SDO HMI 2014-07-05 09:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 23.71 | 0.00 | 11.97 | 6.86 | 258.56 | -4.28 | 115.95 | 0.1801 | 881.6 | 700.2 | |
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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 |
| 0.00 | 1.91 | 0.00 | 0.97 | 5.94 | 276.68 | 13.83 | 281.24 | 0.2435 | 977.0 | 720.3 | |
| 0.00 | 1.00 | 0.00 | 0.50 | -1.85 | 269.38 | 6.53 | 231.68 | 0.1455 | 819.0 | 621.9 | |
| 0.00 | 2.73 | 0.00 | 1.37 | 11.79 | 268.18 | 5.34 | 328.28 | 0.1741 | 1067.0 | 805.2 | |
| 0.00 | 3.18 | 0.00 | 1.59 | 10.15 | 262.57 | -0.27 | 2.26 | 0.1194 | 904.0 | 729.5 | |
| 0.00 | 1.27 | 0.00 | 0.63 | 9.88 | 260.96 | -1.88 | 15.83 | 0.1191 | 977.0 | 857.2 | |
| 0.00 | 1.27 | 0.00 | 0.63 | 4.35 | 260.03 | -2.81 | 70.02 | 0.0523 | 973.0 | 762.1 | |
| 0.00 | 1.09 | 0.00 | 0.54 | 1.39 | 260.03 | -2.81 | 124.59 | 0.0598 | 787.0 | 620.6 | |
| 0.00 | 1.45 | 0.00 | 0.72 | 7.61 | 259.37 | -3.47 | 38.79 | 0.0963 | 973.0 | 810.7 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 1.85 | 254.03 | -8.82 | 99.32 | 0.1560 | 869.0 | 622.8 | |
| 0.00 | 2.54 | 0.00 | 1.29 | 8.02 | 251.64 | -11.21 | 66.71 | 0.2105 | 614.0 | 551.2 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 6.84 | 250.19 | -12.65 | 73.92 | 0.2274 | 837.0 | 638.6 | |
| 0.00 | 2.27 | 0.00 | 1.16 | 3.68 | 248.65 | -14.19 | 88.14 | 0.2459 | 856.0 | 704.5 | |
| 0.00 | 2.73 | 0.00 | 1.42 | 7.06 | 245.61 | -17.24 | 77.06 | 0.3031 | 808.0 | 643.7 | |
| 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. | |