An Improved Method to Derive the Lower Energy Cutoff of non-Thermal Electrons From Hard x-Rays of Solar Flares

Author： Gan W.Q. Li Y.P. Chang J. Tiernan J.M.

ISSN： 0038-0938

Source： Solar Physics, Vol.207, Iss.1, 2002-05, pp. : 137-147

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

Abstract

Related content

An Invariable Point in the Energy Spectra of Non-Thermal Electrons of Solar Flares

By Gan W.Q.

Astrophysics and Space Science, Vol. 260, Iss. 4, 1998-01 ,pp. : 515-519

Springer Publishing Company

Access to resources Recommend Favorite

A Clarification on the invariable point in the power-law energy spectra of non-thermal electrons of solar flares

By Gan W.Q.

Astrophysics and Space Science, Vol. 288, Iss. 4, 2003-01 ,pp. : 451-455

Springer Publishing Company

Access to resources Recommend Favorite

A Clarification on the invariable point in the power-law energy spectra of non-thermal electrons of solar flares

By Gan W.Q.

Astrophysics and Space Science, Vol. 286, Iss. 2, 2003-01 ,pp. : 347-351

Springer Publishing Company

Access to resources Recommend Favorite

The generation of hard X-rays and relativistic protons observed during solar flares

By Podgorny I. Balabin Yu. Vashenyuk E. Podgorny A.

Astronomy Reports, Vol. 54, Iss. 7, 2010-07 ,pp. : 645-656

MAIK Nauka/Interperiodica

Access to resources Recommend Favorite

Hard X-rays, ejecta, and their associated decimetric radio emission in solar flares

By Saint-Hilaire Pascal Benz Arnold

Solar Physics, Vol. 216, Iss. 1-2, 2003-09 ,pp. : 205-224

Springer Publishing Company

Access to resources Recommend Favorite