BibTex format
@article{Raouafi:2023:10.1007/s11214-023-00952-4,
author = {Raouafi, NE and Matteini, L and Squire, J and Badman, ST and Velli, M and Klein, KG and Chen, CHK and Matthaeus, WH and Szabo, A and Linton, M and Allen, RC and Szalay, JR and Bruno, R and Decker, RB and Akhavan-Tafti, M and Agapitov, OV and Bale, SD and Bandyopadhyay, R and Battams, K and Beri, L and Bourouaine, S and Bowen, T and Cattell, C and Chandran, BDG and Chhiber, R and Cohen, CMS and D'Amicis, R and Giacalone, J and Hess, P and Howard, RA and Horbury, TS and Jagarlamudi, VK and Joyce, CJ and Kasper, JC and Kinnison, J and Laker, R and Liewer, P and Malaspina, DM and Mann, I and McComas, DJ and Niembro-Hernandez, T and Panasenco, O and Pokorný, P and Pusack, A and Pulupa, M and Perez, JC and Riley, P and Rouillard, AP and Shi, C and Stenborg, G and Tenerani, A and Verniero, JL and Viall, N and Vourlidas, A and Wood, BE and Woodham, LD and Woolley, T},
doi = {10.1007/s11214-023-00952-4},
journal = {Space Science Reviews},
pages = {1--140},
title = {Parker solar probe: four years of discoveries at solar cycle minimum},
url = {http://dx.doi.org/10.1007/s11214-023-00952-4},
volume = {219},
year = {2023}
}
RIS format (EndNote, RefMan)
TY - JOUR
AB - 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 determine the structure and dynamics of the Sun’s coronal magnetic field, understand how the solar corona and wind are heated and accelerated, and determine what processes accelerate energetic particles. Parker Solar Probe returned a treasure trove of science data that far exceeded quality, significance, and quantity expectations, leading to a significant number of discoveries reported in nearly 700 peer-reviewed publications. The first four years of the 7-year primary mission duration have been mostly during solar minimum conditions with few major solar events. Starting with orbit 8 (i.e., 28 Apr. 2021), Parker flew through the magnetically dominated corona, i.e., sub-Alfvénic solar wind, which is one of the mission’s primary objectives. In this paper, we present an overview of the scientific advances made mainly during the first four years of the Parker Solar Probe mission, which go well beyond the three science objectives that are: (1) Trace the flow of energy that heats and accelerates the solar corona and solar wind; (2) Determine the structure and dynamics of the plasma and magnetic fields at the sources of the solar wind; and (3) Explore mechanisms that accelerate and transport energetic particles.
AU - Raouafi,NE
AU - Matteini,L
AU - Squire,J
AU - Badman,ST
AU - Velli,M
AU - Klein,KG
AU - Chen,CHK
AU - Matthaeus,WH
AU - Szabo,A
AU - Linton,M
AU - Allen,RC
AU - Szalay,JR
AU - Bruno,R
AU - Decker,RB
AU - Akhavan-Tafti,M
AU - Agapitov,OV
AU - Bale,SD
AU - Bandyopadhyay,R
AU - Battams,K
AU - Beri,L
AU - Bourouaine,S
AU - Bowen,T
AU - Cattell,C
AU - Chandran,BDG
AU - Chhiber,R
AU - Cohen,CMS
AU - D'Amicis,R
AU - Giacalone,J
AU - Hess,P
AU - Howard,RA
AU - Horbury,TS
AU - Jagarlamudi,VK
AU - Joyce,CJ
AU - Kasper,JC
AU - Kinnison,J
AU - Laker,R
AU - Liewer,P
AU - Malaspina,DM
AU - Mann,I
AU - McComas,DJ
AU - Niembro-Hernandez,T
AU - Panasenco,O
AU - Pokorný,P
AU - Pusack,A
AU - Pulupa,M
AU - Perez,JC
AU - Riley,P
AU - Rouillard,AP
AU - Shi,C
AU - Stenborg,G
AU - Tenerani,A
AU - Verniero,JL
AU - Viall,N
AU - Vourlidas,A
AU - Wood,BE
AU - Woodham,LD
AU - Woolley,T
DO - 10.1007/s11214-023-00952-4
EP - 140
PY - 2023///
SN - 0038-6308
SP - 1
TI - Parker solar probe: four years of discoveries at solar cycle minimum
T2 - Space Science Reviews
UR - http://dx.doi.org/10.1007/s11214-023-00952-4
UR - https://link.springer.com/article/10.1007/s11214-023-00952-4
UR - http://hdl.handle.net/10044/1/102084
VL - 219
ER -