Parkes observations for project P878 semester 2014OCTS

Measuring the magnetic field and electron density of the solar wind is essential in order to understand the properties of solar corona. Detection of dispersion measure (DM) and Faraday rotation measure (RM) of linearly polarized radio sources occulted by the solar wind provides a unique opportunity...

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Bibliographic Details
Other Authors: xiaopeng You (hasPrincipalInvestigator), CSIRO (isManagedBy)
Format: Dataset
Language:unknown
Published: Commonwealth Scientific and Industrial Research Organisation
Subjects:
pulsars
neutron stars
interstellar medium in and around the Milky Way
magnetic fields
Astronomical and Space Sciences not elsewhere classified
PHYSICAL SCIENCES
ASTRONOMICAL AND SPACE SCIENCES
Faraday
Milky Way
South Pole
South pole
Online Access:https://researchdata.ands.org.au/parkes-observations-project-semester-2014octs/663496

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