SDO HMI 2014-09-13 16:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.96 | 101.81 | 14.32 | 56.02 | -15.77 | 65.62 | 12.10 | 207.42 | 0.4400 | 663.9 | 417.2 | |
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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 |
| 3.73 | 7.20 | 2.07 | 3.99 | -15.85 | 66.87 | 13.34 | 209.74 | 0.4494 | 886.0 | 476.5 | |
| 0.00 | 1.87 | 0.00 | 1.04 | -16.44 | 66.78 | 13.26 | 208.92 | 0.4566 | 632.0 | 561.8 | |
| 2.67 | 80.38 | 1.48 | 44.21 | -15.84 | 66.52 | 12.99 | 209.10 | 0.4465 | 936.3 | 522.1 | |
| 6.40 | -3.00 | 3.53 | -3.00 | -15.67 | 66.22 | 12.69 | 208.73 | 0.4419 | 991.7 | 999999 | |
| 0.00 | 2.93 | 0.00 | 1.62 | -16.12 | 66.18 | 12.65 | 208.15 | 0.4479 | 696.0 | 585.5 | |
| 5.78 | -3.00 | 3.18 | -3.00 | -15.60 | 66.02 | 12.49 | 208.43 | 0.4394 | 1078.4 | 999999 | |
| 7.38 | -3.00 | 4.06 | -3.00 | -15.42 | 65.79 | 12.26 | 208.17 | 0.4354 | 1241.7 | 999999 | |
| 0.00 | 0.98 | 0.00 | 0.54 | -15.98 | 65.72 | 12.19 | 207.44 | 0.4426 | 592.0 | 458.5 | |
| 0.00 | 1.42 | 0.00 | 0.79 | -17.37 | 63.27 | 9.74 | 201.29 | 0.4465 | 771.0 | 560.4 | |
| 0.00 | 0.98 | 0.00 | 0.54 | -17.70 | 61.84 | 8.32 | 198.16 | 0.4439 | -695.0 | -595.1 | |
| 0.00 | 1.16 | 0.00 | 0.64 | -18.83 | 59.49 | 5.96 | 192.64 | 0.4511 | -730.0 | -600.1 | |
| 0.00 | 1.96 | 0.00 | 1.06 | -16.68 | 58.72 | 5.20 | 192.10 | 0.4156 | -767.0 | -690.0 | |
| 0.00 | 2.93 | 0.00 | 1.59 | -16.58 | 58.53 | 5.00 | 191.71 | 0.4134 | -871.0 | -615.9 | |
| 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. | |