Chupp E L (13 results)
Published by J Geophys Res 1967
- Softcover
- Periodical
Seller: Larry W Price Books, Portland, OR, U.S.A.Larry W Price Books
Contact seller5-star sellerCondition: Used - Very good
US$ 6.90
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Pamphlet. Condition: Very Good. Vol 72, No 15, pp. 3809-3816, Illus, Extracted from orig vol, thus begins with title page, trimmed & stapoled pamphlet, else VG.
CANNERY PEAS - BULLETIN 485, WAR EMERGENCY BULLETIN 4, MARCH 1942
Bond, M.C. & Chupp, Charles & Glasgow, Hugh & Leiby, R.W. & Mcnew, G.L. & Raymond, C.B. & Robinson, M.E. & Sayre, C.B.
Published by Cornell University, Ithaca, New York 1942
Seller: Neil Shillington: Bookdealer/Booksearch, hobe sound, FL, U.S.A.Neil Shillington: Bookdealer/Booksearch
Contact seller4-star sellerCondition: Used - Good
US$ 5.81
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Pamphlet. Condition: Good+. 4 pages.

- Hardcover
Seller: Anybook.com, Lincoln, United KingdomAnybook.com
Contact seller5-star sellerCondition: Used - Fair
US$ 13.53
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Condition: Fair. Volume 14. This is an ex-library book and may have the usual library/used-book markings inside.This book has hardback covers. In fair condition, suitable as a study copy. No dust jacket. Please note the Image in this listing is a stock photo and may not match the covers of the actual item,850grams, ISBN:90277069…56.

- Hardcover
Seller: Anybook.com, Lincoln, United KingdomAnybook.com
Contact seller5-star sellerCondition: Used - Good
US$ 16.22
US$ 17.95 shippingShips from United Kingdom to U.S.A.Quantity: 1 available
Condition: Good. Volume 14. This is an ex-library book and may have the usual library/used-book markings inside.This book has hardback covers. In good all round condition. No dust jacket. Please note the Image in this listing is a stock photo and may not match the covers of the actual item,850grams, ISBN:9027706956.
Language: English
Published by Dordrecht, Reidel, 1976
- Softcover
- First Edition
Seller: Buch & Cafe Antiquarius, Bonn, NRW, GermanyBuch & Cafe Antiquarius
Contact seller5-star sellerAssociation member: GIAQ
Condition: Used
US$ 29.32
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8°, original softcover. 1. ed. With numerous illustr., X, 317 p. Shelfmark on spine, stamp, otherwise fine copy. Sprache: Englisch Gewicht in Gramm: 0.

- Softcover
- First Edition
Seller: books4less (Versandantiquariat Petra Gros GmbH & Co. KG), Welling, Germanybooks4less (Versandantiquariat Petra Gros GmbH & Co. KG)
Contact seller5-star sellerCondition: Used - Very good
US$ 99.68
US$ 18.16 shippingShips from Germany to U.S.A.Quantity: 1 available
gebundene Ausgabe. Condition: Gut. 1. Ed. 317 Seiten; Der Erhaltungszustand des hier angebotenen Werks ist trotz seiner Bibliotheksnutzung sehr sauber. Es befindet sich neben dem Rückenschild lediglich ein Bibliotheksstempel im Buch; ordnungsgemäß entwidmet. In ENGLISCHER Sprache. Sprache: Englisch Gewicht in Gramm: 780.

- Softcover
Seller: Ria Christie Collections, Uxbridge, United KingdomRia Christie Collections
Contact seller5-star sellerCondition: New
US$ 131.70
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Condition: New. In.

- Softcover
Seller: moluna, Greven, Germanymoluna
Contact seller5-star sellerCondition: New
US$ 108.21
US$ 55.78 shippingShips from Germany to U.S.A.Quantity: Over 20 available
Kartoniert / Broschiert. Condition: New.
More images- Softcover
Seller: preigu, Osnabrück, Germanypreigu
Contact seller5-star sellerCondition: New
US$ 112.23
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Taschenbuch. Condition: Neu. Gamma-Ray Astronomy | Nuclear Transition Region | E. L. Chupp | Taschenbuch | 336 S. | Englisch | 1976 | Springer Netherland | EAN 9789027706966 | Verantwortliche Person für die EU: Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg, juergen[dot]hartmann[at]springer[dot]com | Anbieter: preigu.

Language: English
Published by Springer Netherlands, Springer Netherlands 1976
- Softcover
Seller: AHA-BUCH GmbH, Einbeck, GermanyAHA-BUCH GmbH
Contact seller5-star sellerCondition: New
US$ 134.12
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Taschenbuch. Condition: Neu. Druck auf Anfrage Neuware - Printed after ordering - Observation of discrete energy electromagnetic emissions from celestial objects in the radio, IR, optical, lN, and X-ray spectral regions has dramatically advanced our know ledge in the field of astrophysics. It is expected that identification of n…uclear 'Y-ray line emissions from any cosmic source would also prove to be a powerful new tool for probing the Universe. Since the publication of Morrison's work in 1958, many experiments were carried out searching for evidence of 'Y-ray lines from cosmic sources, however with little success. Only a few positive experimental results have been reported, in spite of an expenditure of considerable effort by many people: in particular, the possible Galactic Center emission line (473 to 530keV) and 'Y-ray lines at several energies (e. g. , 0. 5 MeV and 2. 2 MeV) associated with large solar flares. Both of these observations are unconfirmed by indepen dent observations (ca. 1975). The high energy 'Y-rays (30MeV) from the Galactic Center are at least partly due to the decay of 1[0 mesons, which are of unique energy (67. 5 MeV) in the 1[0 rest frame only. The reasons for the limited amount of data avail able in this field, even though early theoretical predictions were very optimistic regarding fluxes of nuclear lines, are that experimental efforts are plagued with high backgrounds and low fluxes, and that development of instruments with telescopic properties in the energy range of interest is difficult.

- Softcover
Seller: Mispah books, Redhill, SURRE, United KingdomMispah books
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US$ 186.23
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Paperback. Condition: Very Good. Very Good. book.

Language: English
Published by Springer Netherlands, Springer Netherlands Dez 1976 1976
- Softcover
- Print on Demand
Seller: buchversandmimpf2000, Emtmannsberg, BAYE, Germanybuchversandmimpf2000
Contact seller5-star sellerCondition: New
US$ 125.47
US$ 68.32 shippingShips from Germany to U.S.A.Quantity: 1 available
Taschenbuch. Condition: Neu. This item is printed on demand - Print on Demand Titel. Neuware -Observation of discrete energy electromagnetic emissions from celestial objects in the radio, IR, optical, lN, and X-ray spectral regions has dramatically advanced our know ledge in the field of astrophysics. It is expected that identif…ication of nuclear 'Y-ray line emissions from any cosmic source would also prove to be a powerful new tool for probing the Universe. Since the publication of Morrison's work in 1958, many experiments were carried out searching for evidence of 'Y-ray lines from cosmic sources, however with little success. Only a few positive experimental results have been reported, in spite of an expenditure of considerable effort by many people: in particular, the possible Galactic Center emission line (473 to 530keV) and 'Y-ray lines at several energies (e. g. , 0. 5 MeV and 2. 2 MeV) associated with large solar flares. Both of these observations are unconfirmed by indepen dent observations (ca. 1975). The high energy 'Y-rays (>30MeV) from the Galactic Center are at least partly due to the decay of 1[0 mesons, which are of unique energy (67. 5 MeV) in the 1[0 rest frame only. The reasons for the limited amount of data avail able in this field, even though early theoretical predictions were very optimistic regarding fluxes of nuclear lines, are that experimental efforts are plagued with high backgrounds and low fluxes, and that development of instruments with telescopic properties in the energy range of interest is difficult.Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg 336 pp. Englisch.

- Softcover
- Print on Demand
Seller: BuchWeltWeit Ludwig Meier e.K., Bergisch Gladbach, GermanyBuchWeltWeit Ludwig Meier e.K.
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US$ 181.94
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Taschenbuch. Condition: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -Observation of discrete energy electromagnetic emissions from celestial objects in the radio, IR, optical, lN, and X-ray spectral regions has dramatically advanced our know ledge in the field of astrophysics. It is expected that ide…ntification of nuclear 'Y-ray line emissions from any cosmic source would also prove to be a powerful new tool for probing the Universe. Since the publication of Morrison's work in 1958, many experiments were carried out searching for evidence of 'Y-ray lines from cosmic sources, however with little success. Only a few positive experimental results have been reported, in spite of an expenditure of considerable effort by many people: in particular, the possible Galactic Center emission line (473 to 530keV) and 'Y-ray lines at several energies (e. g. , 0. 5 MeV and 2. 2 MeV) associated with large solar flares. Both of these observations are unconfirmed by indepen dent observations (ca. 1975). The high energy 'Y-rays (30MeV) from the Galactic Center are at least partly due to the decay of 1[0 mesons, which are of unique energy (67. 5 MeV) in the 1[0 rest frame only. The reasons for the limited amount of data avail able in this field, even though early theoretical predictions were very optimistic regarding fluxes of nuclear lines, are that experimental efforts are plagued with high backgrounds and low fluxes, and that development of instruments with telescopic properties in the energy range of interest is difficult. 336 pp. Englisch.