SDO HMI 2011-11-17 19:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.86 | 119.30 | 52.60 | 220.07 | -15.40 | 266.84 | -72.92 | 106.81 | 0.9631 | 246.4 | -30.5 | |
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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 |
| 15.19 | 42.66 | 24.04 | 68.38 | -16.51 | 269.65 | -70.11 | 108.32 | 0.9511 | 534.3 | -44.2 | |
| 0.60 | -1.00 | 0.97 | -1.00 | -16.58 | 269.31 | -70.45 | 108.35 | 0.9529 | -257.7 | 999999 | |
| 3.86 | 9.01 | 6.66 | 15.59 | -17.32 | 268.16 | -71.60 | 108.95 | 0.9590 | 334.1 | -109.1 | |
| 0.00 | 1.72 | 0.00 | 3.16 | -16.69 | 266.92 | -72.85 | 108.13 | 0.9643 | -354.0 | -295.5 | |
| 0.00 | 1.03 | 0.00 | 1.98 | -16.17 | 266.02 | -73.75 | 107.48 | 0.9678 | -417.0 | -374.5 | |
| 3.43 | 42.14 | 6.26 | 77.57 | -14.19 | 266.75 | -73.01 | 105.53 | 0.9635 | 525.9 | 130.0 | |
| 0.00 | 1.29 | 0.00 | 3.36 | -18.10 | 262.10 | -77.66 | 108.98 | 0.9829 | 79.0 | 14.5 | |
| 0.00 | 2.32 | 0.00 | 4.93 | -16.08 | 264.59 | -75.18 | 107.21 | 0.9735 | -371.0 | -369.8 | |
| 0.00 | 4.03 | 0.00 | 10.29 | -17.74 | 262.34 | -77.43 | 108.65 | 0.9820 | -115.0 | -59.0 | |
| 2.66 | -6.00 | 4.88 | -6.00 | -13.77 | 266.57 | -73.19 | 105.07 | 0.9641 | 310.7 | 999999 | |
| 0.00 | 3.00 | 0.00 | 6.34 | -15.76 | 264.69 | -75.08 | 106.90 | 0.9730 | -121.0 | -178.2 | |
| 0.00 | 0.86 | 0.00 | 1.68 | -14.42 | 265.67 | -74.09 | 105.64 | 0.9684 | -327.0 | -309.6 | |
| 4.12 | 11.24 | 9.79 | 26.79 | -13.90 | 262.82 | -76.95 | 104.80 | 0.9790 | -339.0 | -302.9 | |
| 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. | |