SDO HMI 2014-10-09 07:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.99 | 0.00 | 11.98 | 13.91 | 90.77 | 15.44 | 300.15 | 0.3031 | 89.4 | 171.2 | |
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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 | 0.74 | 9.39 | 104.29 | 28.96 | 278.09 | 0.4844 | -785.0 | -623.8 | |
| 0.00 | 0.88 | 0.00 | 0.48 | 8.29 | 100.98 | 25.66 | 276.12 | 0.4327 | -678.0 | -589.2 | |
| 0.00 | 1.40 | 0.00 | 0.76 | 9.25 | 98.36 | 23.03 | 278.93 | 0.3925 | -844.0 | -512.7 | |
| 0.00 | 1.05 | 0.00 | 0.56 | 11.86 | 96.52 | 21.19 | 286.47 | 0.3705 | -761.0 | -660.8 | |
| 0.00 | 1.67 | 0.00 | 0.87 | 11.04 | 94.21 | 18.88 | 285.65 | 0.3313 | -725.0 | -601.1 | |
| 0.00 | 0.88 | 0.00 | 0.48 | 24.08 | 94.91 | 19.58 | 315.54 | 0.4386 | 426.0 | 400.6 | |
| 0.00 | 1.40 | 0.00 | 0.73 | 15.62 | 92.07 | 16.74 | 301.03 | 0.3252 | 727.0 | 533.1 | |
| 0.00 | 1.05 | 0.00 | 0.56 | 20.05 | 90.36 | 15.03 | 314.77 | 0.3446 | 652.0 | 547.4 | |
| 0.00 | 2.19 | 0.00 | 1.13 | 15.95 | 87.88 | 12.55 | 309.23 | 0.2710 | 955.0 | 757.8 | |
| 0.00 | 4.21 | 0.00 | 2.15 | 14.08 | 87.39 | 12.06 | 304.29 | 0.2464 | 787.0 | 720.0 | |
| 0.00 | 1.32 | 0.00 | 0.67 | 14.84 | 87.02 | 11.69 | 307.68 | 0.2486 | 861.0 | 727.4 | |
| 0.00 | 1.23 | 0.00 | 0.63 | 14.73 | 86.95 | 11.62 | 307.44 | 0.2465 | 988.0 | 856.6 | |
| 0.00 | 1.32 | 0.00 | 0.66 | 8.51 | 86.28 | 10.95 | 282.31 | 0.1932 | -913.0 | -638.1 | |
| 0.00 | 0.88 | 0.00 | 0.46 | 20.93 | 85.94 | 10.61 | 325.98 | 0.3088 | 714.0 | 590.8 | |
| 0.00 | 0.96 | 0.00 | 0.49 | 16.72 | 84.65 | 9.32 | 319.66 | 0.2408 | 921.0 | 799.7 | |
| 0.00 | 1.23 | 0.00 | 0.61 | 11.93 | 80.99 | 5.66 | 315.77 | 0.1390 | -894.0 | -772.6 | |
| 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. | |