The Electron Proton Helium INstrument as an example for a Space Weather Radiation Instrument | Journal of Space Weather and Space Climate

Topical Issue - Space Weather Instrumentation

Open Access

Issue		J. Space Weather Space Clim. Volume 10, 2020 Topical Issue - Space Weather Instrumentation


Article Number		53
Number of page(s)		11
DOI		https://doi.org/10.1051/swsc/2020056
Published online		02 November 2020

Banjac S, Gómez-Herrero R, Heber B, Kühl P, Terasa C. 2015. EPHIN anisotropy measurement capability. In: Journal of Physics Conference Series, Vol. 632 of Journal of Physics Conference Series, 012048 p. https://doi.org/10.1088/1742-6596/632/1/012048. [Google Scholar]
Boudouridis A, Rodriguez JV, Kress BT, Dichter BK, Onsager TG. 2020. Development of a Bowtie inversion technique for real-time processing of the GOES-16/-17 SEISS MPS-HI electron channels. Space Weather 18(4): e02403. https://doi.org/10.1029/2019SW002403. [CrossRef] [Google Scholar]
Cohen CMS, Mewaldt RA. 2018. The ground-level enhancement event of September 2017 and other large solar energetic particle events of Cycle 24. Space Weather 16(10): 1616–1623. https://doi.org/10.1029/2018SW002006. [CrossRef] [Google Scholar]
Curdt W, Fleck B. 2015. Solar and galactic cosmic rays observed by SOHO. Cent Eur Astrophys Bull 39 : 109–118. [Google Scholar]
Domingo V, Fleck B, Poland AI. 1995. The SOHO mission: An overview. Sol Phys 162(1–2): 1–37. https://doi.org/10.1007/BF00733425. [Google Scholar]
Dresing N, Gómez-Herrero R, Heber B, Klassen A, Temmer M, Veronig A. 2018. Long-lasting injection of solar energetic electrons into the heliosphere. A&A 613 : A21. https://doi.org/10.1051/0004-6361/201731573. [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
Geant4-Collaboration. 2003. Geant4 – a simulation toolkit. Nucl Instrum Meth Phys Res Sect A: Accel Spectr Detect Assoc Equip 506(3): 250–303. https://doi.org/10.1016/S0168-9002(03)01368-8. [CrossRef] [Google Scholar]
George JS, Lave KA, Wiedenbeck ME, Binns WR, Cummings AC, et al. 2009. Elemental composition and energy spectra of galactic cosmic rays during solar cycle 23. Astrophys J 698(2): 1666–1681. https://doi.org/10.1088/0004-637X/698/2/1666. [NASA ADS] [CrossRef] [Google Scholar]
Gold RE, Krimigis SM, Hawkins SE I, Haggerty DK, Lohr DA, Fiore E, Armstrong TP, Holland G, Lanzerotti LJ. 1998. Electron, proton, and alpha monitor on the advanced composition explorer spacecraft. Space Sci Rev 86 : 541–562. https://doi.org/10.1023/A:1005088115759. [NASA ADS] [CrossRef] [Google Scholar]
Gómez-Herrero R, Rodrguez-Fras MD, del Peral L, Müller-Mellin R, Kunow H. 2002. SOHO/EPHIN observation of a multiple large solar energetic particles event in November 1997. Astropart Phys 17(1): 1–12. https://doi.org/10.1016/S0927-6505(01)00136-0. [CrossRef] [Google Scholar]
Heber B, Wallmann C, Galsdorf D, Herbst K, Kühl P, et al. 2015. Forbush decreases associated to Stealth Coronal Mass Ejections. Cent Eur Astrophys Bull 39 : 75–82. [Google Scholar]
Howard TA, Harrison RA. 2013. Stealth coronal mass ejections: A perspective. Sol Phys 285(1–2): 269–280. https://doi.org/10.1007/s11207-012-0217-0. [NASA ADS] [CrossRef] [Google Scholar]
Jiggens PTA, Gabriel SB, Heynderickx D, Crosby N, Glover A, Hilgers A. 2012. ESA SEPEM project: Peak flux and fluence model. IEEE Trans Nucl Sci 59(4): 1066–1077. https://doi.org/10.1109/TNS.2012.2198242. [CrossRef] [Google Scholar]
Klein K-L, Posner A. 2005. The onset of solar energetic particle events: prompt release of deka-MeV protons and associated coronal activity. A&A 438(3): 1029–1042. https://doi.org/10.1051/0004-6361:20042607. [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
Krucker S, Lin RP. 2000. Two classes of solar proton events derived from onset time analysis. Astrophys J Lett 542(1): L61–L64. https://doi.org/10.1086/312922. [NASA ADS] [CrossRef] [Google Scholar]
Kühl P, Banjac S, Dresing N, Goméz-Herrero R, Heber B, Klassen A, Terasa C. 2015a. Proton intensity spectra during the solar energetic particle events of May 17, 2012 and January 6, 2014. A&A 576 : A120. https://doi.org/10.1051/0004-6361/201424874. [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
Kühl P, Banjac S, Heber B, Labrenz J, Müller-Mellin R, Terasa C. 2015b. Extended measurement capabilities of the electron proton helium instrument aboard SOHO – understanding single detector count rates. Cent Eur Astrophys Bull 39 : 119–124. [Google Scholar]
Kühl P, Dresing N, Heber B, Klassen A. 2017. Solar energetic particle events with protons above 500 MeV between 1995 and 2015 measured with SOHO/EPHIN. Sol Phys 292(1): 10. https://doi.org/10.1007/s11207-016-1033-8. [NASA ADS] [CrossRef] [Google Scholar]
Kühl P, Gómez-Herrero R, Heber B. 2016. Annual cosmic ray spectra from 250 MeV up to 1.6 GeV from 1995–2014 measured with the electron proton helium instrument onboard SOHO. Sol Phys 291(3): 965–974. https://doi.org/10.1007/s11207-016-0879-0. [NASA ADS] [CrossRef] [Google Scholar]
Kühl P, Heber B. 2019. Revising more than 20 years of EPHIN ion flux data – a new data product for space weather applications. Space Weather 17(1): 84–98. https://doi.org/10.1029/2018SW002114. [CrossRef] [Google Scholar]
Lario D, Raouafi NE, Kwon RY, Zhang J, Gómez-Herrero R, Dresing N, Riley P. 2014. The solar energetic particle event on 2013 April 11: an investigation of its solar origin and longitudinal spread. Astrophys J 797(1): 8. https://doi.org/10.1088/0004-637X/797/1/8. [NASA ADS] [CrossRef] [Google Scholar]
Malandraki OE, Crosby NB. 2018. Solar particle radiation storms forecasting and analysis, Vol. 444 , Springer, Berlin, Germany. https://doi.org/10.1007/978-3-319-60051-2. [CrossRef] [Google Scholar]
Marquardt J, Heber B. 2019. Galactic cosmic ray hydrogen spectra and radial gradients in the inner heliosphere measured by the HELIOS experiment 6. A&A 625 : A153. https://doi.org/10.1051/0004-6361/201935413. [CrossRef] [EDP Sciences] [Google Scholar]
Maurin D, Melot F, Taillet R. 2014. A database of charged cosmic rays. A&A 569 : A32. https://doi.org/10.1051/0004-6361/201321344. [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
McComas DJ, Alexander N, Angold N, Bale S, Beebe C, et al. 2016. Integrated science investigation of the Sun (ISIS): Design of the energetic particle investigation. Space Sci Rev 204(1–4): 187–256. https://doi.org/10.1007/s11214-014-0059-1. [NASA ADS] [CrossRef] [Google Scholar]
Mewaldt RA, Cohen CMS, Labrador AW, Leske RA, Mason GM, Desai MI, Looper MD, Mazur JE, Selesnick RS, Haggerty DK. 2005. Proton, helium, and electron spectra during the large solar particle events of October–November 2003. J Geophys Res (Space Phys) 110(A9): A09S18. https://doi.org/10.1029/2005JA011038. [Google Scholar]
Müller-Mellin R, Kunow H, Fleißner V, Pehlke E, Rode E, et al. 1995. COSTEP – comprehensive suprathermal and energetic particle analyser. Sol Phys 162(1): 483–504. [NASA ADS] [CrossRef] [Google Scholar]
Núñez M, Klein K-L, Heber B, Malandraki OE, Zucca P, Labrens J, Reyes-Santiago P, Kuehl P, Pavlos E. 2018. HESPERIA forecasting tools: Real-time and post-event. In: Vol. 444 of Astrophysics and Space Science Library, Springer, Berlin, Germany, pp. 113–131. https://doi.org/10.1007/978-3-319-60051-2_7. [CrossRef] [Google Scholar]
Núñez M, Reyes-Santiago PJ, Malandraki OE. 2017. Real-time prediction of the occurrence of GLE events. Space Weather 15(7): 861–873. https://doi.org/10.1002/2017SW001605. [CrossRef] [Google Scholar]
Paassilta M, Raukunen O, Vainio R, Valtonen E, Papaioannou A, et al. 2017. Catalogue of 55–80 MeV solar proton events extending through solar cycles 23 and 24. J Space Weather Space Clim 7 : A14. https://doi.org/10.1051/swsc/2017013. [CrossRef] [Google Scholar]
Policella N, Oliveira H, Siili T. 2009. SKEYP: AI applied to SOHO keyhole operations. In: 2009 Third IEEE International Conference on Space Mission Challenges for Information Technology, pp. 58–65. [Google Scholar]
Posner A. 2007. Up to 1-hour forecasting of radiation hazards from solar energetic ion events with relativistic electrons. Space Weather 5(5): 05001. https://doi.org/10.1029/2006SW000268. [NASA ADS] [CrossRef] [Google Scholar]
Posner A, Strauss R. 2020. Warning time analysis from SEP simulations of a two-tier REleASE system applied to Mars exploration. Space Weather 18(4): e2019SW002354. https://doi.org/10.1029/2019SW002354. URL https://agupubs.onlinelibrary.wiley.com/doi/abs/10.1029/2019SW002354. [Google Scholar]
Reames. 2019. Element abundances of solar energetic particles and the photosphere, the corona, and the solar wind. Atoms 7(4): 104. https://doi.org/10.3390/atoms7040104. [CrossRef] [Google Scholar]
Richardson IG, Wibberenz G, Cane HV. 1996. The relationship between recurring cosmic ray depressions and corotating solar wind streams at ≤1 AU: IMP 8 and Helios 1 and 2 anticoincidence guard rate observations. J Geophys Res 101(A6): 13483–13496. https://doi.org/10.1029/96JA00547. [NASA ADS] [CrossRef] [Google Scholar]
Rodriguez JV, Sandberg I, Mewaldt RA, Daglis IA, Jiggens P. 2017. Validation of the effect of cross-calibrated GOES solar proton effective energies on derived integral fluxes by comparison with STEREO observations. Space Weather 15(2): 290–309. https://doi.org/10.1002/2016SW001533. [CrossRef] [Google Scholar]
Rodriguez-Pacheco J, Wimmer-Schweingruber RF, Mason GM, Ho GC, Sánchez-Prieto S, et al. 2019. The energetic particle detector. Energetic particle instrument suite for the solar orbiter mission. A&A 642 : 35. https://doi.org/10.1051/0004-6361/201935287. [Google Scholar]
Sandberg I, Jiggens P, Heynderickx D, Daglis IA. 2014. Cross calibration of NOAA GOES solar proton detectors using corrected NASA IMP-8/GME data. Geophys Res Lett 41(13): 4435–4441. https://doi.org/10.1002/2014GL060469. [CrossRef] [Google Scholar]
Sierks H, Elent I, Dröge W, Mann G, Aurass H, Kunow H, Müller-Mellin R, Sequeiros J, McKenna-Lawlor S. 1997. Electron spectra and associated type II and type III radio bursts of the July 9, 1996 solar event. In: International Cosmic Ray Conference, Vol. 1 of International Cosmic Ray Conference, 297 p. [Google Scholar]
Simpson JA, Anglin JD, Balogh A, Bercovitch M, Bouman JM, et al. 1992. The ULYSSES cosmic ray and solar particle investigation. A&A Suppl. 92(2): 365–399. [Google Scholar]
Vainio R, Valtonen E, Heber B, Malandraki OE, Papaioannou A, et al. 2013. The first SEPServer event catalogue 68-MeV solar proton events observed at 1 AU in 1996–2010. J Space Weather Space Clim 3 : A12. https://doi.org/10.1051/swsc/2013030. [CrossRef] [EDP Sciences] [Google Scholar]
Vandenbussche FC. 2006. Saving SOHO. In: SOHO-17. 10 Years of SOHO and Beyond, Vol. 617 of ESA Special Publication, 29 p. [Google Scholar]
Wimmer-Schweingruber RF, Yu J, Böttcher SI, Zhang S, Burmeister S, et al. 2020. The Lunar Lander Neutron and Dosimetry (LND) Experiment on Chang’E 4. Space Sci Rev 216 : 104. [CrossRef] [Google Scholar]
Zhao LL, Qin G, Zhang M, Heber B. 2014. Modulation of galactic cosmic rays during the unusual solar minimum between cycles 23 and 24. J Geophys Res (Space Phys) 119(3): 1493–1506. https://doi.org/10.1002/2013JA019550. [NASA ADS] [CrossRef] [Google Scholar]

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.