Energy estimation of small-scale jets from the quiet-Sun region
arXiv:2403.16193 · doi:10.1051/0004-6361/202449377
Abstract
Context. Solar jets play a role in the coronal heating and the supply of solar wind. Aims. This study calculated the energies of 23 small-scale jets emerging from a quiet-Sun region to investigate their contributions for coronal heating. Conclusions. Our observations suggest that although these jets cannot provide sufficient energy for the heating of the whole quiet-Sun coronal region, they are likely to account for a significant portion of the energy demand in the local regions where the jets occur.
References in corpus (23)
- The Solar Orbiter mission -- Science overview
- Chromospheric Anemone Jets as Evidence of Ubiquitous Reconnection
- Solar Coronal Jets: Observations, Theory, and Modeling
- Small-scale filament eruptions as the driver of solar coronal hole X-ray jets
- Prevalence of Small-scale Jets from the Networks of the Solar Transition Region and Chromosphere
- Thermal Diagnostics with the Atmospheric Imaging Assembly onboard the Solar Dynamics Observatory: A Validated Method for Differential Emission Measure Inversions
- Generation of Solar Spicules and Subsequent Atmospheric Heating
- Magnetic Flux Cancellation as the Trigger of Solar Quiet-Region Coronal Jets
- Magnetic Reconnection as the Driver of the Solar Wind
- Transient small-scale brightenings in the quiet solar corona: a model for campfires observed with Solar Orbiter
- Blobs in recurring EUV jets
- Picoflare jets power the solar wind emerging from a coronal hole on the Sun
- Fine-scale explosive energy release at sites of prospective magnetic flux cancellation in the core of the solar active region observed by Hi-C 2.1, IRIS and SDO
- Quasiperiodic Energy Release and Jets at the Base of Solar Coronal Plumes
- Hi-C 2.1 Observations of Jetlet-like Events at Edges of Solar Magnetic Network Lane
- Ultra-high-resolution Observations of Persistent Null-point Reconnection in the Solar Corona
- Extreme-ultraviolet bursts and nanoflares in the quiet-Sun transition region and corona
- Coronal microjets in quiet-Sun regions observed with the Extreme Ultraviolet Imager onboard Solar Orbiter
- Nanoflare distributions over solar cycle 24 based on SDO/AIA differential emission measure observations
- Capturing transient plasma flows and jets in the solar corona
- Multi-stage reconnection powering a solar coronal jet
- Moving structures in ultraviolet bright points: observations from Solar Orbiter/EUI
- Quasi-periodic microjets driven by granular advection as observed with high-resolution imaging at He I 10830 Å