MODELING IRON ABUNDANCE ENHANCEMENTS IN THE SLOW SOLAR WIND-Reference-Cited by-同舟云学术

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MODELING IRON ABUNDANCE ENHANCEMENTS IN THE SLOW SOLAR WIND

Published:2011-04-26 Issue:2 Volume:732 Page:119
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Byhring H. S.,Cranmer S. R.,Lie-Svendsen Ø.,Habbal S. R.,Esser R.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/732/i=2/a=119/pdf

Reference38 articles.

1. Characterization of the slow wind in the outer corona

2. Effective collision strengths for transitions in Fe XI

3. Slow wind and magnetic topology in the solar minimum corona in 1996–1997

4. Oxygen Abundance and Energy Deposition in the Slow Coronal Wind

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1. The Quiet-Sun Corona;New Millennium Solar Physics;2019

2. Ion Charge States in a Time-Dependent Wave-Turbulence-Driven Model of the Solar Wind;Solar Physics;2019-01

3. SOLAR WIND HEAVY IONS OVER SOLAR CYCLE 23:ACE/SWICS MEASUREMENTS;The Astrophysical Journal;2013-04-17

4. Probing the Fundamental Physics of the Solar Corona with Lunar Solar Occultation Observations;Solar Physics;2012-09-27

5. NEW SOLAR WIND DIAGNOSTIC USING BOTH IN SITU AND SPECTROSCOPIC MEASUREMENTS;The Astrophysical Journal;2012-04-26

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