Turnitin
降AI改写
早检测系统
早降重系统
Turnitin-UK版
万方检测-期刊版
维普编辑部版
Grammarly检测
Paperpass检测
checkpass检测
PaperYY检测
Parker solar probe: Four years of discoveries at solar cycle minimum
Abstract Launched on 12 Aug. 2018, NASA's Parker Solar Probe had completed 13 of its
scheduled 24 orbits around the Sun by Nov. 2022. The mission's primary science goal is to …
scheduled 24 orbits around the Sun by Nov. 2022. The mission's primary science goal is to …
Scaling laws for the energy transfer in space plasma turbulence
One characteristic trait of space plasmas is the multi-scale dynamics resulting from non-
linear transfers and conversions of various forms of energy. Routinely evidenced in a range …
linear transfers and conversions of various forms of energy. Routinely evidenced in a range …
Parker Solar Probe Enters the Magnetically Dominated Solar Corona
The high temperatures and strong magnetic fields of the solar corona form streams of solar
wind that expand through the Solar System into interstellar space. At 09: 33 UT on 28 April …
wind that expand through the Solar System into interstellar space. At 09: 33 UT on 28 April …
Magnetic reconnection as the driver of the solar wind
We present EUV solar observations showing evidence for omnipresent jetting activity driven
by small-scale magnetic reconnection at the base of the solar corona. We argue that the …
by small-scale magnetic reconnection at the base of the solar corona. We argue that the …
Interchange reconnection as the source of the fast solar wind within coronal holes
The fast solar wind that fills the heliosphere originates from deep within regions of open
magnetic field on the Sun called 'coronal holes'. The energy source responsible for …
magnetic field on the Sun called 'coronal holes'. The energy source responsible for …
Alfvénic velocity spikes and rotational flows in the near-Sun solar wind
The prediction of a supersonic solar wind was first confirmed by spacecraft near Earth, and
later by spacecraft at heliocentric distances as small as 62 solar radii. These missions …
later by spacecraft at heliocentric distances as small as 62 solar radii. These missions …
The evolution of the solar wind
How has the solar wind evolved to reach what it is today? In this review, I discuss the long-
term evolution of the solar wind, including the evolution of observed properties that are …
term evolution of the solar wind, including the evolution of observed properties that are …
Vacuum-ultraviolet photodetectors
L Jia, W Zheng, F Huang - PhotoniX, 2020 - Springer
High-performance vacuum-ultraviolet (VUV) photodetectors are of great significance to
space science, radiation monitoring, electronic industry and basic science. Due to the …
space science, radiation monitoring, electronic industry and basic science. Due to the …
In situ observations of large-amplitude Alfvén waves heating and accelerating the solar wind
After leaving the Sun's corona, the solar wind continues to accelerate and cools, but more
slowly than expected for a freely expanding adiabatic gas. Alfvén waves are perturbations of …
slowly than expected for a freely expanding adiabatic gas. Alfvén waves are perturbations of …
Switchbacks in the near-Sun magnetic field: long memory and impact on the turbulence cascade
One of the most striking observations made by Parker Solar Probe during its first solar
encounter is the omnipresence of rapid polarity reversals in a magnetic field that is …
encounter is the omnipresence of rapid polarity reversals in a magnetic field that is …