DE
Member Since 2014
Dr Enrico Landi Landi
University of Michigan Ann Arbor
AGU Research
Search
Filters
Clear All
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
Solar Polar Coronal Hole Spectroscopy with Corrected Abundances and Ion Temperatures
NEW INSIGHTS INTO CORONAL PHYSICS FROM EUV AND UV SPECTROSCOPY I POSTER
spa-solar and heliospheric physics | 13 december 2023
Judit Szente, Enrico Landi, Bart van der Holst
We show a detailed spectroscopic analysis of a coronal hole observation utilizing state-of-the-art 3D MHD modeling to decompose and understand the for...
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
The Cartwheel CME’s Early Evolution Simulated with Non-Equilibrium Charge States for Comparison to High-Resolution EUV Spectroscopic Observations
CONNECTING CORONAL MASS EJECTION INITIATION MECHANISMS TO THEIR OBSERVED PROPAGATION AND IMPACT III ORAL
spa-solar and heliospheric physics | 12 december 2023
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) ...
View Abstract
Spectroscopic observations of the corona in the visible and extreme ultraviolet during the 2017 August 21 total solar eclipse
SOLAR AND HELIOSPHERIC PHYSICS: GENERAL CONTRIBUTIONS II ORAL
spa-solar and heliospheric physics | 16 december 2022
YINGJIE ZHU, Shadia R. Habbal, Adalbert M. Ding, B...
Total solar eclipses are one of the best opportunities to study the elemental composition and plasma properties of the solar corona within 2- 3 Rs abo...
View Abstract
Interpreting the Effects of Non-Equilibrium Ionization on Remote Sensing and In-Situ Observations Using Synthetic Data
CONNECTING REMOTE AND IN SITU OBSERVATIONS TO UNDERSTAND THE DYNAMIC SOLAR WIND AND TRANSIENTS III ORAL
spa-solar and heliospheric physics | 16 december 2022
Judit Szente, Enrico Landi, Bart van der Holst, Ji...
The heavy ion charge states of the solar plasma carry information about the physical processes that occurred as plasma is released from the solar coro...
View Abstract
High-Resolution EUV Spectroscopy of CME Onset and Early Evolution
COORDINATED MULTI-SPACECRAFT OBSERVATIONS IN THE INNER HELIOSPHERE II POSTER
spa-solar and heliospheric physics | 14 december 2022
Elizabeth Wraback, Enrico Landi, Ward Manchester
Coronal mass ejection (CME) onset is a relatively unknown period during the CMEs evolution due to the difficulty of observing it. Coronagraphs block o...
View Abstract