HelioWebUniversity of L'Aquila, Department of Physics
flowchart
I[University of L'Aquila, Department of Physics]
PI["Parent Institutions (1)"]
CI["Child Institutions (0)"]
AW["Affiliated Works (41)"]
CA["Linked Collaborating Authors (2)"]
I== skos:broader ==>PI
CI== skos:broader ==>I
AW== affil ==>I
AW== author ==>CA
click PI "#parent-institutions"
click CI "#child-institutions"
click AW "#affiliated-works"
click CA "#collaborating-authors"
Parent Institutions [?]
Child Institutions [?]
Affiliated Works
sorted by decreasing year, and then by display-name
- A Comprehensive Validation of Global Chemistry Transport Models Against Observations for a Complete 4-year Simulation Period (1995 to 1998)
- On the Role of Coherent and Stochastic Fluctuations in the Radial Evolution of Intermittency of Interplanetary Magnetic Field Fluctuations
- Model-Measurement Comparisons of [OH], [HO2], and P(O3) in Houston
- The Behavior of the Hydroxyl and Hydroperoxyl Radicals During PROPHET2000
- The Behavior of the Hydroxyl and Hydroperoxyl Radicals During TexAQS2000
- Effects of Crustal Layering on Source Parameter Inversion from Coseismic Displacement Data
- Groundwater Carbon Decrease During a Slow Earthquake Swarm in Central Italy
- The ESPERIA Mission
- Clues of Post-seismic Relaxation for the 1915 Fucino Earthquake (Central Italy) From Modeling of Leveling Data
- Recent Seismic Activity of the Messina Straits Area, Italy, and the Magnitude 7, 1908 Messina Earthquake
- Trans-polar Transmission of Pc 3-4 ULF Waves: Results from Cluster and Antarctic Observations
- Improved Understanding of Far-Infrared Radiative Processes in the Earth's Atmosphere
- Solar Wind MHD Turbulence for Different Phases of the Solar Cycle
- Spatial and Temporal Analysis of Magnetic Helicity in the Solar Wind
- THE APRIL 6, 2009 EARTHQUAKE AT L’AQUILA: A PRELIMINARY SEISMO-MAGNETIC ANALYSIS OF MULTIPOINT GROUND-BASED MAGNETIC FIELD MEASUREMENTS
- The June 8, 2000 ULF wave activity: a case study
- The transmission of upstream waves to the magnetosphere: an analysis at widly separated ground stations
- Influence of aerosol chemical composition on N<SUB>2</SUB>O<SUB>5</SUB> uptake: Airborne regional measurements in North-Western Europe
- Morning/Afternoon Asymmetry of Geomagnetic Fluctuations at Discrete Frequencies
- Sudden Impulses: the discrimination between magnetospheric and ionospheric contributions in ground manifestations
- The transmission of upstream waves at polar latitudes through magnetotail lobes
- The transmission of upstream waves to the magnetosphere from middle to high latitude
- ULTIMA: Array of ground-based magnetometer arrays for monitoring magnetospheric and ionospheric perturbations on a global scale
- On the propagation of Sudden Impulses through the magnetosphere:implication of a simple approach
- The Central Raman Laser Facility at the Pierre Auger Observatory
- Effect of the aerosol type uncertainty on the surface reflectance retrieval using CHRIS/PROBA hyperspectral images over land.
- Variation of Ultra-Low Frequency Waves within Solar Wind and Pc5 Fluctuations on the Ground in High Latitudes during Solar Cycle 23
- Biomass Burning Aerosol Vertical Distribution Over the South African-Atlantic Region: Perspectives from Multi-Models and CALIOP Observations
- Global model simulation of single scattering albedo: A sensitivity analysis
- Remote Monitoring of the Plasma Mass Density in the Inner Magnetosphere using Field Line Resonances detected at the European Magnetometer Network EMMA
- Solar Wind Magnetic Field Background Spectrum from Fluid to Kinetic Scales
- ALIF: A New Promising Technique for the Decomposition and Analysis of Nonlinear and Nonstationary Signals
- Application of High Resolution Air-Borne Remote Sensing Observations for Monitoring NOx Emissions
- Quantifying the decadal changes of PM<SUB>2.5</SUB> over New York through a combination of satellite, model and in-situ measurements
- Assessing and communicating uncertainties in PM<SUB>2.5</SUB> estimates derived from satellite aerosol optical depth
- Using Solar Wind Structures as a Rosetta Stone for Understanding Solar Wind Formation
- Evaluation of the particle light scattering enhancement factor within six climate models using surface-based in-situ measurements
- Modeling the Plasma Mass Density of the Inner Magnetosphere From EMMA Magnetometer Network Observations
- Multiharmonic Toroidal Standing Alfven Waves in the Midnight Sector Excited by Solar Wind Source
- Simultaneous occurrence of internally and externally driven ULF waves in the magnetosphere.
- Poloidal ULF Waves During the August 2015 Geomagnetic Storm