D J Gershman
Overview
Explore the profile of D J Gershman including associated specialties, affiliations and a list of published articles.
Author names and details appear as published. Due to indexing inconsistencies, multiple individuals may share a name, and a single author may have variations. MedLuna displays this data as publicly available, without modification or verification
Snapshot
Snapshot
Articles
30
Citations
170
Followers
0
Related Specialties
Related Specialties
Top 10 Co-Authors
Top 10 Co-Authors
Published In
Affiliations
Affiliations
Soon will be listed here.
Recent Articles
11.
Khotyaintsev Y, Graham D, Steinvall K, Alm L, Vaivads A, Johlander A, et al.
Phys Rev Lett
. 2020 Feb;
124(4):045101.
PMID: 32058767
We report electrostatic Debye-scale turbulence developing within the diffusion region of asymmetric magnetopause reconnection with a moderate guide field using observations by the Magnetospheric Multiscale mission. We show that Buneman...
12.
Li W, Graham D, Khotyaintsev Y, Vaivads A, Andre M, Min K, et al.
Nat Commun
. 2020 Jan;
11(1):141.
PMID: 31919351
The Magnetospheric Multiscale (MMS) spacecraft encounter an electron diffusion region (EDR) of asymmetric magnetic reconnection at Earth's magnetopause. The EDR is characterized by agyrotropic electron velocity distributions on both sides...
13.
Hwang K, Choi E, Dokgo K, Burch J, Sibeck D, Giles B, et al.
Geophys Res Lett
. 2019 Oct;
46(12):6287-6296.
PMID: 31598018
While vorticity defined as the curl of the velocity has been broadly used in fluid and plasma physics, this quantity has been underutilized in space physics due to low time...
14.
Phan T, Eastwood J, Shay M, Drake J, Sonnerup B, Fujimoto M, et al.
Nature
. 2019 May;
569(7757):E9.
PMID: 31073227
Change history: In this Letter, the y-axis values in Fig. 3f should go from 4 to -8 (rather than from 4 to -4), the y-axis values in Fig. 3h should...
15.
Eastwood J, Mistry R, Phan T, Schwartz S, Ergun R, Drake J, et al.
Geophys Res Lett
. 2019 Apr;
45(10):4569-4577.
PMID: 31031447
Magnetospheric Multiscale observations are used to probe the structure and temperature profile of a guide field reconnection exhaust ~100 ion inertial lengths downstream from the X-line in the Earth's magnetosheath....
16.
Parashar T, Chasapis A, Bandyopadhyay R, Chhiber R, Matthaeus W, Maruca B, et al.
Phys Rev Lett
. 2019 Jan;
121(26):265101.
PMID: 30636132
We study spectral features of ion velocity and magnetic field correlations in the magnetosheath and in the solar wind using data from the Magnetospheric Multiscale (MMS) spacecraft. High-resolution MMS observations...
17.
Torbert R, Burch J, Phan T, Hesse M, Argall M, Shuster J, et al.
Science
. 2018 Nov;
362(6421):1391-1395.
PMID: 30442767
Magnetic reconnection is an energy conversion process that occurs in many astrophysical contexts including Earth's magnetosphere, where the process can be investigated in situ by spacecraft. On 11 July 2017,...
18.
Turner D, Wilson 3rd L, Liu T, Cohen I, Schwartz S, Osmane A, et al.
Nature
. 2018 Sep;
561(7722):206-210.
PMID: 30209369
Earth and its magnetosphere are immersed in the supersonic flow of the solar-wind plasma that fills interplanetary space. As the solar wind slows and deflects to flow around Earth, or...
19.
Kitamura N, Kitahara M, Shoji M, Miyoshi Y, Hasegawa H, Nakamura S, et al.
Science
. 2018 Sep;
361(6406):1000-1003.
PMID: 30190400
Particle acceleration by plasma waves and spontaneous wave generation are fundamental energy and momentum exchange processes in collisionless plasmas. Such wave-particle interactions occur ubiquitously in space. We present ultrafast measurements...
20.
Phan T, Eastwood J, Shay M, Drake J, Sonnerup B, Fujimoto M, et al.
Nature
. 2018 May;
557(7704):202-206.
PMID: 29743689
Magnetic reconnection in current sheets is a magnetic-to-particle energy conversion process that is fundamental to many space and laboratory plasma systems. In the standard model of reconnection, this process occurs...