group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
55.33 | 327.37 | 78.24 | 469.33 | 13.72 | 173.81 | 69.66 | 283.81 | 0.9369 | -4.3 | -6.6 |
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back to the solar disc SDO HMI 2010-11-18 19:58:57 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 |
4.63 | 171.66 | 7.99 | 289.36 | 12.79 | 177.60 | 73.45 | 282.63 | 0.9592 | 337.3 | -133.8 | |
0.43 | -1.00 | 0.73 | -1.00 | 13.20 | 177.38 | 73.23 | 283.06 | 0.9582 | 170.4 | 999999 | |
21.19 | -1.00 | 35.52 | -1.00 | 12.97 | 177.09 | 72.94 | 282.82 | 0.9568 | -613.0 | 999999 | |
0.60 | -1.00 | 0.98 | -1.00 | 12.83 | 176.58 | 72.43 | 282.70 | 0.9542 | -1018.9 | 999999 | |
0.77 | -1.00 | 1.27 | -1.00 | 12.98 | 176.69 | 72.54 | 282.85 | 0.9548 | -1078.7 | 999999 | |
0.00 | 0.51 | 0.00 | 0.77 | 13.18 | 174.86 | 70.71 | 283.11 | 0.9451 | -334.0 | -363.3 | |
0.00 | 1.29 | 0.00 | 1.88 | 12.59 | 174.39 | 70.24 | 282.51 | 0.9423 | -528.0 | -476.5 | |
0.77 | 6.18 | 1.08 | 8.65 | 13.41 | 173.48 | 69.33 | 283.42 | 0.9372 | 104.7 | -248.9 | |
0.00 | 0.94 | 0.00 | 1.27 | 11.96 | 172.54 | 68.39 | 281.91 | 0.9311 | 90.0 | 83.7 | |
1.89 | 2.92 | 2.52 | 3.90 | 13.49 | 172.34 | 68.19 | 283.56 | 0.9303 | 247.5 | 137.6 | |
0.00 | 6.78 | 0.00 | 8.89 | 12.92 | 171.92 | 67.77 | 282.97 | 0.9275 | 508.0 | 289.5 | |
0.00 | 3.60 | 0.00 | 4.75 | 13.56 | 172.05 | 67.90 | 283.65 | 0.9285 | 572.0 | 429.1 | |
2.40 | 3.69 | 2.82 | 4.33 | 14.71 | 168.94 | 64.79 | 285.11 | 0.9083 | 163.0 | 156.4 | |
22.65 | 129.80 | 25.33 | 145.53 | 15.35 | 167.52 | 63.37 | 285.93 | 0.8984 | 768.3 | 231.4 |
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. |
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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. |
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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. |