SDO HMI 2014-01-11 11:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.48 | 0.00 | 9.93 | -20.72 | 62.07 | 10.30 | 208.06 | 0.3792 | -374.3 | -310.0 | |
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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 | 1.02 | 0.00 | 0.60 | -15.28 | 83.40 | 31.62 | 248.12 | 0.5472 | 532.0 | 429.3 | |
| 0.00 | 1.11 | 0.00 | 0.61 | -18.01 | 74.52 | 22.74 | 236.37 | 0.4435 | 894.0 | 704.8 | |
| 0.00 | 1.28 | 0.00 | 0.71 | -19.57 | 74.37 | 22.59 | 233.20 | 0.4540 | 761.0 | 680.1 | |
| 0.00 | 1.02 | 0.00 | 0.55 | -14.20 | 73.57 | 21.80 | 243.54 | 0.4039 | -871.0 | -707.2 | |
| 0.00 | 1.02 | 0.00 | 0.55 | -14.73 | 72.90 | 21.13 | 241.67 | 0.3978 | -767.0 | -581.2 | |
| 0.00 | 1.62 | 0.00 | 0.90 | -21.67 | 73.02 | 21.24 | 227.80 | 0.4564 | 919.0 | 772.9 | |
| 0.00 | 3.15 | 0.00 | 1.61 | -16.36 | 59.59 | 7.81 | 211.63 | 0.2499 | -733.0 | -726.4 | |
| 0.00 | 0.94 | 0.00 | 0.49 | -24.03 | 56.27 | 4.50 | 191.91 | 0.3489 | -758.0 | -665.0 | |
| 0.00 | 1.28 | 0.00 | 0.65 | -16.30 | 54.59 | 2.81 | 192.64 | 0.2164 | -916.0 | -690.6 | |
| 0.00 | 0.85 | 0.00 | 0.45 | -24.95 | 52.53 | 0.76 | 181.93 | 0.3565 | -880.0 | -741.4 | |
| 0.00 | 1.19 | 0.00 | 0.66 | -30.45 | 52.42 | 0.65 | 181.27 | 0.4448 | -812.0 | -670.6 | |
| 0.00 | 1.02 | 0.00 | 0.54 | -24.13 | 51.85 | 0.07 | 180.20 | 0.3429 | -869.0 | -675.7 | |
| 0.00 | 1.70 | 0.00 | 0.90 | -24.57 | 51.78 | 0.01 | 180.02 | 0.3501 | -903.0 | -734.5 | |
| 0.00 | 1.28 | 0.00 | 0.71 | -29.67 | 42.23 | -9.54 | 161.53 | 0.4566 | -837.0 | -690.1 | |
| 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. | |