SDO HMI 2014-11-13 04:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.28 | 0.00 | 9.82 | -9.26 | 338.52 | 3.13 | 192.96 | 0.2313 | -65.8 | -76.8 | |
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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 | 1.12 | 0.00 | 0.57 | -5.15 | 346.39 | 11.00 | 233.18 | 0.2386 | 875.0 | 677.9 | |
| 0.00 | 0.86 | 0.00 | 0.44 | -8.80 | 343.31 | 7.92 | 213.55 | 0.2476 | 732.0 | 446.7 | |
| 0.00 | 0.77 | 0.00 | 0.40 | -9.98 | 342.42 | 7.04 | 208.14 | 0.2570 | 832.0 | 664.0 | |
| 0.00 | 2.58 | 0.00 | 1.32 | -10.67 | 341.59 | 6.20 | 204.08 | 0.2613 | 962.0 | 753.1 | |
| 0.00 | 1.21 | 0.00 | 0.61 | -6.94 | 340.93 | 5.54 | 208.88 | 0.1994 | 680.0 | 522.1 | |
| 0.00 | 1.29 | 0.00 | 0.66 | -11.16 | 340.87 | 5.48 | 200.87 | 0.2642 | 720.0 | 602.9 | |
| 0.00 | 1.03 | 0.00 | 0.53 | -10.91 | 340.74 | 5.35 | 200.77 | 0.2596 | 643.0 | 479.8 | |
| 0.00 | 1.03 | 0.00 | 0.52 | -9.52 | 337.22 | 1.84 | 188.24 | 0.2215 | -740.0 | -530.3 | |
| 0.00 | 2.24 | 0.00 | 1.14 | -9.92 | 337.11 | 1.72 | 187.48 | 0.2279 | -911.0 | -774.7 | |
| 0.00 | 1.12 | 0.00 | 0.57 | -10.07 | 336.96 | 1.57 | 186.75 | 0.2302 | -830.0 | -697.6 | |
| 0.00 | 0.60 | 0.00 | 0.31 | -10.13 | 336.68 | 1.30 | 185.56 | 0.2307 | -520.0 | -457.1 | |
| 0.00 | 1.03 | 0.00 | 0.52 | -9.40 | 336.08 | 0.69 | 183.16 | 0.2174 | -974.0 | -785.1 | |
| 0.00 | 1.38 | 0.00 | 0.70 | -8.06 | 334.19 | -1.20 | 173.90 | 0.1953 | -902.0 | -669.1 | |
| 0.00 | 1.81 | 0.00 | 0.92 | -10.25 | 333.97 | -1.42 | 173.98 | 0.2329 | -790.0 | -709.1 | |
| 0.00 | 1.21 | 0.00 | 0.61 | -5.93 | 331.72 | -3.66 | 157.89 | 0.1697 | -764.0 | -567.8 | |
| 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. | |