.12 | 84.85 | -52.61 | 99.72 | 0.8052 | -163.4 | 436.8 | |
| 2.94 | -2.00 | 2.47 | -2.00 | -5.41 | 84.52 | -52.95 | 100.01 | 0.8090 | 856.1 | 999999 | |
| 0.00 | 0.87 | 0.00 | 0.72 | -3.47 | 84.72 | -52.74 | 97.67 | 0.8039 | 386.0 | 386.9 | |
| 0.43 | 1.56 | 0.36 | 1.31 | -5.72 | 84.38 | -53.09 | 100.36 | 0.8110 | 486.0 | 377.9 | |
| 19.22 | 56.01 | 16.21 | 47.20 | -4.44 | 84.13 | -53.33 | 98.75 | 0.8114 | 837.3 | 545.5 | |
| 0.00 | 3.03 | 0.00 | 2.56 | -3.64 | 83.86 | -53.61 | 97.73 | 0.8129 | 496.0 | 433.6 | |
| 0.00 | 0.87 | 0.00 | 0.74 | -5.26 | 83.58 | -53.89 | 99.64 | 0.8182 | 347.0 | 284.9 | |
| 3.03 | -6.00 | 2.58 | -6.00 | -4.05 | 83.57 | -53.90 | 98.18 | 0.8165 | 521.9 | 999999 | |
| 0.00 | 2.08 | 0.00 | 1.79 | -4.44 | 83.22 | -54.25 | 98.58 | 0.8205 | 337.0 | 249.7 | |
| 0.00 | 0.26 | 0.00 | 0.23 | -5.27 | 81.54 | -55.93 | 99.27 | 0.8379 | 334.0 | 315.7 | |
| 0.00 | 0.69 | 0.00 | 0.65 | -5.28 | 79.89 | -57.58 | 98.99 | 0.8531 | 449.0 | 428.1 | |
| 0.00 | 0.61 | 0.00 | 0.60 | -5.50 | 78.42 | -59.05 | 98.99 | 0.8663 | -444.0 | -432.7 | |
| 0.52 | 2.25 | 0.54 | 2.33 | -6.68 | 77.00 | -60.47 | 100.09 | 0.8797 | -406.3 | -367.5 | |
| 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. | |