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E-grāmata: Lunar Domes: Properties and Formation Processes

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  • Formāts: PDF+DRM
  • Sērija : Springer Praxis Books
  • Izdošanas datums: 28-Mar-2013
  • Izdevniecība: Springer Verlag
  • Valoda: eng
  • ISBN-13: 9788847026377
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Lunar Domes: Properties and Formation ProcessesPalielināt
  • Formāts: PDF+DRM
  • Sērija : Springer Praxis Books
  • Izdošanas datums: 28-Mar-2013
  • Izdevniecība: Springer Verlag
  • Valoda: eng
  • ISBN-13: 9788847026377
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Lunar domes are structures of volcanic origin which are usually difficult to observe due to their low heights. The Lunar Domes Handbook is a reference work on these elusive features. It provides a collection of images for a large number of lunar domes, including telescopic images acquired with advanced but still moderately intricate amateur equipment as well as recent orbital spacecraft images. Different methods for determining the morphometric properties of lunar domes (diameter, height, flank slope, edifice volume) from image data or orbital topographic data are discussed. Additionally, multispectral and hyperspectral image data are examined, providing insights into the composition of the dome material. Several classification schemes for lunar domes are described, including an approach based on the determined morphometric quantities and spectral analyses. Furthermore, the book provides a description of geophysical models of lunar domes, which yield information about the properties of the lava from which they formed and the depth of the magma source regions below the lunar surface.



This book offers a uniform collection of probe and CCD terrestrial images for each lunar dome, and presents information on morphological measurements and rheologic properties including a novel classification system and a new map of the distribution of domes.

Recenzijas

From the reviews:

In probably the first book ever focused on lunar domes, Lena (independent scholar) and colleagues review what is known about them and add new data. descriptions will interest mainly lunar specialists and perhaps observers looking for viewing targets on the moon. The authors have clearly studied lunar domes in great detail and assembled a wealth of data on them . Summing Up: Recommended. Graduate students through professionals. (B. M. Simonson, Choice, Vol. 51 (4), December, 2013)

Part I Lunar Domes Morphometry, Geophysical Modelling and Formation Processes
1 Volcanism on the Earth and the Moon: Morphometry and Eruption Conditions
3(20)
1.1 Volcanic Processes and Formation of Volcanic Edifices on the Earth and the Moon
3(3)
1.2 Physical Parameters of Dome Formation
6(1)
1.3 Lunar Pyroclastic Deposits
6(2)
1.4 Lunar Cones
8(1)
1.5 Vents of Effusive Lunar Domes
9(1)
1.6 Localization of Lunar Domes
10(13)
1.6.1 Domes in the Maria
10(1)
1.6.2 Domes Inside Craters
10(1)
1.6.3 Domes in Highland Regions
10(5)
1.6.4 Domes Bisected by Rilles
15(3)
1.6.5 Domes with Non-volcanic Hills and Linear Rilles on their Surface
18(1)
1.6.6 Domes with Concentric Craters on their Summit
18(2)
1.6.7 Aligned Lunar Domes, Formation along Crustal Fractures
20(1)
1.6.8 Lunar Intrusive Domes
21(2)
2 Lunar Domes: Morphometric and Rheologic Properties
23(16)
2.1 Observing Lunar Domes
23(1)
2.2 Images Rendered Based on Topographic Data
24(1)
2.3 Image-Based Photogrammetric Measurements
25(2)
2.4 Determination of Morphometric Properties
27(7)
2.4.1 Shadow Length Measurements
27(2)
2.4.2 Photoclinometry and Shape from Shading
29(4)
2.4.3 A Combined DEM Construction Approach
33(1)
2.5 Modelling of Rheologic Properties
34(2)
2.6 Monogenetic and Non-Monogenetic Lunar Effusive Domes
36(1)
2.7 Classification Schemes Based on Qualitative Morphologic Features
36(2)
2.7.1 The Classification Scheme by Westfall (1964)
36(2)
2.7.2 The Classification Scheme by Head and Gifford (1980)
38(1)
2.8 Conclusion
38(1)
3 Determination of Spectral Properties
39(10)
3.1 Spectral Ratios
39(2)
3.2 Diagnostic Spectral Parameters
41(3)
3.3 Petrographic Maps
44(5)
4 Modelling of Lunar Effusive and Intrusive Domes
49(10)
4.1 Modelling of Feeder Dike Dimensions
49(3)
4.2 Time Scales Relevant During Dome Formation
52(2)
4.3 Laccolith Modelling of Putative Intrusive Domes
54(5)
4.3.1 Arguments Against and In Favour of an Intrusive Origin
54(1)
4.3.2 Laccolith Modelling
55(1)
4.3.3 Comparison with Terrestrial Laccoliths
56(3)
5 Lunar Domes Classification Scheme
59(10)
5.1 Classification Based on Principal Component Analysis
59(4)
5.2 Non-monogenetic Lunar Effusive Domes
63(1)
5.3 Classes of Lunar Intrusive Domes
63(2)
5.4 Conclusion
65(4)
Part II Guide to Observing Lunar Domes on the Moon
6 Effusive Bisected Lunar Domes
69(10)
6.1 The Birt Domes
69(3)
6.2 The Domes near the Crater Menelaus
72(5)
6.3 The Bisected Dome near Gassendi
77(2)
7 Effusive Lunar Domes
79(56)
7.1 Effusive Lunar Domes Located from Selenographic Longitude 0° to 90° East
79(26)
7.1.1 Mare Tranquillitatis
79(10)
7.1.2 Mare Vaporum and Hyginus
89(1)
7.1.3 Autolycus
90(1)
7.1.4 Meton
91(4)
7.1.5 Rupes Altai and Piccolomini
95(1)
7.1.6 Fracastorius
96(1)
7.1.7 Mare Fecunditatis
97(1)
7.1.8 Vendelinus
98(2)
7.1.9 Mare Crisium and Yerkes
100(1)
7.1.10 Petavius
101(2)
7.1.11 Mare Undarum
103(2)
7.2 Effusive Lunar Domes Located from Selenographic Longitude 0° to 90° West
105(30)
7.2.1 Palus Putredinis
105(2)
7.2.2 Mare Frigoris and Region Around Archytas
107(1)
7.2.3 Dome Suite near Hortensius and Domes and Swells Between Milichius and Tobias Mayer, Mare Nubium and Aristarchus
108(8)
7.2.4 Capuanus and Palus Epidemiarum
116(2)
7.2.5 Region Around C. Herschel in Mare Imbrium and Sinus Iridum
118(2)
7.2.6 The Doppelmayer Region
120(4)
7.2.7 Region Around Mee
124(1)
7.2.8 Gruithuisen Region
125(2)
7.2.9 Mons Hansten
127(1)
7.2.10 Marius Hills
127(4)
7.2.11 Mons Rumker
131(4)
8 Candidate Lunar Intrusive Domes
135(10)
9 Conclusion
145(4)
Appendix A Lunar dome images 149(8)
Appendix B Further Resources 157(6)
References 163(8)
Index 171
Raffaello Lena was born in Rome on September 1959. He received the Master degree in Pharmaceutical Sciences from the University of Rome La Sapienza in 1985 and the Doctorate degree in Pharmaceutical Sciences from the University of Rome La Sapienza in 1989 in the field of synthesis and pharmacological properties of new molecules. He currently works for the Italian Ministry of Health in Rome, Italy, on food safety. Concerning strictly to astronomic topics he founded the Geologic Lunar Research (GLR) group, association involved in lunar geology and study of lunar domes and their classification. GLR group has produced dozens of published studies of lunar domes, faults and transient phenomena, including a novel classification scheme based on studies carried out during several years (see list below), some of which published in professional Journals (Icarus, PSS). The lunar studies carried out by our group allows to understand the physical conditions and processes of lunar dome eruptions.
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