Welcome to the FMT data base at National University San Luis Gonzaga

The Flare Monitoring Telescope (FMT) is a powerful instrument that performs simultaneous observations of the solar disk at different wavelengths around the H-alpha absorption line (6562.8 A). The scientific objective of the FMT is to monitor continuously the solar flares and filament/prominence eruptions. This in order to improve our understanding of the relationship between these eruptive phenomena and the geo-effectiveness of the associated coronal mass ejections (CMEs), and ultimately the impact on the space-weather.
The FMT is also suitable for detecting large-scale disturbances in the solar chromosphere known as Moreton waves, as well as, for studying the long-term variation of UV radiation.
    Data Policy
    The FMT data is for education and research activities. At the moment the FMT data is not available online, if you would like to use our data please contact us to ciasest@unica.edu.pe

      Latest Images

H-alpha - 0.8A H-alpha + 0.0A H-alpha + 0.8A

Movie (2 min. cadence) Movie (2 min. cadence) Movie (2 min. cadence)
Movie (full frames)
Movie (full frames) Movie (full frames)

Prominence White Light

Movie (2 min. cadence) Movie (2 min. cadence)
Movie (full frames) Movie (full frames)

(Calibration procedures such as dark and flat-field correction are not used in these images)

      FMT Data Archive

    Annual and monthly observation (Coming soon...)

2015-Jan  2015-Feb  2015-Mar  2015-Apr  2015-May  2015-Jun
2015-Jul  2015-Aug  2015-Sep  2015-Oct  2015-Nov  2015-Dec

2014-Jan  2014-Feb  2014-Mar  2014-Apr  2014-May  2014-Jun
2014-Jul  2014-Aug  2014-Sep  2014-Oct  2014-Nov  2014-Dec

2013-Jan  2013-Feb  2013-Mar  2013-Apr  2013-May  2013-Jun
2013-Jul  2013-Aug  2013-Sep  2013-Oct  2013-Nov  2013-Dec

2012-Jan 2012-Feb  2012-Mar  2012-Apr  2012-May  2012-Jun
2012-Jul 2012-Aug  2012-Sep  2012-Oct  2012-Nov  2012-Dec

2011-Jan  2011-Feb  2011-Mar  2011-Apr  2011-May  2011-Jun
2011-Jul   2011-Aug  2011-Sep  2011-Oct  2011-Nov  2011-Dec

2010-Mar  2010-Apr  2010-May  2010-Jun
2010-Jul   2010-Aug  2010-Sep  2010-Oct  2010-Nov  2010-Dec

The CHAIN-project is sponsored and supported by the Astronomical Observatory of Kyoto University, Japan.

  CIASEST & FMT-team