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Enregistrement W2609543370 · doi:10.15407/rpra20.03.247

THE BPD ENERGETIC PARTICLE DETECTOR AS PART OF THE SOLAR X-RAY PHOTOMETER ChemiX FOR THE “INTERHELIOPROBE” INTERPLANETARY MISSION

2015· article· en· W2609543370 sur OpenAlexaboutno aff
Oleksiy Dudnik, E. V. Kurbatov, I. L. Zajtsevsky, J. Sylwester, M. Siarkowski, Mirosław Kowaliński, P. Pоdgórski

Notice bibliographique

RevueRadio physics and radio astronomy · 2015
Typearticle
Langueen
DomainePhysics and Astronomy
ThématiqueSolar and Space Plasma Dynamics
Établissements canadiensnon disponible
Organismes subventionnairesnon disponible
Mots-clésPhysicsInterplanetary scintillationDetectorScintillationScintillatorSolar windAstronomyCoronal mass ejectionOpticsNuclear physicsPlasma

Résumé

récupéré en direct d'OpenAlex

The Background Particle Detector (BPD) is an important block of the Polish-Ukrainian X-ray spectrophotometer ChemiX under development for the “Interhelioprobe” interplanetary mission. The BPD primary objective is to detect incoming charged particle fluxes, measure particle energy spectra and safeguard the instrument in case of emergency. The present work describes the BPD laboratory prototype and current results of adjustment and measurements of its important characteristics, in particular the analog signal processing unit and the source of secondary power supply unit. Laboratory benches designed for controlling the parameters of analog module and for characterization of small-sized organic and inorganic scintillation detectors of high energy charged particles are presented. The functional block diagram of the experimental model of digital signal processing line and information data streaming line designed using ProASIC3E М1А3РЕ1500 FPGA are introduced and explained. The results of respective digital modules’ tests performed by using experimental ModelISim Microsemi ME 10.2c program simulator are also presented. Key words: high energy particles, interplanetary space, satellite device, scintillation detector, printed circuit board, programmable logic device Manuscript submitted 23.02.2015 Radio phys. radio astron. 2015, 20(3): 247-260 REFERENCES 1. MURPHY, N., 2006. Measurement and Instrument Challenges for Future Solar and Heliospheric Missions. In: Joint Assembly AGU, GS, MAS, MSA, SEWG, UGM Abstracts. Baltimore, Maryland, 23-26 May 2006. AGU: Section "SPA-Magnetospheric Physics", Session "Technology Development for Sun / Solar System Connections Science I", SM33C-01. 2. KUZNETSOV V. D. and ZELENYI L. M., 2008. Space projects on Solar-terrestrial physics. Solar-Terrestrial Physics , vol. 1, no. 12, pp. 83–92 (in Russian). 3. KUZNETSOV, V. D., 2012. Solar-terrestrial physics and its application. Physics-Uspekhi , vol. 55, no. 3, pp. 305–314. (in Russian). DOI: https://doi.org/10.3367/UFNe.0182.201203h.0327 4. MULLER, D., MARSDEN, R. G., CYR, O. C. ST. and GILBERT, H. R., 2013. Solar Orbiter - Exploring the Sun–Heliosphere Connection. Sol. Phys ., vol. 285, no. 1-2, pp. 25–70. DOI: https://doi.org/10.1007/s11207-012-0085-7 5. KINNISON, J., LOCKWOOD, M. K., FOX N., CONDE, R. and DRIESMAN, A., 2013. Solar Probe Plus: A mission to touch the Sun. In: IEEE Aerospace Conference Proceedings . Big Sky, Montana, 2-9 March 2013. IEEE: p. 1–11. DOI: https://doi.org/10.1109/AERO.2013.6496957 6. WU, J., SUN, W. Y., ZHENG, J. H., ZHANG, C., LIU, H., YAN, J. G., WANG C., WANG C. B. and WANG S., 2011. Imaging interplanetary CMEs at radio frequency from solar polar orbit. Adv. Space Res ., vol. 48, pp. 943–954. DOI: https://doi.org/10.1016/j.asr.2011.05.001 7. WATANABE, T., 2014. The Solar-C Mission. In: SPIE conference 9143 "Space Telescopes and Instrumentation 2014: Optical, Infrared, and Millimeter Wave" Proceedings . 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SYLWESTER, J., BĄKAŁA, J., PODGÓRSKI, P., KOWALIŃSKI, M., KORDYLEWSKI, Z., GBUREK, S., TRZEBINSKI, W., KUZNETSOV, V. D. and BOLDYREV, S. I., 2012. CHEMIX: a new generation solar soft X-ray Bragg spectrometer. In: V. D. KUZNETSOV, ed. INTERHELIOPROBE Project. Workshop Proceedings . Tarusa, 11–13 May 2011. Moscow, Russia: IZMIRAN, pp. 52–64 (in Russian). 12. SYLWESTER, J., ZIMOVETS, I., KOWALIŃSKI, M., BĄKAŁA J., SIARKOWSKI, M., TRZEBINSKI, W., KUZNETSOV, V. and SZAFORZ, Z., 2014. ChemiX: a new generation bent crystal spectrometer for Interhelioprobe mission to the Sun. In: 40th COSPAR Scientific Assembly Abstracts . Moscow, Russia, 2-10 August 2014. Moscow, COSPAR: Panel D2.4 "The Science with Future Solar missions, from the Sun to the Heliosphere", D2.4-34-14. 13. SYLWESTER, J., SIARKOWSKI, M., SZAFORZ, Z., BĄKAŁA, J., DUDNIK, O., KUZNETSOV, V. D., ZIMOVETS, I. V. and KUZIN, S., 2014. ChemiX – the soft X-ray Bragg spectrometer under development for the Interhelioprobe Mission. In: 13th RHESSI Workshop Abstracts . Brugg/Windisch, Switzerland, 1-4 April 2014. Brugg/Windish, Switzerland: University of Applied Sciences Northwestern Switzerland, Session "Current and Future Instrumentation", p. 17. 14. SYLWESTER, J., KORDYLEWSKI, Z., PŁOCIENIAK, S., SIARKOWSKI, M., KOWALIŃSKI, M., NOWAK, S., TRZEBIŃSKI, W., STĘŚLICKI, M., SYLWESTER, B., STAŃCZYK, E., ZAWERBNY, R., SZAFORZ, Z., PHILLIPS, K. J. H., FĄRNIK, F. and STEPANOV, A., 2015. X-ray Flare Spectra from the DIOGENESS Spectrometer and its concept applied to ChemiX on the Interhelioprobe spacecraft. Sol. Phys . [online]. 20 January, pp. 1–15. DOI: https://doi.org/10.1007/s11207-014-0644-1 15. DUDNIK O. V., SYLWESTER J., SIARKOWSKI M., KOWALIŃSKI M., KURBATOV E. V. and TITOV K. G., 2013. The high energy charge particle detector module in the ChemiX instrument aboard Interhelioprobe mission: the goals, concept and design. In: 13th Ukrainian Conference on Space Research Abstracts. Evpatoria, Crimea, Ukraine, 2-6 September 2013. Kyiv: Space Research Institute, p. 123. 16. DUDNIK, O. V., PRIETO, M., KURBATOV, E. V., SANCHEZ, S., TIMAKOVA, T. G., TITOV, K. G. and PARRA, P., 2012. Asmall-sized device for monitoring of high-energy electrons and nuclei in the outer space. Space Science and Technology, vol. 18, no. 6, pp. 22–34 (in Russian). 17. DUDNIK, O. V., PRIETO, M., KURBATOV, E. V., SANCHEZ S., TIMAKOVA, T. G., SPASSKY, A. V., DUBINA, V. N. and PARRA, P., 2013. SIDRA instrument for measurements of particle fluxes at satellite altitudes. Laboratory prototype. Solar System Research , vol. 47, no. 1, pp. 58–65. DOI: https://doi.org/10.1134/S0038094612060019 18. DUDNIK, O. V., KURBATOV, E. V, SYLWESTER, J., SIARKOWSKI, M., KOWALIŃSKI, M., TARASOV, V. O., ANDRYUSHENKO, L. A., ZAJTSEVSKY, I. L. and VALTONEN, E., 2014. Development of small–sized SIDRA device for monitoring of charged particle fluxes in space. In: O. P. FEDOROV, ed. Space Research in Ukraine, 2012–2014. The Report to the COSPAR . Kyiv, Ukraine: Publ. House "Akademperiodika", pp. 62–67. 19. DUDNIK, O. V., BILOGUB, V. V., KURBATOV, E. V., TIMAKOVA, T. G., DUBINA, V. N., MEZIAT, D. and PRIETO, M., 2009. Compact on-board instrument SIDRA for measurement of particle fluxes & dose rates – concept and first model. In: 9th Ukrainian Conference on Space Research Abstracts . Evpatoria, Crimea, Ukraine, 31 August – 5 September 2009. Kyiv: Space Research Institute, p. 78. 20. DUDNIK, O. V., PRIETO, M., KURBATOV, E. V., SANCHEZ, S., TIMAKOVA, T. G., DUBINA, V. N. and PARRA, P., 2011. First concept of compact instrument SIDRA for measurements of particle fluxes in the space. Journal of Kharkiv National University, phys. series "Nuclei, Particles, Fields" , vol. 969, no. 3(51), pp. 62–66 (in Russian). 21. DUDNIK, O. V., PRIETO, M., KURBATOV, E. V., SANCHEZ, S., TIMAKOVA, T. G., DUBINA, V. N. and PARRA, P., 2012. Onboard instrument SIDRA prototype for measurements of radiation environment in the space. In: 39th COSPAR Scientific Assembly Abstracts . Mysore, India. 14-22 July 2012. COSPAR: Session H0.3 "Technical Development of Instrumentation for Current Missions", STW-B-153 H0.3-0023-12, p. 106. 22. DUDNIK, O. V., PRIETO, M., KURBATOV, E. V., TITOV, K. G., TARASOV, V. O., ANDRYUSHENKO, L. A., SANCHEZ, S. and PARRA, P., 2012. Approaches to signal processing from the light scintillation and semiconductor detectors in the compact satellite instrument SIDRA for monitoring of high energy charge particles. In: 12th Ukrainian Conference on Space Research Abstracts . Evpatoria, Crimea, Ukraine, 3-7 September 2012. Kyiv: Space Research Institute, p. 102. 23. DUDNIK, O. V., PRIETO, M., KURBATOV, E. V., SANCHEZ, S., TITOV, K. G., SYLWESTER, J., GBUREK, S. and PODGÓRSKI, P., 2013. Functional capabilities of the breadboard model of SIDRA satellite-borne instrument. Problems of Atomic Science and Technology, Series "Nuclear Physics Investigations" , vol. 3(85), no. 60, pp. 289–296. 24. DUDNIK, O. V., KURBATOV, E. V., AVILOV, A. M., PRIETO, M., SANCHEZ, S., SPASSKY, A. V., TITOV, K. G., SYLWESTER, J., GBUREK, S. and PODGÓRSKI, P., 2013. Results of the first tests of the SIDRA satellite-borne instrument breadboard model. Problems of Atomic Science and Technology, Series "Nuclear Physics Investigations" , vol. 3(85), no. 60, pp. 297–302. 25. PRIETO, M., DUDNIK, O. V., SANCHEZ, S., KURBATOV, E. V., TIMAKOVA, T. G., TEJEDOR, J. I. G. and TITOV, K. G., 2013. Breadboard model of the SIDRA instrument designed for the measurement of charged particle fluxes in space. J. Instrum., vol. 8, no. 04, id. T04002. DOI: https://doi.org/10.1088/1748-0221/8/04/T04002 26. ANDRYUSHENKO, L. A., TARASOV, V. O., GRINYOV, B. V., DUDNIK, O. V. and KURBATOV, E. V., 2013. Scintillation detector on the base of organic crystal . Patent of Ukraine UA 86274 U (in Ukrainian). 27. KURBATOV, E. V., DUDNIK, O. V., TITOV, K. G., ANDRYUSHENKO, L. A., BOYARINTSEV A. YU., TARASOV, V. A. and VALTONEN, E., 2013. Comparative characteristics of assemblies of small-sized p-terphenyl scintillators and silicon photodetectors. In: XI Conference on high energy physics, nuclear physics and accelerators Abstracts . Kharkiv, Ukraine, 11-15 March, 2013. Kharkiv, Ukraine: National Science Center "Kharkov Institute of Physics and Technology", P. 99.

Récupéré en direct depuis OpenAlex et désinversé. Les résumés ne sont pas conservés dans cette base de données : les index inversés représentent 8,6 Go des 9,3 Go de texte de la base, et le serveur dispose de 13 Go libres.

Comment cette classification a été obtenuedéplier

Prédiction distillée sur la base complète

Imitation des enseignants

Ni prévalence calibrée, ni vérité terrain. Validation humaine à venir. Apprise à partir de 10 348 étiquettes directes de Codex et de 10 348 étiquettes directes de Gemma. Le mode candidate est l'union des têtes enseignantes seuillées; le consensus est leur intersection. Ces sorties portent le statut machine_predicted_unvalidated et ne sont ni des étiquettes humaines ni des étiquettes directes de modèles de pointe.

score de la tête « metaresearch » (Codex)0,000
score de la tête « metaresearch » (Gemma)0,000
Version: codex-gemma-dda1882f352aStatut de validation: machine_predicted_unvalidated
Catégories candidatesaucune
Catégories consensuellesaucune
DomaineSignal candidat: aucune · Signal consensuel: aucune
Devis d'étudeSignal candidat: Autre devis · Signal consensuel: aucune
GenreSignal candidat: Empirique · Signal consensuel: Empirique
Score de désaccord entre enseignants0,592
Score d'incertitude au seuil0,514

Scores Codex et Gemma par catégorie

CatégorieCodexGemma
Métarecherche0,0000,000
Méta-épidémiologie (sens strict)0,0000,000
Méta-épidémiologie (sens large)0,0000,000
Bibliométrie0,0000,000
Études des sciences et des technologies0,0000,000
Communication savante0,0000,000
Science ouverte0,0000,000
Intégrité de la recherche0,0000,000
Charge utile insuffisante (le modèle a refusé de juger)0,0000,000

Scores machine (provisoires)

Les deux têtes enseignantes du modèle étudiant, lues sur ce travail. Un score ordonne la base pour la relecture; il n'affirme jamais une catégorie, et le statut de validation accompagne chaque rangée tel quel.

Scores de référence d'un modèle non mature (critères de maturité non atteints, 7 itérations). Un score ordonne; il n'affirme jamais une catégorie.

Tête enseignante Opus0,010
Tête enseignante GPT0,222
Écart entre enseignants0,212 · la distance entre les deux têtes enseignantes sur ce seul travail
Statut de validationscore_only:v0-immature-baseline · tel quel depuis la passe de notation : score_only signifie que le nombre peut ordonner les travaux, et qu'aucune étiquette de catégorie n'en découle

Classification

machine, non validée

Prédiction automatique; un appel candidat d’une seule tête enseignante, pas un consensus.

Les modèles n’ont appliqué aucune catégorie : rien dans la taxonomie ne correspondait à ce travail.
Devis d'étudeAutre devis
Domainenon disponible
GenreEmpirique

Le détail, modèle par modèle et score par score, se trouve en fin de page sous « Comment cette classification a été obtenue ».

En bref

Citations1
Publié2015
Routes d'admission1
Résumé présentoui

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Même revueRadio physics and radio astronomyMême sujetSolar and Space Plasma DynamicsTravaux en français237 207