Long-Term Fluences of Solar Energetic Particles from H to Fe

Details Long-Term Fluences of Solar Energetic Particles from H to Fe Long-Term Fluences of Solar Energetic Particles from H to Fe

Jun 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ssrv..130..323m&link_type=abstract

Space Science Reviews, Volume 130, Issue 1-4, pp. 323-328

Computer Science

12

Sun: Particle Emission, Sun: Solar Wind, Sun: Abundances, Acceleration Of Particles

Scientific paper

Data from ACE and GOES have been used to measure Solar Energetic Particle (SEP) fluence spectra for H, He, O, and Fe, over the period from October 1997 to December 2005. The measurements were made by four instruments on ACE and the EPS sensor on three GOES satellites and extend in energy from ˜0.1 MeV/nuc to ˜100 MeV/nuc. Fluence spectra for each species were fit by conventional forms and used to investigate how the intensities, composition, and spectral shapes vary from year to year.

Affiliated with

Also associated with

No associations

Rating

Long-Term Fluences of Solar Energetic Particles from H to Fe does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Long-Term Fluences of Solar Energetic Particles from H to Fe, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Long-Term Fluences of Solar Energetic Particles from H to Fe will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1721212