Skip to content
DraconiticResearch
Search Sources API
186,123 studies31 sourcesUpdated 50 min ago
Peer-reviewedCC BY 4.0The Astrophysical Journal Letters

Photospheric Kelvin–Helmholtz Vortices as Possible Drivers of Coronal Heating: Implications of the DKIST Observations

Related

  1. First Statistical Analysis of Photospheric Intensity Vortices with DKIST/VBI
    T. Rees-Crockford, E. Scullion, J. A. McLaughlin +1
    The Astrophysical JournalPeer-reviewedCC BY 4.0Full textSolar & stellar physicsIOP/AASCrossref
  2. DKIST unveils MHD-predicted sub-50 km photospheric vortices
    S. Vargas Dominguez, O. A. Calvo Rebellon, J. S. Castellanos Duran +4
    arXivPreprintCC BY 4.0Full textSolar & stellar physicsarXiv
  3. Kelvin-Helmholtz vortices in the Martian +E hemisphere downstream of crustal magnetic anomalies
    Junxi Niu, Tong Dang, Jiuhou Lei +6
    arXivPreprintCC BY 4.0Full textPlanetary science & exoplanetsSolar & stellar physicsarXiv
  4. Broken Power-law Distributions of Photospheric Magnetic Concentrations and Implications for Solar Dynamo
    Anchuan Song, Yuming Wang, Quanhao Zhang +2
    The Astrophysical JournalPeer-reviewedCC BY 4.0Full textSolar & stellar physicsCrossref
  5. The kinematic Kelvin-Helmholtz instability-driven dynamo: implications for merging compact objects
    James R. Beattie, Amitava Bhattacharjee, Elias R. Most +4
    arXivPreprintCC BY 4.0Full textGalaxiesHigh-energy astrophysicsarXiv
BibTeX
@article{nykyri2026photospheric,
  title = {{Photospheric Kelvin–Helmholtz Vortices as Possible Drivers of Coronal Heating: Implications of the DKIST Observations}},
  author = {Katariina Nykyri},
  journal = {The Astrophysical Journal Letters},
  year = {2026},
  month = nov,
  doi = {10.3847/2041-8213/aeb6c4},
  url = {https://iopscience.iop.org/article/10.3847/2041-8213/aeb6c4},
  note = {CC BY 4.0},
}
RIS
TY  - JOUR
TI  - Photospheric Kelvin–Helmholtz Vortices as Possible Drivers of Coronal Heating: Implications of the DKIST Observations
AU  - Katariina Nykyri
PY  - 2026
DA  - 2026/11/05
JO  - The Astrophysical Journal Letters
DO  - 10.3847/2041-8213/aeb6c4
UR  - https://iopscience.iop.org/article/10.3847/2041-8213/aeb6c4
SN  - 2041-8213
ER  -