Wide angle air Cerenkov detectors

Abstract For a number of important questions in VHE/UHE cosmic ray physics wide angle air Cerenkov detectors offer superior performance compared to scintillator arrays or air Cerenkov telescopes. On hand of the HEGRA air Cerenkov detector AIROBICC the general principle and performance will be discus...
Ausführliche Beschreibung

Gespeichert in:

Autor*in:	Lorenz, E. [verfasserIn]

Format:	Artikel
Sprache:	Englisch

Erschienen:	1996

Schlagwörter:	General Principle Superior Performance Energy Threshold Wide Angle Cerenkov Detector

Anmerkung:	© Kluwer Academic Publishers 1996

Übergeordnetes Werk:	Enthalten in: Space science reviews - Kluwer Academic Publishers, 1962, 75(1996), 1-2 vom: Jan., Seite 169-183
Übergeordnetes Werk:	volume:75 ; year:1996 ; number:1-2 ; month:01 ; pages:169-183

Links:	Volltext

DOI / URN:	10.1007/BF00195033

Katalog-ID:	OLC2033678318

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allfields	10.1007/BF00195033 doi (DE-627)OLC2033678318 (DE-He213)BF00195033-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Lorenz, E. verfasserin aut Wide angle air Cerenkov detectors 1996 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1996 Abstract For a number of important questions in VHE/UHE cosmic ray physics wide angle air Cerenkov detectors offer superior performance compared to scintillator arrays or air Cerenkov telescopes. On hand of the HEGRA air Cerenkov detector AIROBICC the general principle and performance will be discussed. Ideas and prospects for a detector with an energy threshold around 1 to 3 TeV will be presented. General Principle Superior Performance Energy Threshold Wide Angle Cerenkov Detector Enthalten in Space science reviews Kluwer Academic Publishers, 1962 75(1996), 1-2 vom: Jan., Seite 169-183 (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:75 year:1996 number:1-2 month:01 pages:169-183 https://doi.org/10.1007/BF00195033 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_24 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4306 GBV_ILN_4700 AR 75 1996 1-2 01 169-183
spelling	10.1007/BF00195033 doi (DE-627)OLC2033678318 (DE-He213)BF00195033-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Lorenz, E. verfasserin aut Wide angle air Cerenkov detectors 1996 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1996 Abstract For a number of important questions in VHE/UHE cosmic ray physics wide angle air Cerenkov detectors offer superior performance compared to scintillator arrays or air Cerenkov telescopes. On hand of the HEGRA air Cerenkov detector AIROBICC the general principle and performance will be discussed. Ideas and prospects for a detector with an energy threshold around 1 to 3 TeV will be presented. General Principle Superior Performance Energy Threshold Wide Angle Cerenkov Detector Enthalten in Space science reviews Kluwer Academic Publishers, 1962 75(1996), 1-2 vom: Jan., Seite 169-183 (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:75 year:1996 number:1-2 month:01 pages:169-183 https://doi.org/10.1007/BF00195033 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_24 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4306 GBV_ILN_4700 AR 75 1996 1-2 01 169-183
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allfieldsGer	10.1007/BF00195033 doi (DE-627)OLC2033678318 (DE-He213)BF00195033-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Lorenz, E. verfasserin aut Wide angle air Cerenkov detectors 1996 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1996 Abstract For a number of important questions in VHE/UHE cosmic ray physics wide angle air Cerenkov detectors offer superior performance compared to scintillator arrays or air Cerenkov telescopes. On hand of the HEGRA air Cerenkov detector AIROBICC the general principle and performance will be discussed. Ideas and prospects for a detector with an energy threshold around 1 to 3 TeV will be presented. General Principle Superior Performance Energy Threshold Wide Angle Cerenkov Detector Enthalten in Space science reviews Kluwer Academic Publishers, 1962 75(1996), 1-2 vom: Jan., Seite 169-183 (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:75 year:1996 number:1-2 month:01 pages:169-183 https://doi.org/10.1007/BF00195033 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_24 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4306 GBV_ILN_4700 AR 75 1996 1-2 01 169-183
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abstract	Abstract For a number of important questions in VHE/UHE cosmic ray physics wide angle air Cerenkov detectors offer superior performance compared to scintillator arrays or air Cerenkov telescopes. On hand of the HEGRA air Cerenkov detector AIROBICC the general principle and performance will be discussed. Ideas and prospects for a detector with an energy threshold around 1 to 3 TeV will be presented. © Kluwer Academic Publishers 1996
abstractGer	Abstract For a number of important questions in VHE/UHE cosmic ray physics wide angle air Cerenkov detectors offer superior performance compared to scintillator arrays or air Cerenkov telescopes. On hand of the HEGRA air Cerenkov detector AIROBICC the general principle and performance will be discussed. Ideas and prospects for a detector with an energy threshold around 1 to 3 TeV will be presented. © Kluwer Academic Publishers 1996
abstract_unstemmed	Abstract For a number of important questions in VHE/UHE cosmic ray physics wide angle air Cerenkov detectors offer superior performance compared to scintillator arrays or air Cerenkov telescopes. On hand of the HEGRA air Cerenkov detector AIROBICC the general principle and performance will be discussed. Ideas and prospects for a detector with an energy threshold around 1 to 3 TeV will be presented. © Kluwer Academic Publishers 1996
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up_date	2024-07-03T17:58:37.954Z
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