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Measurement of Magnetic Cavitation Driven by Heat Flow in a Plasma

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Measurement of Magnetic Cavitation Driven by Heat Flow in a Plasma. / Arran, C.; Bradford, P.; Dearling, A. et al.
In: Physical review letters, Vol. 131, No. 1, 015101, 06.07.2023.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

Arran, C, Bradford, P, Dearling, A, Hicks, GS, Al-Atabi, S, Antonelli, L, Ettlinger, OC, Khan, M, Read, MP, Glize, K, Notley, M, Walsh, CA, Kingham, RJ, Najmudin, Z, Ridgers, CP & Woolsey, NC 2023, 'Measurement of Magnetic Cavitation Driven by Heat Flow in a Plasma', Physical review letters, vol. 131, no. 1, 015101. https://doi.org/10.1103/PhysRevLett.131.015101

APA

Arran, C., Bradford, P., Dearling, A., Hicks, G. S., Al-Atabi, S., Antonelli, L., Ettlinger, O. C., Khan, M., Read, M. P., Glize, K., Notley, M., Walsh, C. A., Kingham, R. J., Najmudin, Z., Ridgers, C. P., & Woolsey, N. C. (2023). Measurement of Magnetic Cavitation Driven by Heat Flow in a Plasma. Physical review letters, 131(1), Article 015101. https://doi.org/10.1103/PhysRevLett.131.015101

Vancouver

Arran C, Bradford P, Dearling A, Hicks GS, Al-Atabi S, Antonelli L et al. Measurement of Magnetic Cavitation Driven by Heat Flow in a Plasma. Physical review letters. 2023 Jul 6;131(1):015101. doi: 10.1103/PhysRevLett.131.015101

Author

Arran, C. ; Bradford, P. ; Dearling, A. et al. / Measurement of Magnetic Cavitation Driven by Heat Flow in a Plasma. In: Physical review letters. 2023 ; Vol. 131, No. 1.

Bibtex

@article{52b9d1fce40944a289c87c009983ec94,
title = "Measurement of Magnetic Cavitation Driven by Heat Flow in a Plasma",
abstract = "We describe the direct measurement of the expulsion of a magnetic field from a plasma driven by heat flow. Using a laser to heat a column of gas within an applied magnetic field, we isolate Nernst advection and show how it changes the field over a nanosecond timescale. Reconstruction of the magnetic field map from proton radiographs demonstrates that the field is advected by heat flow in advance of the plasma expansion with a velocity vN=(6±2)×105 m/s. Kinetic and extended magnetohydrodynamic simulations agree well in this regime due to the buildup of a magnetic transport barrier.",
author = "C. Arran and P. Bradford and A. Dearling and Hicks, {G. S.} and S. Al-Atabi and L. Antonelli and Ettlinger, {O. C.} and M. Khan and Read, {M. P.} and K. Glize and M. Notley and Walsh, {C. A.} and Kingham, {R. J.} and Z. Najmudin and Ridgers, {C. P.} and Woolsey, {N. C.}",
year = "2023",
month = jul,
day = "6",
doi = "10.1103/PhysRevLett.131.015101",
language = "English",
volume = "131",
journal = "Physical review letters",
issn = "0031-9007",
publisher = "American Physical Society",
number = "1",

}

RIS

TY - JOUR

T1 - Measurement of Magnetic Cavitation Driven by Heat Flow in a Plasma

AU - Arran, C.

AU - Bradford, P.

AU - Dearling, A.

AU - Hicks, G. S.

AU - Al-Atabi, S.

AU - Antonelli, L.

AU - Ettlinger, O. C.

AU - Khan, M.

AU - Read, M. P.

AU - Glize, K.

AU - Notley, M.

AU - Walsh, C. A.

AU - Kingham, R. J.

AU - Najmudin, Z.

AU - Ridgers, C. P.

AU - Woolsey, N. C.

PY - 2023/7/6

Y1 - 2023/7/6

N2 - We describe the direct measurement of the expulsion of a magnetic field from a plasma driven by heat flow. Using a laser to heat a column of gas within an applied magnetic field, we isolate Nernst advection and show how it changes the field over a nanosecond timescale. Reconstruction of the magnetic field map from proton radiographs demonstrates that the field is advected by heat flow in advance of the plasma expansion with a velocity vN=(6±2)×105 m/s. Kinetic and extended magnetohydrodynamic simulations agree well in this regime due to the buildup of a magnetic transport barrier.

AB - We describe the direct measurement of the expulsion of a magnetic field from a plasma driven by heat flow. Using a laser to heat a column of gas within an applied magnetic field, we isolate Nernst advection and show how it changes the field over a nanosecond timescale. Reconstruction of the magnetic field map from proton radiographs demonstrates that the field is advected by heat flow in advance of the plasma expansion with a velocity vN=(6±2)×105 m/s. Kinetic and extended magnetohydrodynamic simulations agree well in this regime due to the buildup of a magnetic transport barrier.

U2 - 10.1103/PhysRevLett.131.015101

DO - 10.1103/PhysRevLett.131.015101

M3 - Journal article

C2 - 37478421

AN - SCOPUS:85164616609

VL - 131

JO - Physical review letters

JF - Physical review letters

SN - 0031-9007

IS - 1

M1 - 015101

ER -