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100 results on '"Campana, D."'

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1. The atmospheric monitoring system of the JEM-EUSO instrument

2. Science and mission status of EUSO-SPB2

3. Time dependence of the flux of helium nuclei in cosmic rays measured by the PAMELA experiment between July 2006 and December 2009

4. Ten years of PAMELA in space

5. GAPS, low-energy antimatter for indirect dark-matter search

6. Atmospheric neutrino oscillations in the macro experiment

7. Time dependence of the e^- flux measured by PAMELA during the July 2006 - December 2009 solar minimum

8. PAMELA's measurements of geomagnetic cutoff variations during solar energetic particle events

9. Latitudinal and radial gradients of galactic cosmic ray protons in the inner heliosphere – PAMELA and Ulysses observations

10. Cosmic-Ray Positron Energy Spectrum Measured by PAMELA

11. Neutrino Astronomy with MACRO

12. New MACRO results on atmospheric neutrino oscillations

13. MACRO results on atmospheric neutrino oscillations

14. The primary cosmic ray composition between 10**15 and 10**16 eV from Extensive Air Showers electromagnetic and TeV muon data

15. Time dependence of the proton flux measured by PAMELA during the July 2006 - December 2009 solar minimum

16. An evaluation of the exposure in nadir observation of the JEM-EUSO mission

17. The cosmic-ray electron flux measured by the PAMELA experiment between 1 and 625 GeV

18. Observations of the December 13 and 14, 2006, Solar Particle Events in the 80 MeV/n - 3 GeV/n range from space with PAMELA detector

19. First detection of geomagnetically trapped antiprotons by the PAMELA experiment

20. PAMELA: Measurements of matter and antimatter in space

21. Experimental study of hadronic interaction model using coincident data from EAS-TOP and MACRO

22. PAMELA results on the cosmic-ray antiproton flux from 60 MeV to 180 GeV in kinetic energy

23. Observation of an anomalous positron abundance in the cosmic radiation

24. STUDY OF THE COSMIC-RAY PRIMARY COMPOSITION AT E0-SIMILAR-TO-1000TEV BY EAS-TOP AND MACRO AT GRAN-SASSO

25. Mass limits for scalar muons, scalar electrons, and winos from e+e− collisions near √ = 91 GeV

26. First Results from the PAMELA Space Mission

27. Cosmic-Ray Positron Identification with the PAMELA experiment

28. The PAMELA space experiment

29. Atmospheric neutrino oscillations from upward throughgoing muon multiple scattering in MACRO

30. Search for diffuse neutrino flux from astrophysical sources with MACRO

31. The cosmic ray proton,helium and CNO fluxes in the 100 TeV energy region from TeV muons and EAS atmospheric Cherenkov light observations of MACRO and EAS-TOP

32. Search for cosmic ray sources using muons detected by the MACRO experiment

33. Search for the sidereal and solar diurnal modulations in the total MACRO muon data set

34. Design of an Antimatter Large Acceptance Detector In Orbit (ALADInO)

35. Matter Effects in Upward-Going Muons and Sterile Neutrino Oscillations

36. Neutrino astronomy with the MACRO detector

37. Observation of the shadowing of cosmic rays by the Moon using a deep underground detector

38. High energy cosmic ray physics with underground muons in MACRO. II. Primary spectra and composition

39. Atmospheric neutrino flux measurement using upgoing muons

40. COINCIDENT OBSERVATION OF AIR CERENKOV LIGHT BY A SURFACE ARRAY AND MUON BUNDLES BY A DEEP UNDERGROUND DETECTOR

41. Study of the primary cosmic ray composition around the knee of the energy spectrum

42. Study of the ultrahigh-energy primary-cosmic-ray composition with the MACRO experiment

43. Extreme Universe Space Observatory on a Super Pressure Balloon 1 calibration: from the laboratory to the desert

44. Time dependence of the flux of helium nuclei in cosmic rays measured by the pamela experiment between 2006 july and 2009 december

45. Spectra of solar neutrons with energies of ~10–1000 MeV in the PAMELA experiment in the flare events of 2006–2015

46. Galactic Cosmic Ray Electrons and Positrons over a Decade of Observations in the PAMELA Experiment

47. Cosmic ray electrons and positrons over decade with the PAMELA experiment

48. Secondary positrons and electrons in near-Earth space in the PAMELA experiment

49. Evidence of energy and charge sign dependence of the recovery time for the December 2006 Forbush event measured by the PAMELA experiment

50. Proton Fluxes Measured by the PAMELA Experiment from the Minimum to the Maximum Solar Activity for Solar Cycle 24

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