Interpreting coronal polarization observations

Solar coronal polarization observations are an underused data product because of the difficulties in interpreting the data and in calculating an inversion. The physics of the polarization is well understood and documented in the literature. The purpose of this paper is to present a general overview on how to interpret polarization signals without calculating an inversion. This is intended to introduce the data to those who are unfamiliar to polarization, and in so doing, make the data more accessible.

To Access Resource:

Questions? Email Resource Support Contact:

  • opensky@ucar.edu
    UCAR/NCAR - Library

Resource Type publication
Temporal Range Begin N/A
Temporal Range End N/A
Temporal Resolution N/A
Bounding Box North Lat N/A
Bounding Box South Lat N/A
Bounding Box West Long N/A
Bounding Box East Long N/A
Spatial Representation N/A
Spatial Resolution N/A
Related Links N/A
Additional Information N/A
Resource Format PDF
Standardized Resource Format PDF
Asset Size N/A
Legal Constraints

Copyright 2012 Astronomical Society of the Pacific.


Access Constraints None
Software Implementation Language N/A

Resource Support Name N/A
Resource Support Email opensky@ucar.edu
Resource Support Organization UCAR/NCAR - Library
Distributor N/A
Metadata Contact Name N/A
Metadata Contact Email opensky@ucar.edu
Metadata Contact Organization UCAR/NCAR - Library

Author Rachmeler, Laurel A.
Casini, Roberto
Gibson, Sarah E.
Publisher UCAR/NCAR - Library
Publication Date 2012-12-01T00:00:00
Digital Object Identifier (DOI) Not Assigned
Alternate Identifier N/A
Resource Version N/A
Topic Category geoscientificInformation
Progress N/A
Metadata Date 2023-08-18T19:02:18.903880
Metadata Record Identifier edu.ucar.opensky::articles:18959
Metadata Language eng; USA
Suggested Citation Rachmeler, Laurel A., Casini, Roberto, Gibson, Sarah E.. (2012). Interpreting coronal polarization observations. UCAR/NCAR - Library. http://n2t.net/ark:/85065/d77p913c. Accessed 23 July 2025.

Harvest Source