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Sökning: WFRF:(Lindqvist A) > Lindqvist P. A

  • Resultat 1-9 av 9
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1.
  • Pedersen, A., Decreau, P., Escoubet, C.P., Gustafsson, G., Laakso, H., Lindqvist, P.-A. , Lybekk, B., Masson, A., Mozer, F. and Vaivads, A. (författare)
  • Four-point high time resolution information on electron densities by the electric field experiments (EFW) on Cluster.
  • 2001
  • Ingår i: Annales Geophysicae. ; 19:6, s. 1483-1489
  • Tidskriftsartikel (refereegranskat)abstract
    • For accurate measurements of electric fields spherical double probes are electronically controlled to be at a positive potential of approximately 1 volt relative to the ambient magnetospheric plasma. The spacecraft will acquire a potential which balance
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2.
  • Andre, M., Behlke, R., Wahlund, J.E., Vaivads, A., Eriksson, A., Tjulin, A., Carozzi, T. D., Cully, C., Gustafsson, G., Sundkvist, D., Khotyaintsev, Y., Cornilleau-Wehrlin, N., Rezeau, L., Maksimovic, M., Lucek, E., Balogh, A., Dunlop, M., Lindqvist, P.A. (författare)
  • Multi-spacecraft observations of broadband waves near the lower hybrid frequency at the Earthward edge of the magnetopause.
  • 2001
  • Ingår i: Annales Geophysicae. ; 19:6, s. 1471-1481
  • Tidskriftsartikel (refereegranskat)abstract
    • Broadband waves around the lower hybrid frequency (around 10 Hz) near the magnetopause are studied, using the four Cluster satellites. These waves are common at the Earthward edge of the boundary layer, consistent with earlier observations, and can have a
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3.
  • Marklund, G.T., Ivchenko, N., Karlsson, T., Fazakerley, A., Dunlop, M., Lindqvist, P.A., Buchert, S., Owen, C., Taylor, M., Vaivalds, A., Carter, P., Andre, M. and Balogh, A. (författare)
  • Temporal evolution of the electric field accelerating electrons away from the auroral ionosphere.
  • 2001
  • Ingår i: Nature. ; 414:6865, s. 724-727
  • Tidskriftsartikel (refereegranskat)abstract
    • The bright night-time aurorae that are visible to the unaided eye are caused by electrons accelerated towards Earth by an upward-pointing electric field(1-3). On adjacent geomagnetic field lines the reverse process occurs: a downward-pointing electric fie
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4.
  • Pedersen, A., et al. (författare)
  • Electron density estimations derived from spacecraft potential measurements on Cluster in tenuous plasma regions
  • 2008
  • Ingår i: Journal of Geophysical Research. - 0148-0227 .- 2156-2202. ; 113:A7, s. A07S33-
  • Tidskriftsartikel (refereegranskat)abstract
    • Spacecraft potential measurements by the EFW electric field experiment on the Cluster satellites can be used to obtain plasma density estimates in regions barely accessible to other type of plasma experiments. Direct calibrations of the plasma density as a function of the measured potential difference between the spacecraft and the probes can be carried out in the solar wind, the magnetosheath, and the plasmashere by the use of CIS ion density and WHISPER electron density measurements. The spacecraft photoelectron characteristic ( photoelectrons escaping to the plasma in current balance with collected ambient electrons) can be calculated from knowledge of the electron current to the spacecraft based on plasma density and electron temperature data from the above mentioned experiments and can be extended to more positive spacecraft potentials by CIS ion and the PEACE electron experiments in the plasma sheet. This characteristic enables determination of the electron density as a function of spacecraft potential over the polar caps and in the lobes of the magnetosphere, regions where other experiments on Cluster have intrinsic limitations. Data from 2001 to 2006 reveal that the photoelectron characteristics of the Cluster spacecraft as well as the electric field probes vary with the solar cycle and solar activity. The consequences for plasma density measurements are addressed. Typical examples are presented to demonstrate the use of this technique in a polar cap/lobe plasma.
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7.
  • Laakso, H., Grard, R., Masson, A., Moullard, O., Bale, S., Mozer, F., Pedersen, A., Andre, M., Eriksson, A., Gustaffson, G. and Lindqvist, P.-A. (författare)
  • Multi-point electric field observations in the high-latitude magnetosphere
  • 2001
  • Ingår i: Les Woolliscroft Memorial Conference Sheffield Space Plasma Meeting: Multipoint Measurements versus Theory. Proceedings (SP-492) (2001) ESA SP-492. - : Noordwijk, Netherlands. ; , s. 27-
  • Konferensbidrag (övrigt vetenskapligt/konstnärligt)abstract
    • The authors use multi-point electric field observations from the four Cluster satellites to study the dynamical behavior of the high-latitude magnetosphere on February 13-14, 2001, 20-02 UT. At 20:00 UT the vehicles enter the cusp where three satellites o
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8.
  • Li, Wenya Y., et al. (författare)
  • Cold Ionospheric Ions in the Magnetic Reconnection Outflow Region
  • 2017
  • Ingår i: Journal of Geophysical Research - Space Physics. - : Blackwell Publishing. - 2169-9380 .- 2169-9402. ; 122:10, s. 10,194-10,202
  • Tidskriftsartikel (refereegranskat)abstract
    • Magnetosheath plasma usually determines properties of asymmetric magnetic reconnection at the subsolar region of Earth's magnetopause. However, cold plasma that originated from the ionosphere can also reach the magnetopause and modify the kinetic physics of asymmetric reconnection. We present a magnetopause crossing with high-density (10–60 cm−3) cold ions and ongoing reconnection from the observation of the Magnetospheric Multiscale (MMS) spacecraft. The magnetopause crossing is estimated to be 300 ion inertial lengths south of the X line. Two distinct ion populations are observed on the magnetosheath edge of the ion jet. One population with high parallel velocities (200–300 km/s) is identified to be cold ion beams, and the other population is the magnetosheath ions. In the deHoffman-Teller frame, the field-aligned magnetosheath ions are Alfvénic and move toward the jet region, while the field-aligned cold ion beams move toward the magnetosheath boundary layer, with much lower speeds. These cold ion beams are suggested to be from the cold ions entering the jet close to the X line. This is the first observation of the cold ionospheric ions in the reconnection outflow region, including the reconnection jet and the magnetosheath boundary layer. 
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  • Resultat 1-9 av 9

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