Evidence for the prolonged existence of >100 MeV solar protons in coronal structures

ISSN： 1063-7729

Source： Astronomy Reports, Vol.47, Iss.11, 2003-11, pp. : 916-924

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

Previous Menu Next

Related content

Solar particle events with helium-over-hydrogen enhancement in the energy range up to 100 MeV nucl^−1

By Torsti J. Kocharov L. Laivola J. Pohjolainen S. Plunkett S.P. Thompson B.J. Kaiser M.L. Reiner M.J.

Solar Physics, Vol. 205, Iss. 1, 2002-01 ,pp. : 123-147

Springer Publishing Company

Access to resources Recommend Favorite

Spectroscopic Studies of the Solar Corona – V. Physical Properties of Coronal Structures

By Singh J. Sakurai T. Ichimoto K. Muneer S.

Solar Physics, Vol. 212, Iss. 2, 2003-02 ,pp. : 343-359

Springer Publishing Company

Access to resources Recommend Favorite

On Temporal Variation of the 0.511 MeV Line in A Solar Flare

By Gan W.Q. Rieger E.

Solar Physics, Vol. 186, Iss. 1, 1999-05 ,pp. : 311-318

Springer Publishing Company

Access to resources Recommend Favorite

Size Distrtibutions of the >10 MeV Solar Proton Events

By Miroshnichenko L.I. Mendoza B. Pérez Enríquez R.

Solar Physics, Vol. 202, Iss. 1, 2001-08 ,pp. : 151-171

Springer Publishing Company

Access to resources Recommend Favorite

Evidence for a new MeV source observed by the COMPTEL experiment aboard CGRO

By Zhang Shu Collmar Werner

Astrophysics and Space Science, Vol. 309, Iss. 1-4, 2007-06 ,pp. : 23-27

Springer Publishing Company

Access to resources Recommend Favorite