VAZZA, FRANCO
 Distribuzione geografica
Continente #
NA - Nord America 10.503
AS - Asia 8.545
EU - Europa 6.401
Continente sconosciuto - Info sul continente non disponibili 688
SA - Sud America 533
AF - Africa 435
OC - Oceania 10
Totale 27.115
Nazione #
US - Stati Uniti d'America 10.272
SG - Singapore 2.287
CN - Cina 2.163
VN - Vietnam 1.974
GB - Regno Unito 1.889
IT - Italia 1.315
DE - Germania 722
HK - Hong Kong 676
FR - Francia 569
SE - Svezia 559
IN - India 413
BR - Brasile 384
KR - Corea 284
RU - Federazione Russa 266
IE - Irlanda 189
FI - Finlandia 183
CI - Costa d'Avorio 147
BD - Bangladesh 142
JP - Giappone 141
CA - Canada 136
NL - Olanda 121
ZA - Sudafrica 109
UA - Ucraina 98
ID - Indonesia 76
EE - Estonia 74
PL - Polonia 73
TG - Togo 72
AR - Argentina 65
JO - Giordania 65
PH - Filippine 63
MX - Messico 52
AT - Austria 51
BG - Bulgaria 50
TR - Turchia 45
TH - Thailandia 38
ES - Italia 36
BE - Belgio 32
IQ - Iraq 30
GR - Grecia 29
SC - Seychelles 28
NG - Nigeria 27
RO - Romania 24
TW - Taiwan 24
SA - Arabia Saudita 23
PK - Pakistan 22
HR - Croazia 21
HU - Ungheria 19
EC - Ecuador 17
CH - Svizzera 16
CO - Colombia 16
CL - Cile 15
CZ - Repubblica Ceca 15
EG - Egitto 13
IR - Iran 12
JM - Giamaica 12
UZ - Uzbekistan 12
CR - Costa Rica 11
AU - Australia 9
MA - Marocco 9
PT - Portogallo 9
TN - Tunisia 9
AL - Albania 8
NP - Nepal 8
PE - Perù 8
UY - Uruguay 8
VE - Venezuela 8
IL - Israele 7
LB - Libano 7
LU - Lussemburgo 7
PY - Paraguay 7
KE - Kenya 6
MY - Malesia 6
AE - Emirati Arabi Uniti 5
LT - Lituania 5
OM - Oman 5
PR - Porto Rico 5
AZ - Azerbaigian 4
DK - Danimarca 4
DZ - Algeria 4
MD - Moldavia 4
BA - Bosnia-Erzegovina 3
BO - Bolivia 3
DO - Repubblica Dominicana 3
ET - Etiopia 3
GT - Guatemala 3
LV - Lettonia 3
SN - Senegal 3
BH - Bahrain 2
GY - Guiana 2
HN - Honduras 2
HT - Haiti 2
MM - Myanmar 2
NI - Nicaragua 2
RS - Serbia 2
SK - Slovacchia (Repubblica Slovacca) 2
A2 - ???statistics.table.value.countryCode.A2??? 1
AM - Armenia 1
BW - Botswana 1
BY - Bielorussia 1
BZ - Belize 1
Totale 26.411
Città #
Southend 1.558
Singapore 1.557
Ashburn 1.109
Fairfield 815
Hong Kong 649
Ho Chi Minh City 518
Hefei 504
San Jose 504
Chandler 493
Hanoi 437
Bologna 436
Woodbridge 379
Dallas 365
Santa Clara 355
Houston 324
Seattle 308
Wilmington 308
Cambridge 281
Council Bluffs 272
Seoul 252
Beijing 240
Princeton 237
Ann Arbor 236
Los Angeles 204
Dublin 183
Boardman 179
Abidjan 147
Lauterbourg 133
Tokyo 113
Munich 102
Lappeenranta 95
Berlin 92
Milan 91
New York 91
Westminster 91
Turin 88
Dong Ket 85
Nanjing 85
Da Nang 76
São Paulo 76
Lomé 72
Redondo Beach 68
Haiphong 66
Amman 65
Helsinki 65
Buffalo 64
Padova 64
San Diego 63
Frankfurt am Main 62
Rome 62
Chicago 57
Jinan 57
Jakarta 56
Bengaluru 55
Warsaw 55
Phoenix 53
Shenyang 50
Guangzhou 49
Saint Petersburg 49
Sofia 49
The Dalles 49
Orem 48
Modena 47
Montreal 44
Shanghai 43
London 40
Redmond 40
Des Moines 39
Tongling 39
Nuremberg 38
Atlanta 37
Hillsboro 37
Fremont 36
San Francisco 34
Norwalk 33
Medford 32
Vienna 31
Hangzhou 30
Mcallen 30
Nanchang 30
Hebei 29
Washington 29
Changsha 28
Tianjin 28
Biên Hòa 27
Falls Church 27
Redwood City 27
Ninh Bình 26
Brooklyn 25
Jiaxing 25
Brussels 24
Denver 24
Paris 24
Zhengzhou 24
Abeokuta 23
Toronto 23
Can Tho 22
Hải Dương 22
Dearborn 21
Thái Nguyên 21
Totale 16.505
Nome #
Astrophysical constraints on the simulation hypothesis for this Universe: why it is (nearly) impossible that we live in a simulation 975
The Quantitative Comparison Between the Neuronal Network and the Cosmic Web 646
LOFAR discovery of radio emission in MACSJ0717.5+3745 406
The turbulent pressure support in galaxy clusters revisited 350
A comparison of cosmological codes: Properties of thermal gas and shock waves in large-scale structures 338
A LOFAR study of non-merging massive galaxy clusters 292
The coma cluster at low frequency array frequencies. I. Insights into particle acceleration mechanisms in the radio bridge 270
Gas clumping in galaxy clusters 266
Fundamental physics with the Square Kilometre Array 263
The scatter in the radial profiles of X-ray luminous galaxy clusters as diagnostic of the thermodynamical state of the ICM 261
The mixing and transport properties of the intra cluster medium: A numerical study using tracers particles 257
The Northern Cross fast radio burst project – I. Overview and pilot observations at 408 MHz 236
How complex is the cosmic web? 232
A radio ridge connecting two galaxy clusters in a filament of the cosmic web 232
Sardinia Radio Telescope observations of Abell 194: The intra-cluster magnetic field power spectrum 228
Universal thermodynamic properties of the intracluster medium over two decades in radius in the X-COP sample 227
Non-thermal pressure support in X-COP galaxy clusters 225
The gas distribution in the outer regions of galaxy clusters 219
Observations of the galaxy cluster CIZA J2242.8+5301 with the Sardinia Radio Telescope 214
New mysteries and challenges from the Toothbrush relic: wideband observations from 550 MHz to 8 GHz 211
Understanding the radio relic emission in the galaxy cluster MACS J0717.5+3745: Spectral analysis 209
A new double radio relic in PSZ1 G096.89+24.17 and a radio relic mass-luminosity relation 207
Physical insights from the spectrum of the radio halo in MACS J0717.5+3745 204
Second-order Fermi Reacceleration Mechanisms and Large-Scale Synchrotron Radio Emission in Intracluster Bridges 202
The challenge of detecting intracluster filaments with Faraday rotation 200
A shock front at the radio relic of Abell 2744 197
Discovering the most elusive radio relic in the sky: Diffuse shock acceleration caught in the act? 196
Resolved magnetic dynamo action in the simulated intracluster medium 194
Simulations and observational tests of primordial magnetic fields from Cosmic Microwave Background constraints 194
Spectro-polarimetric observations of the CIZA J2242.8+5301 northern radio relic: no evidence of high-frequency steepening 193
Turbulent magnetic fields in the merging galaxy cluster MACS J0717.5+3745 190
Magnetic fields and relativistic electrons fill entire galaxy cluster 189
Abell 746: A Highly Disturbed Cluster Undergoing Multiple Mergers 187
Shocks and Non-thermal Particles in Clusters of Galaxies 185
Detecting shocked intergalactic gas with X-ray and radio observations 183
Magnetogenesis and the cosmic web: A joint challenge for radio observations and numerical simulations 182
Enhancing the Spectral Hardening of Cosmic TeV Photons by Mixing with Axionlike Particles in the Magnetized Cosmic Web 180
On the Connection between Turbulent Motions and Particle Acceleration in Galaxy Clusters 180
Particle re-acceleration and Faraday-complex structures in the RXC J1314.4-2515 galaxy cluster 179
A perfect power-law spectrum even at the highest frequencies: The Toothbrush relic 179
Convolutional deep denoising autoencoders for radio astronomical images 179
Deep low-frequency radio observations of Abell 2256. II. The ultra-steep spectrum radio halo 178
The Coma Cluster at LOFAR Frequencies. II. the Halo, Relic, and a New Accretion Relic 177
Probing the origin of extragalactic magnetic fields with Fast Radio Bursts 177
Efficiency of Turbulent Reacceleration by Solenoidal Turbulence and Its Application to the Origin of Radio Megahalos in Cluster Outskirts 176
Massive and refined: A sample of large galaxy clusters simulated at high resolution. I: Thermal gas and properties of shock waves 175
Modelling injection and feedback of cosmic rays in grid-based cosmological simulations: Effects on cluster outskirts 175
Magnetic field evolution in cosmic filaments with LOFAR data 172
Morphology of radio relics-I. What causes the substructure of synchrotron emission? 172
Forecasts for the detection of the magnetised cosmic web from cosmological simulations 171
New filamentary remnant radio emission and duty cycle constraints in the radio galaxy NGC 6086 170
Deep learning based detection of cosmological diffuse radio sources 170
The nature of LOFAR rotation measures and new constraints on magnetic fields in cosmic filaments and on magnetogenesis scenarios 169
Unravelling the origin of large-scale magnetic fields in galaxy clusters and beyond through Faraday Rotation Measures with the SKA 169
Dissecting nonthermal emission in the complex multiple-merger galaxy cluster Abell 2744: Radio and X-ray analysis 168
The thermal and non-thermal components within and between galaxy clusters Abell 399 and Abell 401 167
Turbulence and vorticity in Galaxy clusters generated by structure formation 167
New constraints on the magnetization of the cosmic web using LOFAR Faraday rotation observations 167
A survey of the thermal and non-thermal properties of cosmic filaments 166
Simulations of extragalactic magnetic fields and of their observables 165
Radio haloes in Sunyaev-Zel'dovich-selected clusters of galaxies: The making of a halo? 165
Polarized accretion shocks from the cosmic web 164
Galaxy clusters enveloped by vast volumes of relativistic electrons 160
Evolution of vorticity and enstrophy in the intracluster medium 159
The intracluster magnetic field in the double relic galaxy cluster Abell 2345 159
Do radio relics challenge diffusive shock acceleration? 158
The X-ray/SZ view of the virial region: II. Gas mass fraction 157
Numerical cosmology on the GPU with Enzo and Ramses 155
Constraining magnetic fields in galaxy clusters 155
Fast radio burst dispersion measures and rotation measures and the origin of intergalactic magnetic fields 155
Turbulence in the Intracluster Medium 155
Thermal and non-thermal traces of agn feedback: Results from cosmological amr simulations 154
Why are central radio relics so rare? 154
Analytical model for cluster radio relics 154
Constraining the efficiency of cosmic ray acceleration by cluster shocks 153
Voyage through the hidden physics of the cosmic web 153
Radio relics radio emission from ltishock scenario 153
Simulations of cosmic rays in large-scale structures: Numerical and physical effects 152
Magnetic Field Amplification in Galaxy Clusters and Its Simulation 152
The entropy core in galaxy clusters: Numerical and physical effects in cosmological grid simulations 151
Constraints on the magnetic field in the intercluster bridge A399- A401 150
New constraints on the magnetic field in cosmic web filaments 150
An intergalactic medium temperature from a giant radio galaxy 149
Joint inference on the redshift distribution of fast radio burst and on the intergalactic baryon content 149
On the alignment of haloes, filaments and magnetic fields in the simulated cosmic web 149
Turbulence in the ICM from mergers, cool-core sloshing, and jets: Results from a new multi-scale filtering approach 148
ALMA-SZ DETECTION of A GALAXY CLUSTER MERGER SHOCK at HALF the AGE of the UNIVERSE 148
Propagation of ultrahigh energy cosmic rays in extragalactic magnetic fields: A view from cosmological simulations 147
Electron and proton acceleration efficiency by merger shocks in galaxy clusters 147
Studying the Effect of Shock Obliquity on the γ-ray and Diffuse Radio Emission in Galaxy Clusters 147
Observations of a nearby filament of galaxy clusters with the Sardinia Radio Telescope 146
Polarization of radio relics in galaxy clusters 146
Turbulent gas motions in galaxy cluster simulations: The role of smoothed particle hydrodynamics viscosity 143
Resistively controlled primordial magnetic turbulence decay 142
Simulations of ultra-high energy cosmic rays in the local Universe and the origin of cosmic magnetic fields 142
Turbulent pressure support and hydrostatic mass-bias in the intracluster medium 142
Measurements and simulation of Faraday rotation across the Coma radio relic 141
Simulating the Enrichment of Fossil Radio Electrons by Multiple Radio Galaxies 140
Properties of gas clumps and gas clumping factor in the intra-cluster medium 140
Shock waves in Eulerian cosmological simulations: Main properties and acceleration of cosmic rays 139
Totale 19.631
Categoria #
all - tutte 73.900
article - articoli 0
book - libri 0
conference - conferenze 0
curatela - curatele 0
other - altro 0
patent - brevetti 0
selected - selezionate 0
volume - volumi 0
Totale 73.900


Totale Lug Ago Sett Ott Nov Dic Gen Feb Mar Apr Mag Giu
2021/20222.287 0 90 178 108 261 123 122 274 259 137 377 358
2022/20232.691 244 424 222 333 152 177 115 145 501 104 189 85
2023/2024782 42 117 42 49 83 121 49 45 14 132 25 63
2024/20253.713 124 471 245 294 530 251 249 141 78 163 273 894
2025/20269.860 1.204 964 1.064 604 820 497 1.082 298 1.649 893 409 376
2026/20271.646 874 772 0 0 0 0 0 0 0 0 0 0
Totale 27.115