SDO HMI 2014-09-30 10:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.01 | 0.00 | 11.67 | -22.33 | 196.91 | 4.47 | 190.42 | 0.5117 | -328.5 | -313.2 | |
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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 | 1.32 | 0.00 | 0.78 | -17.19 | 215.06 | 22.62 | 222.79 | 0.5431 | 154.0 | 133.1 | |
| 0.00 | 1.41 | 0.00 | 0.83 | -18.09 | 214.05 | 21.61 | 220.35 | 0.5429 | 751.0 | 525.1 | |
| 0.00 | 1.06 | 0.00 | 0.56 | -7.46 | 207.08 | 14.64 | 226.05 | 0.3496 | 9.0 | -2.1 | |
| 0.00 | 0.79 | 0.00 | 0.49 | -27.26 | 207.36 | 14.92 | 202.38 | 0.6033 | 492.0 | 347.3 | |
| 0.00 | 1.06 | 0.00 | 0.61 | -22.68 | 199.35 | 6.91 | 192.75 | 0.5049 | -682.0 | -548.9 | |
| 0.00 | 2.03 | 0.00 | 1.08 | -14.00 | 198.67 | 6.23 | 196.59 | 0.3705 | -641.0 | -542.7 | |
| 0.00 | 1.59 | 0.00 | 0.89 | -20.25 | 198.62 | 6.18 | 192.57 | 0.4662 | -716.0 | -555.9 | |
| 0.00 | 1.23 | 0.00 | 0.65 | -13.61 | 194.36 | 1.92 | 185.34 | 0.3507 | 3.0 | -3.1 | |
| 0.00 | 1.41 | 0.00 | 0.72 | -7.34 | 192.90 | 0.46 | 181.88 | 0.2446 | -841.0 | -637.4 | |
| 0.00 | 1.23 | 0.00 | 0.74 | -27.11 | 192.90 | 0.46 | 180.73 | 0.5592 | -765.0 | -643.7 | |
| 0.00 | 0.79 | 0.00 | 0.47 | -26.06 | 191.32 | -1.12 | 178.15 | 0.5442 | -607.0 | -527.0 | |
| 0.00 | 3.17 | 0.00 | 2.03 | -32.46 | 190.67 | -1.77 | 177.64 | 0.6349 | -714.0 | -473.5 | |
| 0.00 | 0.71 | 0.00 | 0.45 | -32.83 | 187.94 | -4.50 | 174.09 | 0.6425 | -141.0 | -95.4 | |
| 0.00 | 1.06 | 0.00 | 0.64 | -28.12 | 186.45 | -5.99 | 170.85 | 0.5806 | -484.0 | -528.8 | |
| 0.00 | 1.15 | 0.00 | 0.73 | -30.91 | 182.42 | -10.02 | 166.24 | 0.6297 | -745.0 | -583.0 | |
| 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. | |