group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
48.32 | 299.83 | 26.05 | 161.97 | -24.20 | 250.84 | -11.46 | 152.92 | 0.3993 | 822.3 | 341.4 |
previous
or next observation for the same group /
back to the solar disc SDO HMI 2013-01-05 21:58:54 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 | 1.36 | 0.00 | 0.72 | -24.69 | 261.05 | -1.25 | 176.84 | 0.3621 | 794.0 | 594.7 | |
48.32 | 282.69 | 26.05 | 152.53 | -24.23 | 251.13 | -11.17 | 153.45 | 0.3970 | 1497.4 | 409.0 | |
0.00 | 2.63 | 0.00 | 1.45 | -23.72 | 246.00 | -16.30 | 143.43 | 0.4331 | -667.0 | -586.9 | |
0.00 | 0.59 | 0.00 | 0.33 | -24.82 | 245.76 | -16.55 | 144.64 | 0.4487 | -117.0 | -239.6 | |
0.00 | 1.10 | 0.00 | 0.61 | -24.02 | 245.29 | -17.01 | 142.75 | 0.4434 | -796.0 | -612.2 | |
0.00 | 2.12 | 0.00 | 1.17 | -24.04 | 244.95 | -17.35 | 142.27 | 0.4470 | -885.0 | -701.4 | |
0.00 | 1.19 | 0.00 | 0.66 | -24.39 | 244.83 | -17.47 | 142.60 | 0.4521 | -850.0 | -671.0 | |
0.00 | 1.10 | 0.00 | 0.61 | -23.47 | 244.76 | -17.54 | 141.11 | 0.4422 | -896.0 | -733.1 | |
0.00 | 1.19 | 0.00 | 0.66 | -24.38 | 244.63 | -17.67 | 142.29 | 0.4540 | -791.0 | -533.9 | |
0.00 | 0.93 | 0.00 | 0.52 | -23.97 | 244.69 | -17.61 | 141.77 | 0.4487 | -738.0 | -557.2 | |
0.00 | 2.04 | 0.00 | 1.12 | -23.31 | 244.58 | -17.72 | 140.58 | 0.4422 | -943.0 | -847.6 | |
0.00 | 1.36 | 0.00 | 0.74 | -22.22 | 244.53 | -17.78 | 138.74 | 0.4304 | -929.0 | -720.0 | |
0.00 | 1.53 | 0.00 | 0.85 | -23.34 | 244.17 | -18.13 | 140.01 | 0.4465 | -901.0 | -722.3 |
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. |