SDO HMI 2014-04-11 21:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 24.16 | 0.00 | 12.16 | -13.12 | 302.81 | 2.38 | 194.95 | 0.1737 | 90.6 | -58.6 | |
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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 | 2.21 | 0.00 | 1.13 | -10.81 | 313.49 | 13.06 | 248.23 | 0.2400 | 831.0 | 623.4 | |
| 0.00 | 0.97 | 0.00 | 0.50 | -14.48 | 311.55 | 11.12 | 230.95 | 0.2415 | 761.0 | 634.5 | |
| 0.00 | 0.79 | 0.00 | 0.40 | -12.85 | 311.07 | 10.63 | 235.61 | 0.2190 | 776.0 | 607.8 | |
| 0.00 | 2.29 | 0.00 | 1.16 | -12.22 | 310.73 | 10.30 | 237.31 | 0.2085 | 960.0 | 765.3 | |
| 0.00 | 0.44 | 0.00 | 0.22 | -12.19 | 310.48 | 10.05 | 236.79 | 0.2047 | 558.0 | 635.4 | |
| 0.00 | 1.15 | 0.00 | 0.57 | -12.40 | 306.29 | 5.86 | 221.15 | 0.1523 | 806.0 | 638.5 | |
| 0.00 | 1.50 | 0.00 | 0.75 | -4.67 | 305.85 | 5.42 | 282.33 | 0.0968 | 789.0 | 652.4 | |
| 0.00 | 3.79 | 0.00 | 1.91 | -16.31 | 300.25 | -0.18 | 179.03 | 0.1819 | -763.0 | -363.0 | |
| 0.00 | 2.47 | 0.00 | 1.23 | -13.26 | 298.50 | -1.94 | 165.67 | 0.1334 | -808.0 | -562.4 | |
| 0.00 | 4.32 | 0.00 | 2.16 | -13.44 | 298.34 | -2.09 | 164.92 | 0.1371 | -933.0 | -788.0 | |
| 0.00 | 0.88 | 0.00 | 0.45 | -20.89 | 297.89 | -2.54 | 170.92 | 0.2636 | 785.0 | 535.3 | |
| 0.00 | 0.79 | 0.00 | 0.39 | -8.90 | 296.25 | -4.18 | 126.39 | 0.0900 | -777.0 | -547.7 | |
| 0.00 | 0.97 | 0.00 | 0.49 | -17.17 | 295.65 | -4.78 | 157.92 | 0.2127 | -896.0 | -685.2 | |
| 0.00 | 1.59 | 0.00 | 0.80 | -12.14 | 294.44 | -5.99 | 137.07 | 0.1505 | -820.0 | -574.2 | |
| 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. | |