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Influence of Large-scale Interplanetary Structures on the Propagation of Solar Energetic Particles: The Multispacecraft Event on 2021 October 9

The Astrophysical journal, 2022-07, Vol.934 (1), p.55

2022

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Scientific Analysis within SEPServer – New Perspectives in Solar Energetic Particle Research: The Case Study of the 13 July 2005 Event

Solar physics, 2012-11, Vol.281 (1), p.333-352

2012

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Scanning an Interplanetary Magnetic Cloud Using High-Energy Protons

The Astrophysical journal, 2007-01, Vol.654 (2), p.1121-1127

2007

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High-Energy Protons Associated with Liftoff of a Coronal Mass Ejection

The Astrophysical journal, 2007-04, Vol.659 (1), p.780-787

2007

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Influence of Large-Scale Interplanetary Structures on the Propagation of Solar Energetic Particles: the Multi-Spacecraft Event on 2021 October 9

The Astrophysical journal, 2022-07, Vol.934 (1)

2022

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Great Storm Particle Event on 2000 August 11 Observed by SOHO ERNE

The Astrophysical journal, 2006-02, Vol.638 (1), p.530-538

2006

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Energetic particle experiment ERNE

Solar physics, 1995-12, Vol.162 (1-2), p.505-531

1995

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The 1998 May 2-3 Magnetic Cloud: An Interplanetary "Highway" for Solar Energetic Particles Observed with SOHO /ERNE

The Astrophysical journal, 2004-01, Vol.600 (1), p.L83-L86

2004

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Energetic (∼ 1 to 50 MeV) protons associated with Earth-directed coronal mass ejections

Geophysical research letters, 1998-07, Vol.25 (14), p.2525-2528

1998

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The first SEPServer event catalogue similar to 68-MeV solar proton events observed at 1 AU in 1996-2010

Journal of space weather and space climate, 2013-01, Vol.3

2013

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Energetic (∼10-65 MeV) protons observed by ERNE on August 13-14, 1996: Eruption on the solar back side as a possible source of the event

Journal of Geophysical Research, 1999-05, Vol.104 (A5), p.9903-9909

1999

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Observations of galactic cosmic ray modulation during Earth-directed coronal mass ejections

Geophysical research letters, 1998-08, Vol.25 (15), p.2951-2954

1998

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Specialized detector techniques and electronics of the ERNE instrument onboard SOHO

Nuclear physics. Section B, Proceedings supplement, 1998-02, Vol.61 (3), p.6-11

1998

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Performance of ERNE in particle flux anisotropy measurement

Annales geophysicae (1988), 1996-05, Vol.14 (5), p.503-509

1996

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Energetic and relativistic nuclei and electron experiment of the SOHO mission

Nuclear instruments & methods in physics research. Section A, Accelerators, spectrometers, detectors and associated equipment, 1997-06, Vol.391 (2), p.249-268

1997

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Anomalous Cosmic-Ray Helium, Nitrogen and Oxygen in 1996 - Measurements of the ERNE Instrument on-board SOHO

Solar physics, 1997-01, Vol.170 (1), p.193-204

1997

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Energetic particle investigation using the ERNE instrument

Annales geophysicae (1988), 1996-05, Vol.14 (5), p.497-502

1996

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First Energetic Particle Events Observed by the ERNE Instrument

Solar physics, 1997-01, Vol.170 (1), p.179-191

1997

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Erne observations of energetic particle fluxes

Advances in space research, 1997, Vol.20 (1), p.91-98

1997

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Search of periodic scintillations in cosmic radiation in the range 2–50 mHz

Advances in space research, 1989, Vol.9 (4), p.229-232

1989

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Cosmic-Ray Intensity Oscillations Immediately before and after the GLE on February 16, 1984

Europhysics letters, 1987-05, Vol.3 (10), p.1151-1153

1987

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Energetic (∼10-65 MeV) protons observed by ERNE on August 13-14, 1996 : Eruption on the solar back side as a possible source of the event : Results of the First Whole Sun Month Campaign

Journal of geophysical research, 1999, Vol.104 (A5), p.9903-9909

1999

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Energetic (∼ 1 to 50 MeV) protons associated with Earth-directed coronal mass ejections : Sun-Earth Connections: The ISTP Program

Geophysical research letters, 1998, Vol.25 (14), p.2525-2528

1998

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Analysis of the time structure of the GLE on february 16, 1984

Il nuovo cimento della Società italiana di fisica. Sezione C, Geophysics and space physics, 1987, Vol.10 (1), p.102-108

1987

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Acute changes in oxytocin predict behavioral responses to foundation training in horses

Applied animal behaviour science, 2022-09, Vol.254, p.105707, Article 105707

2022

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Influence of Large-scale Interplanetary Structures on the Propagation of Solar Energetic Particles: The Multispacecraft Event on 2021 October 9

Scientific Analysis within SEPServer – New Perspectives in Solar Energetic Particle Research: The Case Study of the 13 July 2005 Event

Scanning an Interplanetary Magnetic Cloud Using High-Energy Protons

High-Energy Protons Associated with Liftoff of a Coronal Mass Ejection

Influence of Large-Scale Interplanetary Structures on the Propagation of Solar Energetic Particles: the Multi-Spacecraft Event on 2021 October 9

Great Storm Particle Event on 2000 August 11 Observed by SOHO ERNE

Energetic particle experiment ERNE

The 1998 May 2-3 Magnetic Cloud: An Interplanetary "Highway" for Solar Energetic Particles Observed with SOHO /ERNE

Energetic (∼ 1 to 50 MeV) protons associated with Earth-directed coronal mass ejections

The first SEPServer event catalogue similar to 68-MeV solar proton events observed at 1 AU in 1996-2010

Energetic (∼10-65 MeV) protons observed by ERNE on August 13-14, 1996: Eruption on the solar back side as a possible source of the event

Observations of galactic cosmic ray modulation during Earth-directed coronal mass ejections

Specialized detector techniques and electronics of the ERNE instrument onboard SOHO

Performance of ERNE in particle flux anisotropy measurement

Energetic and relativistic nuclei and electron experiment of the SOHO mission

Anomalous Cosmic-Ray Helium, Nitrogen and Oxygen in 1996 - Measurements of the ERNE Instrument on-board SOHO

Energetic particle investigation using the ERNE instrument

First Energetic Particle Events Observed by the ERNE Instrument

Erne observations of energetic particle fluxes

Search of periodic scintillations in cosmic radiation in the range 2–50 mHz

Cosmic-Ray Intensity Oscillations Immediately before and after the GLE on February 16, 1984

Energetic (∼10-65 MeV) protons observed by ERNE on August 13-14, 1996 : Eruption on the solar back side as a possible source of the event : Results of the First Whole Sun Month Campaign

Energetic (∼ 1 to 50 MeV) protons associated with Earth-directed coronal mass ejections : Sun-Earth Connections: The ISTP Program

Analysis of the time structure of the GLE on february 16, 1984

Acute changes in oxytocin predict behavioral responses to foundation training in horses

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