Skip to main content
CenXiv.org
This website is in trial operation, support us!
We gratefully acknowledge support from all contributors.
Contribute
Donate
cenxiv logo > astro-ph > arXiv:1410.8451

Help | Advanced Search

Astrophysics > Solar and Stellar Astrophysics

arXiv:1410.8451 (astro-ph)
[Submitted on 30 Oct 2014 (v1) , last revised 5 Nov 2014 (this version, v2)]

Title: Fast inversion of solar Ca II spectra

Title: 快速反演太阳钙Ⅱ谱线

Authors:C. Beck, D. Prasad Choudhary, R. Rezaei, R.E. Louis
Abstract: We present a fast (<< 1 s per profile) inversion code for solar Ca II lines. The code uses an archive of spectra that are synthesized prior to the inversion under the assumption of local thermodynamic equilibrium (LTE). We show that it can be successfully applied to spectrograph data or more sparsely sampled spectra from two-dimensional spectrometers. From a comparison to a non-LTE inversion of the same set of spectra, we derive a first-order non-LTE correction to the temperature stratifications derived in the LTE approach. The correction factor is close to unity up to log tau ~ -3 and increases to values of 2.5 and 4 at log tau = -6 in the quiet Sun and the umbra, respectively.
Abstract: 我们提出了一种快速(每谱线 << 1 秒)的太阳 Ca II 线反演代码。该代码使用一个光谱档案,这些光谱是在假设局部热动平衡(LTE)条件下预先合成的。我们表明它可以成功应用于光谱仪数据或来自二维分光仪的更稀疏采样的光谱。通过与相同光谱集的非 LTE 反演比较,我们得出了 LTE 方法中推导出的温度分层的首阶非 LTE 校正。校正因子在 log tau ~ -3 以下接近于 1,并且在日冕和本影中分别增加到 log tau = -6 时的 2.5 和 4。
Comments: 8 pages, 10 figures, accepted for publication in ApJ; version updated for an error in the references
Subjects: Solar and Stellar Astrophysics (astro-ph.SR)
Cite as: arXiv:1410.8451 [astro-ph.SR]
  (or arXiv:1410.8451v2 [astro-ph.SR] for this version)
  https://doi.org/10.48550/arXiv.1410.8451
arXiv-issued DOI via DataCite
Related DOI: https://doi.org/10.1088/0004-637X/798/2/100
DOI(s) linking to related resources

Submission history

From: Christian Arthur Rudolf Beck [view email]
[v1] Thu, 30 Oct 2014 17:18:45 UTC (5,385 KB)
[v2] Wed, 5 Nov 2014 16:18:10 UTC (5,385 KB)
Full-text links:

Access Paper:

    View a PDF of the paper titled
  • View Chinese PDF
  • View PDF
  • TeX Source
  • Other Formats
view license
Current browse context:
astro-ph.SR
< prev   |   next >
new | recent | 2014-10
Change to browse by:
astro-ph

References & Citations

  • NASA ADS
  • Google Scholar
  • Semantic Scholar
a export BibTeX citation Loading...

BibTeX formatted citation

×
Data provided by:

Bookmark

BibSonomy logo Reddit logo

Bibliographic and Citation Tools

Bibliographic Explorer (What is the Explorer?)
Connected Papers (What is Connected Papers?)
Litmaps (What is Litmaps?)
scite Smart Citations (What are Smart Citations?)

Code, Data and Media Associated with this Article

alphaXiv (What is alphaXiv?)
CatalyzeX Code Finder for Papers (What is CatalyzeX?)
DagsHub (What is DagsHub?)
Gotit.pub (What is GotitPub?)
Hugging Face (What is Huggingface?)
Papers with Code (What is Papers with Code?)
ScienceCast (What is ScienceCast?)

Demos

Replicate (What is Replicate?)
Hugging Face Spaces (What is Spaces?)
TXYZ.AI (What is TXYZ.AI?)

Recommenders and Search Tools

Influence Flower (What are Influence Flowers?)
CORE Recommender (What is CORE?)
IArxiv Recommender (What is IArxiv?)
  • Author
  • Venue
  • Institution
  • Topic

arXivLabs: experimental projects with community collaborators

arXivLabs is a framework that allows collaborators to develop and share new arXiv features directly on our website.

Both individuals and organizations that work with arXivLabs have embraced and accepted our values of openness, community, excellence, and user data privacy. arXiv is committed to these values and only works with partners that adhere to them.

Have an idea for a project that will add value for arXiv's community? Learn more about arXivLabs.

Which authors of this paper are endorsers? | Disable MathJax (What is MathJax?)
  • About
  • Help
  • contact arXivClick here to contact arXiv Contact
  • subscribe to arXiv mailingsClick here to subscribe Subscribe
  • Copyright
  • Privacy Policy
  • Web Accessibility Assistance
  • arXiv Operational Status
    Get status notifications via email or slack

京ICP备2025123034号