SDO HMI 2014-08-05 14:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.61 | 0.00 | 12.92 | 16.77 | 249.88 | 39.93 | 289.80 | 0.6536 | 591.9 | 479.6 | |
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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 | 0.72 | 0.00 | 0.56 | 8.65 | 260.80 | 50.84 | 276.22 | 0.7734 | 487.0 | 424.5 | |
| 0.00 | 0.99 | 0.00 | 0.74 | 9.88 | 258.83 | 48.88 | 277.84 | 0.7514 | 521.0 | 390.5 | |
| 0.00 | 0.72 | 0.00 | 0.53 | 9.69 | 258.18 | 48.23 | 277.58 | 0.7439 | 521.0 | 402.5 | |
| 0.00 | 0.99 | 0.00 | 0.74 | 15.60 | 258.13 | 48.18 | 285.53 | 0.7472 | 465.0 | 311.5 | |
| 0.00 | 1.18 | 0.00 | 0.87 | 16.89 | 257.98 | 48.03 | 287.27 | 0.7473 | 536.0 | 398.5 | |
| 0.00 | 1.90 | 0.00 | 1.35 | 14.73 | 255.65 | 45.70 | 284.68 | 0.7178 | 637.0 | 456.4 | |
| 0.00 | 0.63 | 0.00 | 0.44 | 11.90 | 254.57 | 44.62 | 280.82 | 0.7020 | 645.0 | 541.0 | |
| 0.00 | 1.18 | 0.00 | 0.75 | 16.13 | 248.00 | 38.05 | 288.34 | 0.6260 | 632.0 | 563.8 | |
| 0.00 | 2.98 | 0.00 | 1.89 | 16.51 | 247.97 | 38.01 | 288.94 | 0.6265 | 479.0 | 479.1 | |
| 0.00 | 1.27 | 0.00 | 0.80 | 16.27 | 247.83 | 37.88 | 288.60 | 0.6241 | 751.0 | 615.1 | |
| 0.00 | 2.71 | 0.00 | 1.66 | 20.64 | 244.05 | 34.10 | 297.11 | 0.5916 | 636.0 | 507.2 | |
| 0.00 | 4.34 | 0.00 | 2.59 | 22.19 | 240.68 | 30.73 | 301.63 | 0.5578 | 793.0 | 526.7 | |
| 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. | |