Konstantinos Tassis

Professor

Panepistemio Kretes

Greece

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Articles (10)

Extragalactic Magnetism with SOFIA (SALSA Legacy Program). V. First Results on the Magnetic Field Orientation of Galaxies

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Year:

2023

Extragalactic Magnetism with SOFIA (SALSA Legacy Program): The Magnetic Fields in the Multiphase Interstellar Medium of the Antennae Galaxies*

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Year:

2023

CO enhancement by magnetohydrodynamic waves

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Year:

2023

Analytic characterization of sub-Alfvénic turbulence energetics

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Year:

2023

GRB 210619B optical afterglow polarization

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Year:

2023

Starlight-polarization-based tomography of the magnetized ISM: PASIPHAE’s line-of-sight inversion method

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Year:

2023

Extragalactic Magnetism with SOFIA (SALSA Legacy Program). IV. Program Overview and First Results on the Polarization Fraction*

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Year:

2022

HI-H2 transition: Exploring the role of the magnetic field

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Year:

2022

Polarization power spectra and dust cloud morphology

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Year:

2022

Dancing with the stars: Stirring up extraordinary turbulence in Galactic center clouds

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Year:

2022

Collaborators (3)

Susan Clark

Assistant Professor

Stanford University

UNITED STATES

William Reach

Institute of Space Sciences

UNITED STATES

Georgia Virginia Panopoulou

Assistant Professor

Chalmers University of Technology

SWEDEN

Konstantinos Tassis

Research Interests

Explore related searches

Contact this professor

Articles (10)

Extragalactic Magnetism with SOFIA (SALSA Legacy Program). V. First Results on the Magnetic Field Orientation of Galaxies

Extragalactic Magnetism with SOFIA (SALSA Legacy Program): The Magnetic Fields in the Multiphase Interstellar Medium of the Antennae Galaxies*

CO enhancement by magnetohydrodynamic waves

Analytic characterization of sub-Alfvénic turbulence energetics

GRB 210619B optical afterglow polarization

Starlight-polarization-based tomography of the magnetized ISM: PASIPHAE’s line-of-sight inversion method

Extragalactic Magnetism with SOFIA (SALSA Legacy Program). IV. Program Overview and First Results on the Polarization Fraction*

HI-H2 transition: Exploring the role of the magnetic field

Polarization power spectra and dust cloud morphology

Dancing with the stars: Stirring up extraordinary turbulence in Galactic center clouds

Collaborators (3)

Susan Clark

William Reach

Georgia Virginia Panopoulou

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