Astrophysical: Solar corona

  • Talk
    Helium Emissions as a Probe for Plasma Temperatures.

    The strongest He II emission in the visible spectral range, at 4686 A, is for the first time observed at a spectral resolution sufficiently high for a line...

  • Talk
    Morphological And Thermal Properties Of The Solar Corona : Diagnostic Tools & Applications

    Progress in our understanding of the Solar corona and its underlying heating and acceleration processes, depends critically on our ability to measure...

  • Publication
    A 2D Model for Coronal Bright Points: Association with Spicules, UV Bursts, Surges, and EUV Coronal Jets

    Coronal bright points (CBPs) are ubiquitous structures in the solar atmosphere composed of hot small-scale loops observed in extreme-ultraviolet (EUV) or X-rays...

  • Publication
    A summary of solar 1-8A measurements from the SMS and GOES satellites, 1977-1981

    The 1-8A band of synodic full-disc solar X-rays (1-8A) W/m(2) were measured nearly continuously from 1975 to 1981 aboard the SMS-1, SMS-2, GOES-1, GOES-2, and...

  • Publication
    Accelerating Non-LTE Synthesis and Inversions with Graph Networks

    The computational cost of fast non-LTE synthesis is one of the challenges that limits the development of 2D and 3D inversion codes. It also makes the...

  • Publication
    An example of the cancellation of magnetic fields during the decay of an active region

    A case of cancellation of magnetic fields is observed during the decay of a small active region. Three different sources of information were simultaneously used...

  • Publication
    Deciphering Solar Coronal Heating: Energizing Small-scale Loops through Surface Convection

    The solar atmosphere is filled with clusters of hot small-scale loops commonly known as coronal bright points (CBPs). These ubiquitous structures stand out in...

  • Publication
    Fast-to-Alfvén Mode Conversion and Ambipolar Heating in Structured Media. II. Numerical Simulation

    This paper studies the effectiveness of production of Alfvén waves in the solar atmosphere through the processes of mode conversion, taking into account several...

  • Publication
    First Metis Detection of the Helium D<SUB>3</SUB> Line Polarization in a Large Eruptive Prominence

    Metis on board Solar Orbiter is the space coronagraph developed by an Italian-German-Czech consortium. It is capable of observing solar corona and various...