Power spectral density of electron flux from Ulysses, 1999-2001

Details Power spectral density of electron flux from Ulysses, 1999-2001 Power spectral density of electron flux from Ulysses, 1999-2001

Feb 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003esasp.517..401t&link_type=abstract

In: Proceedings of SOHO 12 / GONG+ 2002. Local and global helioseismology: the present and future, 27 October - 1 November 2002,

Computer Science

Ulysses, G-Modes, Hiscale

Scientific paper

Fluxes of low-energy (~50-200 keV) electrons measured on the Ulysses HISCALE instrument were of sufficient magnitude to compute reliable power spectra in the frequency range where low-order and degree g- and p-solar modes are expected. Fits to some well-determined l = 1 modes give an estimate of the asymptotic period spacing T0 ≍ 33.23 minutes.

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