X-ray emission from comets and nonmagnetic planets. Theory and comparison with CHANDRA observations

V. D. Shapiro, R. Bingham, B. J. Kellett, K. Quest, D. A. Mendis, P. Bryans, M. Torney, H. P. Summers

Research output: Contribution to journalArticle

3 Citations (Scopus)

Abstract

Mass loading of the solar wind by newly created cometary photoions as well as counterstreaming fluxes of protons in the mantle regions (at the ionospheric boundaries) of nonmagnetic planets (Mars, Venus) result in the modified two stream instability (MTSI) and excitation of the intense lower hybrid wave turbulence. Electrons are efficiently energized by these waves in the magnetic field aligned direction up to KeV energies (confirmed by in situ observations) and interacting with cometary or planetary atmospheres producing X-Ray emission by combination of Bremsstrahlung and line K-shell radiation. Analytical study of the nonlinear evolution of MTSI as well as numerical simulations of instability development in the mantle regions of nonmagnetic planets has been performed and it basically confirms the scenario of electron acceleration. Using the above described mechanism of X-ray emission produced in impacts of energetic electrons with ions and neutrals we employed ADAS-atomic data code to analyze X-ray spectrum emitted by comet Linear and obtained a good fit with recent CHANDRA observations. The theoretical model also predicts strong X-ray emission from nonmagnetic planets such as Mars and Venus.
Original languageEnglish
Pages (from-to)83-87
Number of pages5
JournalPhysica Scripta
VolumeT116
DOIs
Publication statusPublished - 2005
EventInternational Workshop on Theoretical Plasma Physics: Modern Plasma Science - Abdus Salam ICTP, Trieste, Italy
Duration: 5 Jul 200416 Jul 2004

Fingerprint

comets
planets
Mars
Venus (planet)
Electron
Earth mantle
x rays
cometary atmospheres
Mars (planet)
planetary atmospheres
electron acceleration
bremsstrahlung
mars
Theoretical Model
ionospherics
solar wind
Atmosphere
Turbulence
Shell
electrons

Keywords

  • atmospheres
  • solar wind plasma
  • radiation
  • spectra
  • cometary photoions
  • X-ray

Cite this

Shapiro, V. D. ; Bingham, R. ; Kellett, B. J. ; Quest, K. ; Mendis, D. A. ; Bryans, P. ; Torney, M. ; Summers, H. P. / X-ray emission from comets and nonmagnetic planets. Theory and comparison with CHANDRA observations. In: Physica Scripta. 2005 ; Vol. T116. pp. 83-87.
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abstract = "Mass loading of the solar wind by newly created cometary photoions as well as counterstreaming fluxes of protons in the mantle regions (at the ionospheric boundaries) of nonmagnetic planets (Mars, Venus) result in the modified two stream instability (MTSI) and excitation of the intense lower hybrid wave turbulence. Electrons are efficiently energized by these waves in the magnetic field aligned direction up to KeV energies (confirmed by in situ observations) and interacting with cometary or planetary atmospheres producing X-Ray emission by combination of Bremsstrahlung and line K-shell radiation. Analytical study of the nonlinear evolution of MTSI as well as numerical simulations of instability development in the mantle regions of nonmagnetic planets has been performed and it basically confirms the scenario of electron acceleration. Using the above described mechanism of X-ray emission produced in impacts of energetic electrons with ions and neutrals we employed ADAS-atomic data code to analyze X-ray spectrum emitted by comet Linear and obtained a good fit with recent CHANDRA observations. The theoretical model also predicts strong X-ray emission from nonmagnetic planets such as Mars and Venus.",
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X-ray emission from comets and nonmagnetic planets. Theory and comparison with CHANDRA observations. / Shapiro, V. D.; Bingham, R.; Kellett, B. J.; Quest, K.; Mendis, D. A.; Bryans, P.; Torney, M.; Summers, H. P.

In: Physica Scripta, Vol. T116, 2005, p. 83-87.

Research output: Contribution to journalArticle

TY - JOUR

T1 - X-ray emission from comets and nonmagnetic planets. Theory and comparison with CHANDRA observations

AU - Shapiro, V. D.

AU - Bingham, R.

AU - Kellett, B. J.

AU - Quest, K.

AU - Mendis, D. A.

AU - Bryans, P.

AU - Torney, M.

AU - Summers, H. P.

PY - 2005

Y1 - 2005

N2 - Mass loading of the solar wind by newly created cometary photoions as well as counterstreaming fluxes of protons in the mantle regions (at the ionospheric boundaries) of nonmagnetic planets (Mars, Venus) result in the modified two stream instability (MTSI) and excitation of the intense lower hybrid wave turbulence. Electrons are efficiently energized by these waves in the magnetic field aligned direction up to KeV energies (confirmed by in situ observations) and interacting with cometary or planetary atmospheres producing X-Ray emission by combination of Bremsstrahlung and line K-shell radiation. Analytical study of the nonlinear evolution of MTSI as well as numerical simulations of instability development in the mantle regions of nonmagnetic planets has been performed and it basically confirms the scenario of electron acceleration. Using the above described mechanism of X-ray emission produced in impacts of energetic electrons with ions and neutrals we employed ADAS-atomic data code to analyze X-ray spectrum emitted by comet Linear and obtained a good fit with recent CHANDRA observations. The theoretical model also predicts strong X-ray emission from nonmagnetic planets such as Mars and Venus.

AB - Mass loading of the solar wind by newly created cometary photoions as well as counterstreaming fluxes of protons in the mantle regions (at the ionospheric boundaries) of nonmagnetic planets (Mars, Venus) result in the modified two stream instability (MTSI) and excitation of the intense lower hybrid wave turbulence. Electrons are efficiently energized by these waves in the magnetic field aligned direction up to KeV energies (confirmed by in situ observations) and interacting with cometary or planetary atmospheres producing X-Ray emission by combination of Bremsstrahlung and line K-shell radiation. Analytical study of the nonlinear evolution of MTSI as well as numerical simulations of instability development in the mantle regions of nonmagnetic planets has been performed and it basically confirms the scenario of electron acceleration. Using the above described mechanism of X-ray emission produced in impacts of energetic electrons with ions and neutrals we employed ADAS-atomic data code to analyze X-ray spectrum emitted by comet Linear and obtained a good fit with recent CHANDRA observations. The theoretical model also predicts strong X-ray emission from nonmagnetic planets such as Mars and Venus.

KW - atmospheres

KW - solar wind plasma

KW - radiation

KW - spectra

KW - cometary photoions

KW - X-ray

U2 - 10.1238/Physica.Topical.116a00083

DO - 10.1238/Physica.Topical.116a00083

M3 - Article

VL - T116

SP - 83

EP - 87

JO - Physica Scripta

JF - Physica Scripta

SN - 0031-8949

ER -