The Solar Line Emission Dopplerometer project View Full Text


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Article Info

DATE

2021-10-20

AUTHORS

Jean-Marie Malherbe, Pierre Mein, Frédéric Sayède, Pawel Rudawy, Kenneth Phillips, Francis Keenan, Jan Rybák

ABSTRACT

Observations of the dynamics of solar coronal structures are necessary to investigate space weather phenomena and global heating of the corona. The profiles of high temperature lines emitted by the hot plasma are usually integrated by narrow band filters or recorded by classical spectroscopy. We present in this paper details of a new transportable instrument (under construction) for imaging spectroscopy: the Solar Line Emission Dopplerometer (SLED). It uses the Multi-channel Subtractive Double Pass (MSDP) technique, which combines the advantages of both filters and narrow slit spectrographs, i.e. high temporal, spatial and spectral resolutions. The SLED will measure at high cadence (1 Hz) the line-of-sight velocities (Doppler shifts) of hot coronal loops, in the forbidden lines of FeX 6374 Å and FeXIV 5303 Å. It will follow the dynamics of fast evolving events of solar activity such as flares or Coronal Mass Ejections (CMEs), and also study coronal heating by short period waves. Observations will be performed with the coronagraph at the Lomnický Štít Observatory (LSO, in Slovakia) or during total eclipses. The SLED will also observe the dynamics of solar prominences in Hα 6563 Å or He D3 5876 Å lines when mounted on the Białków coronagraph (near Wrocław, Poland). It is fully compatible with polarimetric measurements by various techniques. More... »

PAGES

83-101

References to SciGraph publications

  • 2010-11-02. Search for Rapid Changes in the Visible-Light Corona during the 21 June 2001 Total Solar Eclipse in SOLAR PHYSICS
  • 2019-04-23. A Search for High-Frequency Coronal Brightness Variations in the 21 August 2017 Total Solar Eclipse in SOLAR PHYSICS
  • 2011-12-15. Solar Flares: Magnetohydrodynamic Processes in LIVING REVIEWS IN SOLAR PHYSICS
  • 1977-09. Multi-Channel Subtractive spectrograph and filament observations in SOLAR PHYSICS
  • 2000-04. SECIS: The Solar Eclipse Coronal Eclipse Imaging System in SOLAR PHYSICS
  • 2003-04. Oscillations in the Coronal Green-Line Intensity Observed at Lominický Štít and Norikura Nearly Simultaneously. in SOLAR PHYSICS
  • 2006-03. On Solving the Coronal Heating Problem in SOLAR PHYSICS
  • 1982-03. Doppler shift measurements on the green coronal line—evidence for largescale macroscopic mass motion in JOURNAL OF ASTROPHYSICS AND ASTRONOMY
  • 2010-11-08. Coronal Loops: Observations and Modeling of Confined Plasma in LIVING REVIEWS IN SOLAR PHYSICS
  • 1970-04. Some observed characteristics of solar radar echoes and their implications in SOLAR PHYSICS
  • 2018-03-09. Optical design of visible emission line coronagraph on Indian space solar mission Aditya-L1 in EXPERIMENTAL ASTRONOMY
  • 2002-10-01. Spectroscopic Observation of Coronal Waves in SOLAR PHYSICS
  • 2008-01-11. An Instrument to Measure Coronal Emission Line Polarization in SOLAR PHYSICS
  • 1995-12. The Large Angle Spectroscopic Coronagraph (LASCO) in SOLAR PHYSICS
  • 2021-02-02. Four Decades of Advances from MSDP to S4I and SLED Imaging Spectrometers in SOLAR PHYSICS
  • Identifiers

    URI

    http://scigraph.springernature.com/pub.10.1007/s10686-021-09804-x

    DOI

    http://dx.doi.org/10.1007/s10686-021-09804-x

    DIMENSIONS

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