Evidence for non-Maxwellian electron energy distributions in the solar 
transition region: Si III line ratios from SUMER

Pinfield, D. J.; Keenan, F. P.; Mathioudakis, M.; Phillips, K. H. J.; Curdt, W.; Wilhelm, K.

Item

ITEM ACTIONSEXPORT

Add to Basket

Local TagsRelease HistoryDetailsSummary

Released

Journal Article

Evidence for non-Maxwellian electron energy distributions in the solar transition region: Si III line ratios from SUMER

MPS-Authors

/persons/resource/persons103872

Curdt, W.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

/persons/resource/persons104293

Wilhelm, K.
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

External Resource

No external resources are shared

Fulltext (restricted access)

There are currently no full texts shared for your IP range.

Fulltext (public)

There are no public fulltexts stored in PuRe

Supplementary Material (public)

There is no public supplementary material available

Citation

Pinfield, D. J., Keenan, F. P., Mathioudakis, M., Phillips, K. H. J., Curdt, W., & Wilhelm, K. (1999). Evidence for non-Maxwellian electron energy distributions in the solar transition region: Si III line ratios from SUMER. Astrophysical Journal, 527, 1000-1008.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0014-DCD1-0

Abstract

There is no abstract available