Instruments and Methods for the Radio Detection of High Energy Cosmic Rays:
Gespeichert in:
Format: | Elektronisch E-Book |
---|---|
Sprache: | English |
Veröffentlicht: |
Berlin, Heidelberg
Springer Berlin Heidelberg
2012
|
Schriftenreihe: | Springer Theses, Recognizing Outstanding Ph.D. Research
|
Schlagworte: | |
Online-Zugang: | TUM01 UBT01 Volltext |
Beschreibung: | Cosmic Rays -- Radio Experiments for Air Shower Detection -- Time Calibration of LOPES -- A Reference Beacon for the Auger Engineering Radio Array -- Treatment of Noise -- Lateral Distribution -- Pulse Arrival Time Distributions Cosmic rays consist of elementary particles with enormous energy which originate from outside our solar system and constantly hit the Earth’s atmosphere. Where do these cosmic rays originate? How does nature accelerate the cosmic-ray particles to energies with orders of magnitude beyond the limits of manmade particle accelerators? What can we learn by measuring the interactions of the cosmic rays with the atmosphere? Digital radio-antenna arrays offer a promising, complementary measurement method for high-energy cosmic rays. This thesis reports on substantial advances in the development of the radio technique, which will be used to address these questions in future experiments. |
Beschreibung: | 1 Online-Ressource |
ISBN: | 9783642336607 |
DOI: | 10.1007/978-3-642-33660-7 |
Internformat
MARC
LEADER | 00000nmm a2200000zc 4500 | ||
---|---|---|---|
001 | BV040751394 | ||
003 | DE-604 | ||
005 | 00000000000000.0 | ||
007 | cr|uuu---uuuuu | ||
008 | 130214s2012 |||| o||u| ||||||eng d | ||
020 | |a 9783642336607 |9 978-3-642-33660-7 | ||
024 | 7 | |a 10.1007/978-3-642-33660-7 |2 doi | |
035 | |a (OCoLC)864111589 | ||
035 | |a (DE-599)BVBBV040751394 | ||
040 | |a DE-604 |b ger |e aacr | ||
041 | 0 | |a eng | |
049 | |a DE-703 |a DE-91 | ||
084 | |a PHY 000 |2 stub | ||
245 | 1 | 0 | |a Instruments and Methods for the Radio Detection of High Energy Cosmic Rays |c by Frank G. Schröder |
264 | 1 | |a Berlin, Heidelberg |b Springer Berlin Heidelberg |c 2012 | |
300 | |a 1 Online-Ressource | ||
336 | |b txt |2 rdacontent | ||
337 | |b c |2 rdamedia | ||
338 | |b cr |2 rdacarrier | ||
490 | 0 | |a Springer Theses, Recognizing Outstanding Ph.D. Research | |
500 | |a Cosmic Rays -- Radio Experiments for Air Shower Detection -- Time Calibration of LOPES -- A Reference Beacon for the Auger Engineering Radio Array -- Treatment of Noise -- Lateral Distribution -- Pulse Arrival Time Distributions | ||
500 | |a Cosmic rays consist of elementary particles with enormous energy which originate from outside our solar system and constantly hit the Earth’s atmosphere. Where do these cosmic rays originate? How does nature accelerate the cosmic-ray particles to energies with orders of magnitude beyond the limits of manmade particle accelerators? What can we learn by measuring the interactions of the cosmic rays with the atmosphere? Digital radio-antenna arrays offer a promising, complementary measurement method for high-energy cosmic rays. This thesis reports on substantial advances in the development of the radio technique, which will be used to address these questions in future experiments. | ||
650 | 4 | |a Physics | |
650 | 4 | |a Astrophysics and Astroparticles | |
650 | 4 | |a Particle and Nuclear Physics | |
700 | 1 | |a Schröder, Frank G. |e Sonstige |4 oth | |
856 | 4 | 0 | |u https://doi.org/10.1007/978-3-642-33660-7 |x Verlag |3 Volltext |
912 | |a ZDB-2-PHA | ||
999 | |a oai:aleph.bib-bvb.de:BVB01-025731146 | ||
966 | e | |u https://doi.org/10.1007/978-3-642-33660-7 |l TUM01 |p ZDB-2-PHA |x Verlag |3 Volltext | |
966 | e | |u https://doi.org/10.1007/978-3-642-33660-7 |l UBT01 |p ZDB-2-PHA |x Verlag |3 Volltext |
Datensatz im Suchindex
_version_ | 1804150074835468288 |
---|---|
any_adam_object | |
building | Verbundindex |
bvnumber | BV040751394 |
classification_tum | PHY 000 |
collection | ZDB-2-PHA |
ctrlnum | (OCoLC)864111589 (DE-599)BVBBV040751394 |
discipline | Physik |
doi_str_mv | 10.1007/978-3-642-33660-7 |
format | Electronic eBook |
fullrecord | <?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>02302nmm a2200397zc 4500</leader><controlfield tag="001">BV040751394</controlfield><controlfield tag="003">DE-604</controlfield><controlfield tag="005">00000000000000.0</controlfield><controlfield tag="007">cr|uuu---uuuuu</controlfield><controlfield tag="008">130214s2012 |||| o||u| ||||||eng d</controlfield><datafield tag="020" ind1=" " ind2=" "><subfield code="a">9783642336607</subfield><subfield code="9">978-3-642-33660-7</subfield></datafield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/978-3-642-33660-7</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(OCoLC)864111589</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)BVBBV040751394</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-604</subfield><subfield code="b">ger</subfield><subfield code="e">aacr</subfield></datafield><datafield tag="041" ind1="0" ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="049" ind1=" " ind2=" "><subfield code="a">DE-703</subfield><subfield code="a">DE-91</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">PHY 000</subfield><subfield code="2">stub</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Instruments and Methods for the Radio Detection of High Energy Cosmic Rays</subfield><subfield code="c">by Frank G. Schröder</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="a">Berlin, Heidelberg</subfield><subfield code="b">Springer Berlin Heidelberg</subfield><subfield code="c">2012</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">1 Online-Ressource</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="490" ind1="0" ind2=" "><subfield code="a">Springer Theses, Recognizing Outstanding Ph.D. Research</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">Cosmic Rays -- Radio Experiments for Air Shower Detection -- Time Calibration of LOPES -- A Reference Beacon for the Auger Engineering Radio Array -- Treatment of Noise -- Lateral Distribution -- Pulse Arrival Time Distributions</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">Cosmic rays consist of elementary particles with enormous energy which originate from outside our solar system and constantly hit the Earth’s atmosphere. Where do these cosmic rays originate? How does nature accelerate the cosmic-ray particles to energies with orders of magnitude beyond the limits of manmade particle accelerators? What can we learn by measuring the interactions of the cosmic rays with the atmosphere? Digital radio-antenna arrays offer a promising, complementary measurement method for high-energy cosmic rays. This thesis reports on substantial advances in the development of the radio technique, which will be used to address these questions in future experiments.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Physics</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Astrophysics and Astroparticles</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Particle and Nuclear Physics</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Schröder, Frank G.</subfield><subfield code="e">Sonstige</subfield><subfield code="4">oth</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://doi.org/10.1007/978-3-642-33660-7</subfield><subfield code="x">Verlag</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">ZDB-2-PHA</subfield></datafield><datafield tag="999" ind1=" " ind2=" "><subfield code="a">oai:aleph.bib-bvb.de:BVB01-025731146</subfield></datafield><datafield tag="966" ind1="e" ind2=" "><subfield code="u">https://doi.org/10.1007/978-3-642-33660-7</subfield><subfield code="l">TUM01</subfield><subfield code="p">ZDB-2-PHA</subfield><subfield code="x">Verlag</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="966" ind1="e" ind2=" "><subfield code="u">https://doi.org/10.1007/978-3-642-33660-7</subfield><subfield code="l">UBT01</subfield><subfield code="p">ZDB-2-PHA</subfield><subfield code="x">Verlag</subfield><subfield code="3">Volltext</subfield></datafield></record></collection> |
id | DE-604.BV040751394 |
illustrated | Not Illustrated |
indexdate | 2024-07-10T00:33:09Z |
institution | BVB |
isbn | 9783642336607 |
language | English |
oai_aleph_id | oai:aleph.bib-bvb.de:BVB01-025731146 |
oclc_num | 864111589 |
open_access_boolean | |
owner | DE-703 DE-91 DE-BY-TUM |
owner_facet | DE-703 DE-91 DE-BY-TUM |
physical | 1 Online-Ressource |
psigel | ZDB-2-PHA |
publishDate | 2012 |
publishDateSearch | 2012 |
publishDateSort | 2012 |
publisher | Springer Berlin Heidelberg |
record_format | marc |
series2 | Springer Theses, Recognizing Outstanding Ph.D. Research |
spelling | Instruments and Methods for the Radio Detection of High Energy Cosmic Rays by Frank G. Schröder Berlin, Heidelberg Springer Berlin Heidelberg 2012 1 Online-Ressource txt rdacontent c rdamedia cr rdacarrier Springer Theses, Recognizing Outstanding Ph.D. Research Cosmic Rays -- Radio Experiments for Air Shower Detection -- Time Calibration of LOPES -- A Reference Beacon for the Auger Engineering Radio Array -- Treatment of Noise -- Lateral Distribution -- Pulse Arrival Time Distributions Cosmic rays consist of elementary particles with enormous energy which originate from outside our solar system and constantly hit the Earth’s atmosphere. Where do these cosmic rays originate? How does nature accelerate the cosmic-ray particles to energies with orders of magnitude beyond the limits of manmade particle accelerators? What can we learn by measuring the interactions of the cosmic rays with the atmosphere? Digital radio-antenna arrays offer a promising, complementary measurement method for high-energy cosmic rays. This thesis reports on substantial advances in the development of the radio technique, which will be used to address these questions in future experiments. Physics Astrophysics and Astroparticles Particle and Nuclear Physics Schröder, Frank G. Sonstige oth https://doi.org/10.1007/978-3-642-33660-7 Verlag Volltext |
spellingShingle | Instruments and Methods for the Radio Detection of High Energy Cosmic Rays Physics Astrophysics and Astroparticles Particle and Nuclear Physics |
title | Instruments and Methods for the Radio Detection of High Energy Cosmic Rays |
title_auth | Instruments and Methods for the Radio Detection of High Energy Cosmic Rays |
title_exact_search | Instruments and Methods for the Radio Detection of High Energy Cosmic Rays |
title_full | Instruments and Methods for the Radio Detection of High Energy Cosmic Rays by Frank G. Schröder |
title_fullStr | Instruments and Methods for the Radio Detection of High Energy Cosmic Rays by Frank G. Schröder |
title_full_unstemmed | Instruments and Methods for the Radio Detection of High Energy Cosmic Rays by Frank G. Schröder |
title_short | Instruments and Methods for the Radio Detection of High Energy Cosmic Rays |
title_sort | instruments and methods for the radio detection of high energy cosmic rays |
topic | Physics Astrophysics and Astroparticles Particle and Nuclear Physics |
topic_facet | Physics Astrophysics and Astroparticles Particle and Nuclear Physics |
url | https://doi.org/10.1007/978-3-642-33660-7 |
work_keys_str_mv | AT schroderfrankg instrumentsandmethodsfortheradiodetectionofhighenergycosmicrays |