DE
Member Since 2014
Dr Enrico Landi Landi
University of Michigan Ann Arbor
AGU Research
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Simulations and Diagnostics of CME Charge State Evolution from the Transition Region through Heliosphere
UNDERSTANDING THE ORIGINS AND EVOLUTION OF LARGE-SCALE STRUCTURES IN THE HELIOSPHERE WITH OBSERVATIONS AND MODELING II POSTER
spa-solar and heliospheric physics | 13 december 2024
Elizabeth Wraback, Enrico Landi, Ward Manchester, ...
Charge states freeze-in low in the solar corona and carry information about the inner coronal properties through the heliosphere. In-situ measurements...
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Synthetic Spectroscopic Study of Minor Ions in the Near-Infrared and Visible Corona
SOLAR AND HELIOSPHERIC PHYSICS: GENERAL CONTRIBUTIONS III ORAL
spa-solar and heliospheric physics | 12 december 2024
Judit Szente, Enrico Landi, Bart van der Holst
To contribute to the effort of studying infrared and visible spectral emission and perform plasma diagnostics using observations at these wavelengths,...
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Is the Fe XIX Observed by EUNIS-2021 the 'Smoking Gun' of Nanoflares?
NEW INSIGHTS INTO CORONAL PHYSICS FROM EUV AND UV SPECTROSCOPY I ELIGHTNING
spa-solar and heliospheric physics | 11 december 2024
Adrian N. Daw, Enrico Landi, Douglas Rabin, Jeffre...
The Extreme Ultraviolet Normal Incidence Spectrograph (EUNIS) sounding rocket observed AR 12824 on 2021 May 18 in co-ordination with IRIS and Hinode, ...
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AWSoM Magnetohydrodynamic Simulation of a Solar Active Region: Statistical Analysis of Alfven Wave Dissipation and Reflection, Scaling Laws, and Energy Budget on Coronal Loops
NEW INSIGHTS INTO CORONAL PHYSICS FROM EUV AND UV SPECTROSCOPY II POSTER
spa-solar and heliospheric physics | 11 december 2024
Tong Shi, Ward Manchester, Enrico Landi, Bart van ...
The coronal heating problem has been a major challenge in solar physics. Here, we aim at answering how the physical processes behind the Alfvén w...
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Comparing the Radial Evolution of Slow and Alfvénic Slow Solar Wind with Parker Solar Probe and Solar Orbiter
PARKER SOLAR PROBE’S FURTHEST DESCENT INTO THE SUN’S CORONA I ORAL
spa-solar and heliospheric physics | 09 december 2024
Yeimy Rivera, Samuel T. Badman, Jaye Verniero, Ta...
Decades of remote and in situ observations find that solar wind streams originating from distinct coronal sources evolve differently during transit fr...
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Source region characterization of solar wind sampled during a spacecraft conjunction
TRACING THE BIRTH AND EVOLUTION OF THE SOLAR WIND BY CONNECTING SPACECRAFT CONJUNCTIONS AND REMOTE OBSERVATIONS II POSTER
12 april 2024
Yeimy Rivera, Samuel T. Badman, Enrico Landi, Tan...
With the growing number of solar probes across the inner heliosphere, our community, now more than ever, is well placed to continuously track the form...
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Calibrated Data from the Upgraded Coronal Multi-channel Polarimeter (UCoMP)
INSTRUMENTATION III POSTER
10 april 2024
Michael Galloy, Steven Tomczyk, Enrico Landi, Ben ...
NCAR/HAO has released calibrated data from the new Upgraded Coronal Multi-channel Polarimeter (UCoMP; Landi, Habbal and Tomczyk, 2016). The UCoMP is a...
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The Cartwheel CME’s Evolution in the Low Solar Corona Simulated with Non-Equilibrium Charge States and Spectra for Comparison to High-Resolution EUV Spectroscopic Observations
EARLY EVOLUTION AND CHARACTERISTICS OF HELIOSPHERIC LARGE-SCALE STRUCTURES I ORAL
09 april 2024
Elizabeth Wraback, Enrico Landi, Ward Manchester, ...
High-resolution EUV spectroscopy of the corona provides the most informative diagnostic tool for the early evolution of coronal mass ejections (CMEs) ...
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