A study of cosmic ray flux based on the noise in raw CCD data from solar images

Author:

Shen Z.-N.12ORCID,Qin G.3ORCID

Affiliation:

1. State Key Laboratory of Space Weather; National Space Science Center, Chinese Academy of Sciences; Beijing China

2. College of Earth Sciences; University of Chinese Academy of Sciences; Beijing China

3. School of Science; Harbin Institute of Technology; Shenzhen China

Funder

NNSFC

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Reference17 articles.

1. On the relationship of the 27-day variations of the solar wind velocity and galactic cosmic ray intensity in minimum epoch of solar activity;Alania;Sol. Phys.,2011

2. 27-day variation of the GCR intensity based on corrected and uncorrected for geomagnetic disturbances data of neutron monitors;Alania;J. Phys. Conf. Ser.,2015

3. Maximum entropy method for low contrast images;Chae;J. Korean Astron. Soc.,1994

4. EIT: Extreme-ultraviolet imaging telescope for the SOHO mission;Delaboudinire;Sol. Phys.,1995

5. Measuring proton energies and fluxes using EIT (SOHO) CCD areas outside the solar disk images;Didkovsky;Astron. Nachr.,2006

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