Compact polarization plane rotator for arbitrary angle

Author(s):  
D. Yu. Kulik ◽  
S. O. Steshenko ◽  
A. A. Kirilenko
2017 ◽  
Vol 76 (10) ◽  
pp. 855-864
Author(s):  
D. Yu. Kulik ◽  
S. A. Steshenko ◽  
A. A. Kirilenko

1997 ◽  
Vol 36 (Part 1, No. 5A) ◽  
pp. 2709-2714 ◽  
Author(s):  
Yoshiharu Taniguchi ◽  
Kensuke Murakami ◽  
Hiroshi Kobayashi ◽  
S hosaku Tanaka

Author(s):  
Nataliya Kolmakova ◽  
Sergey Prikolotin ◽  
Andrey Perov ◽  
Vadim Derkach ◽  
Anatoliy Kirilenko

2017 ◽  
Vol 22 (1) ◽  
pp. 15-20 ◽  
Author(s):  
D. Yu. Kulik ◽  
◽  
S. A. Steshenko ◽  
A. A. Kirilenko

1976 ◽  
Vol 32 ◽  
pp. 457-463
Author(s):  
John M. Wilcox ◽  
Leif Svalgaard

SummaryThe sun as a magnetic star is described on the basis of recent work on solar magnetism. Observations at an arbitrary angle to the rotation axis would show a 22-year polar field variation and a 25-day equatorial sector variation. The sector variation would be similar to an oblique rotator with an angle of 90° between the magnetic and rotational axis.


2021 ◽  
Vol 13 (14) ◽  
pp. 2769
Author(s):  
Xiaomei Lu ◽  
Yongxiang Hu ◽  
Ali Omar ◽  
Rosemary Baize ◽  
Mark Vaughan ◽  
...  

Recent studies indicate that the Cloud-Aerosol Lidar with Orthogonal Polarization (CALIOP) aboard the Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observations (CALIPSO) satellite provides valuable information about ocean phytoplankton distributions. CALIOP’s attenuated backscatter coefficients, measured at 532 nm in receiver channels oriented parallel and perpendicular to the laser’s linear polarization plane, are significantly improved in the Version 4 data product. However, due to non-ideal instrument effects, a small fraction of the backscattered optical power polarized parallel to the receiver polarization reference plane is misdirected into the perpendicular channel, and vice versa. This effect, known as polarization crosstalk, typically causes the measured perpendicular signal to be higher than its true value and the measured parallel signal to be lower than its true value. Therefore, the ocean optical properties derived directly from CALIOP’s measured signals will be biased if the polarization crosstalk effect is not taken into account. This paper presents methods that can be used to estimate the CALIOP crosstalk effects from on-orbit measurements. The global ocean depolarization ratios calculated both before and after removing the crosstalk effects are compared. Using CALIOP crosstalk-corrected signals is highly recommended for all ocean subsurface studies.


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