Citation notice #2234 · 2026-07-11 03:18:58.602254+00:00
Detector for fast wave trains in the solar radio emission
Correction
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cites 2021, Physical Review Letters, 126, 135101, doi: 10.1103/PhysRevLett.126.135101, which carries a correction notice dated 2021-03-30. One-hop deterministic notice: the citation edge exists in the Pith bibliography graph; no model judged whether the citation was load-bearing.
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01Evidence
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a rise in the number of non-thermal electrons accelerated during magnetic reconnection. The dynamics of the impulsive phase, once both the acceleration and emission mechanisms are properly taken into account, therefore, provides an estimation of the rate of energy release. But the acceleration process could be suppressed in the strong magnetic field [13]. Determining the spatial extent of the energy release region, remaining one of the principal parameters for estimating the solar flare energetics, is considerably more uncertain. In the microwave or HXR images one may estimate the flare source size by measuring the extent of the emission above the apex of flare-loop coronal arcades at the solar limb and limiting it with
02Event
- Type
- Correction
- Source
- Crossref
- Original DOI
- 10.1103/physrevlett.126.135101
- Notice DOI
- 10.1103/physrevlett.126.135101
- Date
- 2021-03-30
- Title
- Electron Acceleration during Macroscale Magnetic Reconnection
- Reasons
- ['Correction']
- Work
- 2021, Physical Review Letters, 126, 135101, doi: 10.1103/PhysRevLett.126.135101 (2021) Physical Review Letters
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