SDO HMI 2014-11-05 16:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.18 | 0.00 | 7.86 | -21.45 | 77.80 | 3.51 | 188.93 | 0.4457 | 385.3 | 337.8 | |
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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 | 1.21 | 0.00 | 0.70 | -26.31 | 84.55 | 10.25 | 197.61 | 0.5293 | -806.0 | -697.9 | |
| 0.00 | 0.95 | 0.00 | 0.52 | -20.79 | 83.03 | 8.73 | 198.79 | 0.4426 | 710.0 | 576.6 | |
| 0.00 | 0.95 | 0.00 | 0.50 | -14.82 | 82.28 | 7.98 | 202.71 | 0.3492 | 11.0 | 6.9 | |
| 0.00 | 1.21 | 0.00 | 0.67 | -21.07 | 81.79 | 7.49 | 196.09 | 0.4409 | 720.0 | 537.0 | |
| 0.00 | 1.30 | 0.00 | 0.71 | -20.93 | 81.08 | 6.78 | 194.72 | 0.4359 | 631.0 | 531.9 | |
| 0.00 | 1.21 | 0.00 | 0.64 | -14.62 | 80.51 | 6.21 | 198.25 | 0.3359 | 925.0 | 716.1 | |
| 0.00 | 1.64 | 0.00 | 0.90 | -20.89 | 80.63 | 6.33 | 193.81 | 0.4336 | 901.0 | 734.9 | |
| 0.00 | 1.47 | 0.00 | 0.80 | -20.35 | 78.47 | 4.18 | 189.44 | 0.4183 | 813.0 | 693.8 | |
| 0.00 | 0.26 | 0.00 | 0.14 | -16.08 | 78.19 | 3.89 | 190.81 | 0.3496 | -5.0 | 3.3 | |
| 0.00 | 1.47 | 0.00 | 0.82 | -23.55 | 76.49 | 2.19 | 184.34 | 0.4645 | 768.0 | 635.5 | |
| 0.00 | 1.30 | 0.00 | 0.72 | -22.24 | 72.29 | -2.00 | 175.80 | 0.4439 | 766.0 | 589.3 | |
| 0.00 | 1.21 | 0.00 | 0.74 | -28.32 | 58.23 | -16.07 | 155.36 | 0.5865 | -810.0 | -693.5 | |
| 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. | |