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researcher

C. Beck

6 papers hereh-index 11367 citations14 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author1
  • middle author1

Across the 2 of 6 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR4
  • astro-ph2
same name
  • C. Beck — 116 papers, h 47
  • C. Beck — 60 papers, h 23
  • C. Beck — 56 papers, h 24
  • C. Beck — 21 papers, h 26
  • C. Beck — 8 papers, h 12
  • C. Beck — 6 papers, h 3

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20072014
most citedThe signature of chromospheric heating in Ca II H spectra

62 citations · 202 across the 6 of their papers we have counts for

collaborators

4 papers

astro-ph.SR2014★ 26 cited

Fast inversion of solar Ca II spectra

C. Beck, D. Prasad Choudhary, R. Rezaei +1

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…

astro-ph.SR2013

The magnetic configuration of a delta-spot

Horst Balthasar, Christian Beck, Rohan E. Louis +2

Sunspots, which harbor both magnetic polarities within one penumbra, are called delta-spots. They are often associated with flares. Nevertheless, there are only very few detailed o…

astro-ph.SR2012★ 26 cited

The energy of waves in the photosphere and lower chromosphere: III. Inversion setup for Ca II H spectra in local thermal equilibrium

C. Beck, R. Rezaei, K. G. Puschmann

The Ca II H line is one of the strongest lines in the solar spectrum and provides continuous information on the solar atmosphere from the photosphere to the lower chromosphere. We…

astro-ph2007★ 62 cited

The signature of chromospheric heating in Ca II H spectra

C. Beck, W. Schmidt, R. Rezaei +1

We analyze a 1-hour time series of Ca II H intensity spectra and polarimetric spectra around 630 nm to derive the signature of the chromospheric heating and to investigate its rela…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.