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 …
The solar probe plus mission: humanity's first visit to our star
Abstract Solar Probe Plus (SPP) will be the first spacecraft to fly into the low solar corona.
SPP's main science goal is to determine the structure and dynamics of the Sun's coronal …
SPP's main science goal is to determine the structure and dynamics of the Sun's coronal …
Relating streamer flows to density and magnetic structures at the Parker solar probe
AP Rouillard, A Kouloumvakos… - The Astrophysical …, 2020 - iopscience.iop.org
The physical mechanisms that produce the slow solar wind are still highly debated. Parker
Solar Probe's (PSP's) second solar encounter provided a new opportunity to relate in situ …
Solar Probe's (PSP's) second solar encounter provided a new opportunity to relate in situ …
The solar probe cup on the Parker Solar Probe
Abstract Solar Probe Cup (SPC) is a Faraday cup instrument on board NASA's Parker Solar
Probe (PSP) spacecraft designed to make rapid measurements of thermal coronal and solar …
Probe (PSP) spacecraft designed to make rapid measurements of thermal coronal and solar …
The FIELDS instrument suite for Solar Probe Plus: measuring the coronal plasma and magnetic field, plasma waves and turbulence, and radio signatures of solar …
Abstract NASA's Solar Probe Plus (SPP) mission will make the first in situ measurements of
the solar corona and the birthplace of the solar wind. The FIELDS instrument suite on SPP …
the solar corona and the birthplace of the solar wind. The FIELDS instrument suite on SPP …
Prediction and Verification of Parker Solar Probe Solar Wind Sources at 13.3 R⊙
Drawing connections between heliospheric spacecraft and solar wind sources is a vital step
in understanding the evolution of the solar corona into the solar wind and contextualizing in …
in understanding the evolution of the solar corona into the solar wind and contextualizing in …
Understanding coronal heating and solar wind acceleration: Case for in situ near‐Sun measurements
DJ McComas, M Velli, WS Lewis… - Reviews of …, 2007 - Wiley Online Library
The solar wind has been measured directly from 0.3 AU outward, and the Sun's atmosphere
has been imaged from the photosphere out through the corona. These observations have …
has been imaged from the photosphere out through the corona. These observations have …
Solar wind electrons alphas and protons (SWEAP) investigation: Design of the solar wind and coronal plasma instrument suite for solar probe plus
JC Kasper, R Abiad, G Austin, M Balat-Pichelin… - Space Science …, 2016 - Springer
Abstract The Solar Wind Electrons Alphas and Protons (SWEAP) Investigation on Solar
Probe Plus is a four sensor instrument suite that provides complete measurements of the …
Probe Plus is a four sensor instrument suite that provides complete measurements of the …
The origins of hot plasma in the solar corona
The Sun's outer atmosphere, or corona, is heated to millions of degrees, considerably hotter
than its surface or photosphere. Explanations for this enigma typically invoke the deposition …
than its surface or photosphere. Explanations for this enigma typically invoke the deposition …
Solar sources of impulsive solar energetic particle events and their magnetic field connection to the Earth
This paper investigates the solar origin of impulsive solar energetic particle (SEP) events,
often referred to as 3 He-rich flares, by attempting to locate the source regions of 117 events …
often referred to as 3 He-rich flares, by attempting to locate the source regions of 117 events …