lallement r (36 risultati)

Condizione: good. Lallement, Jennifer N (illustratore). This book is in good condition with very minimal damage. Pages may have minimal notes or highlighting. Cover image on the book may vary from photo. Ships out quickly in a secure plastic mailer.

Softcover. Condizione: Très bon. Edition 2015. Ammareal reverse jusqu'à 15% du prix net de cet article à des organisations caritatives. ENGLISH DESCRIPTION Book Condition: Used, Very good. Edition 2015. Ammareal gives back up to 15% of this item's net price to charity organizations.

Paperback. Condizione: Brand New. Lallement, Jennifer N (illustratore). 52 pages. 8.25x8.25x0.13 inches. In Stock.

paperback. Condizione: Good. Our good condition books are generally good for reading but not for gifting or collecting. They could have imperfections such as creasing, fanning, inscriptions, margin notes, yellowing, staining on edge or cover or pages, bumps, scuffs, etc etc (sometimes multiple of these). It's a wide category that encompasses anything that isn't almost-new down to anything that is slightly better than poor. We would NOT recommend gifting Good books - these should be considered reading copies. Our books are dispatched from a Yorkshire former cotton mill. We list via barcode/ISBN so please note that the images are stock images and may not be the exact copy you receive, furthermore the details about edition and year might not be accurate as many publishers reuse the same ISBN for multiple editions and as we simply scan a barcode or enter an ISBN we do not check the validity of the edition data when listing. If you're looking for an exact edition please don't order (at least not without checking with us first, although we don't always have time to check). We aim to dispatch prompty, the service used will depend on order value and book size. We can ship to most countries, see our shipping policies. Payment is via Abe only.

Pictorial Sofcover. Condizione: Good. No Jacket. ships from U.K spine creased, pages clean.Heavy book,will require extra overseas shipping Size: 8 Vo.

couverture souple illustrée. Condizione: Bon exemplaire. 330 pp. Photographies en noir. Cartes.

Hardcover. Condizione: Sehr gut. 413 p. Stamp to front endpaper, else as new. ISBN: 9780792343202 Sprache: Englisch Gewicht in Gramm: 863.

Broché. Condizione: Etat moyen. in-8 Description :Pages 424-482. Tampons de bibliothèque. Soulignements au bic. Déchirures avec manques sur la couverture. Langue : français Nb de volumes : 1.

Hardcover. Condizione: Gut bis sehr gut. GERINGE LAGERSPUREN, SONST SEHR GUT nur a 815 -a-950.

Condizione: New. In.

Condizione: New. In.

Condizione: New.

Condizione: New.

Condizione: New.

Condizione: As New. Unread book in perfect condition.

Condizione: As New. Unread book in perfect condition.

Condizione: New. 2017. 1st Edition. Hardcover. . . . . .

Condizione: New. Gives an overview of knowledge about the local interstellar medium (LISM) surrounding our heliosphere (HS). This volume is the result of the first workshop at ISSI, where both space physicists and astronomers presented their views on the density, velocity, temperature, composition, and morphology of the LISM and how it interacts with the HS. Editor(s): von Steiger, Rudolf; Lallement, R.; Lee, M. A. Series: Space Sciences Series of ISSI. Num Pages: 413 pages, biography. BIC Classification: PGM; PGS. Category: (UP) Postgraduate, Research & Scholarly; (UU) Undergraduate. Dimension: 235 x 155 x 24. Weight in Grams: 866. . 1996. Hardback. . . . .

Condizione: New. pp. 399.

Taschenbuch. Condizione: Neu. The Heliosphere in the Local Interstellar Medium | Proceedings of the First ISSI Workshop 6-10 November 1995, Bern, Switzerland | Rudolf Von Steiger (u. a.) | Taschenbuch | Space Sciences Series of ISSI | xiv | Englisch | 2011 | Springer | EAN 9789401072960 | Verantwortliche Person für die EU: Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg, juergen[dot]hartmann[at]springer[dot]com | Anbieter: preigu.

Gebunden. Condizione: New.

Taschenbuch. Condizione: Neu. Druck auf Anfrage Neuware - Printed after ordering - In summary, we can conclude that the contributions of the different ionization processes to the total ionization rate for the most abundant interstellar species are basically known. The ionization of the noble gases He and Ne is almost completely dominated by photoionization, whereas for H charge-exchange with the solar wind is most important. For other species, such as 0 and Ar, both processes contribute significantly. Electron impact ionization can typically contribute by '' 10% to the total rate in the inner Solar System. Because direct measurements of the solar EUV flux are not yet continuously available, the variation of the ionization rate over the solar cycle still contains a relatively large uncertainty. The recent measurements of pickup ion distributions and of the neutral helium gas provide an independent tool to determine the total ionization rate that can be used to cross calibrate with the results obtained for the individual ionization processes. Acknowledgements The authors are grateful to M. Allen for supplying us with new data on photoioniza tion cross-sections compiled by him. We thank also M. Gruntman for drawing our attention to and support in collecting the most recent data on charge-exchange cross-sections. D. R. was supported by grant No. 2 P03C. 004. 09 from the Com mittee for Scientific Research (Poland). This work was also supported in part through NASA contract NAS7-918, NSF Grant INT-911637, NASA Grant NAGW- 2579.

Buch. Condizione: Neu. Druck auf Anfrage Neuware - Printed after ordering - In summary, we can conclude that the contributions of the different ionization processes to the total ionization rate for the most abundant interstellar species are basically known. The ionization of the noble gases He and Ne is almost completely dominated by photoionization, whereas for H charge-exchange with the solar wind is most important. For other species, such as 0 and Ar, both processes contribute significantly. Electron impact ionization can typically contribute by '' 10% to the total rate in the inner Solar System. Because direct measurements of the solar EUV flux are not yet continuously available, the variation of the ionization rate over the solar cycle still contains a relatively large uncertainty. The recent measurements of pickup ion distributions and of the neutral helium gas provide an independent tool to determine the total ionization rate that can be used to cross calibrate with the results obtained for the individual ionization processes. Acknowledgements The authors are grateful to M. Allen for supplying us with new data on photoioniza tion cross-sections compiled by him. We thank also M. Gruntman for drawing our attention to and support in collecting the most recent data on charge-exchange cross-sections. D. R. was supported by grant No. 2 P03C. 004. 09 from the Com mittee for Scientific Research (Poland). This work was also supported in part through NASA contract NAS7-918, NSF Grant INT-911637, NASA Grant NAGW- 2579.

Paperback. Condizione: Brand New. reprint edition. 414 pages. 9.44x6.31x0.94 inches. In Stock.

Hardcover. Condizione: Brand New. 1st edition. 398 pages. 10.00x6.75x1.00 inches. In Stock.

Paperback. Condizione: Like New. Like New. book.

Condizione: New. Gives an overview of knowledge about the local interstellar medium (LISM) surrounding our heliosphere (HS). This volume is the result of the first workshop at ISSI, where both space physicists and astronomers presented their views on the density, velocity, temperature, composition, and morphology of the LISM and how it interacts with the HS. Editor(s): von Steiger, Rudolf; Lallement, R.; Lee, M. A. Series: Space Sciences Series of ISSI. Num Pages: 413 pages, biography. BIC Classification: PGM; PGS. Category: (UP) Postgraduate, Research & Scholarly; (UU) Undergraduate. Dimension: 235 x 155 x 24. Weight in Grams: 866. . 1996. Hardback. . . . . Books ship from the US and Ireland.

Condizione: new. Questo è un articolo print on demand.

Buch. Condizione: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -In summary, we can conclude that the contributions of the different ionization processes to the total ionization rate for the most abundant interstellar species are basically known. The ionization of the noble gases He and Ne is almost completely dominated by photoionization, whereas for H charge-exchange with the solar wind is most important. For other species, such as 0 and Ar, both processes contribute significantly. Electron impact ionization can typically contribute by '' 10% to the total rate in the inner Solar System. Because direct measurements of the solar EUV flux are not yet continuously available, the variation of the ionization rate over the solar cycle still contains a relatively large uncertainty. The recent measurements of pickup ion distributions and of the neutral helium gas provide an independent tool to determine the total ionization rate that can be used to cross calibrate with the results obtained for the individual ionization processes. Acknowledgements The authors are grateful to M. Allen for supplying us with new data on photoioniza tion cross-sections compiled by him. We thank also M. Gruntman for drawing our attention to and support in collecting the most recent data on charge-exchange cross-sections. D. R. was supported by grant No. 2 P03C. 004. 09 from the Com mittee for Scientific Research (Poland). This work was also supported in part through NASA contract NAS7-918, NSF Grant INT-911637, NASA Grant NAGW- 2579. 420 pp. Englisch.

Taschenbuch. Condizione: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -In summary, we can conclude that the contributions of the different ionization processes to the total ionization rate for the most abundant interstellar species are basically known. The ionization of the noble gases He and Ne is almost completely dominated by photoionization, whereas for H charge-exchange with the solar wind is most important. For other species, such as 0 and Ar, both processes contribute significantly. Electron impact ionization can typically contribute by '' 10% to the total rate in the inner Solar System. Because direct measurements of the solar EUV flux are not yet continuously available, the variation of the ionization rate over the solar cycle still contains a relatively large uncertainty. The recent measurements of pickup ion distributions and of the neutral helium gas provide an independent tool to determine the total ionization rate that can be used to cross calibrate with the results obtained for the individual ionization processes. Acknowledgements The authors are grateful to M. Allen for supplying us with new data on photoioniza tion cross-sections compiled by him. We thank also M. Gruntman for drawing our attention to and support in collecting the most recent data on charge-exchange cross-sections. D. R. was supported by grant No. 2 P03C. 004. 09 from the Com mittee for Scientific Research (Poland). This work was also supported in part through NASA contract NAS7-918, NSF Grant INT-911637, NASA Grant NAGW- 2579. 416 pp. Englisch.