SDO HMI 2014-11-28 01:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.48 | 32.08 | 4.45 | 16.95 | 17.76 | 151.26 | 11.95 | 325.29 | 0.3474 | 6.2 | -42.9 | |
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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 |
| 1.28 | 3.08 | 0.68 | 1.64 | 18.09 | 152.93 | 13.62 | 322.31 | 0.3676 | 1020.1 | 841.2 | |
| 0.00 | 0.43 | 0.00 | 0.23 | 18.06 | 152.45 | 13.13 | 323.24 | 0.3625 | 656.0 | 693.2 | |
| 0.00 | 1.11 | 0.00 | 0.59 | 17.91 | 152.31 | 12.99 | 323.25 | 0.3592 | 843.0 | 769.2 | |
| 1.63 | 6.84 | 0.86 | 3.64 | 18.28 | 152.30 | 12.99 | 323.90 | 0.3639 | 980.6 | 784.8 | |
| 0.00 | 0.77 | 0.00 | 0.41 | 17.72 | 152.20 | 12.88 | 323.16 | 0.3558 | 524.0 | 573.1 | |
| 0.00 | 0.77 | 0.00 | 0.41 | 17.32 | 152.17 | 12.85 | 322.50 | 0.3504 | 809.0 | 595.9 | |
| 0.86 | -4.00 | 0.45 | -4.00 | 18.40 | 152.18 | 12.87 | 324.36 | 0.3644 | 831.7 | 999999 | |
| 0.00 | 0.86 | 0.00 | 0.45 | 17.36 | 151.82 | 12.51 | 323.30 | 0.3474 | 644.0 | 580.4 | |
| 1.11 | 6.84 | 0.58 | 3.60 | 17.52 | 150.60 | 11.28 | 326.31 | 0.3379 | -950.1 | -508.7 | |
| 0.00 | 1.37 | 0.00 | 0.72 | 16.87 | 150.52 | 11.21 | 325.33 | 0.3286 | -951.0 | -754.4 | |
| 0.00 | 1.20 | 0.00 | 0.63 | 17.12 | 150.51 | 11.19 | 325.81 | 0.3317 | -1041.0 | -882.9 | |
| 0.00 | 1.63 | 0.00 | 0.86 | 18.29 | 150.58 | 11.27 | 327.63 | 0.3482 | -693.0 | -504.7 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 17.12 | 150.29 | 10.97 | 326.34 | 0.3297 | -808.0 | -677.4 | |
| 1.97 | 5.73 | 1.03 | 3.01 | 17.55 | 150.15 | 10.84 | 327.40 | 0.3343 | -1183.8 | -825.6 | |
| 1.63 | -14.00 | 0.85 | -14.00 | 17.61 | 150.06 | 10.75 | 327.72 | 0.3344 | -1019.6 | 999999 | |
| 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. | |