DE
Member Since 2014
Dr Enrico Landi Landi
University of Michigan Ann Arbor
AGU Research
Search
Filters
Clear All
Simulations and Diagnostics of CME Charge State Evolution from the Transition Region through Heliosphere
AGU 2024
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...
View Abstract
Synthetic Spectroscopic Study of Minor Ions in the Near-Infrared and Visible Corona
AGU 2024
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,...
View Abstract
AWSoM Magnetohydrodynamic Simulation of a Solar Active Region: Statistical Analysis of Alfven Wave Dissipation and Reflection, Scaling Laws, and Energy Budget on Coronal Loops
AGU 2024
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...
View Abstract
Is the Fe XIX Observed by EUNIS-2021 the 'Smoking Gun' of Nanoflares?
AGU 2024
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, ...
View Abstract
Comparing the Radial Evolution of Slow and Alfvénic Slow Solar Wind with Parker Solar Probe and Solar Orbiter
AGU 2024
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...
View Abstract
Using the Cartwheel CME to Predict EUV Observations of CME Cores for SPICE and EUVST
NEW INSIGHTS INTO CORONAL PHYSICS FROM EUV AND UV SPECTROSCOPY II ORAL
spa-solar and heliospheric physics | 15 december 2023
Elizabeth Wraback, Enrico Landi, Ward Manchester
The early evolution of coronal mass ejections (CME) is a relatively unknown period due to the difficulty of observing it. On-disk observations from EU...
View Abstract
Nonthermal Velocities in a Quiescent Solar Active Region Observed by EUNIS and EIS
NEW INSIGHTS INTO CORONAL PHYSICS FROM EUV AND UV SPECTROSCOPY I POSTER
spa-solar and heliospheric physics | 13 december 2023
Jeffrey W. Brosius, Adrian N. Daw, Douglas Rabin, ...
We present measurements of nonthermal Doppler velocities in quiescent solar active region NOAA 12824 observed simultaneously by the Extreme Ultraviole...
View Abstract
Heating of Heavy Ions in Active Regions Observed by SUMER: Flares, Loop brightening, and Coronal Rain
NEW INSIGHTS INTO CORONAL PHYSICS FROM EUV AND UV SPECTROSCOPY I POSTER
spa-solar and heliospheric physics | 13 december 2023
YINGJIE ZHU, Enrico Landi
Active regions (ARs) are the most dynamic structures in the solar corona, driven by intense magnetic activity that triggers a variety of eruptive and ...
View Abstract