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C. Damiani

5 papers hereh-index 14550 citations35 works total

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

author position
  • first author2
  • middle author2
  • last author1

Across the 5 of 5 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR3
  • astro-ph.EP2
same name
  • C. Damiani — 6 papers, h 5
  • C. Damiani — 5 papers
  • C. Damiani — 3 papers
  • C. Damiani — 3 papers, h 20
  • C. Damiani — 2 papers, h 4
  • C. Damiani — 1 paper

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
20132021
most citedSolar inertial modes: Observations, identification, and diagnostic promise

72 citations · 185 across the 3 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

3 papers · 1 filter

astro-ph.SR2021★ 72 cited

Solar inertial modes: Observations, identification, and diagnostic promise

Laurent Gizon, Robert H. Cameron, Yuto Bekki +10

The oscillations of a slowly rotating star have long been classified into spheroidal and toroidal modes. The spheroidal modes include the well-known 5-min acoustic modes used in he…

astro-ph.SR2020★ 50 cited

Active red giants: close binaries versus single rapid rotators

Patrick Gaulme, Jason Jackiewicz, Federico Spada +7

The objective of this work is to determine what fraction of red-giant (RG) stars shows photometric rotational modulation, and understand its origin. One of the underlying questions…

astro-ph.SR2020

Rossby modes in slowly rotating stars: depth dependence in distorted polytropes with uniform rotation

C. Damiani, R. H. Cameron, A. C. Birch +1

Large-scale Rossby waves have recently been discovered from measurements of horizontal surface and near-surface solar flows (Löptien at al. 2018). We are interested in understandin…

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