Результаты исследований: Научные публикации в периодических изданиях › Обзорная статья › Рецензирование
Jets Downstream of Collisionless Shocks. / Plaschke, Ferdinand; Hietala, Heli; Archer, Martin; Blanco-Cano, Xóchitl; Kajdič, Primož; Karlsson, Tomas; Lee, Sun Hee; Omidi, Nojan; Palmroth, Minna; Roytershteyn, Vadim; Schmid, Daniel; Sergeev, Victor; Sibeck, David.
в: Space Science Reviews, Том 214, № 5, 81, 01.08.2018.Результаты исследований: Научные публикации в периодических изданиях › Обзорная статья › Рецензирование
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TY - JOUR
T1 - Jets Downstream of Collisionless Shocks
AU - Plaschke, Ferdinand
AU - Hietala, Heli
AU - Archer, Martin
AU - Blanco-Cano, Xóchitl
AU - Kajdič, Primož
AU - Karlsson, Tomas
AU - Lee, Sun Hee
AU - Omidi, Nojan
AU - Palmroth, Minna
AU - Roytershteyn, Vadim
AU - Schmid, Daniel
AU - Sergeev, Victor
AU - Sibeck, David
PY - 2018/8/1
Y1 - 2018/8/1
N2 - The magnetosheath flow may take the form of large amplitude, yet spatially localized, transient increases in dynamic pressure, known as “magnetosheath jets” or “plasmoids” among other denominations. Here, we describe the present state of knowledge with respect to such jets, which are a very common phenomenon downstream of the quasi-parallel bow shock. We discuss their properties as determined by satellite observations (based on both case and statistical studies), their occurrence, their relation to solar wind and foreshock conditions, and their interaction with and impact on the magnetosphere. As carriers of plasma and corresponding momentum, energy, and magnetic flux, jets bear some similarities to bursty bulk flows, which they are compared to. Based on our knowledge of jets in the near Earth environment, we discuss the expectations for jets occurring in other planetary and astrophysical environments. We conclude with an outlook, in which a number of open questions are posed and future challenges in jet research are discussed.
AB - The magnetosheath flow may take the form of large amplitude, yet spatially localized, transient increases in dynamic pressure, known as “magnetosheath jets” or “plasmoids” among other denominations. Here, we describe the present state of knowledge with respect to such jets, which are a very common phenomenon downstream of the quasi-parallel bow shock. We discuss their properties as determined by satellite observations (based on both case and statistical studies), their occurrence, their relation to solar wind and foreshock conditions, and their interaction with and impact on the magnetosphere. As carriers of plasma and corresponding momentum, energy, and magnetic flux, jets bear some similarities to bursty bulk flows, which they are compared to. Based on our knowledge of jets in the near Earth environment, we discuss the expectations for jets occurring in other planetary and astrophysical environments. We conclude with an outlook, in which a number of open questions are posed and future challenges in jet research are discussed.
KW - Bow shock
KW - Foreshock
KW - Jets
KW - Magnetopause
KW - Magnetosheath
KW - CORONAL MASS EJECTIONS
KW - LOW-FREQUENCY WAVES
KW - HOT FLOW ANOMALIES
KW - UPSTREAM PRESSURE VARIATIONS
KW - HIGH-SPEED JETS
KW - QUASI-PARALLEL SHOCK
KW - INTERPLANETARY MAGNETIC-FIELD
KW - BURSTY BULK FLOWS
KW - CENTRAL PLASMA SHEET
KW - EARTHS BOW SHOCK
UR - http://www.scopus.com/inward/record.url?scp=85049122845&partnerID=8YFLogxK
U2 - 10.1007/s11214-018-0516-3
DO - 10.1007/s11214-018-0516-3
M3 - Review article
AN - SCOPUS:85049122845
VL - 214
JO - Space Science Reviews
JF - Space Science Reviews
SN - 0038-6308
IS - 5
M1 - 81
ER -
ID: 35372663