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BASS2000 Instruments
This page gives a brief description of the instruments for which BASS2000 makes some data available, either in a systematic observation mode available in our Solar Survey Archive (mainly daily full disk data) or in a long term archive (Long Term Archive). The name of each instrument corresponds to its denomination in our data request forms. Please check the links for more informations on these instruments and their data.

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SPECTRA: The THEMIS-MTR instrument

This instrument allows multi-line spectro-polarimetric observations on the THEMIS telescope (MTR mode). Available wavelengths are currently in the range [430-870] nm and the polarimeter is optimized for 6250Å and 4250Å. A reduction software for these data will soon be available on our site. The observations cover a wide range of subjects, depending on the P.I. program.
THEMIS is a 90 cm telescope built in Tenerife providing 3 observing modes : the MTR mode, the MSDP mode (see below) and the IPM mode (imagery mode archived at Arthemis).

Data: Each channel contains a 2D image, with a variable wavelength across the field of view in one direction. Each channel is centered on a different wavelength across the line profile.

Availability: Starting in 1999 (Long Term Archive); Available one year after the observations (immediately after the observations for the P.I.s).

  • Links for more details:
  • Example of datas
  • The official THEMIS site
  • Our THEMIS page
  • A bibliography
  • Operated by: CNRS-CNR-IAC

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    MSDP: The THEMIS-MSDP instrument

    The Multichannel Subtractive Double Pass mode (MSDP) on THEMIS is a spectro-imager mode allowing a spectral analysis of broad lines (typically Halpha, Na D1 and Na D2) for a 2-D images (9x170 arcsec2 and 25x170 arcsec2). Reduction softwares are available on our site. The observations cover a wide range of subjects, depending on the P.I. program.
    THEMIS is a 90 cm telescope built in Tenerife providing 3 observing mode : the MTR mode (see above), the MSDP mode and the IPM mode (imagery mode archived at Arthemis).

    Data: Spectra for the different Stokes parameters (I+Stokes or I-Stokes, all Stokes parameters are recorded successively), usually for different wavelengths simultaneously (saved in different files). They usually consist of scans over a region (size: 1 or 2 arcminutes times the length of the scan) or of a repeated observation for a given position of the slit.

    Availability: Starting in 1999 (Long Term Archive); Available one year after the observations (immediately after the observations for the P.I.s).

  • Links for more details:
  • Example of datas
  • The official THEMIS site
  • Our MSDP page
  • Our THEMIS page
  • A bibliography
  • Operated by: CNRS-CNR-IAC

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    CORO: The Pic-du-Midi H-alpha coronograph

    The Pic du Midi Coronograph provides H-alpha images of the solar corona and is operated daily by amateur astronomers. The instrument consists of a refractor of diameter 150mm, a narrow-band H-alpha filter and an occulting disk.

    Data: Solar corona images (the disk is occulted) with a cadence of a few minutes

    Availability: Since October 1995. Selection of 1 to 3 representative images are available daily 1 hour after the observation at the Solar Survey Archive. The whole data series (cadence of a few minutes) will soon be available at the Long Term Archive.

  • Links for more details:
  • Example of datas
  • Les observateurs associés
  • A bibliography
  • Operated by: Observatoire Midi-Pyrénées / FIDUCIAL

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    NRH: The Nancay Radioheliograph

    The Nancay Radioheliograph provides 2-D images of the sun at 5 frequencies (between 150 and 450 Mhz) at a cadence of 8 images/second. The instrument consists in 2 linear antenna arrays in EW and NS directions (respectively 19 and 24 antennas), which provide 576 visibilities. The telescope is operated routinely.

    Data: Raw data consists of visibilities. Processed data are 2-D images of the solar radio brightness.

    Availability: Since July 1996, averaged data (128 seconds and 10 seconds) are available at the Solar Survey Archive, as well as summary images and mpeg films. The whole time series (raw data) is available (starting on April 17, 1999) at the Long Term Archive.

  • Links for more details:
  • Example of datas
  • The Nancay page
  • Description of the instrument
  • A bibliography
  • Operated by: Observatoire de Paris, CNRS, Région Centre

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    The Nancay Total Radio Flux Antenna

    This antenna provides daily total radio flux measurement of the sun at 10 frequencies (between 150 and 450 Mhz). The time resolution is 0.1 second.

    Data: Data consist in FITS file of calibrated data.

    Availability: Since January 2001.

  • Links for more details:
  • Example of datas
  • The Nancay page
  • Description of the instrument
  • A bibliography
  • Operated by: Observatoire de Paris, CNRS

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    The Meudon Spectroheliograph

    The spectroheliograph provides images of the solar photosphere (blue wing of the CaII K 3934 Å line, or K1v) and chromosphere (centre of the CaII K 3934 Å line, or K3 ; and H-alpha 6563 Å). Data are acquired once a day by performing scans of the solar disk using a entrance slit and an exit slit.

    Data: Full disk images of the sun at 3 wavelengths. When interesting, an additional image with a larger exposure time is available in K3 for protuberance studies. Synoptic maps for each solar rotation are made from these data.

    Availability: Since 1996. Daily digitized images are available for the period 1996-2001 (Solar Survey Archive) in fits and gif format. Images obtained with a CCD camera are available (since May 2002) for 5 wavelengths in each line. A project to digitize the whole time series (since 1919) is under development. Synoptic maps are also available since rotation 1824 (Dec 12, 1989) at the Solar Survey Archive.

  • Links for more details:
  • Example of datas
  • Pictures and description of the instrument
  • Data description
  • Pictures and history
  • A bibliography
  • for the synoptic maps

    Operated by: Observatoire de Paris-Meudon

    Documents:

    • Spectrohéliographe de Meudon (fr) PDF

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    The Meudon Heliograph

    The heliograph provides 3 images every 1.5 minute of the solar disk in the Halpha line at 3 wavelengths: line core and at 0.5Å from it on each side. A Lyot filter with a 0.5Å bandpass is used. The objective is to detect and observe solar eruptions at a high temporal cadence.

    Data: Full disk Halpha images are available at full resolution in fits format. Movies with half the spatial and temporal resolutions and light curves are made from these data.

    Availability: Since 1999. Mpeg movies are available on our (Solar Survey Archive) as well as light curves (in gif and postscript formats). Original fits images are available on request.

  • Links for more details:
  • Example of datas
  • Pictures and description of the instrument
  • Data description
  • Pictures and history
  • Operated by: Observatoire de Paris-Meudon

    Documents:

    • Héliographe de Meudon avant 2004 (fr) PDF
    • Héliographe CaII raie H 396.8 nm (fr) PDF
    • Héliographe CaII raie K 393.3 nm (fr) PDF
    • Héliographe continu vert 530 nm (fr) PDF
    • Héliographe bande G 430.7 nm (fr) PDF

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    Meudon White Light

    Data: FITS and JPEG white light images of the solar disk.

    Availability: Since 2003. Daily images are available (Solar Survey Archive).

  • Links for more details:
  • Pictures and description of the instrument
  • Operated by: Observatoire de Paris-Meudon

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    Meudon Solar Tower

    Operated by: Observatoire de Paris-Meudon

    Documents:

    • Banc de calibration polarimétrique (fr) PDF
    • Lunette Halpha 656.3 nm (fr) PDF
    • Lunette CaII raie K 393.3 nm (fr) PDF
    • Spectrographe à Double Passage Soustractif Multicanal (fr) PDF
    • Spectrographe classique en simple passage à fente fine (fr) PDF
    • Voie imagerie monochromatique (filtres) à petit champ (fr) PDF

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    The Coupole Tourelle of the Pic du Midi

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    NDA: Nancay Decameter Array

    Data: Spectra for frequencies from 20 to 75 MHz. Full data are available on request, preview images (GIF or PNG) are data integrated over 10 s, summing the two polarizations .(Solar Survey Archive)

    Availability:

  • Links for more details:
  • DAN homepage
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    CLIMSO: Christian Latouche IMageur SOlaire
  • Links for more details:
  • CLIMSO web site
  • Les observateurs associés
  • Operated by: Observatoire Midi-Pyrénées / FIDUCIAL

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    USET: The Uccle Solar Equatorial Table
  • Links for more details:
  • Web site
  • Technical data
  • Operated by: Royal Observatory of Belgium, Brussels

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    Last update: 01 Jun 2017 10:16