SDO HMI 2014-08-22 05:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.45 | 133.40 | 16.19 | 84.29 | 16.48 | 28.10 | 37.93 | 287.93 | 0.6215 | -663.7 | -307.6 | |
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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 |
| 24.46 | 117.83 | 15.56 | 74.96 | 16.35 | 28.68 | 38.51 | 287.52 | 0.6289 | -1059.9 | -350.4 | |
| 0.99 | -1.00 | 0.63 | -1.00 | 16.38 | 28.28 | 38.12 | 287.67 | 0.6238 | -1083.0 | 999999 | |
| 0.00 | 0.99 | 0.00 | 0.62 | 17.91 | 26.85 | 36.68 | 290.54 | 0.6092 | -690.0 | -544.2 | |
| 0.00 | 1.35 | 0.00 | 0.84 | 17.58 | 26.65 | 36.48 | 290.08 | 0.6057 | -675.0 | -509.7 | |
| 0.00 | 1.35 | 0.00 | 0.84 | 17.69 | 26.40 | 36.23 | 290.34 | 0.6028 | -570.0 | -553.5 | |
| 0.00 | 2.25 | 0.00 | 1.38 | 17.04 | 25.89 | 35.73 | 289.45 | 0.5943 | -878.0 | -705.8 | |
| 0.00 | 1.89 | 0.00 | 1.16 | 17.42 | 25.86 | 35.69 | 290.08 | 0.5949 | -810.0 | -597.8 | |
| 0.00 | 1.17 | 0.00 | 0.68 | 16.64 | 21.17 | 31.01 | 290.54 | 0.5291 | 587.0 | 463.5 | |
| 0.00 | 1.44 | 0.00 | 0.84 | 18.50 | 21.16 | 30.99 | 293.93 | 0.5363 | 653.0 | 457.4 | |
| 0.00 | 1.44 | 0.00 | 0.84 | 18.49 | 20.86 | 30.69 | 294.07 | 0.5322 | 696.0 | 596.9 | |
| 0.00 | 2.25 | 0.00 | 1.30 | 16.93 | 20.41 | 30.25 | 291.44 | 0.5198 | 773.0 | 669.6 | |
| 0.00 | 1.44 | 0.00 | 0.83 | 17.22 | 19.70 | 29.53 | 292.34 | 0.5110 | 705.0 | 556.2 | |
| 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. | |