THE EVOLUTION OF SOLAR FLUX FROM 0.1 nm TO 160 μm: QUANTITATIVE ESTIMATES FOR PLANETARY STUDIES-Reference-Cited by-同舟云学术

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THE EVOLUTION OF SOLAR FLUX FROM 0.1 nm TO 160 μm: QUANTITATIVE ESTIMATES FOR PLANETARY STUDIES

Published:2012-09-06 Issue:1 Volume:757 Page:95
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Claire Mark W.,Sheets John,Cohen Martin,Ribas Ignasi,Meadows Victoria S.,Catling David C.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/757/i=1/a=95/pdf

Reference78 articles.

1. The Coronal Heating Paradox

2. Evolution of the solar ionizing flux

3. Sleuthing the Dynamo. II.Hubble Space TelescopeGoddard High Resolution Spectrograph Observations of Solar‐Type Dwarfs in Young Galactic Clusters

4. Solar Models: Current Epoch and Time Dependences, Neutrinos, and Helioseismological Properties

5. Ages for Illustrative Field Stars Using Gyrochronology: Viability, Limitations, and Errors

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