SDO HMI 2014-09-16 05:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.51 | 25.06 | 1.16 | 19.32 | -15.92 | 64.69 | 44.73 | 242.12 | 0.7678 | 150.7 | 272.5 | |
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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 | 1.33 | 0.00 | 1.10 | -17.61 | 67.62 | 47.66 | 241.62 | 0.8030 | 481.0 | 395.5 | |
| 0.00 | 0.98 | 0.00 | 0.77 | -15.18 | 65.98 | 46.02 | 243.67 | 0.7771 | 548.0 | 428.3 | |
| 0.00 | 3.20 | 0.00 | 2.50 | -15.90 | 65.46 | 45.50 | 242.55 | 0.7753 | 572.0 | 498.6 | |
| 0.00 | 2.31 | 0.00 | 1.77 | -14.77 | 65.06 | 45.10 | 243.71 | 0.7662 | 190.0 | 234.7 | |
| 0.00 | 2.49 | 0.00 | 1.93 | -15.64 | 65.12 | 45.16 | 242.69 | 0.7708 | 711.0 | 631.7 | |
| 0.53 | 3.02 | 0.41 | 2.35 | -15.96 | 65.08 | 45.12 | 242.29 | 0.7718 | 664.5 | 582.5 | |
| 0.98 | 4.00 | 0.75 | 3.08 | -15.30 | 64.89 | 44.93 | 242.99 | 0.7669 | 799.3 | 689.5 | |
| 0.00 | 0.98 | 0.00 | 0.74 | -14.27 | 64.62 | 44.66 | 244.09 | 0.7597 | 331.0 | 319.3 | |
| 0.00 | 0.62 | 0.00 | 0.48 | -16.15 | 65.00 | 45.04 | 242.02 | 0.7719 | 373.0 | 384.7 | |
| 0.00 | 0.98 | 0.00 | 0.75 | -16.68 | 64.00 | 44.04 | 240.88 | 0.7646 | -510.0 | -393.8 | |
| 0.00 | 0.62 | 0.00 | 0.48 | -17.25 | 64.12 | 44.17 | 240.27 | 0.7685 | -458.0 | -350.1 | |
| 0.00 | 2.31 | 0.00 | 1.77 | -16.90 | 63.89 | 43.93 | 240.56 | 0.7645 | -595.0 | -416.0 | |
| 0.00 | 0.53 | 0.00 | 0.40 | -16.52 | 62.95 | 42.99 | 240.50 | 0.7535 | -497.0 | -453.5 | |
| 0.00 | 1.69 | 0.00 | 1.20 | -16.83 | 59.46 | 39.50 | 238.05 | 0.7199 | -549.0 | -390.5 | |
| 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. | |