000			03261nam a22005055i 4500
001			978-88-470-2637-7
003			DE-He213
005			20140220082929.0
007			cr nn 008mamaa
008			130330s2013 it | s |||| 0|eng d
020			_a9788847026377 _9978-88-470-2637-7
024	7		_a10.1007/978-88-470-2637-7 _2doi
050		4	_aQB460-466
072		7	_aPHVB _2bicssc
072		7	_aSCI005000 _2bisacsh
082	0	4	_a523.01 _223
100	1		_aLena, Raffaello. _eauthor.
245	1	0	_aLunar Domes _h[electronic resource] : _bProperties and Formation Processes / _cby Raffaello Lena, Christian Wöhler, Jim Phillips, Maria Teresa Chiocchetta.
264		1	_aMilano : _bSpringer Milan : _bImprint: Springer, _c2013.
300			_aXIII, 174 p. 145 illus., 10 illus. in color. _bonline resource.
336			_atext _btxt _2rdacontent
337			_acomputer _bc _2rdamedia
338			_aonline resource _bcr _2rdacarrier
347			_atext file _bPDF _2rda
490	1		_aSpringer Praxis Books
505	0		_aVolcanism on the Earth and the Moon: morphometry and eruption conditions -- Lunar domes: morphometric and rheologic properties -- Determination of spectral properties -- Determination Modelling of lunar effusive and intrusive domes -- Lunar domes classification scheme -- Effusive bisected lunar domes -- Effusive lunar domes -- Candidate lunar intrusive domes -- Conclusion -- Appendix A: Lunar dome images -- Appendix B: Further Resources -- References.
520			_aLunar 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.
650		0	_aPhysics.
650		0	_aPlanetology.
650		0	_aComputer vision.
650	1	4	_aPhysics.
650	2	4	_aAstrophysics and Astroparticles.
650	2	4	_aPlanetology.
650	2	4	_aImage Processing and Computer Vision.
700	1		_aWöhler, Christian. _eauthor.
700	1		_aPhillips, Jim. _eauthor.
700	1		_aChiocchetta, Maria Teresa. _eauthor.
710	2		_aSpringerLink (Online service)
773	0		_tSpringer eBooks
776	0	8	_iPrinted edition: _z9788847026360
830		0	_aSpringer Praxis Books
856	4	0	_uhttp://dx.doi.org/10.1007/978-88-470-2637-7
912			_aZDB-2-PHA
999			_c99209 _d99209