Published December 3, 2004 | Version v1
Report Metadata-only

Fe XVII Emission from Hot, Collisional Plasmas

Creators

Description

The ratios of the Fe XVII 3s → 2p transitions to that of the dominant 3d → 2p transition measured in high-temperature tokamak plasmas are compared to solar and astrophysical observations. Good agreement is found, indicating that the collisional line formation processes active in opacity-free, low-density, high-temperature laboratory plasmas are a good description of those found in astrophysical plasmas

Availability note (English)

Available from http://www.llnl.gov/tid/lof/documents/pdf/314541.pdf; PURL: https://www.osti.gov/servlets/purl/15014392-l6HOH6/native/

Additional details

Identifiers

URL
http://www.llnl.gov/tid/lof/documents/pdf/314541.pdf; https://www.osti.gov/servlets/purl/15014392-l6HOH6/native/;

Publishing Information

Imprint Pagination
vp.
Report number
UCRL-PROC--208689

Conference

Title
Workshop on X-ray Diagnostics of Astrophysical Plasmas
Dates
15-17 Nov 2004
Place
Cambridge, MA (United States)

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
39026003
Subject category
S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
Resource subtype / Literary indicator
Conference, Non-conventional Literature
Descriptors DEI
ASTROPHYSICS; COLLISIONAL PLASMA; EMISSION; ENERGY-LEVEL TRANSITIONS; LAWRENCE LIVERMORE NATIONAL LABORATORY; PLASMA DENSITY
Descriptors DEC
NATIONAL ORGANIZATIONS; PHYSICS; PLASMA; US DOE; US ORGANIZATIONS

Optional Information

Contract/Grant/Project number
W-7405-ENG-48
Notes
PDF-FILE: 5 ; SIZE: 70.3 KBYTES
Funding organization
US Department of Energy (United States)