SDO HMI 2014-11-04 23:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.68 | 0.00 | 12.00 | -21.40 | 78.46 | -5.16 | 169.54 | 0.4426 | 648.4 | 587.0 | |
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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 | 1.30 | 0.00 | 0.71 | -20.68 | 85.55 | 1.94 | 184.33 | 0.4206 | 797.0 | 513.8 | |
| 0.00 | 2.16 | 0.00 | 1.19 | -21.53 | 82.27 | -1.34 | 177.10 | 0.4335 | 706.0 | 611.4 | |
| 0.00 | 1.38 | 0.00 | 0.76 | -21.37 | 81.86 | -1.76 | 176.19 | 0.4312 | 722.0 | 538.8 | |
| 0.00 | 1.47 | 0.00 | 0.80 | -21.04 | 80.68 | -2.93 | 173.56 | 0.4278 | 760.0 | 546.8 | |
| 0.00 | 5.70 | 0.00 | 3.12 | -20.78 | 80.53 | -3.09 | 173.15 | 0.4239 | 746.0 | 677.8 | |
| 0.00 | 1.56 | 0.00 | 0.85 | -20.23 | 78.19 | -5.43 | 167.80 | 0.4215 | 653.0 | 528.2 | |
| 0.00 | 2.76 | 0.00 | 1.52 | -20.57 | 77.06 | -6.56 | 165.57 | 0.4308 | 807.0 | 700.8 | |
| 0.00 | 0.95 | 0.00 | 0.52 | -20.41 | 76.46 | -7.16 | 164.21 | 0.4308 | 851.0 | 674.8 | |
| 0.00 | 1.12 | 0.00 | 0.62 | -20.57 | 76.36 | -7.26 | 164.10 | 0.4337 | 727.0 | 555.0 | |
| 0.00 | 1.12 | 0.00 | 0.63 | -21.98 | 73.14 | -10.48 | 158.90 | 0.4705 | 802.0 | 608.1 | |
| 0.00 | 1.56 | 0.00 | 0.92 | -26.28 | 70.26 | -13.36 | 157.60 | 0.5458 | 743.0 | 585.6 | |
| 0.00 | 0.60 | 0.00 | 0.36 | -24.16 | 65.07 | -18.54 | 148.24 | 0.5535 | -533.0 | -392.1 | |
| 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. | |