| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 70.26 | 240.95 | 88.67 | 308.28 | -11.37 | 17.15 | -67.89 | 99.60 | 0.9216 | -147.1 | -51.5 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-03-31 22:00:32 UT
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 | 1.75 | 0.00 | 1.77 | -10.05 | 23.88 | -61.16 | 97.86 | 0.8727 | 480.0 | 404.9 | |
| 0.00 | 3.42 | 0.00 | 3.50 | -10.04 | 23.44 | -61.60 | 97.86 | 0.8764 | 568.0 | 448.0 | |
| 0.00 | 0.35 | 0.00 | 0.36 | -10.45 | 23.24 | -61.80 | 98.33 | 0.8779 | 517.0 | 548.5 | |
| 4.21 | 7.37 | 4.29 | 7.51 | -9.53 | 23.48 | -61.56 | 97.27 | 0.8762 | 670.8 | 477.2 | |
| 0.00 | 0.70 | 0.00 | 0.73 | -10.57 | 22.99 | -62.05 | 98.49 | 0.8799 | 414.0 | 443.8 | |
| 0.00 | 0.70 | 0.00 | 0.72 | -10.43 | 23.05 | -61.99 | 98.32 | 0.8795 | 390.0 | 452.2 | |
| 0.00 | 1.40 | 0.00 | 1.45 | -9.96 | 22.94 | -62.10 | 97.79 | 0.8805 | 394.0 | 334.8 | |
| 5.79 | 9.91 | 6.07 | 10.41 | -10.83 | 22.57 | -62.47 | 98.80 | 0.8833 | 577.5 | 363.9 | |
| 1.32 | 7.80 | 1.38 | 8.24 | -10.19 | 22.53 | -62.51 | 98.07 | 0.8837 | 407.9 | 335.9 | |
| 0.00 | 1.05 | 0.00 | 1.11 | -10.44 | 22.31 | -62.73 | 98.36 | 0.8854 | 476.0 | 415.1 | |
| 2.02 | -9.00 | 2.14 | -9.00 | -10.19 | 22.20 | -62.84 | 98.08 | 0.8864 | 297.3 | 999999 | |
| 1.49 | 25.69 | 1.61 | 28.29 | -10.56 | 21.66 | -63.38 | 98.52 | 0.8906 | 307.8 | 156.4 | |
| 0.00 | 1.49 | 0.00 | 1.62 | -10.34 | 21.60 | -63.44 | 98.28 | 0.8911 | 155.0 | 146.3 | |
| 2.37 | -12.00 | 2.60 | -12.00 | -10.96 | 21.15 | -63.89 | 98.99 | 0.8944 | 486.5 | 999999 | |
| 7.19 | -12.00 | 8.03 | -12.00 | -11.00 | 20.64 | -64.40 | 99.06 | 0.8983 | 401.3 | 999999 | |
| 0.00 | 1.58 | 0.00 | 1.75 | -10.39 | 20.89 | -64.15 | 98.36 | 0.8966 | 32.0 | -25.8 | |
| 0.61 | 10.87 | 0.69 | 12.35 | -10.32 | 20.49 | -64.55 | 98.30 | 0.8996 | 100.1 | -153.2 | |
| 1.58 | 4.12 | 1.82 | 4.74 | -11.44 | 19.80 | -65.24 | 99.57 | 0.9044 | 494.2 | 391.8 | |
| 0.35 | -18.00 | 0.40 | -18.00 | -11.29 | 19.87 | -65.17 | 99.40 | 0.9039 | 219.2 | 999999 | |
| 0.79 | 1.84 | 0.90 | 2.10 | -10.09 | 20.07 | -64.97 | 98.07 | 0.9028 | 211.9 | 157.0 | |
| 0.00 | 1.93 | 0.00 | 2.24 | -11.11 | 19.58 | -65.46 | 99.21 | 0.9061 | -53.0 | -60.0 | |
| 2.63 | 16.66 | 3.23 | 20.55 | -11.41 | 18.06 | -66.98 | 99.60 | 0.9167 | -338.2 | -250.1 | |
| 0.00 | 1.67 | 0.00 | 2.03 | -10.94 | 18.28 | -66.76 | 99.08 | 0.9153 | -351.0 | -308.6 | |
| 0.00 | 0.79 | 0.00 | 0.98 | -11.86 | 17.75 | -67.29 | 100.11 | 0.9187 | 319.0 | 338.0 | |
| 1.84 | -22.00 | 2.30 | -22.00 | -11.42 | 17.58 | -67.46 | 99.63 | 0.9200 | 427.7 | 999999 | |
| 0.00 | 0.79 | 0.00 | 0.98 | -10.61 | 17.72 | -67.32 | 98.75 | 0.9193 | -233.0 | -292.1 | |
| 1.23 | 2.46 | 1.58 | 3.16 | -12.11 | 16.89 | -68.15 | 100.41 | 0.9244 | 150.9 | 64.6 | |
| 0.00 | 1.49 | 0.00 | 1.89 | -10.84 | 17.29 | -67.75 | 99.02 | 0.9221 | -562.0 | -504.8 | |
| 0.00 | 0.61 | 0.00 | 0.80 | -12.16 | 16.52 | -68.52 | 100.48 | 0.9267 | -60.0 | 35.0 | |
| 0.00 | 4.47 | 0.00 | 5.67 | -10.41 | 17.32 | -67.72 | 98.55 | 0.9220 | -261.0 | -271.3 | |
| 0.53 | 1.75 | 0.67 | 2.24 | -10.90 | 17.01 | -68.03 | 99.10 | 0.9239 | -454.3 | -463.7 | |
| 0.00 | 1.05 | 0.00 | 1.40 | -11.23 | 16.09 | -68.95 | 99.50 | 0.9297 | -494.0 | -475.7 | |
| 0.00 | 1.05 | 0.00 | 1.44 | -10.98 | 15.52 | -69.52 | 99.26 | 0.9334 | -383.0 | -390.5 | |
| 25.61 | 124.96 | 36.02 | 176.57 | -12.04 | 14.83 | -70.21 | 100.43 | 0.9372 | -633.7 | -100.4 | |
| 0.00 | 1.23 | 0.00 | 1.68 | -10.76 | 15.46 | -69.58 | 99.03 | 0.9338 | -500.0 | -462.3 | |
| 10.70 | -34.00 | 14.94 | -34.00 | -11.27 | 15.01 | -70.03 | 99.59 | 0.9364 | -526.5 | 999999 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
|
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. |
||
| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
|
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. |
||
| 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. | |