The FIP and Inverse FIP Effects in Solar and Stellar Coronae

J. Martin Laming
ISSN / E-ISSN
— / —
DOI
10.1007/lrsp-2015-2 ↗
Volume · Issue · Pages
12 · 1 · —
Publisher
Springer International Publishing AG
Article URL
https://doi.org/10.1007/lrsp-2015-2 ↗
Article details
Unverified
Publication date (each date has its type and source)
09 Sep 2015
OpenAlex publication date · source: OpenAlex
Dates on record for this article
TypeDateSource
OpenAlex publication date09 Sep 2015 OpenAlex

Keywords (as given): first ionization potential effect; solar corona; stellar coronae; M dwarfs; solar wind; slow solar wind; fast solar wind; helium depletion; ponderomotive force; magnetohydrodynamic waves; chromosphere; coronal heating; mode conversion; open magnetic field regions

HEC Status at Publication Not the journal's current status

HEC Status at PublicationNot conclusive
Best available information, not a definitive status: HEC status cannot be determined for this date: no HEC list is recorded as in effect on it.
Journal
Living Reviews in Solar Physics
Publication date used
09 Sep 2015 (OpenAlex publication date)
Applicable HEC period
None recorded for this date
Category
—
Recognition status
Unknown (NO_PERIOD_FOR_DATE)
Source
—
Verification status
Not available
This is an automatically generated summary based on the information available on the publication date. Terms & conditions apply.