SDO HMI 2014-11-04 11:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.52 | 0.00 | 8.47 | -22.51 | 73.68 | -16.54 | 150.87 | 0.5176 | 502.0 | 399.2 | |
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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 | 1.12 | 0.00 | 0.62 | -20.99 | 81.24 | -8.99 | 160.95 | 0.4486 | 693.0 | 457.0 | |
| 0.00 | 1.04 | 0.00 | 0.57 | -20.26 | 79.19 | -11.03 | 156.36 | 0.4497 | 677.0 | 549.0 | |
| 0.00 | 1.12 | 0.00 | 0.63 | -20.73 | 78.31 | -11.91 | 155.18 | 0.4619 | 680.0 | 659.6 | |
| 0.00 | 1.04 | 0.00 | 0.59 | -22.66 | 77.46 | -12.77 | 155.50 | 0.4940 | 430.0 | 455.8 | |
| 0.00 | 1.30 | 0.00 | 0.73 | -20.53 | 76.70 | -13.52 | 152.11 | 0.4702 | 824.0 | 596.6 | |
| 0.00 | 0.52 | 0.00 | 0.30 | -22.81 | 76.31 | -13.92 | 153.76 | 0.5034 | 684.0 | 577.8 | |
| 0.00 | 1.38 | 0.00 | 0.78 | -20.64 | 76.07 | -14.16 | 151.15 | 0.4763 | 726.0 | 591.7 | |
| 0.00 | 2.51 | 0.00 | 1.41 | -20.28 | 76.07 | -14.15 | 150.76 | 0.4715 | 800.0 | 620.4 | |
| 0.00 | 1.12 | 0.00 | 0.63 | -20.74 | 75.93 | -14.30 | 151.02 | 0.4787 | 631.0 | 526.5 | |
| 0.00 | 0.43 | 0.00 | 0.24 | -20.54 | 75.85 | -14.38 | 150.67 | 0.4767 | 561.0 | 445.8 | |
| 0.00 | 1.04 | 0.00 | 0.61 | -24.69 | 72.87 | -17.36 | 150.43 | 0.5515 | 664.0 | 480.0 | |
| 0.00 | 1.38 | 0.00 | 0.97 | -28.94 | 58.33 | -31.90 | 139.16 | 0.7095 | -654.0 | -535.7 | |
| 0.00 | 0.52 | 0.00 | 0.39 | -30.87 | 53.87 | -36.36 | 137.77 | 0.7593 | -190.0 | -142.0 | |
| 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. | |