SDO HMI 2014-10-01 15:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.99 | 108.20 | 12.76 | 69.65 | -10.13 | 140.42 | -36.07 | 114.74 | 0.6405 | 338.0 | 289.6 | |
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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 | 0.62 | 0.00 | 0.40 | -14.32 | 142.57 | -33.93 | 122.10 | 0.6408 | 515.0 | 487.9 | |
| 0.00 | 1.14 | 0.00 | 0.77 | -15.83 | 139.83 | -36.67 | 122.13 | 0.6807 | 466.0 | 294.8 | |
| 19.99 | 94.74 | 12.76 | 60.49 | -9.64 | 140.79 | -35.70 | 114.28 | 0.6335 | 987.8 | 388.7 | |
| 0.00 | 1.06 | 0.00 | 0.71 | -14.60 | 139.42 | -37.08 | 120.26 | 0.6777 | 635.0 | 519.5 | |
| 0.00 | 1.58 | 0.00 | 1.03 | -11.29 | 139.96 | -36.54 | 116.12 | 0.6525 | 675.0 | 500.5 | |
| 0.00 | 0.70 | 0.00 | 0.48 | -14.78 | 138.32 | -38.17 | 119.77 | 0.6908 | -750.0 | -671.0 | |
| 0.00 | 0.53 | 0.00 | 0.36 | -13.50 | 138.35 | -38.15 | 118.11 | 0.6834 | -512.0 | -537.8 | |
| 0.00 | 1.06 | 0.00 | 0.72 | -13.59 | 137.97 | -38.53 | 118.00 | 0.6880 | -632.0 | -530.3 | |
| 0.00 | 1.23 | 0.00 | 0.86 | -13.94 | 136.74 | -39.76 | 117.72 | 0.7035 | -562.0 | -471.5 | |
| 0.00 | 1.50 | 0.00 | 1.03 | -12.81 | 136.93 | -39.57 | 116.36 | 0.6956 | -823.0 | -709.8 | |
| 0.00 | 0.44 | 0.00 | 0.30 | -12.52 | 136.98 | -39.52 | 116.01 | 0.6935 | -570.0 | -617.2 | |
| 0.00 | 0.53 | 0.00 | 0.37 | -13.96 | 136.50 | -40.00 | 117.60 | 0.7063 | -405.0 | -380.7 | |
| 0.00 | 0.26 | 0.00 | 0.18 | -12.93 | 136.62 | -39.87 | 116.34 | 0.6996 | -420.0 | -463.0 | |
| 0.00 | 1.14 | 0.00 | 0.79 | -12.46 | 136.51 | -39.99 | 115.67 | 0.6985 | -582.0 | -545.3 | |
| 0.00 | 1.67 | 0.00 | 1.16 | -12.55 | 136.17 | -40.33 | 115.59 | 0.7027 | -596.0 | -445.8 | |
| 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. | |