C Alex Young (36 results)

Soft Cover. Condition: Very Good. First Edition. ----------pulp magazine, digest size. Notable stories in this issue are What Thin Partitions by Clifton & Apostolides, and Humpty Dumpty (the final Baldy story) by Kuttner and Moore. Reading crease, some front cover rubbing, edgewear, pen numbers on front cover, at least a VG copy. Miller (front cover) (illustrator).…

Soft cover. Condition: Very Good. First Edition. (xii) 307 pp. Trade paperback format. Lightly rubbed on the corners with a flat uncreased spine; no interior markings. Wraparound cover art by Michael Carroll. Subtitled: Tales of Mars from the Magazine of Fantasy and Science Fiction. This anthology contains: We Can Remember It for You Wholesale - a novelette by Philip K. Dick; In the Hall of the Martian Kings - a novella by John Varley; The Wilderness by Ray Bradbury; Mars Is Ours by Alfred Coppel; Crime on Mars by Arthur C. Clarke; Purple Priestess of the Mad Moon by Leigh Brackett; A Rose for Ecclesiastes - a novelette by Roger Zelazny; Hellas Is Florida - a novelette by Gordon Eklund and Gregory Benford; The First Mars Mission by Robert F. Young; The Last Mars Trip by Michael Cassutt; The Great Martian Pyramid Hoax by Jerry Oltion; and Pictures from an Expedition - a novella by Alex Irvine. Size: 8vo. Michael Carroll; (illustrator). Book.…

SingleIssueMagazine. Condition: Very Good-. Vol. LII, No. 1. Edited by John W. Campbell, Jr.Cover art by Miller for "What Thin Partitions" (novelette) by Mark Clifton & Alex Apostolides. Includes "Humpty Dumpty" (novelette) by Lewis Padgett (Henry Kuttner & C. L. Moore); "Little Joe" by Algis Budrys; "The Garden in the Forest" by Robert F. Young; "Gimmick" by Katherine MacLean. Articles: "Destruction from Atomic Weapons" by Lt. Theodore S. Simpson, USAF; "Venus of Troy" by Daniel Whitton. Readers' Departments: "The Editor's Page: Emotional Senses"; "In Times to Come"; "The Analytical Laboratory"; "The Reference Library" by P. Schuyler Miller; "Brass Tacks". Illustrated by Freas, Miller, von Dongen and Vidmer. Scars at spine ends with short tear at heel; corner wear; creasing; tanning; a little musty; foredge heel bumped. Book.…

SingleIssueMagazine. Condition: Very Good. Vol. LII, No. 1. Edited by John W. Campbell, Jr.Cover art by Miller for "What Thin Partitions" (novelette) by Mark Clifton & Alex Apostolides. Includes "Humpty Dumpty" (novelette) by Lewis Padgett (Henry Kuttner & C. L. Moore); "Little Joe" by Algis Budrys; "The Garden in the Forest" by Robert F. Young; "Gimmick" by Katherine MacLean. Articles: "Destruction from Atomic Weapons" by Lt. Theodore S. Simpson, USAF; "Venus of Troy" by Daniel Whitton. Readers' Departments: "The Editor's Page: Emotional Senses"; "In Times to Come"; "The Analytical Laboratory"; "The Reference Library" by P. Schuyler Miller; "Brass Tacks". Illustrated by Freas, Miller, von Dongen and Vidmer. Short spine tears; edgewear; creasing. Book. …

Condition: New.

Condition: New.

Condition: As New. Unread book in perfect condition.

Condition: New. In.

Condition: New.

Condition: As New. Unread book in perfect condition.

Condition: New. In.

Condition: New.

Condition: New.

Condition: New. pp. iv + 289.

Condition: New. 2009th edition.

Taschenbuch. Condition: Neu. Druck auf Anfrage Neuware - Printed after ordering - The SECCHI A and B instrument suites (Howard et al. , 2006) onboard the two STEREO mission spacecraft (Kaiser, 2005) are each composed of: one Extreme Ultra-Violet Imager (EUVI), two white-light coronagraphs (COR1 and COR2), and two wide-angle heliospheric imagers (HI1 and HI2). Technical descriptions of EUVI, COR1 and the HIs can be found in Wuelser et al. (2004), Thompson et al. (2003), and De se et al. (2003), respectively. The images produced by SECCHI represent a data visualization challenge: i) the images are 2048×2048 pixels (except for the HIs, which are usually binned onboard 2×2), thus the vast majority of computer displays are not able to display them at full frame and full r- olution, and ii) more importantly, the ve instruments of SECCHI A and B were designed to be able to track Coronal Mass Ejections from their onset (with EUVI) to their pro- gation in the heliosphere (with the HIs), which implies that a set of SECCHI images that covers the propagation of a CME from its initiation site to the Earth is composed of im- 1 ages with very different spatial resolutions - from 1. 7 arcsecondspixel for EUVI to 2. 15 1 arcminutespixel for HI2, i. e. 75 times larger. A similar situation exists with the angular scales of the physical objects, since the size of a CME varies by orders of magnitude as it expands in the heliosphere.…

Hardcover. Condition: Brand New. 1st edition. 292 pages. 9.30x6.30x0.60 inches. In Stock.

Paperback. Condition: Brand New. 289 pages. 9.21x6.14x0.70 inches. In Stock.

Condition: As New. Unread book in perfect condition.

Condition: Sehr gut. Zustand: Sehr gut | Seiten: 296 | Sprache: Englisch | Produktart: Bücher | The SECCHI A and B instrument suites (Howard et al. , 2006) onboard the two STEREO mission spacecraft (Kaiser, 2005) are each composed of: one Extreme Ultra-Violet Imager (EUVI), two white-light coronagraphs (COR1 and COR2), and two wide-angle heliospheric imagers (HI1 and HI2). Technical descriptions of EUVI, COR1 and the HIs can be found in Wuelser et al. (2004), Thompson et al. (2003), and De?se et al. (2003), respectively. The images produced by SECCHI represent a data visualization challenge: i) the images are 2048×2048 pixels (except for the HIs, which are usually binned onboard 2×2), thus the vast majority of computer displays are not able to display them at full frame and full r- olution, and ii) more importantly, the ?ve instruments of SECCHI A and B were designed to be able to track Coronal Mass Ejections from their onset (with EUVI) to their pro- gation in the heliosphere (with the HIs), which implies that a set of SECCHI images that covers the propagation of a CME from its initiation site to the Earth is composed of im- ?1 ages with very different spatial resolutions ¿ from 1. 7 arcsecondspixel for EUVI to 2. 15 ?1 arcminutespixel for HI2, i. e. 75 times larger. A similar situation exists with the angular scales of the physical objects, since the size of a CME varies by orders of magnitude as it expands in the heliosphere.…

Hardcover. Condition: Like New. LIKE NEW. SHIPS FROM MULTIPLE LOCATIONS. book.

Condition: As New. Unread book in perfect condition.

PAP. Condition: New. New Book. Delivered from our UK warehouse in 4 to 14 business days. THIS BOOK IS PRINTED ON DEMAND. Established seller since 2000.

Leather Bound. Condition: New. Language: English. {Size: 14.60 x 22.86 cms} Presenting an Exquisite Leather-Bound Edition, expertly crafted with Original Natural Leather that gracefully adorns the spine and corners. The allure continues with Golden Leaf Printing that adds a touch of elegance, while Hand Embossing on the rounded spine lends an artistic flair. This masterpiece has been meticulously reprinted in 2026, utilizing the invaluable guidance of the original edition published many years ago in 1803. The contents of this book are presented in classic black and white. Its durability is ensured through a meticulous sewing binding technique, enhancing its longevity. Imprinted on top-tier quality paper. A team of professionals has expertly processed each page, delicately preserving its content without alteration. Due to the vintage nature of these books, every page has been manually restored for legibility. However, in certain instances, occasional blurriness, missing segments, or faint black spots might persist. We sincerely hope for your understanding of the challenges we faced with these books. Recognizing their significance for readers seeking insight into our historical treasure, we've diligently restored and reissued them. Our intention is to offer this valuable resource once again. We eagerly await your feedback, hoping that you'll find it appealing and will generously share your thoughts and recommendations. Lang: - English, Vol:- Volume 21, Pages:- 200, Print on Demand. If it is a multi-volume set, then it is only a single volume. We are specialised in Customisation of books, if you wish to opt different color leather binding, you may contact us. This service is chargeable. Product Disclaimer: Kindly be informed that, owing to the inherent nature of leather as a natural material, minor discolorations or textural variations may be perceptible. Explore the FOLIO EDITION (12x19 Inches): Available Upon Request. Volume 21 200.…

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Buch. Condition: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -The SECCHI A and B instrument suites (Howard et al. , 2006) onboard the two STEREO mission spacecraft (Kaiser, 2005) are each composed of: one Extreme Ultra-Violet Imager (EUVI), two white-light coronagraphs (COR1 and COR2), and two wide-angle heliospheric imagers (HI1 and HI2). Technical descriptions of EUVI, COR1 and the HIs can be found in Wuelser et al. (2004), Thompson et al. (2003), and De se et al. (2003), respectively. The images produced by SECCHI represent a data visualization challenge: i) the images are 2048×2048 pixels (except for the HIs, which are usually binned onboard 2×2), thus the vast majority of computer displays are not able to display them at full frame and full r- olution, and ii) more importantly, the ve instruments of SECCHI A and B were designed to be able to track Coronal Mass Ejections from their onset (with EUVI) to their pro- gation in the heliosphere (with the HIs), which implies that a set of SECCHI images that covers the propagation of a CME from its initiation site to the Earth is composed of im- 1 ages with very different spatial resolutions - from 1. 7 arcsecondspixel for EUVI to 2. 15 1 arcminutespixel for HI2, i. e. 75 times larger. A similar situation exists with the angular scales of the physical objects, since the size of a CME varies by orders of magnitude as it expands in the heliosphere. 296 pp. Englisch.…

Taschenbuch. Condition: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -The SECCHI A and B instrument suites (Howard et al. , 2006) onboard the two STEREO mission spacecraft (Kaiser, 2005) are each composed of: one Extreme Ultra-Violet Imager (EUVI), two white-light coronagraphs (COR1 and COR2), and two wide-angle heliospheric imagers (HI1 and HI2). Technical descriptions of EUVI, COR1 and the HIs can be found in Wuelser et al. (2004), Thompson et al. (2003), and De se et al. (2003), respectively. The images produced by SECCHI represent a data visualization challenge: i) the images are 2048×2048 pixels (except for the HIs, which are usually binned onboard 2×2), thus the vast majority of computer displays are not able to display them at full frame and full r- olution, and ii) more importantly, the ve instruments of SECCHI A and B were designed to be able to track Coronal Mass Ejections from their onset (with EUVI) to their pro- gation in the heliosphere (with the HIs), which implies that a set of SECCHI images that covers the propagation of a CME from its initiation site to the Earth is composed of im- 1 ages with very different spatial resolutions - from 1. 7 arcsecondspixel for EUVI to 2. 15 1 arcminutespixel for HI2, i. e. 75 times larger. A similar situation exists with the angular scales of the physical objects, since the size of a CME varies by orders of magnitude as it expands in the heliosphere. 296 pp. Englisch.…

Condition: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Only book that focuses on the intersection between the fields of solar physics and image processingDiscusses state-of-the-art techniquesThe SECCHI A and B instrument suites (Howard et al. , 2006) onboard the two STEREO mission spacecraft (. …

Condition: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Only book that focuses on the intersection between the fields of solar physics and image processingDiscusses state-of-the-art techniquesThe SECCHI A and B instrument suites (Howard et al. , 2006) onboard the two STEREO mission spacecraft (. …

Buch. Condition: Neu. nach der Bestellung gedruckt Neuware - Printed after ordering - The SECCHI A and B instrument suites (Howard et al. , 2006) onboard the two STEREO mission spacecraft (Kaiser, 2005) are each composed of: one Extreme Ultra-Violet Imager (EUVI), two white-light coronagraphs (COR1 and COR2), and two wide-angle heliospheric imagers (HI1 and HI2). Technical descriptions of EUVI, COR1 and the HIs can be found in Wuelser et al. (2004), Thompson et al. (2003), and De se et al. (2003), respectively. The images produced by SECCHI represent a data visualization challenge: i) the images are 2048×2048 pixels (except for the HIs, which are usually binned onboard 2×2), thus the vast majority of computer displays are not able to display them at full frame and full r- olution, and ii) more importantly, the ve instruments of SECCHI A and B were designed to be able to track Coronal Mass Ejections from their onset (with EUVI) to their pro- gation in the heliosphere (with the HIs), which implies that a set of SECCHI images that covers the propagation of a CME from its initiation site to the Earth is composed of im- 1 ages with very different spatial resolutions - from 1. 7 arcsecondspixel for EUVI to 2. 15 1 arcminutespixel for HI2, i. e. 75 times larger. A similar situation exists with the angular scales of the physical objects, since the size of a CME varies by orders of magnitude as it expands in the heliosphere.…