SDO HMI 2014-11-14 11:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.15 | 33.72 | 7.30 | 24.03 | 8.59 | 4.25 | 45.87 | 279.16 | 0.7209 | -224.5 | -73.4 | |
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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 |
| 0.95 | 11.44 | 0.70 | 8.41 | 8.12 | 6.08 | 47.70 | 278.32 | 0.7423 | -543.6 | -488.5 | |
| 0.00 | 0.60 | 0.00 | 0.44 | 8.54 | 6.15 | 47.76 | 278.88 | 0.7434 | -409.0 | -335.4 | |
| 3.87 | -1.00 | 2.84 | -1.00 | 8.22 | 5.96 | 47.58 | 278.46 | 0.7410 | -814.8 | 999999 | |
| 2.15 | -1.00 | 1.58 | -1.00 | 8.04 | 5.93 | 47.55 | 278.22 | 0.7405 | -842.6 | 999999 | |
| 0.00 | 3.36 | 0.00 | 2.44 | 8.21 | 5.34 | 46.96 | 278.50 | 0.7337 | -788.0 | -668.0 | |
| 0.00 | 1.38 | 0.00 | 0.99 | 8.31 | 5.05 | 46.66 | 278.67 | 0.7304 | -688.0 | -563.6 | |
| 0.00 | 3.27 | 0.00 | 2.35 | 8.11 | 4.84 | 46.46 | 278.41 | 0.7278 | -808.0 | -662.1 | |
| 0.00 | 0.60 | 0.00 | 0.42 | 9.75 | 3.51 | 45.12 | 280.82 | 0.7134 | 649.0 | 539.9 | |
| 0.00 | 1.98 | 0.00 | 1.37 | 9.87 | 2.59 | 44.21 | 281.13 | 0.7025 | 583.0 | 455.4 | |
| 0.00 | 0.69 | 0.00 | 0.48 | 10.48 | 2.41 | 44.02 | 282.02 | 0.7010 | 535.0 | 518.9 | |
| 2.06 | 7.48 | 1.41 | 5.12 | 8.70 | 1.90 | 43.52 | 279.54 | 0.6926 | 803.7 | 645.6 | |
| 1.12 | 2.92 | 0.77 | 2.01 | 9.77 | 1.95 | 43.57 | 281.08 | 0.6944 | 790.3 | 627.0 | |
| 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. | |