SDO HMI 2014-09-04 14:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.61 | 0.00 | 10.95 | 9.73 | 179.15 | 5.67 | 195.91 | 0.1974 | -341.2 | -229.7 | |
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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 | 1.43 | 0.00 | 0.73 | 11.50 | 188.13 | 14.64 | 287.62 | 0.2611 | -746.0 | -614.4 | |
| 0.00 | 1.07 | 0.00 | 0.55 | 5.93 | 187.43 | 13.95 | 265.49 | 0.2415 | -842.0 | -651.6 | |
| 0.00 | 2.23 | 0.00 | 1.14 | 11.17 | 186.11 | 12.63 | 288.52 | 0.2272 | -1087.0 | -873.5 | |
| 0.00 | 1.16 | 0.00 | 0.59 | 10.96 | 186.04 | 12.56 | 287.71 | 0.2251 | -1023.0 | -785.2 | |
| 0.00 | 1.16 | 0.00 | 0.59 | 10.78 | 185.97 | 12.49 | 287.02 | 0.2231 | -860.0 | -671.5 | |
| 0.00 | 1.16 | 0.00 | 0.59 | 5.74 | 185.65 | 12.16 | 263.72 | 0.2119 | -814.0 | -755.2 | |
| 0.00 | 1.70 | 0.00 | 0.86 | 5.95 | 185.46 | 11.98 | 264.64 | 0.2083 | -999.0 | -875.6 | |
| 0.00 | 3.13 | 0.00 | 1.58 | 6.00 | 185.06 | 11.58 | 264.61 | 0.2014 | -825.0 | -677.4 | |
| 0.00 | 0.98 | 0.00 | 0.50 | 11.11 | 185.04 | 11.56 | 289.68 | 0.2097 | -738.0 | -573.2 | |
| 0.00 | 2.50 | 0.00 | 1.24 | 10.27 | 172.70 | -0.78 | 14.12 | 0.0551 | 945.0 | 702.0 | |
| 0.00 | 1.16 | 0.00 | 0.59 | 14.74 | 164.19 | -9.30 | 49.71 | 0.2057 | 847.0 | 651.6 | |
| 0.00 | 2.50 | 0.00 | 1.26 | 10.39 | 163.90 | -9.58 | 70.79 | 0.1741 | 853.0 | 768.7 | |
| 0.00 | 1.43 | 0.00 | 0.73 | 15.39 | 161.80 | -11.68 | 53.47 | 0.2440 | 853.0 | 655.2 | |
| 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. | |