Coronal loops: observations and modeling of confined plasma
F Reale - Living Reviews in Solar Physics, 2014 - Springer
Coronal loops are the building blocks of the X-ray bright solar corona. They owe their
brightness to the dense confined plasma, and this review focuses on loops mostly as …
brightness to the dense confined plasma, and this review focuses on loops mostly as …
The solar extreme ultraviolet monitor for MAVEN
Abstract The Extreme Ultraviolet (EUV) monitor is an instrument on the NASA Mars
Atmosphere and Volatile EvolutioN (MAVEN) mission, designed to measure the variability of …
Atmosphere and Volatile EvolutioN (MAVEN) mission, designed to measure the variability of …
The Helioseismic and Magnetic Imager (HMI) Investigation for the Solar Dynamics Observatory (SDO)
Abstract The Helioseismic and Magnetic Imager (HMI) instrument and investigation as a part
of the NASA Solar Dynamics Observatory (SDO) is designed to study convection-zone …
of the NASA Solar Dynamics Observatory (SDO) is designed to study convection-zone …
Global energetics of thirty-eight large solar eruptive events
We have evaluated the energetics of 38 solar eruptive events observed by a variety of
spacecraft instruments between 2002 February and 2006 December, as accurately as the …
spacecraft instruments between 2002 February and 2006 December, as accurately as the …
Initial Calibration of the Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observatory (SDO)
P Boerner, C Edwards, J Lemen, A Rausch… - The Solar Dynamics …, 2012 - Springer
Abstract The Atmospheric Imaging Assembly (AIA) instrument onboard the Solar Dynamics
Observatory (SDO) is an array of four normal-incidence reflecting telescopes that image the …
Observatory (SDO) is an array of four normal-incidence reflecting telescopes that image the …
CHIANTI—an atomic database for emission lines. XVI. Version 10, further extensions
G Del Zanna, KP Dere, PR Young… - The Astrophysical …, 2021 - iopscience.iop.org
We present version 10 of the CHIANTI package. In this release, we provide updated atomic
models for several helium-like ions and for all the ions of the beryllium, carbon, and …
models for several helium-like ions and for all the ions of the beryllium, carbon, and …
Mars Global Ionosphere‐Thermosphere Model: Solar cycle, seasonal, and diurnal variations of the Mars upper atmosphere
Abstract A new Mars Global Ionosphere‐Thermosphere Model (M‐GITM) is presented that
combines the terrestrial GITM framework with Mars fundamental physical parameters, ion …
combines the terrestrial GITM framework with Mars fundamental physical parameters, ion …
Solar UV and X-ray spectral diagnostics
G Del Zanna, HE Mason - Living Reviews in Solar Physics, 2018 - Springer
X-ray and ultraviolet (UV) observations of the outer solar atmosphere have been used for
many decades to measure the fundamental parameters of the solar plasma. This review …
many decades to measure the fundamental parameters of the solar plasma. This review …
The MAVEN EUVM model of solar spectral irradiance variability at Mars: Algorithms and results
Solar extreme ultraviolet (EUV) radiation is a primary energy input to the Mars atmosphere,
causing ionization and driving photochemical processes above approximately 100 km …
causing ionization and driving photochemical processes above approximately 100 km …
Emirates Mars mission characterization of Mars atmosphere dynamics and processes
H Almatroushi, H AlMazmi, N AlMheiri… - Space Science …, 2021 - Springer
Abstract The Emirates Mars Mission (EMM)–Hope Probe–was developed to understand
Mars atmospheric circulation, dynamics, and processes through characterization of the Mars …
Mars atmospheric circulation, dynamics, and processes through characterization of the Mars …