SDO HMI 2014-01-16 08:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 74.60 | 359.57 | 41.41 | 199.53 | -16.21 | 12.17 | 24.60 | 242.60 | 0.4519 | 925.3 | 376.1 | |
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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 |
| 34.45 | 208.48 | 19.27 | 116.66 | -16.58 | 13.07 | 25.50 | 242.61 | 0.4667 | 1155.6 | 345.7 | |
| 5.87 | -1.00 | 3.27 | -1.00 | -16.59 | 12.70 | 25.13 | 242.28 | 0.4617 | 1355.8 | 999999 | |
| 2.47 | -1.00 | 1.37 | -1.00 | -16.60 | 12.50 | 24.93 | 242.10 | 0.4590 | 1258.4 | 999999 | |
| 0.00 | 1.45 | 0.00 | 0.80 | -16.85 | 12.16 | 24.59 | 241.31 | 0.4559 | 200.0 | 205.4 | |
| 0.00 | 2.64 | 0.00 | 1.45 | -14.88 | 11.44 | 23.87 | 244.81 | 0.4340 | -14.0 | 4.8 | |
| 0.00 | 0.77 | 0.00 | 0.42 | -16.72 | 11.57 | 24.00 | 241.06 | 0.4470 | 605.0 | 467.4 | |
| 31.13 | 137.29 | 17.13 | 75.46 | -15.73 | 11.34 | 23.77 | 242.92 | 0.4376 | 1324.9 | 517.6 | |
| 0.68 | -7.00 | 0.37 | -7.00 | -14.95 | 11.15 | 23.58 | 244.42 | 0.4303 | 894.4 | 999999 | |
| 0.00 | 0.43 | 0.00 | 0.24 | -19.48 | 10.50 | 22.93 | 234.54 | 0.4529 | 686.0 | 644.2 | |
| 0.00 | 1.19 | 0.00 | 0.64 | -15.18 | 7.23 | 19.66 | 240.07 | 0.3762 | -815.0 | -703.7 | |
| 0.00 | 1.19 | 0.00 | 0.64 | -15.07 | 7.05 | 19.48 | 240.14 | 0.3730 | -979.0 | -727.6 | |
| 0.00 | 1.28 | 0.00 | 0.68 | -16.92 | 6.33 | 18.76 | 234.89 | 0.3777 | -839.0 | -692.3 | |
| 0.00 | 1.19 | 0.00 | 0.63 | -16.16 | 5.25 | 17.68 | 235.18 | 0.3568 | -903.0 | -690.1 | |
| 0.00 | 1.11 | 0.00 | 0.59 | -19.19 | 4.28 | 16.71 | 226.94 | 0.3733 | -940.0 | -691.1 | |
| 0.00 | 2.55 | 0.00 | 1.32 | -12.31 | 3.43 | 15.86 | 243.03 | 0.3010 | -852.0 | -668.8 | |
| 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. | |