File:Effective neutrino cross sections.png

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Effective_neutrino_cross_sections.png(430 × 284 pixels, file size: 15 KB, MIME type: image/png)

Summary[edit | edit source]

Description

The effective neutrino cross sections by plasma instability.

Source

The image appears on a website entitled, "Anticorrelation Between Neutrino Flux and Activity in the Sun" at http://adsabs.harvard.edu/abs/1995ICRC....4.1259T.

Date

28 August 1995

Author

Yukio Tomozawa

Rationale

No free licensed or public domain alternatives known to exist to show the effective neutrino cross sections by plasma instability regarding anticorrelation between neutrino flux and activity in the Sun, about 1995.

Permission

Fair Use

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File history

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Date/TimeThumbnailDimensionsUserComment
current20:42, 2 June 2018Thumbnail for version as of 20:42, 2 June 2018430 × 284 (15 KB)Marshallsumter (discuss | contribs){{Information1 |Description = The effective neutrino cross sections by plasma instability. |Source = The image appears on a website entitled, "Anticorrelation Between Neutrino Flux and Activity in the Sun" at http://adsabs.harvard.edu/abs/1995ICRC....4.1259T. |Date = 28 August 1995 |Author = Yukio Tomozawa |Rationale = No free licensed or public domain alternatives known to exist to show the effective neutrino cross sections by plasma instability regarding anticorrelation between neutrino flu...

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