SDO HMI 2014-01-12 18:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.46 | 0.00 | 9.37 | -23.24 | 53.84 | 19.08 | 219.56 | 0.4806 | -535.7 | -390.5 | |
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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 | 1.36 | 0.00 | 0.89 | -21.02 | 72.77 | 38.02 | 242.25 | 0.6521 | 810.0 | 613.6 | |
| 0.00 | 0.93 | 0.00 | 0.60 | -22.99 | 71.06 | 36.31 | 238.51 | 0.6416 | 786.0 | 630.6 | |
| 0.00 | 1.36 | 0.00 | 0.80 | -16.58 | 65.07 | 30.32 | 245.30 | 0.5347 | -785.0 | -549.9 | |
| 0.00 | 1.19 | 0.00 | 0.68 | -16.74 | 62.04 | 27.28 | 243.02 | 0.4946 | -744.0 | -617.6 | |
| 0.00 | 1.19 | 0.00 | 0.66 | -16.21 | 58.52 | 23.77 | 241.21 | 0.4434 | -804.0 | -632.4 | |
| 0.00 | 1.10 | 0.00 | 0.61 | -18.06 | 58.50 | 23.74 | 237.49 | 0.4559 | -860.0 | -740.6 | |
| 0.00 | 0.85 | 0.00 | 0.47 | -18.99 | 58.16 | 23.40 | 235.37 | 0.4584 | -867.0 | -720.3 | |
| 0.00 | 1.10 | 0.00 | 0.59 | -20.56 | 49.36 | 14.61 | 219.90 | 0.3697 | -667.0 | -540.1 | |
| 0.00 | 0.93 | 0.00 | 0.54 | -33.17 | 47.92 | 13.17 | 201.48 | 0.5229 | -430.0 | -452.6 | |
| 0.00 | 1.02 | 0.00 | 0.59 | -33.25 | 44.62 | 9.87 | 196.46 | 0.5078 | -520.0 | -460.2 | |
| 0.00 | 1.27 | 0.00 | 0.70 | -28.58 | 42.42 | 7.67 | 195.88 | 0.4300 | -720.0 | -436.9 | |
| 0.00 | 0.93 | 0.00 | 0.51 | -29.20 | 41.78 | 7.03 | 194.22 | 0.4368 | -823.0 | -613.5 | |
| 0.00 | 1.02 | 0.00 | 0.56 | -29.53 | 41.53 | 6.78 | 193.53 | 0.4408 | -758.0 | -557.7 | |
| 0.00 | 1.02 | 0.00 | 0.54 | -23.77 | 39.52 | 4.77 | 192.85 | 0.3437 | -911.0 | -702.2 | |
| 0.00 | 1.19 | 0.00 | 0.63 | -25.44 | 38.47 | 3.72 | 189.22 | 0.3672 | -743.0 | -584.6 | |
| 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. | |