SDO HMI 2014-11-24 15:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.88 | 0.00 | 12.51 | -12.93 | 227.01 | 42.63 | 249.60 | 0.7062 | 262.6 | 271.8 | |
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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 | 1.03 | 0.00 | 0.74 | -12.86 | 228.74 | 44.37 | 250.35 | 0.7262 | 282.0 | 251.2 | |
| 0.00 | 1.80 | 0.00 | 1.29 | -13.04 | 228.57 | 44.20 | 250.05 | 0.7248 | 503.0 | 412.4 | |
| 0.00 | 1.28 | 0.00 | 0.92 | -12.77 | 228.51 | 44.13 | 250.40 | 0.7233 | 521.0 | 424.9 | |
| 0.00 | 1.11 | 0.00 | 0.79 | -12.55 | 228.16 | 43.79 | 250.58 | 0.7186 | 625.0 | 537.0 | |
| 0.00 | 0.60 | 0.00 | 0.43 | -12.85 | 228.19 | 43.81 | 250.17 | 0.7199 | 613.0 | 536.6 | |
| 0.00 | 1.20 | 0.00 | 0.85 | -12.76 | 228.00 | 43.62 | 250.23 | 0.7174 | 521.0 | 427.1 | |
| 0.00 | 2.48 | 0.00 | 1.76 | -13.03 | 227.89 | 43.52 | 249.83 | 0.7170 | 804.0 | 673.5 | |
| 0.00 | 0.94 | 0.00 | 0.67 | -13.61 | 227.89 | 43.52 | 249.05 | 0.7190 | 625.0 | 527.3 | |
| 0.00 | 1.03 | 0.00 | 0.72 | -12.93 | 227.62 | 43.24 | 249.86 | 0.7136 | 554.0 | 533.8 | |
| 0.00 | 1.11 | 0.00 | 0.78 | -12.93 | 227.41 | 43.03 | 249.79 | 0.7111 | 644.0 | 547.2 | |
| 0.00 | 1.11 | 0.00 | 0.79 | -14.12 | 227.55 | 43.18 | 248.23 | 0.7169 | 620.0 | 520.1 | |
| 0.00 | 0.77 | 0.00 | 0.51 | -9.99 | 223.78 | 39.41 | 252.58 | 0.6576 | -418.0 | -427.7 | |
| 0.00 | 1.11 | 0.00 | 0.74 | -13.57 | 223.45 | 39.08 | 247.23 | 0.6669 | -643.0 | -565.0 | |
| 0.00 | 1.37 | 0.00 | 0.90 | -12.77 | 223.07 | 38.69 | 248.21 | 0.6589 | -662.0 | -609.7 | |
| 0.00 | 0.94 | 0.00 | 0.62 | -13.17 | 223.06 | 38.69 | 247.63 | 0.6605 | -650.0 | -493.5 | |
| 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. | |